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Publications

To acknowledge the support by DFG within the priority program SPP 1992 please add the following acknowledgement to your publications:

XX acknowledges the support of the DFG priority program SPP 1992 “Exploring the Diversity of Extrasolar Planets (XX XXXX/XX)”

Current number of publications: 389

Year
  • 2018
  • 2019
  • 2020
  • 2021
  • 2022
  • 2023
  • 2024
  1. E. W. Guenther, E. Goffo, D. Sebastian, A. M. S. Smith, C. M. Persson, M. Fridlund, D. Gandolfi, J. Korth

    A new mass and radius determination of the ultra-short period planet K2-106b and the fluffy planet K2-106c

    bib

    @misc{guenther2024new,
    title={A new mass and radius determination of the ultra-short period planet K2-106b and the fluffy planet K2-106c},
    author={E. W. Guenther and E. Goffo and D. Sebastian and A. M. S. Smith and C. M. Persson and M. Fridlund and D. Gandolfi and J. Korth},
    year={2024},
    eprint={2402.09322},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP}
    }

    arXiv
  2. L. M. Bernabò, Sz. Csizmadia, A. M. S. Smith, H. Rauer, A. P. Hatzes, M. Esposito, D. Gandolfi, J. Cabrera

    Evidence of apsidal motion and a possible co-moving companion star detected in the WASP-19 system

    bib

    @article{Bernabo_2024,
    title={Evidence of apsidal motion and a possible co-moving companion star detected in the WASP-19 system},
    ISSN={1432-0746},
    url={http://dx.doi.org/10.1051/0004-6361/202346852},
    DOI={10.1051/0004-6361/202346852},
    journal={Astronomy & Astrophysics},
    publisher={EDP Sciences},
    author={Bernabo, L.M. and Csizmadia, Sz. and Smith, A.M.S. and Rauer, H. and Hatzes, A. and Esposito, M. and Gandolfi, D. and Cabrera, J.},
    year={2024},
    month=jan }

    DOI arXiv
  3. B. Akinsanmi, S. C. C. Barros, M. Lendl, L. Carone, P. E. Cubillos, A. Bekkelien, A. Fortier, H. -G. Florén, A. Collier Cameron, G. Boué, G. Bruno, B. O. Demory, A. Brandeker, S. G. Sousa, T. G. Wilson, A. Deline, A. Bonfanti, G. Scandariato, M. J. Hooton, A. C. M. Correia, O. D. S. Demangeon, A. M. S. Smith, V. Singh, Y. Alibert, R. Alonso, J. Asquier,, T. Bárczy, D. Barrado Navascues, W. Baumjohann, M. Beck, T. Beck, W. Benz, N. Billot, X. Bonfils, L. Borsato, C. Broeg, M. Buder, S. Charnoz, Sz. Csizmadia, M. B. Davies, M. Deleuil, L. Delrez, D. Ehrenreich, A. Erikson, J. Farinato, L. Fossati, M. C. V. Fridlund, D. Gandolfi, M. Gillon, M. Guedel, M. N. Guenther, A. Heitzmann, Ch. Helling, S. Hoyer, K. G. Isaak, L. Kiss, K. W. F. Lam, J. Laskar, A. Lecavelier des Etangs, D. Magrin, P. F. L. Maxted, M. Mecina, C. Mordasini, V. Nascimbeni, G. Olofsson, R. Ottensamer, I. Pagano, E. Pallé, G. Peter, D. Piazza, G. Piotto, D. Pollacco, D. Queloz, R. Ragazzoni, N. Rando, H. Rauer, I. Ribas, N. C. Santos, D. Ségransan, A. E. Simon, M. Stalport, G. M. Szabó, N. Thomas, S. Udry, V. Van Grootel, J. Venturini, E. Villaver, N. A. Walton

    The tidal deformation and atmosphere of WASP-12b from its phase curve

    bib

    @misc{akinsanmi2024tidal,
    title={The tidal deformation and atmosphere of WASP-12b from its phase curve},
    author={B. Akinsanmi and S. C. C. Barros and M. Lendl and L. Carone and P. E. Cubillos and A. Bekkelien and A. Fortier and H. -G. Florén and A. Collier Cameron and G. Boué and G. Bruno and B. -O. Demory and A. Brandeker and S. G. Sousa and T. G. Wilson and A. Deline and A. Bonfanti and G. Scandariato and M. J. Hooton and A. C. M. Correia and O. D. S. Demangeon and A. M. S. Smith and V. Singh and Y. Alibert and R. Alonso and J. Asquier and T. Bárczy and D. Barrado Navascues and W. Baumjohann and M. Beck and T. Beck and W. Benz and N. Billot and X. Bonfils and L. Borsato and Ch. Broeg and M. Buder and S. Charnoz and Sz. Csizmadia and M. B. Davies and M. Deleuil and L. Delrez and D. Ehrenreich and A. Erikson and J. Farinato and L. Fossati and M. Fridlund and D. Gandolfi and M. Gillon and M. Güdel and M. N. Günther and A. Heitzmann and Ch. Helling and S. Hoyer and K. G. Isaak and L. L. Kiss and K. W. F. Lam and J. Laskar and A. Lecavelier des Etangs and D. Magrin and P. F. L. Maxted and M. Mecina and Ch. Mordasini and V. Nascimbeni and G. Olofsson and R. Ottensamer and I. Pagano and E. Pallé and G. Peter and D. Piazza and G. Piotto and D. Pollacco and D. Queloz and R. Ragazzoni and N. Rando and H. Rauer and I. Ribas and N. C. Santos and D. Ségransan and A. E. Simon and M. Stalport and Gy. M. Szabó and N. Thomas and S. Udry and V. Van Grootel and J. Venturini and E. Villaver and N. A. Walton},
    year={2024},
    eprint={2402.10486},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP}
    }

    arXiv
  4. M. Nowak, S. Lacour, R. Abuter, A. Amorim, R. Asensio-Torres, W. Balmer, M. Benisty, J. -P. Berger, H. Beust, S. Blunt, A. Boccaletti, M. Bonnefoy, H. Bonnet, M. S. Bordoni, G. Bourdarot, W. Brandner, F. Cantalloube, B. Charnay, G. Chauvin, A. Chavez, E. Choquet, V. Christiaens, Y. Clénet, V. Coudé du Foresto, A. Cridland, G. R. Davies, R. Dembet, J. Dexter, A. Drescher, G. Duvert, A. Eckart, F. Eisenhauer, N. M. Foerster Schreiber, P. Garcia, R. Garcia Lopez, T. Gardner, E. Gendron, R. Genzel, S. Gillessen, J. H. Girard, S. Grant, X. Haubois, G. Heißel, T. Henning, S. Hinkley, S. Hippler, M. Houllé, Z. Hubert, L. Jocou, J. Kammerer, M. Keppler, P. Kervella, L. Kreidberg, N. T. Kurtovic, A. M. Lagrange, V. Lapeyrère, J. -B. Le Bouquin, P. Léna, D. Lutz, A. L. Maire, F. Mang, G.-D. Marleau, A. Mérand, J. D. Monnier, C. Mordasini, D. Mouillet, E. Nasedkin, G. P. P. L. Otten, T. Ott, C. Paladini, T. Paumard, K. Perraut, G. Perrin, O. Pfuhl, N. Pourré, L. Pueyo, D. C. Ribeiro, E. Rickman, Z. Rustamkulov, J. Shangguan, T. Shimizu, D. K. Sing, E. Stadler, T. Stolker, O. Straub, C. Straubmeier, E. Sturm, M. Subroweit, L. J. Tacconi, E. van Dishoeck, A. Vigan, F. Vincent, S. D. Fellenberg, J. J. Wang, F. Widmann, T. Winterhalder, J. Woillez, S. Yazici, A. Young, the GRAVITY Collaboration

    A catalogue of dual-field interferometric binary calibrators

    bib

    @misc{nowak2024catalogue,
    title={A catalogue of dual-field interferometric binary calibrators},
    author={M. Nowak and S. Lacour and R. Abuter and A. Amorim and R. Asensio-Torres and W. O. Balmer and M. Benisty and J. -P. Berger and H. Beust and S. Blunt and A. Boccaletti and M. Bonnefoy and H. Bonnet and M. S. Bordoni and G. Bourdarot and W. Brandner and F. Cantalloube and B. Charnay and G. Chauvin and A. Chavez and E. Choquet and V. Christiaens and Y. Clénet and V. Coudé du Foresto and A. Cridland and R. Davies and R. Dembet and J. Dexter and A. Drescher and G. Duvert and A. Eckart and F. Eisenhauer and N. M. Förster Schreiber and P. Garcia and R. Garcia Lopez and T. Gardner and E. Gendron and R. Genzel and S. Gillessen and J. H. Girard and S. Grant and X. Haubois and G. Heißel and T. Henning and S. Hinkley and S. Hippler and M. Houllé and Z. Hubert and L. Jocou and J. Kammerer and M. Keppler and P. Kervella and L. Kreidberg and N. T. Kurtovic and A. -M. Lagrange and V. Lapeyrère and J. -B. Le Bouquin and P. Léna and D. Lutz and A. -L. Maire and F. Mang and G. -D. Marleau and A. Mérand and J. D. Monnier and C. Mordasini and D. Mouillet and E. Nasedkin and T. Ott and G. P. P. L. Otten and C. Paladini and T. Paumard and K. Perraut and G. Perrin and O. Pfuh and N. Pourré and L. Pueyo and D. C. Ribeiro and E. Rickman and Z. Rustamkulov and J. Shangguan and T. Shimizu and D. Sing and J. Stadler and T. Stolker and O. Straub and C. Straubmeier and E. Sturm and M. Subroweit and L. J. Tacconi and E. F. van Dishoeck and A. Vigan and F. Vincent and S. D. von Fellenberg and J. J. Wang and F. Widmann and T. O. Winterhalder and J. Woillez and Ş. Yazıcı and A. Young and the GRAVITY Collaboration},
    year={2024},
    eprint={2402.05019},
    archivePrefix={arXiv},
    primaryClass={astro-ph.IM}
    }

    arXiv
  5. G. Andama, J. Mah, B. Bitsch

    Which stars can form planets: Planetesimal formation at low metallicities

    bib

    @misc{andama2024stars,
    title={Which stars can form planets: Planetesimal formation at low metallicities},
    author={Geoffrey Andama and Jingyi Mah and Bertram Bitsch},
    year={2024},
    eprint={2401.16155},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP}
    }

    arXiv
  6. S. Dreizler, R. Luque, I. Ribas, V. Koseleva, H. L. Ruh, E. Nagel, F. J. Pozuelos, M. Zechmeister, A. Reiners, J. A. Caballero, P. J. Amado, V. J. S. Béjar, J. L. Bean, M. Brady, C. Cifuentes, M. Gillon, A. P. Hatzes, Th. Henning, D. Kasper, D. Montes, J. C. Morales, C. Murray, E. Pallé, A. Quirrenbach, A. Seifahrt, A. Schweitzer, J. Stürmer, G. Kári Stefánsson, J. I. Vico-Linares

    Teegarden’s Star revisited: A nearby planetary system with at least three planets

    bib

    @misc{dreizler2024teegardens,
    title={Teegarden's Star revisited: A nearby planetary system with at least three planets},
    author={S. Dreizler and R. Luque and I. Ribas and V. Koseleva and H. L. Ruh and E. Nagel and F. J. Pozuelos and M. Zechmeister and A. Reiners and J. A. Caballero and P. J. Amado and V. J. S. Béjar and J. L. Bean and M. Brady and C. Cifuentes and M. Gillon and A. P. Hatzes and Th. Henning and D. Kasper and D. Montes and J. C. Morales and C. A. Murray and E. Pallé and A. Quirrenbach and A. Seifahrt and A. Schweitzer and J. Stürmer and G. Stefánsson and J. I. Vico Linares},
    year={2024},
    eprint={2402.00923},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP}
    }

    arXiv
  7. P. Wulff, U. R. Christensen, W. Dietrich, J. Wicht

    The Effects of a Stably Stratified Region with radially varying Electrical Conductivity on the Formation of Zonal Winds on Gas Planets

    bib

    @misc{wulff2024effects,
    title={The Effects of a Stably Stratified Region with radially varying Electrical Conductivity on the Formation of Zonal Winds on Gas Planets},
    author={Paula N. Wulff and Ulrich R. Christensen and Wieland Dietrich and Johannes Wicht},
    year={2024},
    eprint={2402.00073},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP}
    }

    arXiv
  8. A. Psaridi, H. P. Osborn, F. Bouchy, M. Lendl, L. Parc, N. Billot, C. Broeg, S. G. Sousa, V. Adibekyan, O. Attia, A. Bonfanti, A. Chakraborty, K. A. Collins, J. Davoult, E. Delgado Mena, N. Grieves, T. Guillot, A. Heitzmann, R. Helled, C. Hellier, J. M. Jenkins, R. Luque, T. G. Wilson, J. N. Winn, C. Ziegler, J. Venturini, Y. Alibert, A. Brandeker, W. Baumjohann, X. Bonfils, Sz. Csizmadia, M. Beck, T. Beck, M. Deleuil, B. O. Demory, M. Fridlund, A. Lecavelier des Etangs, D. Magrin, C. Mordasini, G. Piotto, D. Pollacco, H. Rauer, N. Rando, R. West, C. N. Watkins, N. A. Walton, I. Walter, E. Villaver, V. Van Grootel, C. Corral Van Damme, S. Udry, T. A. Pritchard, N. Thomas, G. M. Szabó, M. Steller, M. Stalport, A. M. S. Smith, A. Simon, G. Scandariato, D. Ségransan, S. Seager, I. Ribas, C. Reimers, D. Ramos, R. Ragazzoni, D. Queloz, G. Peter, E. Pallé, I. Pagano, R. Ottensamer, G. Olofsson, L. D. Nielsen, V. Nascimbeni, F. Murgas, P. F. L. Maxted, K. W. F. Lam, L. Kiss, J. Laskar, J. Hagelberg, M. Guedel, P. E. Cubillos, S. Charnoz, A. Deline, L. Delrez, K. G. Isaak, S. Hoyer, D. Ehrenreich, T. Daylan, C. Helling, S. McDermott, C. Lovis

    Discovery of two warm mini-Neptunes with contrasting densities orbiting the young K3V star TOI-815

    bib

    @misc{psaridi2024discovery,
    title={Discovery of two warm mini-Neptunes with contrasting densities orbiting the young K3V star TOI-815},
    author={Angelica Psaridi and Hugh Osborn and François Bouchy and Monika Lendl and Léna Parc and Nicolas Billot and Christopher Broeg and Sérgio G. Sousa and Vardan Adibekyan and Omar Attia and Andrea Bonfanti and Hritam Chakraborty and Karen A. Collins and Jeanne Davoult and Elisa Delgado-Mena and Nolan Grieves and Tristan Guillot and Alexis Heitzmann and Ravit Helled and Coel Hellier and Jon M. Jenkins and Henrik Knierim and Andreas Krenn and JackJ. Lissauer and Rafael Luque and David Rapetti and Nuno C. Santos and Olga Suárez and Julia Venturini and Francis P. Wilkin and Thomas G. Wilson and Joshua N. Winn and Carl Ziegler and Tiziano Zingales and Yann Alibert and Alexis Brandeker and Jo Ann Egger and Davide Gandolfi and Matthew J. Hooton and Amy Tuson and Solène Ulmer-Moll and Lyu Abe and Romain Allart and Roi Alonso and David R. Anderson and Guillem Anglada and Tamas Bárczy and David Barrado and Susana C. C. Barros and Wolfgang Baumjohann and Mathias Beck and Thomas Beck and Willy Benz and Xavier Bonfils and Luca Borsato and Vincent Bourrier and David R. Ciardi and Andrew Collier Cameron and Sébastien Charnoz and Marion Cointepas and Szilárd Csizmadia and Patricio Cubillos and Gaspare Lo Curto and Melvyn B. Davies and Tansu Daylan and Magali Deleuil and Adrien Deline and Laetitia Delrez and Olivier D. S. Demangeon and Brice-Olivier Demory and Caroline Dorn and Xavier Dumusque and David Ehrenreich and Anders Erikson and Alain Lecavelier des Etangs and Elena Diana de Miguel Ferreras and Andrea Fortier and Luca Fossati and Yolanda G. C. Frensch and Malcolm Fridlund and Michaël Gillon and Manuel Güdel and Maximilian N. Günther and Janis Hagelberg and Christiane Helling and Sergio Hoyer and Kate G. Isaak and Laszlo L. Kiss and Kristine Lam and Jacques Laskar and Baptiste Lavie and Christophe Lovis and Demetrio Magrin and Luca Marafatto and Pierre Maxted and Scott McDermott and Djamel Mékarnia and Christoph Mordasini and Felipe Murgas and Valerio Nascimbeni and Louise D. Nielsen and Göran Olofsson and Roland Ottensamer and Isabella Pagano and Enric Pallé and Gisbert Peter and Giampaolo Piotto and Don Pollacco and Didier Queloz and Roberto Ragazzoni and Devin Ramos and Nicola Rando and Heike Rauer and Christian Reimers and Ignasi Ribas and Sara Seager and Damien Ségransan and Gaetano Scandariato and Attila Simon and Alexis M. S. Smith and Manu Stalport and Manfred Steller and Gyula Szabó and Nicolas Thomas and Tyler A. Pritchard and Stéphane Udry and Carlos Corral Van Damme and Valérie Van Grootel and Eva Villaver and Ingo Walter and Nicholas Walton and Cristilyn N. Watkins and Richard G. West},
    year={2024},
    eprint={2401.15709},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP}
    }

    arXiv
  9. T. Rometsch, L. M. Jordan, T.W. Moldenhauer, D. Wehner, S. Rendon Restrepo, T. W. A. Müller, G. Picogna, W. Kley, C. P. Dullemond

    FargoCPT: A 2D Multi-Physics Code for Simulating the Interaction of Disks with Stars, Planets and Particles

    bib

    @misc{rometsch2024fargocpt,
    title={FargoCPT: A 2D Multi-Physics Code for Simulating the Interaction of Disks with Stars, Planets and Particles},
    author={Thomas Rometsch and Lucas M. Jordan and Tobias W. Moldenhauer and Dennis Wehner and Steven Rendon Restrepo and Tobias W. A. Müller and Giovanni Picogna and Wilhelm Kley and Cornelis P. Dullemond},
    year={2024},
    eprint={2401.16203},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP}
    }

    arXiv
  10. G.-D. Marleau, Y. Aoyama, J. Hashimoto, Y. Zhou

    Revisiting the Helium and Hydrogen Accretion Indicators at TWA 27B: Weak Mass Flow at Near-Freefall Velocity

    bib

    @misc{marleau2024revisiting,
    title={Revisiting the Helium and Hydrogen Accretion Indicators at TWA 27B: Weak Mass Flow at Near-Freefall Velocity},
    author={Gabriel-Dominique Marleau and Yuhiko Aoyama and Jun Hashimoto and Yifan Zhou},
    year={2024},
    eprint={2401.04763},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP}
    }

    arXiv
  11. E. Brown, S. C. Marsden, S. V. Jeffers, A. Heitzmann, J. R. Barnes, C. P. Folsom

    The variable magnetic field of V889 Her and the challenge of detecting exoplanets around young Suns using Gaussian process regression

    bib

    @misc{brown2024variable,
    title={The variable magnetic field of V889 Her and the challenge of detecting exoplanets around young Suns using Gaussian process regression},
    author={E. L. Brown and S. C. Marsden and S. V. Jeffers and A. Heitzmann and J. R. Barnes and C. P. Folsom},
    year={2024},
    eprint={2401.12408},
    archivePrefix={arXiv},
    primaryClass={astro-ph.SR}
    }

    DOI arXiv
  12. L. Benkendorff, F. Flammini Dotti, K. Stock, M. X. Cai, R. Spurzem

    Hot Jupiter formation in dense star clusters

    bib

    @misc{benkendorff2024hot,
    title={Hot Jupiter Formation in Dense Star Clusters},
    author={Leonard Benkendorff and Francesco Flammini Dotti and Katja Stock and Maxwell Xu Cai and Rainer Spurzem},
    year={2024},
    eprint={2401.11613},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP}
    }

    arXiv
  13. Y. Shan, D. Revilla, S. L. Skrzypinski, S. Dreizler, V. J. S. Béjar, J. A. Caballero, C. Cardona Guillén, C. Cifuentes, B. Fuhrmeister, A. Reiners, S. Vanaverbeke, I. Ribas, A. Quirrenbach, P. J. Amado, F. J. Aceituno, V. Casanova, M. Cortés-Contreras, F. Dubois, P. Gorrini, Th. Henning, E. Herrero, S. V. Jeffers, J. Kemmer, S. Lalitha, N. Lodieu, L. Logie, M. J. López-González, S. Martín-Ruiz, D. Montes, J. C. Morales, E. Nagel, E. Pallé, V. Perdelwitz, M. Pérez-Torres, D. Pollacco, S. Rau, C. Rodríguez López, E. Rodríguez, P. Schöfer, W. Seifert, A. Sota, M. R. Zapatero Osorio, M. Zechmeister

    CARMENES input catalog of M dwarfs: VII. New rotation periods for the survey stars and their correlations with stellar activity

    bib

    @misc{shan2024carmenes,
    title={CARMENES input catalog of M dwarfs: VII. New rotation periods for the survey stars and their correlations with stellar activity},
    author={Yutong Shan and Daniel Revilla and Sebastian L. Skrzypinski and Stefan Dreizler and Victor J. S. Bejar and Jose A. Caballero and Carlos Cardona Guillen and Carlos Cifuentes and Birgit Fuhrmeister and Ansgar Reiners and Siegfried Vanaverbeke and Ignasi Ribas and Andreas Quirrenbach and Pedro J. Amado and Francisco J. Aceituno and Victor Casanova and Miriam Cortes-Contreras and Franky Dubois and Paula Gorrini and Thomas Henning and Enrique Herrero and Sandra V. Jeffers and Jonas Kemmer and Sairam Lalitha and Nicolas Lodieu and Ludwig Logie and Maria J. Lopez Gonzalez and Susanna Martin-Ruiz and David Montes and Juan Carlos Morales and Evangelos Nagel and Enric Palle and Volker Perdelwitz and Miguel Perez-Torres and Don Pollacco and Steve Rau and Cristina Rodriguez Lopez and Eloy Rodriguez and Patrick Schoefer and Walter Seifert and Alfredo Sota and Maria Rosa Zapatero Osorio and Mathias Zechmeister},
    year={2024},
    eprint={2401.09550},
    archivePrefix={arXiv},
    primaryClass={astro-ph.SR}
    }

    arXiv
  14. S. Czesla, M. Lampón, D. Cont, F. Lesjak, J. Orell-Miquel, J. Sanz-Forcada, E. Nagel, L. Nortmann, K. Molaverdikhani, M. López-Puertas, F. Yan, A. Quirrenbach, J. A. Caballero, E. Pallé, J. Aceituno, P. J. Amado, Th. Henning, S. Khalafinejad, D. Montes, A. Reiners, I. Ribas, A. Schweitzer

    The elusive atmosphere of WASP-12 b / High-resolution transmission spectroscopy with CARMENES

    bib

    @misc{czesla2024elusive,
    title={The elusive atmosphere of WASP-12 b / High-resolution transmission spectroscopy with CARMENES},
    author={S. Czesla and M. Lampón and D. Cont and F. Lesjak and J. Orell-Miquel and J. Sanz-Forcada and E. Nagel and L. Nortmann and K. Molaverdikhani and M. López-Puertas and F. Yan and A. Quirrenbach and J. A. Caballero and E. Pallé and J. Aceituno and P. J. Amado and Th. Henning and S. Khalafinejad and D. Montes and A. Reiners and I. Ribas and A. Schweitzer},
    year={2024},
    eprint={2401.02195},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP}
    }

    arXiv
  15. K. Namekata, V. S. Airapetian, P. Petit, H. Maehara, K. Ikuta, S. Inoue, R. R. Paudel, Z. Arzoumanian, A. A. Avramova-Boncheva, K. Gendreau, S. V. Jeffers, S. Marsden, M. Mori, C. Neiner, A. A. Vidotto, K. Shibata

    Multiwavelength Campaign Observations of a Young Solar-type Star, EK Draconis. I. Discovery of Prominence Eruptions Associated with Superflares

    bib

    @misc{namekata2023multiwavelength,
    title={Multiwavelength Campaign Observations of a Young Solar-type Star, EK Draconis. I. Discovery of Prominence Eruptions Associated with Superflares},
    author={Kosuke Namekata and Vladimir S. Airapetian and Pascal Petit and Hiroyuki Maehara and Kai Ikuta and Shun Inoue and Yuta Notsu and Rishi R. Paudel and Zaven Arzoumanian and Antoaneta A. Avramova-Boncheva and Keith Gendreau and Sandra V. Jeffers and Stephen Marsden and Julien Morin and Coralie Neiner and Aline A. Vidotto and Kazunari Shibata},
    year={2023},
    eprint={2311.07380},
    archivePrefix={arXiv},
    primaryClass={astro-ph.SR}
    }

    arXiv
  16. M. I. Swayne, P. F. L. Maxted, A. Triaud, S. G. Sousa, A. Deline, D. Ehrenreich, S. Hoyer, G. Olofsson, I. Boisse, A. Duck, S. Gill, D. Martin, J. McCormac, C. M. Persson, A. Santerne, D. Sebastian, M. R. Standing, L. Acuna, Y. Alibert, R. Alonso, G. Anglada, T. Bárczy, D. Barrado Navascues, S. C. C. Barros, W. Baumjohann, T. A. Baycroft, M. Beck, T. Beck, W. Benz, N. Billot, X. Bonfils, L. Borsato, V. Bourrier, A. Brandeker, C. Broeg, A. Carmona, S. Charnoz, A. Collier Cameron, P. Cortés-Zuleta, Sz. Csizmadia, P. E. Cubillos, M. B. Davies, M. Deleuil, X. Delfosse, L. Delrez, O. D. S. Demangeon, B. O. Demory, G. Dransfield, A. Erikson, A. Fortier, T. Forveille, L. Fossati, M. Fridlund, D. Gandolfi, M. Gillon, M. Guedel, M. N. Guenther, N. Hara, E. M. Hébrard, N. Heidari, C. Hellier, Ch. Helling, K. G. Isaak, F. Kerschbaum, F. Kiefer, L. Kiss, V. Kunovac, S. Lalitha, K. W. F. Lam, J. Laskar, A. Lecavelier des Etangs, M. Lendl, D. Magrin, L. Marafatto, E. Martioli, N. J. Miller, C. Mordasini, C. Moutou, V. Nascimbeni, R. Ottensamer, I. Pagano, E. Pallé, G. Peter, D. Piazza, G. Piotto, D. Pollacco, D. Queloz, R. Ragazzoni, N. Rando, H. Rauer, I. Ribas, N. C. Santos, G. Scandariato, D. Ségransan, A. E. Simon, A. M. S. Smith, J. Southworth, M. Stalport, G. M. Szabó, N. Thomas, S. Udry, B. Ulmer, V. Van Grootel, J. Venturini, N. A. Walton, E. Willett, T. G. Wilson

    The EBLM Project- XI. Mass, radius, and effective temperature measurements for 23 M-dwarf companions to solar-type stars observed with CHEOPS

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    year={2023},
    eprint={2312.11339},
    archivePrefix={arXiv},
    primaryClass={astro-ph.SR}
    }

    DOI arXiv
  17. N. Nossir, L. Dalil-Essakali, A. Belafhal

    Generation of optical vortices by flat-topped beam diffracted with a radial phase shift spiral zone plate

    DOI
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    VLTI/GRAVITY Provides Evidence the Young, Substellar Companion HD 136164 Ab Formed Like a “Failed Star”

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    archivePrefix={arXiv},
    primaryClass={astro-ph.SR}
    }

    DOI arXiv
  19. J. D. Melon Fuksman, M. Flock, H. Klahr

    Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks II. Secondary instabilities and stability regions

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    @misc{fuksman2023vertical,
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    eprint={2312.06890},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP}
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    arXiv
  20. C. Dominik, C. P. Dullemond

    The bouncing barrier revisited: Impact on key planet formation processes and observational signatures

    bib

    @misc{dominik2023bouncing,
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    author={Carsten Dominik and Cornelis Dullemond},
    year={2023},
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    archivePrefix={arXiv},
    primaryClass={astro-ph.EP}
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    arXiv
  21. A. Bonfanti, M. Brady, T. G. Wilson, J. Venturini, J. A. Egger, A. Brandeker, S. G. Sousa, M. Lendl, A. E. Simon, D. Queloz, G. Olofsson, V. Adibekyan, Y. Alibert, L. Fossati, M. J. Hooton, D. Kubyshkina, R. Luque, F. Murgas, A. J. Mustill, N. C. Santos, V. Van Grootel, R. Alonso, J. Asquier,, T. Bandy, T. Bárczy, D. Barrado Navascues, S. C. C. Barros, W. Baumjohann, J. L. Bean, M. Beck, T. Beck, W. Benz, M. Bergomi, N. Billot, L. Borsato, C. Broeg, A. Collier Cameron, Sz. Csizmadia, P. E. Cubillos, M. B. Davies, M. Deleuil, A. Deline, L. Delrez, O. D. S. Demangeon, B. O. Demory, D. Ehrenreich, A. Erikson, A. Fortier, M. C. V. Fridlund, D. Gandolfi, M. Gillon, M. Guedel, M. N. Guenther, A. Heitzmann, Ch. Helling, S. Hoyer, K. G. Isaak, D. Kasper, L. Kiss, K. W. F. Lam, J. Laskar, A. Lecavelier des Etangs, D. Magrin, P. F. L. Maxted, C. Mordasini, V. Nascimbeni, R. Ottensamer, I. Pagano, E. Pallé, G. Peter, G. Piotto, D. Pollacco, R. Ragazzoni, N. Rando, H. Rauer, I. Ribas, G. Scandariato, D. Ségransan, A. Seifahrt, A. M. S. Smith, M. Stalport, G. Kári Stefánsson, M. Steinberger, J. Stürmer, G. M. Szabó, N. Thomas, S. Udry, E. Villaver, N. A. Walton, K. Westerdorff, T. Zingales

    Characterising TOI-732 b and c: New insights into the M-dwarf radius and density valley

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  22. E. Pallé, K. Biazzo, E. Bolmont, P. Mollière, K. Poppenhaeger, J. Birkby, M. Brogi, G. Chauvin, A. Chiavassa, H. J. Hoeijmakers, E. Lellouch, C. Lovis, R. Maiolino, L. Nortmann, H. Parviainen, L. Pino, M. Turbet, J. Wender, S. Albrecht, S. Antoniucci, S. C. C. Barros, A. Beaudoin, B. Benneke, I. Boisse, A. S. Bonomo, F. Borsa, A. Brandeker, W. Brandner, L. A. Buchhave, A. -L. Cheffot, R. Deborde, F. Debras, R. Doyon, P. Di Marcantonio, P. Giacobbe, J. I. González Hernández, R. Helled, L. Kreidberg, P. Machado, J. Maldonado, A. Marconi, B. L. Canto Martins, A. Miceli, C. Mordasini, M. N'Diaye, A. Niedzielski, B. Nisini, M. Zechmeister, A. Zanutta, A. Simonnin, E. Rauscher, S. Reffert, N. Sanna

    Ground-breaking Exoplanet Science with the ANDES spectrograph at the ELT

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    eprint={2311.17075},
    archivePrefix={arXiv},
    primaryClass={astro-ph.IM}
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    arXiv
  23. A. Krieger, S. Wolf

    Improving Monte Carlo radiative transfer in the regime of high optical depths: The minimum scattering order

    bib

    @misc{krieger2023improving,
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    year={2023},
    eprint={2311.13252},
    archivePrefix={arXiv},
    primaryClass={astro-ph.IM}
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    arXiv
  24. J. -V. Harre, A. M. S. Smith

    The Apparent Tidal Decay of WASP-4 b Can Be Explained by the Rømer Effect

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    @article{Harre_2023,
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    arXiv
  25. K. Herbst, A. Bartenschlager, J. L. Grenfell, N. Iro, M. Sinnhuber, B. Taysum, F. Wunderlich, N. Engelbrecht, J. Light, K. Moloto, J. -V. Harre, H. Rauer, F. Schreier

    Impact of Cosmic Rays on Atmospheric Ion Chemistry and Spectral Transmission Features of TRAPPIST-1e

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    year={2023},
    eprint={2311.04684},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP}
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    arXiv
  26. S. Kálmán, Sz. Csizmadia, A. E. Simon, K. W. F. Lam, A. Deline, J. -V. Harre, G. M. Szabó

    Modelling the light curves of transiting exomoons: a zero-order photodynamic agent added to the Transit and Light Curve Modeller

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    @misc{kálmán2023modelling,
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    year={2023},
    eprint={2311.04647},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP}
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    DOI arXiv
  27. V. Singh, G. Scandariato, A. M. S. Smith, P. E. Cubillos, M. Lendl, N. Billot, A. Fortier, D. Queloz, S. G. Sousa, Sz. Csizmadia, A. Brandeker, L. Carone, T. G. Wilson, B. Akinsanmi, J. A. Patel, A. Krenn, O. D. S. Demangeon, G. Bruno, I. Pagano, M. J. Hooton, J. Cabrera, N. C. Santos, Y. Alibert, R. Alonso, J. Asquier,, T. Bárczy, D. Barrado Navascues, S. C. C. Barros, W. Baumjohann, M. Beck, T. Beck, W. Benz, M. Bergomi, A. Bonfanti, X. Bonfils, L. Borsato, C. Broeg, S. Charnoz, A. Collier Cameron, M. B. Davies, M. Deleuil, A. Deline, L. Delrez, B. O. Demory, D. Ehrenreich, A. Erikson, L. Fossati, M. Fridlund, D. Gandolfi, M. Gillon, M. Guedel, M. N. Guenther, J. -V. Harre, A. Heitzmann, Ch. Helling, S. Hoyer, K. G. Isaak, L. Kiss, K. W. F. Lam, J. Laskar, A. Lecavelier des Etangs, D. Magrin, P. F. L. Maxted, H. Mischler, C. Mordasini, V. Nascimbeni, G. Olofsson, R. Ottensamer, E. Pallé, G. Peter, G. Piotto, D. Pollacco, R. Ragazzoni, N. Rando, H. Rauer, I. Ribas, S. Salmon, D. Ségransan, A. E. Simon, M. Stalport, M. Steinberger, G. M. Szabó, N. Thomas, S. Udry, B. Ulmer, V. Van Grootel, J. Venturini, E. Villaver, N. A. Walton, T. Zingales

    CHEOPS observations of KELT-20 b/MASCARA-2 b: an aligned orbit and signs of variability from a reflective dayside

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    arXiv
  28. M. Rengel, J. Adamczewski

    Radiative transfer and inversion codes for characterizing planetary atmospheres: an overview

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    url = {https://doi.org/10.3389%2Ffspas.2023.1176740},

    year = 2023,
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    publisher = {Frontiers Media {SA}
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    volume = {10},

    author = {M. Rengel and J. Adamczewski},

    title = {Radiative transfer and inversion codes for characterizing planetary atmospheres: an overview},

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    DOI arXiv
  29. A. Krieger, S. Wolf

    Improving Monte Carlo radiative transfer simulations: A shift of framework

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    arXiv
  30. H. L. M. Osborne, V. Van Eylen, E. Goffo, D. Gandolfi, G. Nowak, C. M. Persson, J. Livingston, A. Weeks, E. Pallé, R. Luque, C. Hellier, I. Carleo, S. Redfield, T. Hirano, M. Garbaccio Gili, J. Alarcon, O. Barragán, N. Casasayas-Barris, M. R. Díaz, M. Esposito, J. S. Jenkins, E. Knudstrup, F. Murgas, J. Orell-Miquel, F. Rodler, L. M. Serrano, M. Stangret, S. H. Albrecht, A. Alqasim, W. D. Cochran, H. J. Deeg, M. Fridlund, A. P. Hatzes, J. Korth, K. W. F. Lam

    TOI-544 b: a potential water-world inside the radius valley in a two-planet system

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    arXiv
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    arXiv
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    arXiv
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    arXiv
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    arXiv
  35. C. Danti, B. Bitsch, J. Mah

    Composition of giant planets: the roles of pebbles and planetesimals

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    arXiv
  36. S. K. Betti, K. B. Follete, K. Ward-Duong, A. E. Peck, Y. Aoyama, J. Bary, B. Dacus, B. Edwards, G.-D. Marleau, K. Mohamed, J. Palmo, C. Plunkett, C. Robinson, H. Wang

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    arXiv
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    Microlensing Discovery and Characterization Efficiency in the Vera C. Rubin Legacy Survey of Space and Time

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    arXiv
  38. S. V. Jeffers, S. Kiefer, T. S. Metcalfe

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    arXiv
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    arXiv
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    arXiv
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    Lens mass estimate in the Galactic disk extreme parallax microlensing event Gaia19dke

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    arXiv
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    arXiv
  45. J. Mah, B. Bitsch, I. Pascucci, T. Henning

    Close-in ice lines and the super-stellar C/O ratio in discs around very low-mass stars

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    arXiv
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    arXiv
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    @misc{metcalfe2023asteroseismology,
    title={Asteroseismology and Spectropolarimetry of the Exoplanet Host Star $\lambda$ Serpentis},
    author={Travis S. Metcalfe and Derek Buzasi and Daniel Huber and Marc H. Pinsonneault and Jennifer L. van Saders and Thomas R. Ayres and Sarbani Basu and Jeremy J. Drake and Ricky Egeland and Oleg Kochukhov and Pascal Petit and Steven H. Saar and Victor See and Keivan G. Stassun and Yaguang Li and Timothy R. Bedding and Sylvain N. Breton and Adam J. Finley and Rafael A. Garcia and Hans Kjeldsen and Martin B. Nielsen and J. M. Joel Ong and Jakob L. Rorsted and Amalie Stokholm and Mark L. Winther and Catherine A. Clark and Diego Godoy-Rivera and Ilya V. Ilyin and Klaus G. Strassmeier and Sandra V. Jeffers and Stephen C. Marsden and Aline A. Vidotto and Sallie Baliunas and Willie Soon},
    year={2023},
    eprint={2308.09808},
    archivePrefix={arXiv},
    primaryClass={astro-ph.SR}
    }

    arXiv
  49. J. A. Patel, J. A. Egger, T. G. Wilson, V. Bourrier, L. Carone, M. Beck, D. Ehrenreich, S. G. Sousa, W. Benz, A. Deline, Y. Alibert, K. W. F. Lam, M. Lendl, R. Alonso, G. Anglada, T. Bárczy, D. Barrado, S. C. C. Barros, W. Baumjohann, T. Beck, N. Billot, X. Bonfils, C. Broeg, M. D. Busch, J. Cabrera, S. Charnoz, A. Collier Cameron, Sz. Csizmadia, M. B. Davies, M. Deleuil, L. Delrez, O. D. S. Demangeon, B. O. Demory, A. Erikson, A. Fortier, L. Fossati, M. Fridlund, D. Gandolfi, M. Gillon, M. Guedel, K. Heng, S. Hoyer, K. G. Isaak, L. Kiss, E. Kopp, J. Laskar, A. Lecavelier des Etangs, C. Lovis, D. Magrin, P. F. L. Maxted, V. Nascimbeni, G. Olofsson, R. Ottensamer, I. Pagano, E. Pallé, G. Peter, G. Piotto, D. Pollacco, D. Queloz, R. Ragazzoni, N. Rando, F. Ratti, H. Rauer, I. Ribas, N. C. Santos, G. Scandariato, D. Ségransan, A. E. Simon, A. M. S. Smith, M. Steller, G. M. Szabó, N. Thomas, B. Ulmer, V. Van Grootel, V. Viotto, N. A. Walton

    CHEOPS and TESS view of the ultra-short period super-Earth TOI-561 b

    bib

    @misc{patel2023cheops,
    title={CHEOPS and TESS view of the ultra-short period super-Earth TOI-561 b},
    author={J. A. Patel and J. A. Egger and T. G. Wilson and V. Bourrier and L. Carone and M. Beck and D. Ehrenreich and S. G. Sousa and W. Benz and A. Brandeker and A. Deline and Y. Alibert and K. W. F. Lam and M. Lendl and R. Alonso and G. Anglada and T. Bárczy and D. Barrado and S. C. C. Barros and W. Baumjohann and T. Beck and N. Billot and X. Bonfils and C. Broeg and M. -D. Busch and J. Cabrera and S. Charnoz and A. Collier Cameron and Sz. Csizmadia and M. B. Davies and M. Deleuil and L. Delrez and O. D. S. Demangeon and B. -O. Demory and A. Erikson and A. Fortier and L. Fossati and M. Fridlund and D. Gandolfi and M. Gillon and M. Güdel and K. Heng and S. Hoyer and K. G. Isaak and L. L. Kiss and E. Kopp and J. Laskar and A. Lecavelier des Etangs and C. Lovis and D. Magrin and P. F. L. Maxted and V. Nascimbeni and G. Olofsson and R. Ottensamer and I. Pagano and E. Pallé and G. Peter and G. Piotto and D. Pollacco and D. Queloz and R. Ragazzoni and N. Rando and F. Ratti and H. Rauer and I. Ribas and N. C. Santos and G. Scandariato and D. Ségransan and A. E. Simon and A. M. S. Smith and M. Steller and Gy. M. Szabó and N. Thomas and S. Udry and B. Ulmer and V. Van Grootel and V. Viotto and N. A. Walton},
    year={2023},
    eprint={2308.08687},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP}
    }

    arXiv
  50. J. A. Patel, J. A. Egger, T. G. Wilson, V. Bourrier, L. Carone, M. Beck, D. Ehrenreich, S. G. Sousa, W. Benz, A. Brandeker, A. Deline, Y. Alibert, K. W. F. Lam, M. Lendl, R. Alonso, G. Anglada, T. Bárczy, D. Barrado, S. C. C. Barros, W. Baumjohann, T. Beck, N. Billot, X. Bonfils, C. Broeg, M. D. Busch, J. Cabrera, S. Charnoz, A. Collier Cameron, Sz. Csizmadia, M. B. Davies, M. Deleuil, L. Delrez, O. D. S. Demangeon, B. O. Demory, A. Erikson, A. Fortier, L. Fossati, M. C. V. Fridlund, D. Gandolfi, M. Gillon, M. Guedel, K. Heng, S. Hoyer, K. G. Isaak, L. Kiss, E. Kopp, J. Laskar, A. Lecavelier des Etangs, C. Lovis, D. Magrin, P. F. L. Maxted, V. Nascimbeni, G. Olofsson, R. Ottensamer, I. Pagano, E. Pallé, G. Peter, G. Piotto, D. Pollacco, D. Queloz, R. Ragazzoni, N. Rando, F. Ratti, H. Rauer, I. Ribas, N. C. Santos, G. Scandariato, D. Ségransan, A. E. Simon, A. M. S. Smith, M. Steller, G. M. Szabó, N. Thomas, S. Udry, B. Ulmer, V. Van Grootel, V. Viotto, N. A. Walton

    CHEOPS and TESS view of the ultra-short-period super-Earth TOI-561 b

    bib

    @article{Patel_2023,
    title={CHEOPS and TESS view of the ultra-short-period super-Earth TOI-561 b},
    volume={679},
    ISSN={1432-0746},
    url={http://dx.doi.org/10.1051/0004-6361/202244946},
    DOI={10.1051/0004-6361/202244946},
    journal={Astronomy & Astrophysics},
    publisher={EDP Sciences},
    author={Patel, J. A. and Egger, J. A. and Wilson, T. G. and Bourrier, V. and Carone, L. and Beck, M. and Ehrenreich, D. and Sousa, S. G. and Benz, W. and Brandeker, A. and Deline, A. and Alibert, Y. and Lam, K. W. F. and Lendl, M. and Alonso, R. and Anglada, G. and Bárczy, T. and Barrado, D. and Barros, S. C. C. and Baumjohann, W. and Beck, T. and Billot, N. and Bonfils, X. and Broeg, C. and Busch, M.-D. and Cabrera, J. and Charnoz, S. and Collier Cameron, A. and Csizmadia, Sz. and Davies, M. B. and Deleuil, M. and Delrez, L. and Demangeon, O. D. S. and Demory, B.-O. and Erikson, A. and Fortier, A. and Fossati, L. and Fridlund, M. and Gandolfi, D. and Gillon, M. and Güdel, M. and Heng, K. and Hoyer, S. and Isaak, K. G. and Kiss, L. L. and Kopp, E. and Laskar, J. and Lecavelier des Etangs, A. and Lovis, C. and Magrin, D. and Maxted, P. F. L. and Nascimbeni, V. and Olofsson, G. and Ottensamer, R. and Pagano, I. and Pallé, E. and Peter, G. and Piotto, G. and Pollacco, D. and Queloz, D. and Ragazzoni, R. and Rando, N. and Ratti, F. and Rauer, H. and Ribas, I. and Santos, N. C. and Scandariato, G. and Ségransan, D. and Simon, A. E. and Smith, A. M. S. and Steller, M. and Szabó, Gy. M. and Thomas, N. and Udry, S. and Ulmer, B. and Van Grootel, V. and Viotto, V. and Walton, N. A.},
    year={2023},
    month=nov, pages={A92} }

    DOI arXiv
  51. J. -V. Harre, A. M. S. Smith, T. Hirano, Sz. Csizmadia, A. Triaud, D. R. Anderson

    The Orbit of Warm Jupiter WASP-106 b is aligned with its Star

    bib

    @misc{harre2023orbit,
    title={The Orbit of Warm Jupiter WASP-106 b is aligned with its Star},
    author={Jan-Vincent Harre and Alexis M. S. Smith and Teruyuki Hirano and Szilárd Csizmadia and Amaury H. M. J. Triaud and David R. Anderson},
    year={2023},
    eprint={2308.07165},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP}
    }

    arXiv
  52. D. Muley, J. D. Melon Fuksman, H. Klahr

    Three-temperature radiation hydrodynamics with PLUTO: Tests and applications to protoplanetary disks

    bib

    @misc{muley2023threetemperature,
    title={Three-temperature radiation hydrodynamics with PLUTO: Tests and applications to protoplanetary disks},
    author={Dhruv Muley and Julio David Melon Fuksman and Hubert Klahr},
    year={2023},
    eprint={2308.03504},
    archivePrefix={arXiv},
    primaryClass={astro-ph.IM}
    }

    arXiv
  53. D. Hintz, S. Peacock, T. Barman, B. Fuhrmeister, E. Nagel, A. Schweitzer, S. V. Jeffers, I. Ribas, A. Reiners, A. Quirrenbach, P. J. Amado, V. J. S. Béjar, J. A. Caballero, A. P. Hatzes, D. Montes

    Modeling the Chromosphere and Transition Region of Planet-hosting Star GJ 436

    bib

    @misc{hintz2023modeling,
    title={Modeling the Chromosphere and Transition Region of Planet-hosting Star GJ 436},
    author={Dominik Hintz and Sarah Peacock and Travis Barman and Birgit Fuhrmeister and Evangelos Nagel and Andreas Schweitzer and Sandra V. Jeffers and Ignasi Ribas and Ansgar Reiners and Andreas Quirrenbach and Pedro J. Amado and Victor J. S. Bejar and Jose A. Caballero and Artie P. Hatzes and David Montes},
    year={2023},
    eprint={2307.13857},
    archivePrefix={arXiv},
    primaryClass={astro-ph.SR}
    }

    arXiv
  54. F. Lesjak, L. Nortmann, F. Yan, D. Cont, A. Reiners, N. Piskunov, A. P. Hatzes, L. Boldt-Christmas, S. Czesla, U. Heiter, O. Kochukhov, A. Lavail, E. Nagel, A. D. Rains, M. Rengel, F. Rodler, U. Seemann, D. Shulyak

    Retrieval of the dayside atmosphere of WASP-43b with CRIRES+

    bib

    @misc{lesjak2023retrieval,
    title={Retrieval of the dayside atmosphere of WASP-43b with CRIRES+},
    author={F. Lesjak and L. Nortmann and F. Yan and D. Cont and A. Reiners and N. Piskunov and A. Hatzes and L. Boldt-Christmas and S. Czesla and U. Heiter and O. Kochukhov and A. Lavail and E. Nagel and A. D. Rains and M. Rengel and F. Rodler and U. Seemann and D. Shulyak},
    year={2023},
    eprint={2307.11627},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP}
    }

    arXiv
  55. J. Cabrera, D. Gandolfi, L. M. Serrano, Sz. Csizmadia, J. A. Egger, P. Baumeister, A. Krenn, W. Benz, A. Deline, H. -G. Florén, A. Collier Cameron, V. Adibekyan, Y. Alibert, S. E. Bellomo, L. Delrez, L. Fossati, A. Fortier, S. Grziwa, S. Hoyer, A. Bonfanti, S. Salmon, S. G. Sousa, T. G. Wilson, J. Alarcon, R. Alonso, G. Anglada-Escudé, T. Bárczy, O. Barragán, D. Barrado, S. C. C. Barros, W. Baumjohann, M. Beck, T. Beck, L. M. Bernabò, N. Billot, X. Bonfils, L. Borsato, A. Brandeker, C. Broeg, Ó. Carrión-González, S. Charnoz, D. R. Ciardi, W. D. Cochran, K. A. Collins, K. I. Collins, D. M. Conti, M. B. Davies, H. J. Deeg, M. Deleuil, O. D. S. Demangeon, B. O. Demory, D. Ehrenreich, A. Erikson, M. Esposito, M. C. V. Fridlund, M. Gillon, E. Goffo, M. Guedel, E. W. Guenther, J. -V. Harre, K. Heng, M. J. Hooton, K. G. Isaak, J. M. Jenkins, L. Kiss, E. Knudstrup, K. W. F. Lam, J. Laskar, A. Lecavelier des Etangs, M. Lendl, C. Lovis, R. Luque, D. Magrin, P. F. L. Maxted, A. Muresan, V. Nascimbeni, G. Olofsson, H. P. Osborn, H. L. M. Osborne, R. Ottensamer, I. Pagano, E. Pallé, C. M. Persson, G. Peter, G. Piotto, D. Pollacco, D. Queloz, R. Ragazzoni, N. Rando, H. Rauer, S. Redfield, I. Ribas, G. R. Ricker, F. Rodler, N. C. Santos, G. Scandariato, S. Seager, D. Ségransan, A. E. Simon, A. M. S. Smith, M. Steller, G. M. Szabó, N. Thomas, N. Tosi, J. D. Twicken, S. Udry, V. Van Eylen, V. Van Grootel, N. A. Walton, J. N. Winn

    The planetary system around HD 190622 (TOI-1054). Measuring the gas content of low-mass planets orbiting F-stars

    DOI
  56. G.-D. Marleau, R. Kuiper, W. Béthune, C. Mordasini

    The Planetary Accretion Shock. III. Smoothing-free 2.5D Simulations and Calculation of Hα Emission

    bib

    @article{Marleau_2023,
    doi = {10.3847/1538-4357/accf12},

    url = {https://doi.org/10.3847%2F1538-4357%2Faccf12},

    year = 2023,
    month = {jul},

    publisher = {American Astronomical Society},

    volume = {952},

    number = {1},

    pages = {89},

    author = {Gabriel-Dominique Marleau and Rolf Kuiper and William B{\'{e}
    }thune and Christoph Mordasini},

    title = {The Planetary Accretion Shock. {III}. Smoothing-free 2.5D Simulations and Calculation of H$\upalpha$ Emission},

    journal = {The Astrophysical Journal}
    }

    DOI arXiv
  57. E. Goffo, D. Gandolfi, J. A. Egger, A. J. Mustill, S. H. Albrecht, T. Hirano, O. Kochukhov, N. Astudillo-Defru, O. Barragán, L. M. Serrano, A. P. Hatzes, Y. Alibert, E. W. Guenther, F. Dai, K. W. F. Lam, Sz. Csizmadia, A. M. S. Smith, L. Fossati, R. Luque, F. Rodler, M. L. Winther, J. L. Rørsted, J. Alarcon, X. Bonfils, W. D. Cochran, H. J. Deeg, J. M. Jenkins, J. Korth, J. H. Livingston, A. Meech, F. Murgas, J. Orell-Miquel, H. L. M. Osborne, E. Pallé, C. M. Persson, S. Redfield, G. R. Ricker, S. Seager, R. Vanderspek, V. Van Eylen, J. N. Winn

    Company for the ultra-high density, ultra-short period sub-Earth GJ 367 b: discovery of two additional low-mass planets at 11.5 and 34 days

    bib

    @misc{goffo2023company,
    title={Company for the ultra-high density, ultra-short period sub-Earth GJ 367 b: discovery of two additional low-mass planets at 11.5 and 34 days},
    author={Elisa Goffo and Davide Gandolfi and Jo Ann Egger and Alexander J. Mustill and Simon H. Albrecht and Teruyuki Hirano and Oleg Kochukhov and Nicola Astudillo-Defru and Oscar Barragan and Luisa M. Serrano and Artie P. Hatzes and Yann Alibert and Eike Guenther and Fei Dai and Kristine W. F. Lam and Szilárd Csizmadia and Alexis M. S. Smith and Luca Fossati and Rafael Luque and Florian Rodler and Mark L. Winther and Jakob L. Rørsted and Javier Alarcon and Xavier Bonfils and William D. Cochran and Hans J. Deeg and Jon M. Jenkins and Judith Korth and John H. Livingston and Annabella Meech and Felipe Murgas and Jaume Orell-Miquel and Hannah L. M. Osborne and Enric Palle and Carina M. Persson and Seth Redfield and George R. Ricker and Sara Seager and Roland Vanderspek and Vincent Van Eylen and Joshua N. Winn},
    year={2023},
    eprint={2307.09181},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP}
    }

    arXiv
  58. K. Barkaoui, F. J. Pozuelos, C. Hellier, B. Smalley, L. D. Nielsen, C. Dorn, P. Niraula, M. Gillon, J. de Wit, R. Helled, S. Müller, E. Jehin, B. O. Demory, V. Van Grootel, A. Soubkiou, M. Ghachoui, D. R. Anderson, Z. Benkhaldoun, F. Bouchy, A. Burdanov, L. Delrez, E. Ducrot, L. Garcia, A. Jabiri, M. Lendl, P. F. L. Maxted, C. Murray, P. Pihlmann Pedersen, D. Queloz, D. Sebastian, O. Turner, S. Udry, M. Timmermans, A. Triaud, R. G. West

    WASP-193b: An extremely low-density super-Neptune

    bib

    @misc{barkaoui2023wasp193b,
    title={WASP-193b: An extremely low-density super-Neptune},
    author={Khalid Barkaoui and Francisco J. Pozuelos and Coel Hellier and Barry Smalley and Louise D. Nielsen and Caroline Dorn and Prajwal Niraula and Michaël Gillon and Julien de Wit and Ravit Helled and Simon Müller and Emmanuel Jehin and Brice-Olivier Demory and V. Van Grootel and Abderahmane Soubkiou and Mourad Ghachoui and David. R. Anderson and Zouhair Benkhaldoun and Francois Bouchy and Artem Burdanov and Laetitia Delrez and Elsa Ducrot and Lionel Garcia and Abdelhadi Jabiri and Monika Lendl and Pierre F. L. Maxted and Catriona A. Murray and Peter Pihlmann Pedersen and Didier Queloz and Daniel Sebastian and Oliver Turner and Stephane Udry and Mathilde Timmermans and Amaury H. M. J. Triaud and Richard G. West},
    year={2023},
    eprint={2307.08350},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP}
    }

    arXiv
  59. A. Chomez, V. Squicciarini, A. M. Lagrange, P. Delorme, G. Viswanath, M. Janson, O. Flasseur, G. Chauvin, M. Langlois, P. Rubini, S. Bergeon, D. Albert, M. Bonnefoy, S. Desidera, N. Engler, R. Gratton, Th. Henning, E. E. Mamajek, G.-D. Marleau, M. R. Meyer, S. Reffert, S. C. Ringqvist, M. Samland

    An imaged 15Mjup companion within a hierarchical quadruple system

    bib

    @misc{chomez2023imaged,
    title={An imaged 15Mjup companion within a hierarchical quadruple system},
    author={A. Chomez and V. Squicciarini and A. -M. Lagrange and P. Delorme and G. Viswanath and M. Janson and O. Flasseur and G. Chauvin and M. Langlois and P. Rubini and S. Bergeon and D. Albert and M. Bonnefoy and S. Desidera and N. Engler and R. Gratton and T. Henning and E. E. Mamajek and G. -D. Marleau and M. R. Meyer and S. Reffert and S. C. Ringqvist and M. Samland},
    year={2023},
    eprint={2307.01195},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP}
    }

    arXiv
  60. P. Heeren, R. Tronsgaard, F. Grundahl, S. Reffert, A. Quirrenbach, P. L. Pallé

    Pyodine: an open, flexible reduction software for iodine-calibrated precise radial velocities

    bib

    @article{Heeren_2023,
    doi = {10.1051/0004-6361/202244441},

    url = {https://doi.org/10.1051%2F0004-6361%2F202244441},

    year = 2023,
    month = {jun},

    publisher = {{EDP} Sciences},

    volume = {674},

    pages = {A164},

    author = {Paul Heeren and Ren{\'{e}
    } Tronsgaard and Frank Grundahl and Sabine Reffert and Andreas Quirrenbach and Pere L. Pall{\'{e}}},

    title = {Pyodine: an open, flexible reduction software for iodine-calibrated precise radial velocities},

    journal = {Astronomy {\&}amp$\mathsemicolon$ Astrophysics}
    }

    DOI arXiv
  61. P. Baumeister, N. Tosi

    ExoMDN: Rapid characterization of exoplanet interior structures with Mixture Density Networks

    bib

    @misc{baumeister2023exomdn,
    title={ExoMDN: Rapid characterization of exoplanet interior structures with Mixture Density Networks},
    author={Philipp Baumeister and Nicola Tosi},
    year={2023},
    eprint={2306.09002},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP}
    }

    arXiv
  62. K. G. Kislyakova, L. Noack, E. Sanchis, L. Fossati, G. G. Valyavin, G. J. Golabek, M. Guedel

    Induction heating of planetary interiors in white dwarf systems

    DOI
  63. P. Baumeister, N. Tosi, C. Brachmann, J. L. Grenfell, L. Noack

    Redox state and interior structure control on the long-term habitability of stagnant-lid planets

    bib

    @article{Baumeister_2023,
    doi = {10.1051/0004-6361/202245791},

    url = {https://doi.org/10.1051%2F0004-6361%2F202245791},

    year = 2023,
    month = {jul},

    publisher = {{EDP} Sciences},

    volume = {675},

    pages = {A122},

    author = {Philipp Baumeister and Nicola Tosi and Caroline Brachmann and John Lee Grenfell and Lena Noack},

    title = {Redox state and interior structure control on the long-term habitability of stagnant-lid planets},

    journal = {Astronomy {\&}amp$\mathsemicolon$ Astrophysics}
    }

    DOI arXiv
  64. S. Czesla, P. C. Schneider, J. H. M. M. Schmitt, S. Freund, M. Salvato, J. Buchner, J. Robrade

    Likelihood of the sky. Bayesian treatment of the geometric two-catalog matching problem

    DOI
  65. K. Wu, M. B. N. Kouwenhoven, R. Spurzem, X. Pang

    Influence of planets on debris disks in star clusters I: the 50 AU Jupiter

    bib

    @misc{wu2023influence,
    title={Influence of planets on debris disks in star clusters I: the 50 AU Jupiter},
    author={Kai Wu and M. B. N. Kouwenhoven and Rainer Spurzem and Xiaoying Pang},
    year={2023},
    eprint={2306.01283},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP}
    }

    DOI arXiv
  66. K. Wu, M. B. N. Kouwenhoven, R. Spurzem, X. Pang

    Influence of planets on debris discs in star clusters – I. The 50 au Jupiter

    bib

    article{Wu_2023,
    doi = {10.1093/mnras/stad1673},

    url = {https://doi.org/10.1093%2Fmnras%2Fstad1673},

    year = 2023,
    month = {jun},

    publisher = {Oxford University Press ({OUP})},

    volume = {523},

    number = {4},

    pages = {4801--4817},

    author = {Kai Wu and M B N Kouwenhoven and Rainer Spurzem and Xiaoying Pang},

    title = {Influence of planets on debris discs in star clusters {\textendash} I. The 50 au Jupiter},

    journal = {Monthly Notices of the Royal Astronomical Society}
    }

    DOI arXiv
  67. S. C. Marsden, D. Evensberget, E. Brown, C. Neiner, J. M. Seach, J. Morin, P. Petit, S. V. Jeffers, C. P. Folsom

    The magnetic field and stellar wind of the mature late-F star χ Draconis A

    bib

    @article{10.1093/mnras/stad925,
    author = {Marsden, S C and Evensberget, D and Brown, E L and Neiner, C and Seach, J M and Morin, J and Petit, P and Jeffers, S V and Folsom, C P},
    title = "{The magnetic field and stellar wind of the mature late-F star χ Draconis A}",
    journal = {Monthly Notices of the Royal Astronomical Society},
    volume = {522},
    number = {1},
    pages = {792-810},
    year = {2023},
    month = {03},
    abstract = "{F stars lie in the transition region between cool stars with dynamo generated fields and hot star fossil fields and offer an interesting window into the generation of magnetic fields in shallow convection zones. In this paper, we investigate the magnetic field of the mature F7V primary of the bright χ Draconis system. χ Dra was observed in circularly polarized light at four epochs from 2014 through to 2019 using the NARVAL spectropolarimeter at the Téléscope Bernard Lyot. Using the technique of least-squares deconvolution, we created high signal-to-noise line profiles from which we were able to measure the radial velocity of both the primary and secondary and use these to improve the orbital parameters of the system. Additionally, we used the technique of Zeeman Doppler imaging to reconstruct the large-scale magnetic field geometry of the primary at the four epochs. The magnetic maps show that χ Dra A has a predominately dipolar poloidal magnetic field at all epochs with the magnetic axis well aligned with the stellar rotation axis. The large-scale features of the magnetic field appear to be relatively stable over the ∼5 yr time base of our observations, with no evidence of any polarity reversals. We used the magnetic field maps to model the wind from χ Dra A at all epochs, showing that the mass-loss from the stellar wind of χ Dra A is 3–6 times the current solar value, while the angular momentum loss from the wind is around 3–4 times the solar value.}",
    issn = {0035-8711},
    doi = {10.1093/mnras/stad925},
    url = {https://doi.org/10.1093/mnras/stad925},
    eprint = {https://academic.oup.com/mnras/article-pdf/522/1/792/49994667/stad925.pdf},
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    DOI
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    arXiv
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  73. H. Klahr, H. Baehr, J. D. Melon Fuksman

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  75. S. Müller, R. Helled

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    arXiv
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    arXiv
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    title = {About the atomic and molecular databases in the planetary community -- A contribution in the Laboratory Astrophysics Data WG IAU 2022 GA session},

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    arXiv
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    The CARMENES search for exoplanets around M dwarfs. Wolf 1069 b: Earth-mass planet in the habitable zone of a nearby, very low-mass star

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    arXiv
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    arXiv
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    }n and A E Simon and L Fossati and C M Persson and M Fridlund and S Salmon and S Hoyer and H P Osborn and T G Wilson and I Y Georgieva and Gr Nowak and R Luque and J A Egger and V Abidekyan and R Alonso and G Anglada Escud{\'{e}} and T B{\'{a}}rczy and D Barrado and S C C Barros and W Baumjohann and T Beck and A Bekkelien and W Benz and N Billot and X Bonfils and A Brandeker and C Broeg and S Charnoz and A Collier Cameron and Sz Csizmadia and M B Davies and M Deleuil and L Delrez and O D S Demangeon and B-O Demory and D Ehrenreich and A Erikson and A Fortier and D Futyan and D Gandolfi and M Gillon and M Guedel and P Guterman and J Laskar and D W Latham and A Lecavelier des Etangs and M Lendl and C Lovis and K Heng and K G Isaak and L Kiss and D Magrin and P F L Maxted and V Nascimbeni and G Olofsson and R Ottensamer and I Pagano and E Pall{\'{e}} and G Peter and G Piotto and D Pollacco and D Queloz and I Ribas and R Ragazzoni and N Rando and H Rauer and N C Santos and G Scandariato and S Seager and D S{\'{e}}gransan and L M Serrano and A M S Smith and S G Sousa and M Steller and Gy M Szab{\'{o}} and N Thomas and S Udry and V Van Grootel and N A Walton and J N Winn},

    title = {Discovery of {TOI}-1260d and the characterisation of the multi-planet system},

    journal = {Monthly Notices of the Royal Astronomical Society}
    }

    arXiv
  104. K. W. F. Lam, J. Cabrera, M. J. Hooton, Y. Alibert, A. Bonfanti, M. Beck, A. Deline, H. -G. Florén, A. E. Simon, L. Fossati, C. M. Persson, M. C. V. Fridlund, S. Salmon, S. Hoyer, H. P. Osborn, T. G. Wilson, I. Georgieva, G. Nowak, R. Luque, J. A. Egger, V. Adibekyan, R. Alonso, G. Anglada-Escudé, T. Bárczy, D. Barrado, S. C. C. Barros, W. Baumjohann, T. Beck, A. Bekkelien, W. Benz, N. Billot, X. Bonfils, A. Brandeker, C. Broeg, S. Charnoz, A. Collier Cameron, Sz. Csizmadia, M. B. Davies, M. Deleuil, L. Delrez, O. D. S. Demangeon, B. O. Demory, D. Ehrenreich, A. Erikson, A. Fortier, D. Futyan, D. Gandolfi, M. Gillon, M. Guedel, P. Guterman, J. Laskar, D. W. Latham, A. Lecavelier des Etangs, M. Lendl, C. Lovis, K. Heng, K. G. Isaak, L. Kiss, D. Magrin, P. F. L. Maxted, V. Nascimbeni, G. Olofsson, R. Ottensamer, I. Pagano, E. Pallé, G. Peter, G. Piotto, D. Pollacco, D. Queloz, I. Ribas, R. Ragazzoni, N. Rando, H. Rauer, N. C. Santos, G. Scandariato, S. Seager, D. Ségransan, L. M. Serrano, A. M. S. Smith, S. G. Sousa, M. Steller, G. M. Szabó, N. Thomas, S. Udry, V. Van Grootel, N. A. Walton, J. N. Winn

    Discovery of TOI-1260d and the characterization of the multiplanet system

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    url = {https://doi.org/10.1093%2Fmnras%2Fstac3639},

    year = 2022,
    month = {dec},

    publisher = {Oxford University Press ({OUP})},

    volume = {519},

    number = {1},

    pages = {1437--1451},

    author = {K W F Lam and J Cabrera and M J Hooton and Y Alibert and A Bonfanti and M Beck and A Deline and H-G Flor{\'{e}
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    title = {Discovery of {TOI}-1260d and the characterization of the multiplanet system},

    journal = {Monthly Notices of the Royal Astronomical Society}
    }

    DOI arXiv
  105. B. Fuhrmeister, S. Czesla, V. Perdelwitz, E. Nagel, J. H. M. M. Schmitt, S. V. Jeffers, J. A. Caballero, M. Zechmeister, D. Montes, A. Reiners, Á. López-Gallifa, I. Ribas, A. Quirrenbach, P. J. Amado, D. Galadí-Enríquez, V. J. S. Béjar, C. Danielski, A. P. Hatzes, A. Kaminski, M. Kürster, J. C. Morales, M. R. Zapatero Osorio

    The CARMENES search for exoplanets around M dwarfs. Variability on long timescales as seen in chromospheric indicators

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    @misc{https://doi.org/10.48550/arxiv.2212.03514,
    doi = {10.48550/ARXIV.2212.03514},

    url = {https://arxiv.org/abs/2212.03514},

    author = {Fuhrmeister, B. and Czesla, S. and Perdelwitz, V. and Nagel, E. and Schmitt, J. H. M. M. and Jeffers, S. V. and Caballero, J. A. and Zechmeister, M. and Montes, D. and Reiners, A. and López-Gallifa, Á. and Ribas, I. and Quirrenbach, A. and Amado, P. J. and Galadí-Enríquez, D. and Béjar, V. J. S. and Danielski, C. and Hatzes, A. P. and Kaminski, A. and Kürster, M. and Morales, J. C. and Osorio, M. R. Zapatero},

    keywords = {Solar and Stellar Astrophysics (astro-ph.SR), Earth and Planetary Astrophysics (astro-ph.EP), FOS: Physical sciences, FOS: Physical sciences},

    title = {The CARMENES search for exoplanets around M dwarfs. Variability on long timescales as seen in chromospheric indicators},

    publisher = {arXiv},

    year = {2022},

    copyright = {Creative Commons Attribution Non Commercial No Derivatives 4.0 International}
    }

    arXiv
  106. V. J. Sterken, L. R. Baalmann, B. T. Draine, E. Godenko, K. Herbst, H. -W. Hsu, S. Hunziker, V. V. Izmodenov, R. Lallement, J. D. Slavin

    Dust in and Around the Heliosphere and Astrospheres

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    Planetary Line-to-accretion Luminosity Scaling Relations: Extrapolating to Higher-order Hydrogen Lines

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    @article{Marleau_2022,
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    url = {https://dx.doi.org/10.3847/2515-5172/acaa34},
    year = {2022},
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    publisher = {The American Astronomical Society},
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    pages = {262},
    author = {Gabriel-Dominique Marleau and Yuhiko Aoyama},
    title = {Planetary Line-to-accretion Luminosity Scaling Relations: Extrapolating to Higher-order Hydrogen Lines},
    journal = {Research Notes of the AAS},
    abstract = {Aoyama et al. provided scaling relations between hydrogen-line luminosities and the accretion luminosity for planetary-mass objects. These fits should be an improvement over blind extrapolations of stellar relations. The fits go up only to the n = 8 electron energy level, but higher-n Balmer lines have been observed in the near-UV with UVES. We extend the scaling relations to higher-n levels for the Balmer and other series by fitting the fit coefficients (a, b) themselves and extrapolating them. Within the assumption of an accretion shock as the source of line emission, these fits should be robust for accreting planetary-mass objects.}
    }

    DOI
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    Radial velocity confirmation of a hot super-Neptune discovered by TESS with a warm Saturn-mass companion

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    @misc{https://doi.org/10.48550/arxiv.2211.17035,
    doi = {10.48550/ARXIV.2211.17035},

    url = {https://arxiv.org/abs/2211.17035},

    author = {Knudstrup, E. and Gandolfi, D. and Nowak, G. and Persson, C. M. and Furlan, E. and Livingston, J. and Matthews, E. and Lundkvist, M. S. and Winther, M. L. and Rørsted, J. L. and Albrecht, S. H. and Goffo, E. and Carleo, I. and Deeg, H. J. and Collins, K. A. and Narita, N. and Isaacson, H. and Redfield, S. and Dai, F. and Hirano, T. and Murphy, J. M. Akana and Beard, C. and Buchhave, L. A. and Cary, S. and Chontos, A. and Crossfield, I. and Cochran, W. D. and Conti, D. and Dalba, P. A. and Esposito, M. and Fajardo-Acosta, S. and Giacalone, S. and Grunblatt, S. K. and Guerra, P. and Hatzes, A. P. and Holcomb, R. and Horta, F. G. and Howard, A. W. and Huber, D. and Jenkins, J. M. and Kabáth, P. and Kane, S. and Korth, J. and Lam, K. W. F. and Lester, K. V. and Matson, R. and McLeod, K. K. and Orell-Miquel, J. and Murgas, F. and Palle, E. and Polanski, A. S. and Ricker, G. and Robertson, P. and Rubenzahl, R. and Schlieder, J E. and Seager, S. and Smith, A. M. S. and Tenenbaum, P. and Turtelboom, E. and Vanderspek, R. and Weiss, L. and Winn, J.},

    keywords = {Earth and Planetary Astrophysics (astro-ph.EP), FOS: Physical sciences, FOS: Physical sciences},

    title = {Radial velocity confirmation of a hot super-Neptune discovered by TESS with a warm Saturn-mass companion},

    publisher = {arXiv},

    year = {2022},

    copyright = {Creative Commons Attribution 4.0 International}
    }

    arXiv
  109. A. Papaioannou, K. Herbst, T. Ramm, E. W. Cliver, D. Lario, A. M. Astrid

    Revisiting Empirical Solar Energetic Particle Scaling Relations I. Solar flares

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    url = {https://arxiv.org/abs/2211.15312},

    author = {Papaioannou, Athanasios and Herbst, Konstantin and Ramm, Tobias and Cliver, Edward W. and Lario, David and Veronig, Astrid M.},

    keywords = {Solar and Stellar Astrophysics (astro-ph.SR), High Energy Astrophysical Phenomena (astro-ph.HE), Space Physics (physics.space-ph), FOS: Physical sciences, FOS: Physical sciences},

    title = {Revisiting Empirical Solar Energetic Particle Scaling Relations I. Solar flares},

    publisher = {arXiv},

    year = {2022},

    copyright = {Creative Commons Attribution 4.0 International}
    }

    arXiv
  110. O. Zakhozhay, R. Launhardt, T. Trifonov, M. Kürster, S. Reffert, T. Henning, R. Brahm, J. I. Vines, G.-D. Marleau, J. A. Patel

    Radial velocity survey for planets around young stars (RVSPY). A transiting warm super-Jovian planet around HD 114082, a young star with a debris disk

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    url = {https://doi.org/10.1051%2F0004-6361%2F202244747},

    year = 2022,
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    publisher = {{EDP} Sciences},

    volume = {667},

    pages = {L14},

    author = {Olga V. Zakhozhay and Ralf Launhardt and Trifon Trifonov and Martin Kürster and Sabine Reffert and Thomas Henning and Rafael Brahm and Jos{\'{e}
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    title = {Radial velocity survey for planets around young stars ({RVSPY})},

    journal = {Astronomy {\&}amp$\mathsemicolon$ Astrophysics}
    }

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    Examining the orbital decay targets KELT-9 b, KELT-16 b and WASP-4 b, and the transit-timing variations of HD 97658 b

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    url = {https://arxiv.org/abs/2211.05646},

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    keywords = {Earth and Planetary Astrophysics (astro-ph.EP), FOS: Physical sciences, FOS: Physical sciences},

    title = {Examining the orbital decay targets KELT-9 b, KELT-16 b and WASP-4 b, and the transit-timing variations of HD 97658 b},

    publisher = {arXiv},

    year = {2022},

    copyright = {Creative Commons Attribution Non Commercial No Derivatives 4.0 International}
    }

    arXiv
  112. T. Pfeil, M. Cranmer, S. Ho, P. J. Armitage, T. Birnstiel, H. Klahr

    A Neural Network Subgrid Model of the Early Stages of Planet Formation

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    @misc{https://doi.org/10.48550/arxiv.2211.04160,
    doi = {10.48550/ARXIV.2211.04160},

    url = {https://arxiv.org/abs/2211.04160},

    author = {Pfeil, Thomas and Cranmer, Miles and Ho, Shirley and Armitage, Philip J. and Birnstiel, Tilman and Klahr, Hubert},

    keywords = {Earth and Planetary Astrophysics (astro-ph.EP), Machine Learning (cs.LG), FOS: Physical sciences, FOS: Physical sciences, FOS: Computer and information sciences, FOS: Computer and information sciences},

    title = {A Neural Network Subgrid Model of the Early Stages of Planet Formation},

    publisher = {arXiv},

    year = {2022},

    copyright = {arXiv.org perpetual, non-exclusive license}
    }

    arXiv
  113. F. Murgas, G. Nowak, T. Masseron, H. Parviainen, R. Luque, E. Pallé, J. Korth, I. Carleo, S. Csizmadia, E. Esparza-Borges, A. Alqasim, W. D. Cochran, F. Dai, H. J. Deeg, D. Gandolfi, E. Goffo, P. Kabáth, K. W. F. Lam, J. Livingston, A. Muresan, H. L. M. Osborne, C. M. Persson, L. M. Serrano, A. M. S. Smith, V. Van Eylen, J. Orell-Miquel, N. R. Hinkel, D. Galán, M. Puig-Subirà, M. Stangret, A. Fukui, T. Kagetani, N. Narita, D. R. Ciardi, C. Ziegler, C. Briceño, N. Law, A. W. Mann, J. M. Jenkins, D. W. Latham, S. N. Quinn, G. Ricker, S. Seager, A. Shporer, E. B. Ting, R. Vanderspek, J. N. Winn

    HD 20329b: An ultra-short-period planet around a solar-type star found by TESS

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    @misc{https://doi.org/10.48550/arxiv.2211.02547,
    doi = {10.48550/ARXIV.2211.02547},

    url = {https://arxiv.org/abs/2211.02547},

    author = {Murgas, F. and Nowak, G. and Masseron, T. and Parviainen, H. and Luque, R. and Pallé, E. and Korth, Judith and Carleo, I. and Csizmadia, Sz. and Esparza-Borges, E. and Alqasim, Ahlam and Cochran, William D. and Dai, Fei and Deeg, Hans J. and Gandolfi, D. and Goffo, Elisa and Kabáth, Petr and Lam, K. W. F. and Livingston, John and Muresan, Alexandra and Osborne, H. L. M. and Persson, Carina M. and Serrano, L. M. and Smith, Alexis M. S. and Van Eylen, Vincent and Orell-Miquel, J. and Hinkel, Natalie R. and Galán, D. and Puig-Subirà, M. and Stangret, M. and Fukui, A. and Kagetani, T. and Narita, N. and Ciardi, David R. and Boyle, Andrew W. and Ziegler, Carl and Briceño, César and Law, Nicholas and Mann, Andrew W. and Jenkins, Jon M. and Latham, David W. and Quinn, Samuel N. and Ricker, G. and Seager, S. and Shporer, Avi and Ting, Eric B. and Vanderspek, R. and Winn, Joshua N.},

    keywords = {Earth and Planetary Astrophysics (astro-ph.EP), Solar and Stellar Astrophysics (astro-ph.SR), FOS: Physical sciences, FOS: Physical sciences},

    title = {HD 20329b: An ultra-short-period planet around a solar-type star found by TESS},

    publisher = {arXiv},

    year = {2022},

    copyright = {Creative Commons Attribution 4.0 International}
    }

    arXiv
  114. J. Orell-Miquel, G. Nowak, F. Murgas, E. Pallé, G. Morello, R. Luque, M. Badenas-Agusti, I. Ribas, M. Lafarga, N. Espinoza, J. C. Morales, M. Zechmeister, A. Alqasim, W. D. Cochran, D. Gandolfi, E. Goffo, P. Kabáth, J. Korth, K. W. F. Lam, J. Livingston, A. Muresan, C. M. Persson, V. Van Eylen

    HD 191939 revisited: New and refined planet mass determinations, and a new planet in the habitable zone

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    year = 2023,
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    publisher = {{EDP} Sciences},

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    pages = {A40},

    author = {J. Orell-Miquel and G. Nowak and F. Murgas and E. Palle and G. Morello and R. Luque and M. Badenas-Agusti and I. Ribas and M. Lafarga and N. Espinoza and J. C. Morales and M. Zechmeister and A. Alqasim and W. D. Cochran and D. Gandolfi and E. Goffo and P. Kab{\'{a}
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    title = {{HD} 191939 revisited: New and refined planet mass determinations, and a new planet in the habitable zone},

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    DOI arXiv
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    TOI-2196 b: Rare planet in the hot Neptune desert transiting a G-type star

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    publisher = {{EDP} Sciences},

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    pages = {A184},

    author = {Carina M. Persson and Iskra Y. Georgieva and Davide Gandolfi and Lorena Acuna and Artem Aguichine and Alexandra Muresan and Eike Guenther and John Livingston and Karen A. Collins and Fei Dai and Malcolm Fridlund and Elisa Goffo and James S. Jenkins and Petr Kab{\'{a}
    }th and Judith Korth and Alan M. Levine and Luisa M. Serrano and Jos{\'{e}} Vines and Oscar Barragan and Ilaria Carleo and Knicole D. Colon and William D. Cochran and Jessie L. Christiansen and Hans J. Deeg and Magali Deleuil and Diana Dragomir and Massimiliamo Esposito and Tianjun Gan and Sascha Grziwa and Artie P. Hatzes and Katharine Hesse and Keith Horne and Jon M. Jenkins and John F. Kielkopf and P. Klagyivik and Kristine W. F. Lam and David W. Latham and Rafa Luque and Jaume Orell-Miquel and Annelies Mortier and Olivier Mousis and Noria Narita and Hannah L. M. Osborne and Enric Palle and Riccardo Papini and George R. Ricker and Hendrik Schmerling and Sara Seager and Keivan G. Stassun and Vincent Van Eylen and Roland Vanderspek and Gavin Wang and Joshua N. Winn and Bill Wohler and Roberto Zambelli and Carl Ziegler},

    title = {{TOI}-2196 b: Rare planet in the hot Neptune desert transiting a G-type star},

    journal = {Astronomy {\&}amp$\mathsemicolon$ Astrophysics}
    }

    DOI arXiv
  116. H. Rahmati, S. Czesla, S. Khalafinejad, P. Mollière

    Transmission spectroscopy of WASP-7 b with UVES. Detection of Na I D2 and tentative D1 line absorption

    bib

    @article{Rahmati_2022,
    doi = {10.1051/0004-6361/202243955},

    url = {https://doi.org/10.1051%2F0004-6361%2F202243955},

    year = 2022,
    month = {nov},

    publisher = {{EDP} Sciences},

    volume = {668},

    pages = {A24},

    author = {Hossein Rahmati and Stefan Czesla and Sara Khalafinejad and Paul Molli{\`{e}
    }re},

    title = {Transmission spectroscopy of {WASP}-7 b with {UVES}},

    journal = {Astronomy {\&}amp$\mathsemicolon$ Astrophysics}
    }

    DOI arXiv
  117. P. Wulff, W. Dietrich, U. R. Christensen, J. Wicht

    Zonal winds in the gas planets driven by convection above a stably stratified layer

    bib

    @article{10.1093/mnras/stac3045,
    author = {Wulff, Paula N and Dietrich, W and Christensen, U R and Wicht, J},
    title = "{Zonal winds in the gas planets driven by convection above a stably stratified layer}",
    journal = {Monthly Notices of the Royal Astronomical Society},
    volume = {517},
    number = {4},
    pages = {5584-5593},
    year = {2022},
    month = {10},
    abstract = "{The analysis of the recent gravity measurements of Jupiter and Saturn reveal that the zonal winds observed on their surfaces reach several thousand kilometres deep into their atmospheres. However, it remains unclear which mechanism prevents them from penetrating deeper. Recent models suggest that a stably stratified region would yield the desired effect. In this numerical study we systematically explore the dynamics of flow in a rotating spherical shell where the lower third is stably stratified while convection in the outer region drives multiple zonal winds, similar to those observed on Jupiter or Saturn. When using a rigid lower boundary condition, only an equatorial jet pair is formed without an underlying stable layer. When including a stable layer, fierce multiple jets also develop at mid to high latitudes, once the stable stratification is strong enough to effectively decouple the jet dynamics from the lower boundary. We find that the decay of the jet amplitude near the stable layer boundary is controlled by Ω/N, where Ω is the rotation rate and N the Brunt-Väisälä frequency that quantifies the degree of stable stratification. Furthermore, the penetration distance of the jets is proportional to the jet width. In the convective region, the winds are invariant along the axis of rotation, whereas their extension in the stable layer tends to become radially aligned.}",
    issn = {0035-8711},
    doi = {10.1093/mnras/stac3045},
    url = {https://doi.org/10.1093/mnras/stac3045},
    eprint = {https://academic.oup.com/mnras/article-pdf/517/4/5584/46951621/stac3045.pdf},
    }

    DOI
  118. P. Chaturvedi, P. Bluhm, E. Nagel, A. P. Hatzes, G. Morello, M. Brady, J. Korth, K. Molaverdikhani, D. Kossakowski, J. A. Caballero, E. W. Guenther, E. Pallé, N. Espinoza, A. Seifahrt, N. Lodieu, C. Cifuentes, E. Furlan, P. J. Amado, T. Barclay, J. L. Bean, V. J. S. Béjar, G. Bergond, A. W. Boyle, D. R. Ciardi, K. A. Collins, K. I. Collins, E. Esparza-Borges, A. Fukui, C. L. Gnilka, R. Goeke, P. Guerra, T. Henning, E. Herrero, S. B. Howell, S. V. Jeffers, J. M. Jenkins, E. L. N. Jensen, D. Kasper, T. Kodama, D. W. Latham, M. J. López-González, R. Luque, D. Montes, J. C. Morales, M. Mori, F. Murgas, N. Narita, G. Nowak, H. Parviainen, V. M. Passegger, A. Quirrenbach, S. Reffert, A. Reiners, I. Ribas, G. R. Ricker, E. Rodríguez, C. Rodríguez López, M. Schlecker, R. P. Schwarz, A. Schweitzer, S. Seager, G. Kári Stefánsson, C. Stockdale, L. Tal-Or, J. D. Twicken, S. Vanaverbeke, G. Wang, N. Watanabe, J. N. Winn, M. Zechmeister

    TOI-1468: A system of two transiting planets, a super-Earth and a mini-Neptune, on opposite sides of the radius valley

    bib

    @article{Chaturvedi_2022,
    doi = {10.1051/0004-6361/202244056},

    url = {https://doi.org/10.1051%2F0004-6361%2F202244056},

    year = 2022,
    month = {oct},

    publisher = {{EDP} Sciences},

    volume = {666},

    pages = {A155},

    author = {P. Chaturvedi and P. Bluhm and E. Nagel and A. P. Hatzes and G. Morello and M. Brady and J. Korth and K. Molaverdikhani and D. Kossakowski and J. A. Caballero and E. W. Guenther and E. Pall{\'{e}
    } and N. Espinoza and A. Seifahrt and N. Lodieu and C. Cifuentes and E. Furlan and P. J. Amado and T. Barclay and J. Bean and V. J. S. B{\'{e}}jar and G. Bergond and A. W. Boyle and D. Ciardi and K. A. Collins and K. I. Collins and E. Esparza-Borges and A. Fukui and C. L. Gnilka and R. Goeke and P. Guerra and Th. Henning and E. Herrero and S. B. Howell and S. V. Jeffers and J. M. Jenkins and E. L. N. Jensen and D. Kasper and T. Kodama and D. W. Latham and M. J. L{\'{o}}pez-Gonz{\'{a}}lez and R. Luque and D. Montes and J. C. Morales and M. Mori and F. Murgas and N. Narita and G. Nowak and H. Parviainen and V. M. Passegger and A. Quirrenbach and S. Reffert and A. Reiners and I. Ribas and G. R. Ricker and E. Rodriguez and C. Rodr{\'{\i}}guez-L{\'{o}}pez and M. Schlecker and R. P. Schwarz and A. Schweitzer and S. Seager and G. Stef{\'{a}}nsson and C. Stockdale and L. Tal-Or and J. D. Twicken and S. Vanaverbeke and G. Wang and D. Watanabe and J. N. Winn and M. Zechmeister},

    title = {{TOI}-1468: A system of two transiting planets, a super-Earth and a mini-Neptune, on opposite sides of the radius valley},

    journal = {Astronomy {\&}amp$\mathsemicolon$ Astrophysics}
    }

    DOI arXiv
  119. R. Luque, G. Nowak, T. Hirano, D. Kossakowski, E. Pallé, M. Nixon, G. Morello, P. J. Amado, S. H. Albrecht, J. A. Caballero, C. Cifuentes, W. D. Cochran, H. J. Deeg, S. Dreizler, E. Esparza-Borges, A. Fukui, D. Gandolfi, E. Goffo, E. W. Guenther, A. P. Hatzes, T. Henning, P. Kabáth, K. Kawauchi, J. Korth, T. Kotani, T. Kudo, M. Kuzuhara, M. Lafarga, K. W. F. Lam, J. Livingston, J. C. Morales, A. Muresan, F. Murgas, N. Narita, H. L. M. Osborne, H. Parviainen, V. M. Passegger, C. M. Persson, A. Quirrenbach, S. Redfield, S. Reffert, A. Reiners, I. Ribas, L. M. Serrano, M. Tamura, V. Van Eylen, N. Watanabe, M. R. Zapatero Osorio

    Precise mass determination for the keystone sub-Neptune planet transiting the mid-type M dwarf G 9-40

    bib

    @article{Luque_2022,
    doi = {10.1051/0004-6361/202244426},

    url = {https://doi.org/10.1051%2F0004-6361%2F202244426},

    year = 2022,
    month = {oct},

    publisher = {{EDP} Sciences},

    volume = {666},

    pages = {A154},

    author = {R. Luque and G. Nowak and T. Hirano and D. Kossakowski and E. Pall{\'{e}
    } and M. C. Nixon and G. Morello and P. J. Amado and S. H. Albrecht and J. A. Caballero and C. Cifuentes and W. D. Cochran and H. J. Deeg and S. Dreizler and E. Esparza-Borges and A. Fukui and D. Gandolfi and E. Goffo and E. W. Guenther and A. P. Hatzes and T. Henning and P. Kabath and K. Kawauchi and J. Korth and T. Kotani and T. Kudo and M. Kuzuhara and M. Lafarga and K. W. F. Lam and J. Livingston and J. C. Morales and A. Muresan and F. Murgas and N. Narita and H. L. M. Osborne and H. Parviainen and V. M. Passegger and C. M. Persson and A. Quirrenbach and S. Redfield and S. Reffert and A. Reiners and I. Ribas and L. M. Serrano and M. Tamura and V. Van Eylen and N. Watanabe and M. R. Zapatero Osorio},

    title = {Precise mass determination for the keystone sub-Neptune planet transiting the mid-type M dwarf G 9-40},

    journal = {Astronomy {\&}amp$\mathsemicolon$ Astrophysics}
    }

    DOI arXiv
  120. O. Voelkel, H. Klahr, C. Mordasini, A. Emsenhuber

    Exploring multiple generations of planetary embryos

    bib

    @article{Voelkel_2022,
    doi = {10.1051/0004-6361/202141830},

    url = {https://doi.org/10.1051%2F0004-6361%2F202141830},

    year = 2022,
    month = {oct},

    publisher = {{EDP} Sciences},

    volume = {666},

    pages = {A90},

    author = {Oliver Voelkel and Hubert Klahr and Christoph Mordasini and Alexandre Emsenhuber},

    title = {Exploring multiple generations of planetary embryos},

    journal = {Astronomy {\&}amp$\mathsemicolon$ Astrophysics}
    }

    DOI arXiv
  121. W. Dietrich, S. Kumar, A. J. Poser, M. French, N. Nettelmann, R. Redmer, J. Wicht

    Magnetic induction processes in hot Jupiters, application to KELT-9b

  122. G. Olmschenk, D. P. Bennett, I. A. Bond, W. Zang, Y. K. Jung, J. C. Yee, E. Bachelet, F. Abe, R. K. Barry, A. Bhattacharya, H. Fujii, A. Fukui, Y. Hirao, S. Ishitani Silva, Y. Itow, R. Kirikawa, I. Kondo, N. Koshimoto, Y. Matsubara, S. Matsumoto, S. Miyazaki, B. Munford, Y. Muraki, A. Okamura, C. Ranc, N. J. Rattenbury, Y. Satoh, T. Sumi, D. Suzuki, T. Toda, P. J. Tristram, A. Vandorou, H. Yama, M. D. Albrow, S. M. Cha, S. J. Chung, A. Gould, C. Han, K. H. Hwang, D. J. Kim, H. W. Kim, S. L. Kim, C. U. Lee, D. J. Lee, Y. Lee, B. G. Park, R. W. Pogge, Y. H. Ryu, I. G. Shin, Y. Shvartzvald, G. Christie, T. Cooper, J. Drummond, J. Green, S. Hennerley, J. McCormick, L. A. G. Monard, T. Natusch, I. Porritt, T. G. Tan, S. Mao, D. Maoz, M. T. Penny, W. Zhu, V. Bozza, A. Cassan, M. Dominik, M. Hundertmark, R. Figuera Jaimes, K. Kruszyńska, K. A. Rybicki, R. A. Street, Y. Tsapras, J. Wambsganss, L. Wyrzykowski, P. Zieliński, G. Rau

    MOA-2020-BLG-208: Cool Sub-Saturn Planet Within Predicted Desert

    bib

    @misc{https://doi.org/10.48550/arxiv.2210.02436,
    doi = {10.48550/ARXIV.2210.02436},

    url = {https://arxiv.org/abs/2210.02436},

    author = {Olmschenk, Greg and Bennett, David P. and Bond, Ian A. and Zang, Weicheng and Jung, Youn Kil and Yee, Jennifer C. and Bachelet, Etienne and Abe, Fumio and Barry, Richard K. and Bhattacharya, Aparna and Fujii, Hirosane and Fukui, Akihiko and Hirao, Yuki and Silva, Stela Ishitani and Itow, Yoshitaka and Kirikawa, Rintaro and Kondo, Iona and Koshimoto, Naoki and Matsubara, Yutaka and Matsumoto, Sho and Miyazaki, Shota and Munford, Brandon and Muraki, Yasushi and Okamura, Arisa and Ranc, Clément and Rattenbury, Nicholas J. and Satoh, Yuki and Sumi, Takahiro and Suzuki, Daisuke and Toda, Taiga and Tristram, Paul J. and Vandorou, Katie and Yama, Hibiki and Albrow, Michael D. and Cha, Sang-Mok and Chung, Sun-Ju and Gould, Andrew and Han, Cheongho and Hwang, Kyu-Ha and Kim, Dong-Jin and Kim, Hyoun-Woo and Kim, Seung-Lee and Lee, Chung-Uk and Lee, Dong-Joo and Lee, Yongseok and Park, Byeong-Gon and Pogge, Richard W. and Ryu, Yoon-Hyun and Shin, In-Gu and Shvartzvald, Yossi and Christie, Grant and Cooper, Tony and Drummond, John and Green, Jonathan and Hennerley, Steve and McCormick, Jennie and Monard, L. A. G. and Natusch, Tim and Porritt, Ian and Tan, Thiam-Guan and Mao, Shude and Maoz, Dan and Penny, Matthew T. and Zhu, Wei and Bozza, V. and Cassan, Arnaud and Dominik, Martin and Hundertmark, Markus and Jaimes, R. Figuera and Kruszyńska, K. and Rybicki, K. A. and Street, R. A. and Tsapras, Y. and Wambsganss, Joachim and Wyrzykowski, Ł. and Zieliński, P. and Rau, Gioia},

    keywords = {Earth and Planetary Astrophysics (astro-ph.EP), Astrophysics of Galaxies (astro-ph.GA), FOS: Physical sciences, FOS: Physical sciences},

    title = {MOA-2020-BLG-208: Cool Sub-Saturn Planet Within Predicted Desert},

    publisher = {arXiv},

    year = {2022},

    copyright = {arXiv.org perpetual, non-exclusive license}
    }

    arXiv
  123. T. Trifonov, A. Wollbold, M. Kürster, J. Eberhardt, S. Stock, T. Henning, S. Reffert, R. P. Butler, S. S. Vogt, A. Reiners, M. H. Lee, B. Bitsch, M. Zechmeister, F. Rodler, V. Perdelwitz, L. Tal-Or, J. Rybizki, P. Heeren, D. Gandolfi, O. Barragán, O. Zakhozhay, P. Sarkis, M. Tala-Pinto, D. Kossakowski, V. Wolthoff, S. S. Brems, V. M. Passegger

    A New Third Planet and the Dynamical Architecture of the HD 33142 Planetary System

    bib

    @article{Trifonov_2022,
    doi = {10.3847/1538-3881/ac7ce0},

    url = {https://doi.org/10.3847%2F1538-3881%2Fac7ce0},

    year = 2022,
    month = {sep},

    publisher = {American Astronomical Society},

    volume = {164},

    number = {4},

    pages = {156},

    author = {Trifon Trifonov and Anna Wollbold and Martin Kürster and Jan Eberhardt and Stephan Stock and Thomas Henning and Sabine Reffert and R. Paul Butler and Steven S. Vogt and Ansgar Reiners and Man Hoi Lee and Bertram Bitsch and Mathias Zechmeister and Florian Rodler and Volker Perdelwitz and Lev Tal-Or and Jan Rybizki and Paul Heeren and Davide Gandolfi and Oscar Barrag{\'{a}
    }n and Olga Zakhozhay and Paula Sarkis and Marcelo Tala Pinto and Diana Kossakowski and Vera Wolthoff and Stefan S. Brems and Vera Maria Passegger},

    title = {A New Third Planet and the Dynamical Architecture of the {HD} 33142 Planetary System{\ast}},

    journal = {The Astronomical Journal}
    }

    DOI arXiv
  124. G. Maciejewski, M. Fernández, A. Sota, P. J. Amado, D. Dimitrov, Y. Nikolov, J. Ohlert, M. Mugrauer, R. Bischoff, T. Heyne, F. Hildebrandt, W. Stenglein, A. A. Arévalo, S. Neira, L. A. Riesco, V. Sánchez Martínez, M. M. Verdugo

    Planet-star interactions with precise transit timing. III. Entering the regime of dynamical tides

    bib

    @article{Maciejewski_2022,
    doi = {10.1051/0004-6361/202244280},

    url = {https://doi.org/10.1051%2F0004-6361%2F202244280},

    year = 2022,
    month = {nov},

    publisher = {{EDP} Sciences},

    volume = {667},

    pages = {A127},

    author = {G. Maciejewski and M. Fern{\'{a}
    }ndez and A. Sota and P. J. Amado and D. Dimitrov and Y. Nikolov and J. Ohlert and M. Mugrauer and R. Bischoff and T. Heyne and F. Hildebrandt and W. Stenglein and A. A. Ar{\'{e}}valo and S. Neira and L. A. Riesco and V. S{\'{a}}nchez Mart{\'{\i}}nez and M. M. Verdugo},

    title = {Planet-star interactions with precise transit timing},

    journal = {Astronomy {\&}amp$\mathsemicolon$ Astrophysics}
    }

    DOI arXiv
  125. O. Zakhozhay, R. Launhardt, A. Müller, S. S. Brems, P. Eigenthaler, M. Gennaro, A. Hempel, M. Hempel, T. Henning, G. M. Kennedy, S. Kim, M. Kürster, R. Lachaume, Y. Manerikar, J. A. Patel, A. Pavlov, S. Reffert, T. Trifonov

    RVSPY — Radial Velocity Survey for Planets around Young Stars. Target characterization and high-cadence survey

    bib

    @article{Zakhozhay_2022,
    doi = {10.1051/0004-6361/202244213},

    url = {https://doi.org/10.1051%2F0004-6361%2F202244213},

    year = 2022,
    month = {nov},

    publisher = {{EDP} Sciences},

    volume = {667},

    pages = {A63},

    author = {Olga V. Zakhozhay and Ralf Launhardt and Andre Müller and Stefan S. Brems and Paul Eigenthaler and Mario Gennaro and Angela Hempel and Maren Hempel and Thomas Henning and Grant M. Kennedy and Sam Kim and Martin Kürster and R{\'{e}
    }gis Lachaume and Yashodhan Manerikar and Jayshil A. Patel and Alexey Pavlov and Sabine Reffert and Trifon Trifonov},

    title = {Radial Velocity Survey for Planets around Young stars ({RVSPY})},

    journal = {Astronomy {\&}amp$\mathsemicolon$ Astrophysics}
    }

    arXiv
  126. A. W. H. Kamlah, R. Spurzem, P. Berczik, M. Arca Sedda, F. Flammini Dotti, N. Neumayer, X. Pang, Q. Shu, A. Tanikawa, M. Giersz

    The impact of stellar evolution on rotating star clusters: the gravothermal-gravogyro catastrophe and the formation of a bar of black holes

    bib

    @article{10.1093/mnras/stac2281,
    author = {Kamlah, A W H and Spurzem, R and Berczik, P and Sedda, M Arca and Dotti, F Flammini and Neumayer, N and Pang, X and Shu, Q and Tanikawa, A and Giersz, M},
    title = "{The impact of stellar evolution on rotating star clusters: the gravothermal-gravogyro catastrophe and the formation of a bar of black holes}",
    journal = {Monthly Notices of the Royal Astronomical Society},
    volume = {516},
    number = {3},
    pages = {3266-3283},
    year = {2022},
    month = {08},
    abstract = "{We present results from a suite of eight direct N-body simulations, performed with nbody6++ GPU, representing realistic models of rotating star clusters with up to 1.1 × 105 stars. Our models feature primordial (hard) binaries, a continuous mass spectrum, differential rotation, and tidal mass-loss induced by the overall gravitational field of the host galaxy. We explore the impact of rotation and stellar evolution on the star cluster dynamics. In all runs for rotating star clusters, we detect a previously predicted mechanism: an initial phase of violent relaxation followed by the so-called gravogyro catastrophe. We find that the gravogyro catastrophe reaches a finite amplitude, which depends in strength on the level of the bulk rotation, and then levels off. After this phase, the angular momentum is transferred from high-mass to low-mass particles in the cluster (both stars and compact objects). Simultaneously, the system becomes gravothermally unstable and collapses, thus undergoing the so-called gravothermal-gravogyro catastrophe. Comparing models with and without stellar evolution, we find an interesting difference. When stellar evolution is not considered, the whole process proceeds at a faster pace. The population of heavy objects tends to form a triaxial structure that rotates in the cluster centre. When stellar evolution is considered, we find that such a rotating bar is populated by stellar black holes and their progenitors. The triaxial structure becomes axisymmetric over time, but we also find that the models without stellar evolution suffer repeated gravogyro catastrophes as sufficient angular momentum and mass are removed by the tidal field.}",
    issn = {0035-8711},
    doi = {10.1093/mnras/stac2281},
    url = {https://doi.org/10.1093/mnras/stac2281},
    eprint = {https://academic.oup.com/mnras/article-pdf/516/3/3266/45877622/stac2281.pdf},
    }

    DOI arXiv
  127. M. Schlecker, R. Burn, S. Sabotta, A. Seifert, T. Henning, A. Emsenhuber, C. Mordasini, S. Reffert, Y. Shan, H. Klahr

    RV-detected planets around M dwarfs: Challenges for core accretion models

    bib

    @article{Schlecker_2022,
    doi = {10.1051/0004-6361/202142543},

    url = {https://doi.org/10.1051%2F0004-6361%2F202142543},

    year = 2022,
    month = {aug},

    publisher = {{EDP} Sciences},

    volume = {664},

    pages = {A180},

    author = {M. Schlecker and R. Burn and S. Sabotta and A. Seifert and Th. Henning and A. Emsenhuber and C. Mordasini and S. Reffert and Y. Shan and H. Klahr},

    title = {{RV}-detected planets around M dwarfs: Challenges for core accretion models},

    journal = {Astronomy {\&}amp$\mathsemicolon$ Astrophysics}
    }

    DOI arXiv
  128. F. Feng, R. P. Butler, S. S. Vogt, M. S. Clement, C. G. Tinney, K. Cui, M. Aizawa, H. R. A. Jones, J. Bailey, J. A. Burt, B. D. Carter, J. D. Crane, F. Flammini Dotti, B. Holden, B. Ma, M. Ogihara, R. Oppenheimer, S. O'Toole, S. A. Shectman, R. A. Wittenmyer, S. Wang, D. J. Wright, Y. Xuan

    3D Selection of 167 Substellar Companions to Nearby Stars

    bib

    @article{Feng_2022,
    doi = {10.3847/1538-4365/ac7e57},

    url = {https://doi.org/10.3847%2F1538-4365%2Fac7e57},

    year = 2022,
    month = {aug},

    publisher = {American Astronomical Society},

    volume = {262},

    number = {1},

    pages = {21},

    author = {Fabo Feng and R. Paul Butler and Steven S. Vogt and Matthew S. Clement and C. G. Tinney and Kaiming Cui and Masataka Aizawa and Hugh R. A. Jones and J. Bailey and Jennifer Burt and B. D. Carter and Jeffrey D. Crane and Francesco Flammini Dotti and Bradford Holden and Bo Ma and Masahiro Ogihara and Rebecca Oppenheimer and S. J. O'Toole and Stephen A. Shectman and Robert A. Wittenmyer and Sharon X. Wang and D. J. Wright and Yifan Xuan},

    title = {3D Selection of 167 Substellar Companions to Nearby Stars},

    journal = {The Astrophysical Journal Supplement Series}
    }

    DOI arXiv
  129. J. D. Melon Fuksman, H. Klahr

    No Self-shadowing Instability in 2D Radiation Hydrodynamical Models of Irradiated Protoplanetary Disks

    bib

    @article{David_Melon_Fuksman_2022,
    doi = {10.3847/1538-4357/ac7fee},

    url = {https://doi.org/10.3847%2F1538-4357%2Fac7fee},

    year = 2022,
    month = {aug},

    publisher = {American Astronomical Society},

    volume = {936},

    number = {1},

    pages = {16},

    author = {Julio David Melon Fuksman and Hubert Klahr},

    title = {No Self-shadowing Instability in 2D Radiation Hydrodynamical Models of Irradiated Protoplanetary Disks},

    journal = {The Astrophysical Journal}
    }

    DOI arXiv
  130. J. Light, S. E. S. Ferreira, N. Engelbrecht, K. Scherer, K. Herbst

    On the numerical modelling of astrospheres, including those of luminous blue variable stars, and the modulation of cosmic rays within

    bib

    @article{10.1093/mnras/stac2312,
    author = {Light, Juandré and Ferreira, S E S and Engelbrecht, N E and Scherer, K and Herbst, K},
    title = "{On the numerical modelling of astrospheres, including those of luminous blue variable stars, and the modulation of cosmic rays within}",
    journal = {Monthly Notices of the Royal Astronomical Society},
    volume = {516},
    number = {3},
    pages = {3284-3296},
    year = {2022},
    month = {08},
    abstract = "{Luminous blue variable-type stars are massive O-type stars that show variable outflow parameters. These stars can also undergo eruptions where a large amount of mass is ejected in a very short duration. The astrospheres of these stars are modelled using a magnetohydrodynamic model including the effect of radiative cooling. The variation in outflow parameters is demonstrated to lead to a variation in number density up to the termination shock, after which there is no effect in the post-shocked regions. On the other hand, eruptions increase the size of the astrosphere and cause the termination shock to oscillate between the inner boundary and the astropause. Galactic cosmic ray modulation within these types of astrospheres is also studied using a 1D stochastic differential equation model. It is shown that, even though these astrospheres are considerably larger than the heliosphere, calculated cosmic ray differential intensities remain larger than what is observed in the heliosphere at Earth, implying lower levels of modulation related to larger cosmic ray diffusion coefficients. During eruptive events, modelled cosmic ray intensities fluctuate due to the oscillating termination shock, and varying plasma parameters. It is also shown that such behaviour, can in principle, lead to the acceleration of these particles, but the results of this study, due to the 1D approach taken to solving the Parker transport equation, are argued to represent an upper limit to this phenomenon.}",
    issn = {0035-8711},
    doi = {10.1093/mnras/stac2312},
    url = {https://doi.org/10.1093/mnras/stac2312},
    eprint = {https://academic.oup.com/mnras/article-pdf/516/3/3284/45877633/stac2312.pdf},
    }

    DOI
  131. P. Gorrini, N. Astudillo-Defru, S. Dreizler, M. Damasso, R. F. Díaz, X. Bonfils, S. V. Jeffers, J. R. Barnes, F. Del Sordo, J. M. Almenara, E. Artigau, F. Bouchy, D. Charbonneau, X. Delfosse, R. Doyon, P. Figueira, T. Forveille, C. A. Haswell, M. J. López-González, C. Melo, R. Mennickent, G. Gaisné, N. Morales, F. Murgas, F. Pepe, E. Rodríguez, N. C. Santos, L. Tal-Or, Y. Tsapras, S. Udry

    Detailed stellar activity analysis and modelling of GJ 832. Reassessment of the putative habitable zone planet GJ 832c

    bib

    @article{Gorrini_2022,
    doi = {10.1051/0004-6361/202243063},

    url = {https://doi.org/10.1051%2F0004-6361%2F202243063},

    year = 2022,
    month = {aug},

    publisher = {{EDP} Sciences},

    volume = {664},

    pages = {A64},

    author = {P. Gorrini and N. Astudillo-Defru and S. Dreizler and M. Damasso and R. F. D{\'{\i}
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    title = {Detailed stellar activity analysis and modelling of {GJ} 832},

    journal = {Astronomy {\&}amp$\mathsemicolon$ Astrophysics}
    }

    DOI arXiv
  132. S. Hinkley, S. Lacour, G.-D. Marleau, A. M. Lagrange, J. J. Wang, J. Kammerer, A. Cumming, M. Nowak, L. Rodet, T. Stolker, W. Balmer, S. Ray, M. Bonnefoy, P. Mollière, C. Lazzoni, G. M. Kennedy, C. Mordasini, R. Abuter, S. Aigrain, A. Amorim, R. Asensio-Torres, C. Babusiaux, M. Benisty, J. -P. Berger, H. Beust, S. Blunt, A. Boccaletti, A. J. Bohn, H. Bonnet, G. Bourdarot, W. Brandner, F. Cantalloube, P. Caselli, B. Charnay, G. Chauvin, A. Chomez, E. Choquet, V. Christiaens, Y. Clénet, V. Coudé du Foresto, A. Cridland, P. Delorme, R. Dembet, P. T. de Zeeuw, A. Drescher, G. Duvert, A. Eckart, F. Eisenhauer, H. Feuchtgruber, F. Galland, P. Garcia, R. Garcia Lopez, T. Gardner, E. Gendron, R. Genzel, S. Gillessen, J. H. Girard, A. Grandjean, X. Haubois, G. Heißel, Th. Henning, S. Hippler

    Direct Discovery of the Inner Exoplanet in the HD206893 System

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    keywords = {Earth and Planetary Astrophysics (astro-ph.EP), Solar and Stellar Astrophysics (astro-ph.SR), FOS: Physical sciences, FOS: Physical sciences},

    title = {Direct Discovery of the Inner Exoplanet in the HD206893 System},

    publisher = {arXiv},

    year = {2022},

    copyright = {Creative Commons Attribution 4.0 International}
    }

    arXiv
  133. O. Zakhozhay, R. Launhardt, A. Müller, S. S. Brems, P. Eigenthaler, M. Gennaro, A. Hempel, M. Hempel, T. Henning, G. M. Kennedy, S. Kim, M. Kürster, R. Lachaume, Y. Manerikar, J. A. Patel, A. Pavlov, S. Reffert, T. Trifonov

    Radial Velocity Survey for Planets around Young stars (RVSPY). Target characterisation and high-cadence survey

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  134. V. Squicciarini, R. Gratton, M. Janson, E. E. Mamajek, G. Chauvin, P. Delorme, M. Langlois, A. Vigan, S. C. Ringqvist, G. Meeus, S. Reffert, M. Kenworthy, M. R. Meyer, M. Bonnefoy, M. Bonavita, D. Mesa, M. Samland, S. Desidera, V. D'Orazi, N. Engler, E. Alecian, A. Miglio, T. Henning, S. P. Quanz, L. Mayer, O. Flasseur, G.-D. Marleau

    A scaled-up planetary system around a supernova progenitor

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    @article{Squicciarini_2022,
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    url = {https://doi.org/10.1051%2F0004-6361%2F202243675},

    year = 2022,
    month = {aug},

    publisher = {{EDP} Sciences},

    volume = {664},

    pages = {A9},

    author = {V. Squicciarini and R. Gratton and M. Janson and E. E. Mamajek and G. Chauvin and P. Delorme and M. Langlois and A. Vigan and S. C. Ringqvist and G. Meeus and S. Reffert and M. Kenworthy and M. R. Meyer and M. Bonnefoy and M. Bonavita and D. Mesa and M. Samland and S. Desidera and V. D'Orazi and N. Engler and E. Alecian and A. Miglio and T. Henning and S. P. Quanz and L. Mayer and O. Flasseur and G.-D. Marleau},

    title = {A scaled-up planetary system around a supernova progenitor},

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    }

    DOI arXiv
  135. K. Breivik, A. J. Connolly, K. E. S. Ford, M. Jurić, R. Mandelbaum, A. A. Miller, D. Norman, K. Olsen, W. O'Mullane, A. Price-Whelan, T. Sacco, J. L. Sokoloski, A. Villar, V. Acquaviva, T. Ahumada, Y. AlSayyad, C. S. Alves, I. Andreoni, T. Anguita, H. J. Best, F. B. Bianco, R. Bonito, A. Bradshaw, C. J. Burke, A. Rodrigues de Campos, M. Cantiello, N. Caplar, C. O. Chandler, J. Chan, L. Nicolaci da Costa, S. Danieli, J. R. A. Davenport, G. Fabbian, J. Fagin, A. Gagliano, C. Gall, N. Garavito Camargo, E. Gawiser, S. Gezari, A. Gomboc, A. X. Gonzalez-Morales, M. J. Graham, J. Gschwend, L. P. Guy, R. A. Street, Y. Tsapras, M. J. Holmann, H. H. Hsieh, M. Hundertmark, D. Ilić, E. E. O. Ishida, T. Jurkić, A. Kannawadi, A. Kosakowski, A. B. Kovačević, J. Kubica, F. Lanusse, I. Lazar, W. G. Levine, X. Li, J. Lu, G. J. M. Luna, A. A. Mahabal, A. I. Malz

    From Data to Software to Science with the Rubin Observatory LSST

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    @misc{https://doi.org/10.48550/arxiv.2208.02781,
    doi = {10.48550/ARXIV.2208.02781},

    url = {https://arxiv.org/abs/2208.02781},

    author = {Breivik, Katelyn and Connolly, Andrew J. and Ford, K. E. Saavik and Jurić, Mario and Mandelbaum, Rachel and Miller, Adam A. and Norman, Dara and Olsen, Knut and O'Mullane, William and Price-Whelan, Adrian and Sacco, Timothy and Sokoloski, J. L. and Villar, Ashley and Acquaviva, Viviana and Ahumada, Tomas and AlSayyad, Yusra and Alves, Catarina S. and Andreoni, Igor and Anguita, Timo and Best, Henry J. and Bianco, Federica B. and Bonito, Rosaria and Bradshaw, Andrew and Burke, Colin J. and de Campos, Andresa Rodrigues and Cantiello, Matteo and Caplar, Neven and Chandler, Colin Orion and Chan, James and da Costa, Luiz Nicolaci and Danieli, Shany and Davenport, James R. A. and Fabbian, Giulio and Fagin, Joshua and Gagliano, Alexander and Gall, Christa and Camargo, Nicolás Garavito and Gawiser, Eric and Gezari, Suvi and Gomboc, Andreja and Gonzalez-Morales, Alma X. and Graham, Matthew J. and Gschwend, Julia and Guy, Leanne P. and Holman, Matthew J. and Hsieh, Henry H. and Hundertmark, Markus and Ilić, Dragana and Ishida, Emille E. O. and Jurkić, Tomislav and Kannawadi, Arun and Kosakowski, Alekzander and Kovačević, Andjelka B. and Kubica, Jeremy and Lanusse, François and Lazar, Ilin and Levine, W. Garrett and Li, Xiaolong and Lu, Jing and Luna, Gerardo Juan Manuel and Mahabal, Ashish A. and Malz, Alex I. and Mao, Yao-Yuan and Medan, Ilija and Moeyens, Joachim and Nikolić, Mladen and Nikutta, Robert and O'Dowd, Matt and Olsen, Charlotte and Pearson, Sarah and Pedraza, Ilhuiyolitzin Villicana and Popinchalk, Mark and Popović, Luka C. and Pritchard, Tyler A. and Quint, Bruno C. and Radović, Viktor and Ragosta, Fabio and Riccio, Gabriele and Riley, Alexander H. and Rożek, Agata and Sánchez-Sáez, Paula and Sarro, Luis M. and Saunders, Clare and Savić, Đorđe V. and Schmidt, Samuel and Scott, Adam and Shirley, Raphael and Smotherman, Hayden R. and Stetzler, Steven and Storey-Fisher, Kate and Street, Rachel A. and Trilling, David E. and Tsapras, Yiannis and Ustamujic, Sabina and van Velzen, Sjoert and Vázquez-Mata, José Antonio and Venuti, Laura and Wyatt, Samuel and Yu, Weixiang and Zabludoff, Ann},

    keywords = {Instrumentation and Methods for Astrophysics (astro-ph.IM), FOS: Physical sciences, FOS: Physical sciences},

    title = {From Data to Software to Science with the Rubin Observatory LSST},

    publisher = {arXiv},

    year = {2022},

    copyright = {arXiv.org perpetual, non-exclusive license}
    }

    arXiv
  136. J. Tayar, F. D. Moyano, M. Soares-Furtado, A. Escorza, M. Joyce, S. L. Martell, R. A. García, S. N. Breton, S. Mathis, S. Mathur, V. Delsanti, S. Kiefer, S. Reffert, D. M. Bowman, T. Van Reeth, S. Shetye, C. Gehan, S. K. Grunblatt

    Spinning up the Surface: Evidence for Planetary Engulfment or Unexpected Angular Momentum Transport?

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    @article{Tayar_2022,
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    url = {https://doi.org/10.3847%2F1538-4357%2Fac9312},

    year = 2022,
    month = {nov},

    publisher = {American Astronomical Society},

    volume = {940},

    number = {1},

    pages = {23},

    author = {Jamie Tayar and Facundo D. Moyano and Melinda Soares-Furtado and Ana Escorza and Meridith Joyce and Sarah L. Martell and Rafael A. Garc{\'{\i}
    }a and Sylvain N. Breton and St{\'{e}}phane Mathis and Savita Mathur and Vincent Delsanti and Sven Kiefer and Sabine Reffert and Dominic M. Bowman and Timothy Van Reeth and Shreeya Shetye and Charlotte Gehan and Samuel K. Grunblatt},

    title = {Spinning up the Surface: Evidence for Planetary Engulfment or Unexpected Angular Momentum Transport?},

    journal = {The Astrophysical Journal}
    }

    DOI arXiv
  137. E. Bachelet, Y. Tsapras, A. Gould, R. A. Street, D. P. Bennett, M. P. G. Hundertmark, V. Bozza, D. M. Bramich, A. Cassan, M. Dominik, K. Horne, S. Mao, A. Saha, J. Wambsganss, W. Zang, ROME/REA Team, F. Abe, R. Barry, A. Bhattacharya, I. A. Bond, A. Fukui, H. Fujii, Y. Hirao, Y. Itow, R. Kirikawa, I. Kondo, N. Koshimoto, Y. Matsubara, S. Matsumoto, S. Miyazaki, Y. Muraki, G. Olmschenk, C. Ranc, A. Okamura, N. J. Rattenbury, Y. Satoh, T. Sumi, D. Suzuki, S. Ishitani Silva, T. Toda, P. J. Tristram, A. Vandorou, H. Yama, MOA Collaboration, M. D. Albrow, S. J. Chung, C. Han, K. H. Hwang, Y. K. Jung, Y. H. Ryu, I. G. Shin, Y. Shvartzvald, J. C. Yee, S. M. Cha, D. J. Kim, S. L. Kim, C. U. Lee, D. J. Lee, Y. Lee, B. G. Park, R. W. Pogge, KMTNet Collaboration, A. Udalski, P. Mróz, R. Poleski, J. Skowron, M. K. Szymański, I. Soszyński, P. Pietrukowicz, S. Kozlowski, K. Ulaczyk, K. A. Rybicki, P. Iwanek, M. Wrona, M. Gromadzki, OGLE Collaboration

    MOA-2019-BLG-008Lb: A New Microlensing Detection of an Object at the Planet/Brown Dwarf Boundary

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    year = 2022,
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    publisher = {American Astronomical Society},

    volume = {164},

    number = {3},

    pages = {75},

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  138. S. Kálmán, G. M. Szabó, Sz. Csizmadia

    The power of wavelets in analysis of transit and phase curves in presence of stellar variability and instrumental noise III. Accuracy of transit parameters

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    arXiv
  139. D. Atri, C. MacArthur, S. Devata, K. Herbst, D. Gakis, S. Mathur, M. Villarreal-Gomez, G. Carla Bassani, R. Parisi, A. Al Bakr, T. Witzens

    Crewed Missions to Mars: Modeling the Impact of Astrophysical Charged Particles on Astronauts and Their Health

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    url = {https://arxiv.org/abs/2208.00892},

    author = {Atri, Dimitra and MacArthur, Caitlin and Devata, Sriram and Herbst, Konstantin and Gakis, Dionysios and Mathur, Shireen and Villarreal-Gomez, Maria and Bassani, Giulia Carla and Parisi, Roberto and Bakr, Azza Al and Witzens, Tammy},

    keywords = {Space Physics (physics.space-ph), Earth and Planetary Astrophysics (astro-ph.EP), FOS: Physical sciences, FOS: Physical sciences},

    title = {Crewed Missions to Mars: Modeling the Impact of Astrophysical Charged Particles on Astronauts and Their Health},

    publisher = {arXiv},

    year = {2022},

    copyright = {arXiv.org perpetual, non-exclusive license}
    }

    arXiv
  140. S. Petrus, G. Chauvin, M. Bonnefoy, P. Tremblin, B. Charnay, P. Delorme, G.-D. Marleau, A. Bayo, E. Manjavacas, A. M. Lagrange, P. Mollière, P. Palma-Bifani, J. -S. Biller, B. Jenkins

    X-SHYNE: X-shooter spectra of young exoplanet analogs. I. A medium-resolution 0.65-2.5μm one-shot spectrum of VHS\,1256-1257 b

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    url = {https://arxiv.org/abs/2207.06622},

    author = {Petrus, Simon and Chauvin, Gaël and Bonnefoy, Mickaël and Tremblin, Pascal and Charnay, Benjamin and Delorme, Philippe and Marleau, Gabriel-Dominique and Bayo, Amelia and Manjavacas, Elena and Lagrange, Anne-Marie and Mollière, Paul and Palma-Bifani, Paulina and Jenkins, Beth Biller James-S.},

    keywords = {Earth and Planetary Astrophysics (astro-ph.EP), Solar and Stellar Astrophysics (astro-ph.SR), FOS: Physical sciences, FOS: Physical sciences},

    title = {X-SHYNE: X-shooter spectra of young exoplanet analogs. I. A medium-resolution 0.65-2.5$\mathrm{μm}$ one-shot spectrum of VHS\,1256-1257 b},

    publisher = {arXiv},

    year = {2022},

    copyright = {arXiv.org perpetual, non-exclusive license}
    }

    arXiv
  141. B. Bitsch, A. D. Schneider, L. Kreidberg

    How drifting and evaporating pebbles shape giant planets. III. The formation of WASP-77A b and τ Boötis b

  142. N. Godoy, J. Olofsson, A. Bayo, A. C. Cheetham, R. Launhardt, G. Chauvin, G. M. Kennedy, S. S. Brems, G. Cugno, J. H. Girard, T. Henning, A. Müller, A. Musso Barcucci, F. Pepe, S. P. Quanz, A. Quirrenbach, S. Reffert, E. L. Rickman, M. Samland, D. Ségransan, T. Stolker

    ISPY – NaCo Imaging Survey for Planets around Young stars. CenteR: The impact of centering and frame selection

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    url = {https://doi.org/10.1051%2F0004-6361%2F202040024},

    year = 2022,
    month = {jul},

    publisher = {{EDP} Sciences},

    volume = {663},

    pages = {A53},

    author = {N. Godoy and J. Olofsson and A. Bayo and A. C. Cheetham and R. Launhardt and G. Chauvin and G. M. Kennedy and S. S. Brems and G. Cugno and J. H. Girard and Th. Henning and A. Müller and A. Musso Barcucci and F. Pepe and S. P. Quanz and A. Quirrenbach and S. Reffert and E. L. Rickman and M. Samland and D. S{\'{e}
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    title = {{ISPY} {\textendash} {NaCo} Imaging Survey for Planets around Young stars},

    journal = {Astronomy {\&}amp$\mathsemicolon$ Astrophysics}
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    DOI arXiv
  143. S. V. Jeffers, J. R. Barnes, P. Schöfer, A. Quirrenbach, M. Zechmeister, P. J. Amado, J. A. Caballero, M. Fernández, E. Rodríguez, I. Ribas, A. Reiners, C. Cardona Guillén, C. Cifuentes, S. Czesla, A. P. Hatzes, M. Kürster, D. Montes, J. C. Morales, S. Pedraz, S. Sadegi

    The CARMENES search for exoplanets around M dwarfs. Benchmarking the impact of activity in high-precision radial velocity measurements

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    url = {https://doi.org/10.1051%2F0004-6361%2F202141880},

    year = 2022,
    month = {jul},

    publisher = {{EDP} Sciences},

    volume = {663},

    pages = {A27},

    author = {S. V. Jeffers and J. R. Barnes and P. Schöfer and A. Quirrenbach and M. Zechmeister and P. J. Amado and J. A. Caballero and M. Fern{\'{a}
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    title = {The {CARMENES} search for exoplanets around M dwarfs},

    journal = {Astronomy {\&}amp$\mathsemicolon$ Astrophysics}
    }

    DOI arXiv
  144. K. C. Sahu, J. Anderson, S. Casertano, H. E. Bond, A. Udalski, M. Dominik, A. Calamida, A. Bellini, T. M. Brown, M. Rejkuba, V. Bajaj, N. Kains, H. C. Ferguson, C. L. Fryer, P. Yock, P. Mróz, S. Kozlowski, P. Pietrukowicz, R. Poleski, J. Skowron, I. Soszyński, M. K. Szymański, K. Ulaczyk, L. Wyrzykowski, R. K. Barry, D. P. Bennett, I. A. Bond, Y. Hirao, S. Ishitani Silva, I. Kondo, N. Koshimoto, C. Ranc, N. J. Rattenbury, T. Sumi, D. Suzuki, P. J. Tristram, A. Vandorou, J. P. Beaulieu, J. B. Marquette, A. Cole, P. Fouqué, K. Hill, S. Dieters, C. Coutures, D. Dominis-Prester, C. Bennett, E. Bachelet, J. Menzies, M. Albrow, K. Pollard, A. Gould, J. C. Yee, W. Allen, L. A. Almeida, G. Christie, J. Drummond, A. Gal-Yam, E. Gorbikov, F. Jablonski, C. H. Lee, D. Maoz, I. Manulis, J. McCormick, T. Natusch, R. W. Pogge, Y. Shvartzvald, U. G. Jørgensen, K. A. Alsubai, M. I. Andersen, V. Bozza, S. Calchi Novati, M. J. Burgdorf, T. C. Hinse, M. Hundertmark, T. -O. Husser, E. Kerins, P. Longa-Peña, L. Mancini, M. T. Penny, S. Rahvar, D. Ricci, S. Sajadian, J. Skottfelt, C. Snodgrass, J. Southworth, J. Tregloan-Reed, J. Wambsganss, O. Wertz, Y. Tsapras, R. A. Street, D. M. Bramich, K. Horne, I. A. Steele, The RoboNet Collaboration

    An Isolated Stellar-Mass Black Hole Detected Through Astrometric Microlensing

    bib

    @article{Sahu_2022,
    doi = {10.3847/1538-4357/ac739e},

    url = {https://doi.org/10.3847%2F1538-4357%2Fac739e},

    year = 2022,
    month = {jul},

    publisher = {American Astronomical Society},

    volume = {933},

    number = {1},

    pages = {83},

    author = {Kailash C. Sahu and Jay Anderson and Stefano Casertano and Howard E. Bond and Andrzej Udalski and Martin Dominik and Annalisa Calamida and Andrea Bellini and Thomas M. Brown and Marina Rejkuba and Varun Bajaj and No{\'{e}
    } Kains and Henry C. Ferguson and Chris L. Fryer and Philip Yock and Przemek Mr{\'{o}}z and Szymon Koz{\l}owski and Pawe{\l} Pietrukowicz and Radek Poleski and Jan Skowron and Igor Soszy{\'{n}}ski and Micha{\l} K. Szyma{\'{n}}ski and Krzysztof Ulaczyk and {\L}ukasz Wyrzykowski and Richard K. Barry and David P. Bennett and Ian A. Bond and Yuki Hirao and Stela Ishitani Silva and Iona Kondo and Naoki Koshimoto and Cl{\'{e}}ment Ranc and Nicholas J. Rattenbury and Takahiro Sumi and Daisuke Suzuki and Paul J. Tristram and Aikaterini Vandorou and Jean-Philippe Beaulieu and Jean-Baptiste Marquette and Andrew Cole and Pascal Fouqu{\'{e}} and Kym Hill and Stefan Dieters and Christian Coutures and Dijana Dominis-Prester and Clara Bennett and Etienne Bachelet and John Menzies and Michael Albrow and Karen Pollard and Andrew Gould and Jennifer C. Yee and William Allen and Leonardo A. Almeida and Grant Christie and John Drummond and Avishay Gal-Yam and Evgeny Gorbikov and Francisco Jablonski and Chung-Uk Lee and Dan Maoz and Ilan Manulis and Jennie McCormick and Tim Natusch and Richard W. Pogge and Yossi Shvartzvald and Uffe G. J{\o}rgensen and Khalid A. Alsubai and Michael I. Andersen and Valerio Bozza and Sebastiano Calchi Novati and Martin Burgdorf and Tobias C. Hinse and Markus Hundertmark and Tim-Oliver Husser and Eamonn Kerins and Penelope Longa-Pe{\~{n}}a and Luigi Mancini and Matthew Penny and Sohrab Rahvar and Davide Ricci and Sedighe Sajadian and Jesper Skottfelt and Colin Snodgrass and John Southworth and Jeremy Tregloan-Reed and Joachim Wambsganss and Olivier Wertz and Yiannis Tsapras and Rachel A. Street and D. M. Bramich and Keith Horne and Iain A. Steele},

    title = {An Isolated Stellar-mass Black Hole Detected through Astrometric Microlensing{\ast}},

    journal = {The Astrophysical Journal}
    }

    DOI arXiv
  145. K. Kruszyńska, L. Wyrzykowski, K. A. Rybicki, M. Maskoliunas, E. Bachelet, N. Rattenbury, P. Mróz, P. Zieliński, K. Howil, Z. Kaczmarek, S. T. Hodgkin, N. Ihanec, I. Gezer, M. Gromadzki, P. Mikolajczyk, A. Stankevičiutė, V. Čepas, E. Pakštienė, K. Šiškauskaitė, J. Zdanavičius, V. Bozza, M. Dominik, R. Figuera Jaimes, A. Fukui, M. Hundertmark, N. Narita, R. Street, Y. Tsapras, M. Bronikowski, M. Jabłońska, A. Jabłonowska, O. Ziólkowska

    Lens parameters for Gaia18cbf – a long gravitational microlensing event in the Galactic plane

    bib

    @article{Kruszy_ska_2022,
    doi = {10.1051/0004-6361/202142602},

    url = {https://doi.org/10.1051%2F0004-6361%2F202142602},

    year = 2022,
    month = {jun},

    publisher = {{EDP} Sciences},

    volume = {662},

    pages = {A59},

    author = {K. Kruszy{\'{n}
    }ska and {\L}. Wyrzykowski and K. A. Rybicki and M. Maskoli{\={u}}nas and E. Bachelet and N. Rattenbury and P. Mr{\'{o}}z and P. Zieli{\'{n}}ski and K. Howil and Z. Kaczmarek and S. T. Hodgkin and N. Ihanec and I. Gezer and M. Gromadzki and P. Miko{\l}ajczyk and A. Stankevi{\v{c}}i{\={u}}t{\.{e}} and V. {\v{C}}epas and E. Pak{\v{s}}tien{\.{e}} and K. {\v{S}}i{\v{s}}kauskait{\.{e}} and J. Zdanavi{\v{c}}ius and V. Bozza and M. Dominik and R. Figuera Jaimes and A. Fukui and M. Hundertmark and N. Narita and R. Street and Y. Tsapras and M. Bronikowski and M. Jab{\l}o{\'{n}}ska and A. Jab{\l}onowska and O. Zi{\'{o}}{\l}kowska},

    title = {Lens parameters for $\less$i$\greater$Gaia$\less$/i$\greater$18cbf {\textendash} a long gravitational microlensing event in the Galactic plane},

    journal = {Astronomy {\&}amp$\mathsemicolon$ Astrophysics}
    }

    DOI arXiv
  146. W. Zang, Y. Shvartzvald, A. Udalski, J. C. Yee, C. U. Lee, T. Sumi, X. Zhang, H. Yang, S. Mao, S. Calchi Novati, A. Gould, W. Zhu, C. A. Beichman, G. Bryden, S. Carey, B. S. Gaudi, C. B. Henderson, P. Mróz, J. Skowron, R. Poleski, M. K. Szymański, I. Soszyński, P. Pietrukowicz, S. Kozlowski, K. Ulaczyk, K. A. Rybicki, P. Iwanek, M. Wrona, M. D. Albrow, S. J. Chung, C. Han, K. H. Hwang, Y. K. Jung, Y. H. Ryu, I. G. Shin, S. M. Cha, D. J. Kim, H. W. Kim, S. L. Kim, D. J. Lee, Y. Lee, B. G. Park, R. W. Pogge, I. A. Bond, F. Abe, R. Barry, D. P. Bennett, A. Bhattacharya, M. Donachie, H. Fujii, A. Fukui, Y. Hirao, Y. Itow, R. Kirikawa, I. Kondo, N. Koshimoto, M. C. A. Li, Y. Matsubara, Y. Muraki, S. Miyazaki, C. Ranc, N. J. Rattenbury, Y. Satoh, H. Shoji, D. Suzuki, Y. Tanaka, P. J. Tristram, T. Yamawaki, A. Yonehara, E. Bachelet, M. P. G. Hundertmark, R. Figuera Jaimes, D. Maoz, M. T. Penny, R. A. Street, Y. Tsapras

    OGLE-2018-BLG-0799Lb: a q 2.7 × 10^-3 planet with Spitzer parallax

    bib

    @article{Zang_2022,
    doi = {10.1093/mnras/stac1631},

    url = {https://doi.org/10.1093%2Fmnras%2Fstac1631},

    year = 2022,
    month = {jun},

    publisher = {Oxford University Press ({OUP})},

    volume = {514},

    number = {4},

    pages = {5952--5968},

    author = {Weicheng Zang and Yossi Shvartzvald and Andrzej Udalski and Jennifer C Yee and Chung-Uk Lee and Takahiro Sumi and Xiangyu Zhang and Hongjing Yang and Shude Mao and Sebastiano Calchi Novati and Andrew Gould and Wei Zhu and Charles A Beichman and Geoffery Bryden and Sean Carey and B Scott Gaudi and Calen B Henderson and Przemek Mr{\'{o}
    }z and Jan Skowron and Radoslaw Poleski and Micha{\l} K Szyma{\'{n}}ski and Igor Soszy{\'{n}}ski and Pawe{\l} Pietrukowicz and Szymon Koz{\l}owski and Krzysztof Ulaczyk and Krzysztof A Rybicki and Patryk Iwanek and Marcin Wrona and Michael D Albrow and Sun-Ju Chung and Cheongho Han and Kyu-Ha Hwang and Youn Kil Jung and Yoon-Hyun Ryu and In-Gu Shin and Sang-Mok Cha and Dong-Jin Kim and Hyoun-Woo Kim and Seung-Lee Kim and Dong-Joo Lee and Yongseok Lee and Byeong-Gon Park and Richard W Pogge and Ian A Bond and Fumio Abe and Richard Barry and David P Bennett and Aparna Bhattacharya and Martin Donachie and Hirosane Fujii and Akihiko Fukui and Yuki Hirao and Yoshitaka Itow and Rintaro Kirikawa and Iona Kondo and Naoki Koshimoto and Man Cheung Alex Li and Yutaka Matsubara and Yasushi Muraki and Shota Miyazaki and Cl{\'{e}}ment Ranc and Nicholas J Rattenbury and Yuki Satoh and Hikaru Shoji and Daisuke Suzuki and Yuzuru Tanaka and Paul J Tristram and Tsubasa Yamawaki and Atsunori Yonehara and Etienne Bachelet and Markus P G Hundertmark and R Figuera Jaimes and Dan Maoz and Matthew T Penny and Rachel A Street and Yiannis Tsapras},

    title = {{OGLE}-2018-{BLG}-0799Lb: a $\less$i$\greater$q$\less$/i$\greater$ $\sim$ 2.7~{\texttimes}~10-3 planet with $\less$i$\greater$Spitzer$\less$/i$\greater$ parallax},

    journal = {Monthly Notices of the Royal Astronomical Society}
    }

    DOI arXiv
  147. S. V. Jeffers, R. H. Cameron, S. C. Marsden, S. Boro Saikia, C. P. Folsom, M. M. Jardine, J. Morin, P. Petit, V. See, A. A. Vidotto, U. Wolter, M. Mittag

    The crucial role of surface magnetic fields for stellar dynamos: ϵ Eridani, 61 Cygni A, and the Sun

    bib

    @article{Jeffers_2022,
    doi = {10.1051/0004-6361/202142202},

    url = {https://doi.org/10.1051%2F0004-6361%2F202142202},

    year = 2022,
    month = {may},

    publisher = {{EDP} Sciences},

    volume = {661},

    pages = {A152},

    author = {S. V. Jeffers and R. H. Cameron and S. C. Marsden and S. Boro Saikia and C. P. Folsom and M. M. Jardine and J. Morin and P. Petit and V. See and A. A. Vidotto and U. Wolter and M. Mittag},

    title = {The crucial role of surface magnetic fields for stellar dynamos: $\less$i$\greater$ϵ$\less$/i$\greater$ Eridani, 61 Cygni A, and the Sun},

    journal = {Astronomy {\&}amp$\mathsemicolon$ Astrophysics}
    }

    DOI arXiv
  148. V. Wolthoff, S. Reffert, A. Quirrenbach, M. I. Jones, R. A. Wittenmyer, J. M. Jenkins

    Precise radial velocities of giant stars. XVI. Planet occurrence rates from the combined analysis of the Lick, EXPRESS, and PPPS giant star surveys

    bib

    @article{Wolthoff_2022,
    doi = {10.1051/0004-6361/202142501},

    url = {https://doi.org/10.1051%2F0004-6361%2F202142501},

    year = 2022,
    month = {may},

    publisher = {{EDP} Sciences},

    volume = {661},

    pages = {A63},

    author = {Vera Wolthoff and Sabine Reffert and Andreas Quirrenbach and Mat{\'{\i}
    }as I. Jones and Robert A. Wittenmyer and James S. Jenkins},

    title = {Precise radial velocities of giant stars},

    journal = {Astronomy {\&}amp$\mathsemicolon$ Astrophysics}
    }

    DOI arXiv
  149. K. Herbst, L. R. Baalmann, A. Bykov, N. Engelbrecht, S. E. S. Ferreira, V. V. Izmodenov, S. D. Korolkov, K. P. Levenfish, J. L. Linsky, D. M. -A. Meyer, K. Scherer, R. Du Toit Strauss

    Astrospheres of Planet-Hosting Cool Stars and Beyond ⋅ When Modeling Meets Observations

    DOI
  150. E. Brown, S. V. Jeffers, S. C. Marsden, J. Morin, S. Boro Saikia, P. Petit, M. M. Jardine, V. See, A. A. Vidotto, M. W. Mengel, M. N. Dahlkemper, BCool Collaboration

    Linking chromospheric activity and magnetic field properties for late-type dwarf stars

    bib

    @article{Brown_2022,
    doi = {10.1093/mnras/stac1291},

    url = {https://doi.org/10.1093%2Fmnras%2Fstac1291},

    year = 2022,
    month = {may},

    publisher = {Oxford University Press ({OUP})},

    volume = {514},

    number = {3},

    pages = {4300--4319},

    author = {E L Brown and S V Jeffers and S C Marsden and J Morin and S Boro~Saikia and P Petit and M M Jardine and V See and A A Vidotto and M W Mengel and M N Dahlkemper and the~BCool~Collaboration},

    title = {Linking chromospheric activity and magnetic field properties for late-type dwarf stars},

    journal = {Monthly Notices of the Royal Astronomical Society}
    }

    DOI arXiv
  151. K. Herbst, J. L. Grenfell, M. Sinnhuber, F. Wunderlich

    INCREASE : An updated model suite to study the INfluence of Cosmic Rays on Exoplanetary AtmoSpherEs

    bib

    @article{https://doi.org/10.1002/asna.20210072,
    author = {Herbst, Konstantin and Grenfell, John Lee and Sinnhuber, Miriam and Wunderlich, Fabian},
    title = {INCREASE: An updated model suite to study the INfluence of Cosmic Rays on Exoplanetary AtmoSpherEs},
    journal = {Astronomische Nachrichten},
    volume = {343},
    number = {4},
    pages = {e210072},
    keywords = {atmospheres, biosignatures, cosmic rays, habitability},
    doi = {https://doi.org/10.1002/asna.20210072},
    url = {https://onlinelibrary.wiley.com/doi/abs/10.1002/asna.20210072},
    eprint = {https://onlinelibrary.wiley.com/doi/pdf/10.1002/asna.20210072},
    abstract = {Abstract Exoplanets are as diverse as they are fascinating. They vary from ultrahot Jupiter-like low-density planets to presumed gas-ice-rock mixture worlds such as GJ 1214b or worlds as LHS 1140b, which features twice the Earth's bulk density. Regarding the great diversity of exoplanetary atmospheres, much remains to be explored. For a few selected objects such as GJ1214b, Proxima Centauri b, and the TRAPPIST-1 planets, the first observations of their atmospheres have already been achieved or are expected in the near future with the launch of the James Webb Space Telescope envisaged in October 2021. However, in order to interpret these observations, model studies of planetary atmospheres that account for various processes—such as atmospheric escape, outgassing, climate, photochemistry, as well as the physics of air showers and the transport of stellar energetic particles and galactic cosmic rays through the stellar astrospheres and planetary magnetic fields—are necessary. Here, we present our model suite INCREASE, a planned extension of the model suite discussed in Herbst, Grenfell, et al. (2019).},
    year = {2022}
    }

    DOI
  152. L. M. Serrano, D. Gandolfi, A. J. Mustill, O. Barragán, J. Korth, F. Dai, S. Redfield, M. Fridlund, K. W. F. Lam, M. R. Díaz, S. Grziwa, K. A. Collins, J. H. Livingston, W. D. Cochran, C. Hellier, S. E. Bellomo, T. Trifonov, F. Rodler, J. Alarcon, J. M. Jenkins, D. W. Latham, G. Ricker, S. Seager, R. Vanderspek, J. N. Winn, S. Albrecht, K. I. Collins, S. Csizmadia, T. Daylan, H. J. Deeg, M. Esposito, M. Fausnaugh, I. Georgieva, E. Goffo, E. W. Guenther, A. P. Hatzes, S. B. Howell, E. L. N. Jensen, R. Luque, A. W. Mann, F. Murgas, H. L. M. Osborne, E. Pallé, C. M. Persson, P. Rowden, A. Rudat, A. M. S. Smith, J. D. Twicken, V. Van Eylen, C. Ziegler

    A low-eccentricity migration pathway for a 13-h-period Earth analogue in a four-planet system

  153. E. V. Turtelboom, L. M. Weiss, C. D. Dressing, G. Nowak, E. Pallé, C. Beard, S. Blunt, C. Brinkman, A. Chontos, Z. R. Claytor, F. Dai, P. A. Dalba, S. Giacalone, E. Gonzales, C. K. Harada, M. L. Hill, R. Holcomb, J. Korth, J. Lubin, T. Masseron, M. Macdougall, A. W. Mayo, T. Močnik, J. M. Akana Murphy, A. S. Polanski, M. Rice, R. A. Rubenzahl, N. Scarsdale, K. G. Stassun, D. B. Tyler, J. Van Zandt, I. Crossfield, H. J. Deeg, B. Fulton, D. Gandolfi, A. W. Howard, D. Huber, H. Isaacson, S. R. Kane, K. W. F. Lam, R. Luque, E. L. Martín, G. Morello, J. Orell-Miquel, E. A. Petigura, P. Robertson, A. Roy, V. Van Eylen, D. Baker, A. A. Belinski, A. Bieryla, D. R. Ciardi, K. A. Collins, N. Cutting, D. J. Della-Rose, T. B. Ellingsen, E. Furlan, T. Gan, C. L. Gnilka, P. Guerra, S. B. Howell, M. Jimenez, D. W. Latham, M. Larivière, K. V. Lester, J. Lillo-Box, L. Luker, C. R. Mann, P. Plavchan, B. Safonov, B. Skinner, I. A. Strakhov, J. Wittrock, D. Caldwell, Z. Essack, J. M. Jenkins, E. V. Quintana, G. R. Ricker, R. Vanderspek, S. Seager, J. N. Winn

    The TESS-Keck Survey. XI. Mass Measurements for Four Transiting sub-Neptunes orbiting K dwarf TOI-1246

  154. P. Schöfer, S. V. Jeffers, A. Reiners, M. Zechmeister, B. Fuhrmeister, M. Lafarga, I. Ribas, A. Quirrenbach, P. J. Amado, J. A. Caballero, G. Anglada-Escudé, F. F. Bauer, V. J. S. Béjar, M. Cortés-Contreras, E. Díez Alonso, S. Dreizler, E. W. Guenther, O. Herbort, E. N. Johnson, A. Kaminski, M. Kürster, D. Montes, J. C. Morales, S. Pedraz, L. Tal-Or

    The CARMENES search for exoplanets around M dwarfs. Rotational variation in activity indicators of Ross 318, YZ CMi, TYC 3529-1437-1, and EV Lac

  155. A. P. Hatzes, D. Gandolfi, J. Korth, F. Rodler, S. Sabotta, M. Esposito, O. Barragán, V. Van Eylen, J. H. Livingston, L. M. Serrano, R. Luque, A. M. S. Smith, S. Redfield, C. M. Persson, M. Pätzold, E. Pallé, G. Nowak, H. L. M. Osborne, N. Narita, S. Mathur, K. W. F. Lam, P. Kabáth, M. C. Johnson, E. W. Guenther, S. Grziwa, E. Goffo, M. Fridlund, M. Endl, H. J. Deeg, S. Csizmadia, W. D. Cochran, L. González-Cuesta, P. Chaturvedi, I. Carleo, J. Cabrera, P. G. Beck, S. Albrecht

    A Radial Velocity Study of the Planetary System of π Mensae: Improved Planet Parameters for π Mensae c and a Third Planet on a 125 Day Orbit

    bib

    @article{Hatzes_2022,
    doi = {10.3847/1538-3881/ac5dcb},

    url = {https://doi.org/10.3847%2F1538-3881%2Fac5dcb},

    year = 2022,
    month = {apr},

    publisher = {American Astronomical Society},

    volume = {163},

    number = {5},

    pages = {223},

    author = {Artie P. Hatzes and Davide Gandolfi and Judith Korth and Florian Rodler and Silvia Sabotta and Massimiliano Esposito and Oscar Barrag{\'{a}
    }n and Vincent Van Eylen and John H. Livingston and Luisa Maria Serrano and Rafael Luque and Alexis M. S. Smith and Seth Redfield and Carina M. Persson and Martin Pätzold and Enric Palle and Grzegorz Nowak and Hannah L. M. Osborne and Norio Narita and Savita Mathur and Kristine W. F. Lam and Petr Kab{\'{a}}th and Marshall C. Johnson and Eike W. Guenther and Sascha Grziwa and Elisa Goffo and Malcolm Fridlund and Michael Endl and Hans J. Deeg and Szilard Csizmadia and William D. Cochran and Luc{\'{\i}}a Gonz{\'{a}}lez Cuesta and Priyanka Chaturvedi and Ilaria Carleo and Juan Cabrera and Paul G. Beck and Simon Albrecht},

    title = {A Radial Velocity Study of the Planetary System of $\uppi$ Mensae: Improved Planet Parameters for $\uppi$ Mensae c and a Third Planet on a 125 Day Orbit},

    journal = {The Astronomical Journal}
    }

    DOI arXiv
  156. N. Engelbrecht, A. Vogt, K. Herbst, R. Du Toit Strauss, R. A. Burger

    Revisiting the Revisited Palmer Consensus: New Insights from Jovian Electron Transport

    bib

    @article{Engelbrecht_2022,
    doi = {10.3847/1538-4357/ac58f5},
    url = {https://doi.org/10.3847/1538-4357/ac58f5},
    year = 2022,
    month = {apr},
    publisher = {American Astronomical Society},
    volume = {929},
    number = {1},
    pages = {8},
    author = {N. Eugene Engelbrecht and Adrian Vogt and Konstantin Herbst and R. Du Toit Strauss and R. A. Burger},
    title = {Revisiting the Revisited Palmer Consensus: New Insights from Jovian Electron Transport},
    journal = {The Astrophysical Journal},
    abstract = {Novel insights into the behavior of the diffusion coefficients of charged particles in the inner heliosphere are of great importance to any study of the transport of these particles and are especially relevant with regard to the transport of low-energy electrons. The present study undertakes an exhaustive investigation into the diffusion parameters needed to reproduce low-energy electron intensities as observed at Earth, using a state-of-the-art 3D cosmic ray transport code. To this end, the transport of Jovian electrons is considered, as Jupiter represents the predominant source of these particles in the inner heliosphere, and because a careful comparison of model results with observations taken during periods of good and poor magnetic connectivity between Earth and Jupiter allows for conclusions to be drawn as to both parallel and perpendicular diffusion coefficients. This study then compares these results with the predictions made by various scattering theories. Best-fit parameters for parallel and perpendicular mean free paths at 1 au fall reasonably well within the span of observational values reported by previous studies, but best-fit radial and rigidity dependences vary widely. However, a large number of diffusion parameters lead to reasonable to-good fits to observations, and it is argued that considerable caution must be exercised when comparing theoretical results for diffusion coefficients with diffusion parameters calculated from particle transport studies.}
    }

    DOI
  157. J. Eberhardt, T. Trifonov, M. Kürster, S. Stock, T. Henning, A. Wollbold, S. Reffert, M. H. Lee, M. Zechmeister, F. Rodler, O. Zakhozhay, P. Heeren, D. Gandolfi, O. Barragán, M. Tala-Pinto, V. Wolthoff, P. Sarkis, S. S. Brems

    Dynamical Architecture of the HD 107148 Planetary System

    bib

    @article{Eberhardt_2022,
    doi = {10.3847/1538-3881/ac53b2},

    url = {https://doi.org/10.3847%2F1538-3881%2Fac53b2},

    year = 2022,
    month = {apr},

    publisher = {American Astronomical Society},

    volume = {163},

    number = {5},

    pages = {198},

    author = {Jan Eberhardt and Trifon Trifonov and Martin Kürster and Stephan Stock and Thomas Henning and Anna Wollbold and Sabine Reffert and Man Hoi Lee and Mathias Zechmeister and Florian Rodler and Olga Zakhozhay and Paul Heeren and Davide Gandolfi and Oscar Barrag{\'{a}
    }n and Marcelo Tala Pinto and Vera Wolthoff and Paula Sarkis and Stefan S. Brems},

    title = {Dynamical Architecture of the {HD} 107148 Planetary System},

    journal = {The Astronomical Journal}
    }

    DOI arXiv
  158. H. Q. Tran, P. B. Bowler, M. Endl, W. D. Cochran, P. J. MacQueen, D. Gandolfi, C. M. Persson, M. Fridlund, E. Pallé, G. Nowak, H. J. Deeg, R. Luque, J. H. Livingston, P. Kabáth, J. Laskar, J. Subjak, S. B. Howell, S. H. Albrecht, K. A. Collins, M. Esposito, S. Grziwa, V. Van Eylen, E. Goffo, C. Huang, J. M. Jenkins, M. Karjalainen, R. Karjalainen, E. Knudstrup, J. Korth, K. W. F. Lam, D. W. Latham, A. Levine, H. L. M. Osborne, S. N. Quinn, S. Redfield, G. R. Ricker, S. Seager, L. M. Serrano, A. M. S. Smith, J. D. Twicken, J. N. Winn

    TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to have Originated from High-Eccentricity Migration

  159. J. Mah, R. Brasser, J. M. Y. Woo, A. Bouvier, S. J. Mojzsis

    Evidence of a primordial isotopic gradient in the inner region of the solar protoplanetary disc

  160. O. Barragán, D. J. Armstrong, D. Gandolfi, I. Carleo, A. A. Vidotto, C. Villarreal D'Angelo, A. Oklopčić, H. Isaacson, D. Oddo, K. Collins, M. Fridlund, S. G. Sousa, C. M. Persson, C. Hellier, S. Howell, A. W. Howard, S. Redfield, N. Eisner, I. Georgieva, D. Dragomir, D. Bayliss, L. D. Nielsen, B. Klein, S. Aigrain, X. Zhang, J. Teske, J. D. Twicken, J. Jenkins, M. Esposito, V. Van Eylen, F. Rodler, V. Adibekyan, J. Alarcon, D. R. Anderson, J. M. Akana Murphy, D. Barrado, S. C. C. Barros, B. Benneke, F. Bouchy, E. M. Bryant, R. P. Butler, J. A. Burt, J. Cabrera, S. L. Casewell, P. Chaturvedi, R. Cloutier, W. D. Cochran, J. D. Crane, I. Crossfield, N. Crouzet, K. I. Collins, F. Dai, H. J. Deeg, A. Deline, O. D. S. Demangeon, X. Dumusque, P. Figueira, E. Furlan, C. L. Gnilka, M. R. Goad, E. Goffo, F. Gutiérrez-Canales, A. Hadjigeorghiou, Z. Hartman, A. P. Hatzes, M. Harris, B. A. Henderson, T. Hirano, S. Hojjatpanah, S. Hoyer, P. Kabáth, J. Korth, J. Lillo-Box, R. Luque, M. Marmier, T. Močnik, A. Muresan, F. Murgas, E. Nagel, H. L. M. Osborne, A. Osborn, H. P. Osborn, E. Pallé, M. Raimbault, G. R. Ricker, R. A. Rubenzahl, C. Stockdale, N. C. Santos, N. Scott, R. P. Schwarz, S. Shectman, S. Seager, D. Ségransan, L. M. Serrano, M. Skarka, A. M. S. Smith, J. Subjak, T. G. Tan, S. Udry, C. A. Watson, P. J. Wheatley, R. West, J. N. Winn, S. Wang, A. Wolfgang, C. Ziegler

    The young HD 73583 (TOI-560) planetary system: two 10-M⊕ mini-Neptunes transiting a 500-Myr-old, bright, and active K dwarf

    bib

    @article{Barrag_n_2022,
    doi = {10.1093/mnras/stac638},

    url = {https://doi.org/10.1093%2Fmnras%2Fstac638},

    year = 2022,
    month = {mar},

    publisher = {Oxford University Press ({OUP})},

    volume = {514},

    number = {2},

    pages = {1606--1627},

    author = {O Barrag{\'{a}
    }n and D J Armstrong and D Gandolfi and I Carleo and A A Vidotto and C Villarreal~D'Angelo and A Oklop{\v{c}}i{\'{c}} and H Isaacson and D Oddo and K Collins and M Fridlund and S G Sousa and C M Persson and C Hellier and S Howell and A Howard and S Redfield and N Eisner and I Y Georgieva and D Dragomir and D Bayliss and L D Nielsen and B Klein and S Aigrain and M Zhang and J Teske and J D Twicken and J Jenkins and M Esposito and V Van~Eylen and F Rodler and V Adibekyan and J Alarcon and D R Anderson and J M Akana~Murphy and D Barrado and S C C Barros and B Benneke and F Bouchy and E M Bryant and R P Butler and J Burt and J Cabrera and S Casewell and P Chaturvedi and R Cloutier and W D Cochran and J Crane and I Crossfield and N Crouzet and K I Collins and F Dai and H J Deeg and A Deline and O D S Demangeon and X Dumusque and P Figueira and E Furlan and C Gnilka and M R Goad and E Goffo and F Guti{\'{e}}rrez-Canales and A Hadjigeorghiou and Z Hartman and A P Hatzes and M Harris and B Henderson and T Hirano and S Hojjatpanah and S Hoyer and P Kab{\'{a}}th and J Korth and J Lillo-Box and R Luque and M Marmier and T Mo{\v{c}}nik and A Muresan and F Murgas and E Nagel and H L M Osborne and A Osborn and H P Osborn and E Palle and M Raimbault and G R Ricker and R A Rubenzahl and C Stockdale and N C Santos and N Scott and R P Schwarz and S Shectman and M Raimbault and S Seager and D S{\'{e}}gransan and L M Serrano and M Skarka and A M S Smith and J {\v{S}}ubjak and T G Tan and S Udry and C Watson and P J Wheatley and R West and J N Winn and S X Wang and A Wolfgang and C Ziegler},

    title = {The young {HD} 73583 ({TOI}-560) planetary system: two 10-M$\oplus$ mini-Neptunes transiting a 500-Myr-old, bright, and active K dwarf},

    journal = {Monthly Notices of the Royal Astronomical Society}
    }

    DOI arXiv
  161. A. Krieger, S. Wolf

    Feasibility of detecting and characterizing embedded low-mass giant planets in gaps in the VIS/NIR wavelength range

  162. A. P. Hatzes, D. Gandolfi, J. Korth, F. Rodler, S. Sabotta, M. Esposito, O. Barragán, J. H. Livingston, V. Van Eylen, L. M. Serrano, R. Luque, A. M. S. Smith, S. Redfield, C. M. Persson, E. Pallé, M. Paetzold, G. Nowak, H. L. M. Osborne, N. Narita, S. Mathur, K. W. F. Lam, P. Kabáth, M. C. Johnson, E. W. Guenther, S. Grziwa, E. Goffo, M. Fridlund, M. Endl, H. J. Deeg, Sz. Csizmadia, W. D. Cochran, L. González-Cuesta, P. Chaturvedi, I. Carleo, J. Cabrera, P. G. Beck, S. Albrecht

    A Radial Velocity Study of the Planetary System of Pi Mensae: Improved Planet Parameters for PI Mensae c and a Third Planet on a 125-d Orbit

  163. K. Stock, D. Veras, M. X. Cai, R. Spurzem, S. Portegies Zwart

    Birth cluster simulations of planetary systems with multiple super-Earths: initial conditions for white dwarf pollution drivers

  164. J. Kemmer, S. Dreizler, D. Kossakowski, S. Stock, A. Quirrenbach, J. A. Caballero, P. J. Amado, K. A. Collins, N. Espinoza, E. Herrero, J. M. Jenkins, D. W. Latham, J. Lillo-Box, N. Narita, E. Pallé, A. Reiners, I. Ribas, G. Ricker, E. Rodríguez, S. Seager, R. Vanderspek, R. Wells, J. Winn, F. J. Aceituno, V. J. S. Béjar, T. Barclay, P. Bluhm, P. Chaturvedi, C. Cifuentes, K. I. Collins, M. Cortés-Contreras, B. O. Demory, M. Fausnaugh, Y. Gómez Maqueo Chew, D. Galadí-Enríquez, T. Gan, M. Gillon, A. Golovin, A. P. Hatzes, Th. Henning, C. Huang, S. V. Jeffers, A. Kaminski, M. Kunimoto, M. Kürster, M. J. López-González, M. Lafarga, R. Luque, J. McCormac, K. Molaverdikhani, D. Montes, J. C. Morales, V. M. Passegger, S. Reffert, L. Sabin, P. Schöfer, N. Schanche, M. Schlecker, U. Schroffenegger, R. P. Schwarz, A. Schweitzer, A. Sota, P. Tenenbaum, T. Trifonov, S. Vanaverbeke, M. Zechmeister

    Discovery and mass measurement of the hot, transiting, Earth-sized planet, GJ 3929 b

  165. B. Ercolano, C. Rab, K. Molaverdikhani, B. Edwards, T. Preibisch, L. Testi, I. Kamp, W. -F. Thi

    Observations of PAHs in the atmospheres of discs and exoplanets

    bib

    @article{10.1093/mnras/stac505,
    author = {Ercolano, Barbara and Rab, Christian and Molaverdikhani, Karan and Edwards, Billy and Preibisch, Thomas and Testi, Leonardo and Kamp, Inga and Thi, Wing-Fai},
    title = "{Observations of PAHs in the atmospheres of discs and exoplanets}",
    journal = {Monthly Notices of the Royal Astronomical Society},
    volume = {512},
    number = {1},
    pages = {430-438},
    year = {2022},
    month = {02},
    abstract = "{Polycyclic aromatic hydrocarbons (PAHs) play a key role in the chemical and hydrodynamical evolution of the atmospheres of exoplanets and planet-forming discs. If they can survive the planet formation process, PAHs are likely to be involved in pre-biotic chemical reactions eventually leading to more complex molecules such as amino acids and nucleotides, which form the basis for life as we know it. However, the abundance and specific role of PAHs in these environments is largely unknown due to limitations in sensitivity and range of wavelength of current and previous space-borne facilities. Upcoming infrared space spectroscopy missions, such as Twinkle and Ariel, present a unique opportunity to detect PAHs in the atmospheres of exoplanets and planet-forming discs. In this work, we present synthetic observations based on conservative numerical modelling of typical planet-forming discs and a transiting hot Saturnian planet around solar-type star. Our models show that Twinkle and Ariel might both be able to detect the 3.3 \\$\\mu\\$m PAH feature within reasonable observing time in discs and transiting planets, assuming that PAHs are present with an abundance of at least one-tenth of the interstellar medium value.}",
    issn = {0035-8711},
    doi = {10.1093/mnras/stac505},
    url = {https://doi.org/10.1093/mnras/stac505},
    eprint = {https://academic.oup.com/mnras/article-pdf/512/1/430/42897794/stac505.pdf},
    }

    DOI arXiv
  166. T.W. Moldenhauer, R. Kuiper, W. Kley, C. W. Ormel

    Recycling of the first atmospheres of embedded planets: Dependence on core mass and optical depth

  167. J. Subjak, M. Endl, P. Chaturvedi, R. Karjalainen, W. D. Cochran, M. Esposito, D. Gandolfi, K. W. F. Lam, K. G. Stassun, J. Žák, N. Lodieu, H. M. J. Boffin, P. J. MacQueen, A. P. Hatzes, E. W. Guenther, I. Georgieva, S. Grziwa, H. Schmerling, M. Skarka, M. Blažek, M. Karjalainen, M. Špoková, H. Isaacson, A. W. Howard, C. Burke, V. Van Eylen, M. C. V. Fridlund, E. Goffo, B. Falk, J. M. Jenkins, J. Korth, J. J. Lissauer, J. H. Livingston, R. Luque, A. Muresan, H. P. Osborn, E. Pallé, C. M. Persson, S. Redfield, G. R. Ricker, S. Seager, L. M. Serrano, A. M. S. Smith, P. Kabáth

    TOI-1268b: the youngest, hot, Saturn-mass transiting exoplanet

  168. N. Davari, R. Capuzzo-Dolcetta, R. Spurzem

    Stability of planetary systems within the S-star cluster: the Solar system analogues

    bib

    @article{10.1093/mnras/stac462,
    author = {Davari, N and Capuzzo–Dolcetta, R and Spurzem, R},
    title = "{Stability of planetary systems within the S-star cluster: the Solar system analogues}",
    journal = {Monthly Notices of the Royal Astronomical Society},
    year = {2022},
    month = {02},
    abstract = "{A dynamically relaxed dense cluster comprised of about 40 stars (the so-called S-stars) inhabits the central region of the Galaxy. Their stars revolve around the Sgr A* massive object. To understand the dynamical evolution of planetary systems in a particular environment like that around Sgr A*, we carry out direct N–body simulations of planetary systems embedded in the S–star cluster. In this work, we investigate the short-term stability of the planets orbiting around S-stars after their close interactions with the central massive black hole of our galaxy. We find that planetary systems go through encounters with the SMBH and the nearby stars. We determine the frequency and the strength of planetary systems’ encounters with the nearby stars as these encounters remarkably increase for systems assigned to S-stars closer to the SMBH. The SMBH severely destabilizes the planetary systems, though we noted that the small oscillations in the mutual eccentricity and inclination of the planetary system could be caused by the planet–planet coupling and the near-resonance effect between the two planets. We obtain estimates of the fraction of survivor planets (\\$\\sim 51\\\\%\\$), and find that planets stripped from their hosting star are generally captured on close orbits around Sgr A*. We notify while gas giants are tidally disrupted, terrestrial planets do not. We estimate that Sgr A* flares can be due to the tidal disruption events of starless giant planets.}",
    issn = {0035-8711},
    doi = {10.1093/mnras/stac462},
    url = {https://doi.org/10.1093/mnras/stac462},
    note = {stac462},
    eprint = {https://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stac462/42549403/stac462.pdf},
    }

    DOI arXiv
  169. A. Papaioannou, A. Kouloumvakos, A. Mishev, R. Vainio, K. Herbst, I. Usoskin, A. P. Rouillard, A. Anastasiadis, R. Wimmer-Schweingruber, J. Gieseler, P. Kühl

    The First Ground Level Enhancement of Solar Cycle 25 on 28 October 2021

  170. A. Papaioannou, A. Kouloumvakos, A. Mishev, R. Vainio, I. Usoskin, K. Herbst, A. P. Rouillard, A. Anastasiadis, J. Gieseler, R. Wimmer-Schweingruber, P. Kühl

    The first ground-level enhancement of solar cycle 25 on 28 October 2021

    bib

    @article{Papaioannou_2022,
    doi = {10.1051/0004-6361/202142855},

    url = {https://doi.org/10.1051%2F0004-6361%2F202142855},

    year = 2022,
    month = {apr},

    publisher = {{EDP} Sciences},

    volume = {660},

    pages = {L5},

    author = {A. Papaioannou and A. Kouloumvakos and A. Mishev and R. Vainio and I. Usoskin and K. Herbst and A. P. Rouillard and A. Anastasiadis and J. Gieseler and R. Wimmer-Schweingruber and P. Kühl},

    title = {The first ground-level enhancement of solar cycle 25 on 28 October 2021},

    journal = {Astronomy {\&}amp$\mathsemicolon$ Astrophysics}
    }

    DOI arXiv
  171. J. Eberhardt, T. Trifonov, M. Kürster, S. Stock, Th. Henning, A. Wollbold, S. Reffert, M. H. Lee, M. Zechmeister, F. Rodler, O. Zakhozhay, P. Heeren, D. Gandolfi, O. Barragán, M. Tala-Pinto, V. Wolthoff, P. Sarkis, S. S. Brems

    Dynamical architecture of the HD 107148 system

  172. E. González-Álvarez, M. R. Zapatero Osorio, J. Sanz-Forcada, J. A. Caballero, S. Reffert, V. J. S. Béjar, A. P. Hatzes, E. Herrero, S. V. Jeffers, J. Kemmer, M. J. López-González, R. Luque, K. Molaverdikhani, G. Morello, E. Nagel, A. Quirrenbach, E. Rodríguez, C. Rodríguez López, M. Schlecker, A. Schweitzer, S. Stock, V. M. Passegger, T. Trifonov, P. J. Amado, D. Baker, P. T. Boyd, C. Cadieux, D. Charbonneau, K. A. Collins, R. Doyon, S. Dreizler, N. Espinoza, G. Fűrész, E. Furlan, K. Hesse, S. B. Howell, J. M. Jenkins, R. C. Kidwell, D. W. Latham, K. K. McLeod, D. Montes, J. C. Morales, T. O'Dwyer, S. Pedraz, A. Reiners, I. Ribas, S. N. Quinn, C. Schnaible, S. Seager, B. Skinner, J. C. Smith, R. P. Schwarz, A. Shporer, R. Vanderspek, J. N. Winn

    A multi-planetary system orbiting the early-M dwarf TOI-1238

  173. J. L. Grenfell, F. Wunderlich, M. Sinnhuber, K. Herbst, R. Lehmann, M. Scheucher, S. Gebauer, G. Arnold, H. Rauer

    Atmospheric processes affecting methane on Mars

  174. T. N. Delage, S. Okuzumi, M. Flock, P. Pinilla, N. Dzyurkevich

    Steady-state accretion in magnetized protoplanetary disks

  175. M. Rengel, D. Shulyak, P. Hartogh, H. Sagawa, R. Moreno, C. Jarchow, D. Breitschwerdt

    Ground-based HCN submillimetre measurements in Titan’s atmosphere: an intercomparison with Herschel observations

  176. O. Voelkel, H. Klahr, C. Mordasini, A. Emsenhuber

    On the multiple generations of planetary embryos

  177. R. Bischoff, St. Raetz, M. Fernández, R. Neuhäuser, M. Mugrauer, C. Huang, W. P. Chen, A. Sota, J. Jiménez Ortega, V. V. Hambaryan, P. Zieliński, M. Dróżdż, W. Ogloza, W. Stenglein, E. Hohmann, K. -U. Michel

    Young Exoplanet Transit Initiative follow-up observations of the T Tauri star CVSO 30 with transit-like dips

    bib

    @article{10.1093/mnras/stac293,
    author = {Bischoff, R and Raetz, St and Fernández, M and Mugrauer, M and Neuhäuser, R and Huang, P C and Chen, W P and Sota, A and Jiménez Ortega, J and Hambaryan, V V and Zieliński, P and Dróżdż, M and Ogłoza, W and Stenglein, W and Hohmann, E and Michel, K-U},
    title = "{Young Exoplanet Transit Initiative follow-up observations of the T Tauri star CVSO 30 with transit-like dips}",
    journal = {Monthly Notices of the Royal Astronomical Society},
    volume = {511},
    number = {3},
    pages = {3487-3500},
    year = {2022},
    month = {02},
    abstract = "{The T Tauri star CVSO 30, also known as PTFO 8-8695, was studied intensively with ground-based telescopes as well as with satellites over the last decade. It showed a variable light curve with additional repeating planetary transit-like dips every ∼10.8 h. However, these dimming events changed in depth and duration since their discovery and from autumn 2018 on, they were not even present or near the predicted observing times. As reason for the detected dips and their changes within the complex light curve, e.g. a disintegrating planet, a circumstellar dust clump, stellar spots, possible multiplicity, and orbiting clouds at a Keplerian co-rotating radius were discussed and are still under debate. In this paper, we present additional optical monitoring of CVSO 30 with the meter class telescopes of the Young Exoplanet Transit Initiative in Asia and Europe over the last 7 yr and characterize CVSO 30 with the new Early Data Release 3 of the European Space Agency-Gaia mission. As a result, we describe the evolution of the dimming events in the optical wavelength range since 2014 and present explanatory approaches for the observed variabilities. We conclude that orbiting clouds of gas at a Keplerian co-rotating radius are the most promising scenario to explain most changes in CVSO 30’s light curve.}",
    issn = {0035-8711},
    doi = {10.1093/mnras/stac293},
    url = {https://doi.org/10.1093/mnras/stac293},
    eprint = {https://academic.oup.com/mnras/article-pdf/511/3/3487/42571812/stac293.pdf},
    }

    DOI arXiv
  178. D. Mesa, C. Ginski, R. Gratton, S. Ertel, K. Wagner, M. Bonavita, D. Fedele, M. Meyer, T. Henning, M. Langlois, A. Garufi, S. Antoniucci, R. Claudi, D. Defrère, S. Desidera, M. Janson, N. Pawellek, E. Rigliaco, V. Squicciarini, A. Zurlo, A. Boccaletti, M. Bonnefoy, F. Cantalloube, G. Chauvin, M. Feldt, J. Hagelberg, E. Hugot, A. M. Lagrange, C. Lazzoni, D. Maurel, C. Perrot, C. Petit, D. Rouan, A. Vigan

    Signs of late infall and possible planet formation around DR Tau using VLT/SPHERE and LBTI/LMIRCam

  179. E. W. Guenther

    The impact of faculae on the radius determination of exoplanets: the case of the M-star GJ 1214

    bib

    @article{10.1093/mnras/stac108,
    author = {Guenther, Eike W},
    title = "{The impact of faculae on the radius determination of exoplanets: the case of the M-star GJ 1214}",
    journal = {Monthly Notices of the Royal Astronomical Society},
    volume = {511},
    number = {1},
    pages = {1115-1120},
    year = {2022},
    month = {01},
    abstract = "{Precise measurements of exoplanets radii are of key importance for our understanding of the origin and nature of these objects. Measurement of the planet radii using the transit method has reached a precision that the effects of stellar surface features have to be taken into account. While the effects from spots have already been studied in detail, our knowledge of the effects caused by faculae is still limited. This is particularly the case for M-stars. Faculae can pose a problem if they are inhomogeneously distributed on the stellar surface. Using the eclipse mapping method, we study the distribution of the faculae on the surface of GJ 1214 using the Ca ii H\\&K lines as tracers. In order to assess the homogeneity of the distribution in a quantitative way, we introduce the inhomogeneity factor (IHF). IHF is 0 per cent if the distribution is homogeneous, positive, if the plage regions are preferentially located along the path of the planet, and negative, if they are preferentially located outside the path of the planet. For GJ 1214, we derive a rather small value of \\$\\rm IHF=7.7\_\\{-7.7\\}^\\{+12.0\\}\\{\\{\\ \\rm per\\ cent\\}\\}\\$. We discuss the relevance of this result in the context of the PLATO and ARIEL missions.}",
    issn = {0035-8711},
    doi = {10.1093/mnras/stac108},
    url = {https://doi.org/10.1093/mnras/stac108},
    eprint = {https://academic.oup.com/mnras/article-pdf/511/1/1115/42385991/stac108.pdf},
    }

    DOI arXiv
  180. S. Boro Saikia, T. Lueftinger, C. P. Folsom, A. Antonova, E. Alecian, S.-F. Donati, M. Guedel, J. C. Hall, S. V. Jeffers, O. Kochukhov, S. C. Marsden, Y. T. Metodieva, M. Mittag, J. Morin, V. Perdelwitz, P. Petit, M. Schmid, A. A. Vidotto

    Time evolution of magnetic activity cycles in young suns: The curious case of κ Ceti

  181. D. Ó Fionnagáin, R. D. Kavanagh, A. A. Vidotto, S. V. Jeffers, P. Petit, S. Marsden, J. Morin, A. Golden

    Coronal Mass Ejections and Type II Radio Emission Variability during a Magnetic Cycle on the Solar-type Star ϵ Eridani

    bib

    @article{_Fionnag_in_2022,
    doi = {10.3847/1538-4357/ac35de},
    url = {https://doi.org/10.3847/1538-4357/ac35de},
    year = 2022,
    month = {jan},
    publisher = {American Astronomical Society},
    volume = {924},
    number = {2},
    pages = {115},
    author = {D{\'{u}}alta {\'{O}} Fionnag{\'{a}}in and Robert D. Kavanagh and Aline A. Vidotto and Sandra V. Jeffers and Pascal Petit and Stephen Marsden and Julien Morin and Aaron Golden},
    title = {Coronal Mass Ejections and Type {II} Radio Emission Variability during a Magnetic Cycle on the Solar-type Star ϵ Eridani},
    journal = {The Astrophysical Journal},
    abstract = {We simulate possible stellar coronal mass ejection (CME) scenarios over the magnetic cycle of ϵ Eridani (18 Eridani; HD 22049). We use three separate epochs from 2008, 2011, and 2013, and estimate the radio emission frequencies associated with these events. These stellar eruptions have proven to be elusive, although a promising approach to detect and characterize these phenomena are low-frequency radio observations of potential type II bursts as CME-induced shocks propagate through the stellar corona. Stellar type II radio bursts are expected to emit below 450 MHz, similarly to their solar counterparts. We show that the length of time these events remain above the ionospheric cutoff is not necessarily dependent on the stellar magnetic cycle, but more on the eruption location relative to the stellar magnetic field. We find that these type II bursts would remain within the frequency range of LOFAR for a maximum of 20–30 minutes post-eruption for the polar CMEs (50 minutes for second harmonics). We find evidence of slower equatorial CMEs, which result in slightly longer observable windows for the 2008 and 2013 simulations. Stellar magnetic geometry and strength have a significant effect on the detectability of these events. We place the CMEs in the context of the stellar mass-loss rate (27–48× solar mass-loss rate), showing that they can amount to 3%–50% of the stellar wind mass-loss rate for ϵ Eridani. Continuous monitoring of likely stellar CME candidates with low-frequency radio telescopes will be required to detect these transient events.}
    }

    DOI arXiv
  182. D. Cont, F. Yan, A. Reiners, L. Nortmann, K. Molaverdikhani, M. Stangret, Th. Henning, I. Ribas, A. Quirrenbach, J. A. Caballero, M. R. Zapatero Osorio, P. J. Amado, J. Aceituno, N. Casasayas-Barris, S. Czesla, A. Kaminski, M. López-Puertas, D. Montes, J. C. Morales, G. Morello, E. Nagel, A. Sánchez-López, E. Sedaghati, M. Zechmeister

    Silicon in the dayside atmospheres of two ultra-hot Jupiters

  183. A. Vogt, N. Engelbrecht, N. Eugene, B. Heber, A. Kopp, K. Herbst

    Numerical and experimental evidence for a new interpretation of residence times in space

  184. J. Mah, R. Brasser, A. Bouvier, S. J. Mojzsis

    Effects of pebble accretion on the growth and composition of planetesimals in the inner Solar system

    bib

    @article{10.1093/mnras/stab3766,
    author = {Mah, J and Brasser, R and Bouvier, A and Mojzsis, S J},
    title = "{Effects of pebble accretion on the growth and composition of planetesimals in the inner Solar system}",
    journal = {Monthly Notices of the Royal Astronomical Society},
    volume = {511},
    number = {1},
    pages = {158-175},
    year = {2021},
    month = {12},
    abstract = "{Recent work has shown that aside from the classical view of collisions by increasingly massive planetesimals, the accretion of mm to m-sized ‘pebbles’ can also reproduce the mass–orbit distribution of the terrestrial planets. Here, we perform N-body simulations to study the effects of pebble accretion on to growing planetesimals of different diameters located in the inner Solar system. The simulations are run to occur during the lifetime of the gas disc while also simultaneously taking Jupiter’s growth into account. We find that pebble accretion can increase the mass in the solid disc by at least a few times its initial mass with reasonable assumptions that pebbles fragment to smaller sized grains at the snow line and that gas-disc-induced orbital migration effects are in force. Such a large contribution in mass by pebbles would seem to imply that the isotopic composition of the inner Solar system should be similar to the pebble source (i.e. outer Solar system). This implication appears to violate the observed nucleosynthetic isotopic dichotomy of the sampled Solar system. Thus, pebble accretion played little or no role in terrestrial planet formation.}",
    issn = {0035-8711},
    doi = {10.1093/mnras/stab3766},
    url = {https://doi.org/10.1093/mnras/stab3766},
    eprint = {https://academic.oup.com/mnras/article-pdf/511/1/158/42362609/stab3766.pdf},
    }
    author={Mah, J and Brasser, R and Bouvier, A and Mojzsis, S J},
    year={2021},
    month={Dec},
    pages={158–175} }

    DOI arXiv
  185. G.-D. Marleau, Y. Aoyama, R. Kuiper, K. Follette, N. J. Turner, G. Cugno, C. F. Manara, S. Y. Haffert, D. Kitzmann, S. C. Ringqvist, K. R. Wagner, R. van Boekel, S. Sallum, M. Janson, T. O. B. Schmidt, L. Venuti, C. Lovis, C. Mordasini

    Accreting protoplanets: Spectral signatures and magnitude of gas and dust extinction at H α

  186. K. A. Rybicki, L. Wyrzykowski, E. Bachelet, A. Cassan, P. Zieliński, A. Gould, S. Calchi Novati, J. C. Yee, Y. H. Ryu, M. Gromadzki, P. Mikolajczyk, N. Ihanec, K. Kruszyńska, F. J. Hambsch, S. Zola, S. J. Fossey, S. Awiphan, N. Nakharutai, F. Lewis, E. F. Olivares, S. Hodgkin, A. Delgado, E. Breedt, D. L. Harrison, M. van Leeuwen, G. Rixon, T. Wevers, A. Yoldas, A. Udalski, M. K. Szymański, I. Soszyński, P. Pietrukowicz, J. Skowron, R. Poleski, K. Ulaczyk, P. Mróz, P. Iwanek, M. Wrona, R. A. Street, Y. Tsapras, M. Hundertmark, M. Dominik, C. Beichman, G. Bryden, S. Carey, B. S. Gaudi, C. Henderson, Y. Shvartzvald, W. Zang, W. Zhu, G. Christie, J. Green, S. Hennerley, J. McCormick, L. A. G. Monard, T. Natusch, R. W. Pogge, I. Gezer, A. Gurgul, Z. Kaczmarek, M. Konacki, M. C. Lam, M. Maskoliunas, E. Pakštienė, M. Ratajczak, A. Stankevičiutė, J. Zdanavičius, O. Ziólkowska

    Single-lens mass measurement in the high-magnification microlensing event Gaia19bld located in the Galactic disc

  187. E. Bachelet, P. Zieliński, M. Gromadzki, I. Gezer, K. A. Rybicki, K. Kruszyńska, N. Ihanec, L. Wyrzykowski, R. A. Street, Y. Tsapras, M. Hundertmark, A. Cassan, D. Harbeck, M. Rabus

    A spectroscopic follow-up for Gaia19bld

  188. E. Marfil, H. M. Tabernero, D. Montes, J. A. Caballero, F. J. Lázaro, J. I. González Hernández, E. Nagel, V. M. Passegger, A. Schweitzer, I. Ribas, A. Reiners, A. Quirrenbach, P. J. Amado, C. Cifuentes, M. Cortés-Contreras, S. Dreizler, C. Duque-Arribas, D. Galadí-Enríquez, Th. Henning, S. V. Jeffers, A. Kaminski, M. Kürster, M. Lafarga, Á. López-Gallifa, J. C. Morales, Y. Shan, M. Zechmeister

    The CARMENES search for exoplanets around M dwarfs. Stellar atmospheric parameters of target stars with SteParSyn

  189. M. Küffmeier, C. P. Dullemond, S. Reissl, F. G. Goicovic

    Misaligned disks induced by infall

  190. S. Khalafinejad, K. Molaverdikhani, J. Blecic, M. Mallonn, L. Nortmann, J. A. Caballero, H. Rahmati, A. Kaminski, S. Sadegi, E. Nagel, L. Carone, P. J. Amado, M. Azzaro, F. F. Bauer, N. Casasayas-Barris, S. Czesla, C. von Essen, L. Fossati, M. Guedel, Th. Henning, M. López-Puertas, M. Lendl, T. Lueftinger, D. Montes, M. Oshagh, A. Quirrenbach, E. Pallé, S. Reffert, A. Reiners, I. Ribas, S. Stock, F. Yan, M. R. Zapatero Osorio, M. Zechmeister

    Probing the atmosphere of WASP-69 b with low- and high-resolution transmission spectroscopy

  191. D. Kossakowski, J. Kemmer, P. Bluhm, S. Stock, J. A. Caballero, V. J. S. Béjar, C. Cardona Guillén, N. Lodieu, K. A. Collins, M. Oshagh, M. Schlecker, N. Espinoza, E. Pallé, Th. Henning, L. Kreidberg, M. Kürster, P. J. Amado, D. R. Anderson, J. C. Morales, S. Cartwright, D. Charbonneau, P. Chaturvedi, C. Cifuentes, D. M. Conti, M. Cortés-Contreras, S. Dreizler, D. Galadí-Enríquez, P. Guerra, R. Hart, C. Hellier, C. Henze, E. Herrero, S. V. Jeffers, J. M. Jenkins, E. L. N. Jensen, A. Kaminski, J. Kielkopf, M. Kunimoto, M. Lafarga, D. W. Latham, J. Lillo-Box, R. Luque, K. Molaverdikhani, D. Montes, G. Morello, E. H. Morgan, G. Nowak, A. Pavlov, M. Perger, E. V. Quintana, A. Quirrenbach, S. Reffert, A. Reiners, G. Ricker, I. Ribas, C. Rodríguez López, M. R. Zapatero Osorio, S. Seager, P. Schöfer, A. Schweitzer, T. Trifonov, S. Vanaverbeke, R. Vanderspek, R. West, J. Winn, M. Zechmeister

    TOI-1201 b: A mini-Neptune transiting a bright and moderately young M dwarf

  192. M. Janson, R. Gratton, L. Rodet, A. Vigan, M. Bonnefoy, P. Delorme, E. E. Mamajek, S. Reffert, L. Stock, G.-D. Marleau, M. Langlois, G. Chauvin, S. Desidera, S. C. Ringqvist, L. Mayer, G. Viswanath, V. Squicciarini, M. R. Meyer, M. Samland, S. Petrus, R. Helled, M. Kenworthy, S. P. Quanz, B. Biller, T. Henning, D. Mesa, N. Engler, J. C. Carson

    A wide-orbit giant planet in the high-mass b Centauri binary system

  193. A. Cassan, C. Ranc, O. Absil, L. Wyrzykowski, K. A. Rybicki, E. Bachelet, J. -B. Le Bouquin, M. Hundertmark, R. Street, J. Surdej, Y. Tsapras, J. Wambsganss, O. Wertz

    Microlensing mass measurement from images of rotating gravitational arcs

    DOI
  194. T. Stolker, S. Y. Haffert, A. Y. Kesseli, R. G. van Holstein, Y. Aoyama, J. Brinchmann, G. Cugno, J. H. Girard, G.-D. Marleau, M. R. Meyer, J. Milli, S. P. Quanz, I. A. G. Snellen, K. O. Todorov

    Characterizing the Protolunar Disk of the Accreting Companion GQ Lupi B

    bib

    @article{Stolker_2021,
    doi = {10.3847/1538-3881/ac2c7f},
    url = {https://doi.org/10.3847/1538-3881/ac2c7f},
    year = 2021,
    month = {dec},
    publisher = {American Astronomical Society},
    volume = {162},
    number = {6},
    pages = {286},
    author = {Tomas Stolker and Sebastiaan Y. Haffert and Aurora Y. Kesseli and Rob G. van Holstein and Yuhiko Aoyama and Jarle Brinchmann and Gabriele Cugno and Julien H. Girard and Gabriel-Dominique Marleau and Michael R. Meyer and Julien Milli and Sascha P. Quanz and Ignas A. G. Snellen and Kamen O. Todorov},
    title = {Characterizing the Protolunar Disk of the Accreting Companion {GQ} Lupi B{\ast}},
    journal = {The Astronomical Journal},
    abstract = {GQ Lup B is a young and accreting, substellar companion that appears to drive a spiral arm in the circumstellar disk of its host star. We report high-contrast imaging observations of GQ Lup B with VLT/NACO at 4–5 μm and medium-resolution integral field spectroscopy with VLT/MUSE. The optical spectrum is consistent with an M9 spectral type, shows characteristics of a low-gravity atmosphere, and exhibits strong Hα emission. The H − M′ color is ≳1 mag redder than field dwarfs with similar spectral types, and a detailed analysis of the spectral energy distribution (SED) from optical to mid-infrared wavelengths reveals excess emission in the L′, NB4.05, and M′ bands. The excess flux is well described by a blackbody component with T disk ≈ 460 K and R disk ≈ 65 R J and is expected to trace continuum emission from small grains in a protolunar disk. We derive an extinction of A V ≈ 2.3 mag from the broadband SED with a suspected origin in the vicinity of the companion. We also combine 15 yr of astrometric measurements and constrain the mutual inclination with the circumstellar disk to 84 ± 9 deg, indicating a tumultuous dynamical evolution or a stellar-like formation pathway. From the measured Hα flux and the estimated companion mass, M p ≈ 30 M J, we derive an accretion rate of . We speculate that the disk is in a transitional stage in which the assembly of satellites from a pebble reservoir has opened a central cavity while GQ Lup B is in the final stages of its formation.}
    }

    DOI arXiv
  195. E. Pallé, S. Seager, A. M. S. Smith, J. D. Twicken, J. N. Winn, P. J. Wheatley, B. Benneke, M. N. Günther, D. R. Anderson, D. J. Armstrong, O. Barragán, K. A. Collins, K. I. Collins, D. Conti, I. Crossfield, S. Gill, M. Fausnaugh, H. M. Relles, F. X. Schmider, R. P. Schwarz, S. Udry

    Transit timings variations in the three-planet system: TOI-270

    bib

    @article{10.1093/mnras/stab3483,
    author = {Kaye, Laurel and Vissapragada, Shreyas and Günther, Maximilian N and Aigrain, Suzanne and Mikal-Evans, Thomas and Jensen, Eric L N and Parviainen, Hannu and Pozuelos, Francisco J and Abe, Lyu and Acton, Jack S and Agabi, Abdelkrim and Alves, Douglas R and Anderson, David R and Armstrong, David J and Barkaoui, Khalid and Barragán, Oscar and Benneke, Björn and Boyd, Patricia T and Brahm, Rafael and Bruni, Ivan and Bryant, Edward M and Burleigh, Matthew R and Casewell, Sarah L and Ciardi, David and Cloutier, Ryan and Collins, Karen A and Collins, Kevin I and Conti, Dennis M and Crossfield, Ian J M and Crouzet, Nicolas and Daylan, Tansu and Dragomir, Diana and Dransfield, Georgina and Fabrycky, Daniel and Fausnaugh, Michael and Fuűrész, Gábor and Gan, Tianjun and Gill, Samuel and Gillon, Michaël and Goad, Michael R and Gorjian, Varoujan and Greklek-McKeon, Michael and Guerrero, Natalia and Guillot, Tristan and Jehin, Emmanuël and Jenkins, J S and Lendl, Monika and Kamler, Jacob and Kane, Stephen R and Kielkopf, John F and Kunimoto, Michelle and Marie-Sainte, Wenceslas and McCormac, James and Mékarnia, Djamel and Morales, Farisa Y and Moyano, Maximiliano and Palle, Enric and Parmentier, Vivien and Relles, Howard M and Schmider, François-Xavier and Schwarz, Richard P and Seager, S and Smith, Alexis M S and Tan, Thiam-Guan and Taylor, Jake and Triaud, Amaury H M J and Twicken, Joseph D and Udry, Stephane and Vines, J I and Wang, Gavin and Wheatley, Peter J and Winn, Joshua N},
    title = "{Transit timings variations in the three-planet system: TOI-270}",
    journal = {Monthly Notices of the Royal Astronomical Society},
    volume = {510},
    number = {4},
    pages = {5464-5485},
    year = {2021},
    month = {12},
    abstract = "{We present ground- and space-based photometric observations of TOI-270 (L231-32), a system of three transiting planets consisting of one super-Earth and two sub-Neptunes discovered by TESS around a bright (K-mag = 8.25) M3V dwarf. The planets orbit near low-order mean-motion resonances (5:3 and 2:1) and are thus expected to exhibit large transit timing variations (TTVs). Following an extensive observing campaign using eight different observatories between 2018 and 2020, we now report a clear detection of TTVs for planets c and d, with amplitudes of ∼10 min and a super-period of ∼3 yr, as well as significantly refined estimates of the radii and mean orbital periods of all three planets. Dynamical modelling of the TTVs alone puts strong constraints on the mass ratio of planets c and d and on their eccentricities. When incorporating recently published constraints from radial velocity observations, we obtain masses of \\$M\_\\{\\mathrm\\{b\\}\\}=1.48\\pm 0.18\\, M\_\\oplus\\$, \\$M\_\\{\\mathrm\\{c\\}\\}=6.20\\pm 0.31\\, M\_\\oplus\\$, and \\$M\_\\{\\mathrm\\{d\\}\\}=4.20\\pm 0.16\\, M\_\\oplus\\$ for planets b, c, and d, respectively. We also detect small but significant eccentricities for all three planets : eb = 0.0167 ± 0.0084, ec = 0.0044 ± 0.0006, and ed = 0.0066 ± 0.0020. Our findings imply an Earth-like rocky composition for the inner planet, and Earth-like cores with an additional He/H2O atmosphere for the outer two. TOI-270 is now one of the best constrained systems of small transiting planets, and it remains an excellent target for atmospheric characterization.}",
    issn = {0035-8711},
    doi = {10.1093/mnras/stab3483},
    url = {https://doi.org/10.1093/mnras/stab3483},
    eprint = {https://academic.oup.com/mnras/article-pdf/510/4/5464/42358035/stab3483.pdf},
    }

    DOI
  196. K. W. F. Lam, Sz. Csizmadia, N. Astudillo-Defru, X. Bonfils, D. Gandolfi, Sebastiano Padovan, M. Esposito, C. Hellier, T. Hirano, J. Livingston, F. Murgas, A. M. S. Smith, K. A. Collins, S. Mathur, R. A. García, S. Howell, N. C. Santos, F. Dai, G. R. Ricker, R. Vanderspek, D. W. Latham, S. Seager, J. N. Winn, J. M. Jenkins, S. Albrecht, J. M. Almenara, E. Artigau, O. Barragán, F. Bouchy, J. Cabrera, D. Charbonneau, P. Chaturvedi, A. Chaushev, J. L. Christiansen, W. D. Cochran, X. Delfosse, R. F. Díaz, R. Doyon, P. Eigmüller, P. Figueira, T. Forveille, M. Fridlund, E. Goffo, I. Georgieva, S. Grziwa, E. W. Guenther, A. P. Hatzes, M. C. Johnson, P. Kabáth, E. Knudstrup, J. Korth, J. J. Lissauer, C. Lovis, R. Luque, R. Morris, N. Narita, H. Osborne, F. Pepe, C. M. Persson, S. N. Quinn, H. Rauer, S. Redfield, J. E. Schlieder, D. Ségransan, L. M. Serrano, J. C. Smith, J. Subjak, J. D. Twicken, S. Udry, V. Van Eylen, M. Vezie, J. R. de Meideiros, G. Gaisné, P. Lewin, C. Melo, E. H. Morgan, M. Mayor

    GJ 367b: A dense, ultrashort-period sub-Earth planet transiting a nearby red dwarf star

    bib

    @article{doi:10.1126/science.aay3253,
    author = {Kristine W. F. Lam and Szilárd Csizmadia and Nicola Astudillo-Defru and Xavier Bonfils and Davide Gandolfi and Sebastiano Padovan and Massimiliano Esposito and Coel Hellier and Teruyuki Hirano and John Livingston and Felipe Murgas and Alexis M. S. Smith and Karen A. Collins and Savita Mathur and Rafael A. Garcia and Steve B. Howell and Nuno C. Santos and Fei Dai and George R. Ricker and Roland Vanderspek and David W. Latham and Sara Seager and Joshua N. Winn and Jon M. Jenkins and Simon Albrecht and Jose M. Almenara and Etienne Artigau and Oscar Barragán and François Bouchy and Juan Cabrera and David Charbonneau and Priyanka Chaturvedi and Alexander Chaushev and Jessie L. Christiansen and William D. Cochran and José R. De Meideiros and Xavier Delfosse and Rodrigo F. Díaz and René Doyon and Philipp Eigmüller and Pedro Figueira and Thierry Forveille and Malcolm Fridlund and Guillaume Gaisné and Elisa Goffo and Iskra Georgieva and Sascha Grziwa and Eike Guenther and Artie P. Hatzes and Marshall C. Johnson and Petr Kabáth and Emil Knudstrup and Judith Korth and Pablo Lewin and Jack J. Lissauer and Christophe Lovis and Rafael Luque and Claudio Melo and Edward H. Morgan and Robert Morris and Michel Mayor and Norio Narita and Hannah L. M. Osborne and Enric Palle and Francesco Pepe and Carina M. Persson and Samuel N. Quinn and Heike Rauer and Seth Redfield and Joshua E. Schlieder and Damien Ségransan and Luisa M. Serrano and Jeffrey C. Smith and Ján Šubjak and Joseph D. Twicken and Stéphane Udry and Vincent Van Eylen and Michael Vezie },
    title = {GJ 367b: A dense, ultrashort-period sub-Earth planet transiting a nearby red dwarf star},
    journal = {Science},
    volume = {374},
    number = {6572},
    pages = {1271-1275},
    year = {2021},
    doi = {10.1126/science.aay3253},

    URL = {https://www.science.org/doi/abs/10.1126/science.aay3253},
    eprint = {https://www.science.org/doi/pdf/10.1126/science.aay3253}
    ,
    abstract = { The mass and radius of an exoplanet determine its mean density, which provides information about the possible interior structure. Lam et al. have identified a planet on a 7.7-hour orbit around a nearby red dwarf star. The authors determined the planet’s radius from the transit, then used radial velocity observations to measure the mass. They found a sub-Earth–sized planet with a density almost equivalent to pure iron. Its high surface temperature is close to the vaporization point of iron, suggesting that it is the iron core of a planet that has lost its outer mantle. —KTS The nearby exoplanet GJ 367b has a density consistent with pure iron. Ultrashort-period (USP) exoplanets have orbital periods shorter than 1 day. Precise masses and radii of USP exoplanets could provide constraints on their unknown formation and evolution processes. We report the detection and characterization of the USP planet GJ 367b using high-precision photometry and radial velocity observations. GJ 367b orbits a bright (V-band magnitude of 10.2), nearby, and red (M-type) dwarf star every 7.7 hours. GJ 367b has a radius of 0.718 ± 0.054 Earth-radii and a mass of 0.546 ± 0.078 Earth-masses, making it a sub-Earth planet. The corresponding bulk density is 8.106 ± 2.165 grams per cubic centimeter—close to that of iron. An interior structure model predicts that the planet has an iron core radius fraction of 86 ± 5\%, similar to that of Mercury’s interior. }
    }

    DOI arXiv
  197. A. M. S. Smith, S. N. Breton, Sz. Csizmadia, F. Dai, D. Gandolfi, R. A. García, A. W. Howard, H. Isaacson, J. Korth, K. W. F. Lam, S. Mathur, G. Nowak, F. Pérez Hernández, C. M. Persson, S. H. Albrecht, O. Barragán, J. Cabrera, W. D. Cochran, H. J. Deeg, M. Fridlund, I. Georgieva, E. Goffo, E. W. Guenther, A. P. Hatzes, P. Kabáth, J. H. Livingston, R. Luque, S. Redfield, F. Rodler, L. M. Serrano, V. Van Eylen

    K2-99 revisited: a non-inflated warm Jupiter, and a temperate giant planet on a 522-d orbit around a subgiant

    bib

    @article{10.1093/mnras/stab3497,
    author = {Smith, A M S and Breton, S N and Csizmadia, Sz and Dai, F and Gandolfi, D and García, R A and Howard, A W and Isaacson, H and Korth, J and Lam, K W F and Mathur, S and Nowak, G and Pérez Hernández, F and Persson, C M and Albrecht, S H and Barragán, O and Cabrera, J and Cochran, W D and Deeg, H J and Fridlund, M and Georgieva, I Y and Goffo, E and Guenther, E W and Hatzes, A P and Kabath, P and Livingston, J H and Luque, R and Palle, E and Redfield, S and Rodler, F and Serrano, L M and Van Eylen, V},
    title = "{K2-99 revisited: a non-inflated warm Jupiter, and a temperate giant planet on a 522-d orbit around a subgiant}",
    journal = {Monthly Notices of the Royal Astronomical Society},
    volume = {510},
    number = {4},
    pages = {5035-5049},
    year = {2021},
    month = {12},
    abstract = "{We report new photometric and spectroscopic observations of the K2-99 planetary system. Asteroseismic analysis of the short-cadence light curve from K2’s Campaign 17 allows us to refine the stellar properties. We find K2-99 to be significantly smaller than previously thought, with R⋆ = 2.55 ± 0.02 R⊙. The new light curve also contains four transits of K2-99 b, which we use to improve our knowledge of the planetary properties. We find the planet to be a non-inflated warm Jupiter, with Rb = 1.06 ± 0.01 \\$\\mathrm\\{R\_\\{\\rm Jup\\}\\}\\$. 60 new radial velocity measurements from HARPS, HARPS-N, and HIRES enable the determination of the orbital parameters of K2-99 c, which were previously poorly constrained. We find that this outer planet has a minimum mass Mcsin ic = 8.4 ± 0.2 \\$\\mathrm\\{M\_\\{\\rm Jup\\}\\}\\$, and an eccentric orbit (ec = 0.210 ± 0.009) with a period of 522.2 ± 1.4 d. Upcoming TESS observations in 2022 have a good chance of detecting the transit of this planet, if the mutual inclination between the two planetary orbits is small.}",
    issn = {0035-8711},
    doi = {10.1093/mnras/stab3497},
    url = {https://doi.org/10.1093/mnras/stab3497},
    eprint = {https://academic.oup.com/mnras/article-pdf/510/4/5035/42245480/stab3497.pdf},
    }

    DOI arXiv
  198. Q. Li, W. Xiao, R. Wang, Z. Chen

    Diatom based reconstruction of climate evolution through the Last Glacial Maximum to Holocene in the Cosmonaut Sea, East Antarctica

    bib

    @article{LI2021104960,
    title = {Diatom based reconstruction of climate evolution through the Last Glacial Maximum to Holocene in the Cosmonaut Sea, East Antarctica},
    journal = {Deep Sea Research Part II: Topical Studies in Oceanography},
    volume = {194},
    pages = {104960},
    year = {2021},
    issn = {0967-0645},
    doi = {https://doi.org/10.1016/j.dsr2.2021.104960},
    url = {https://www.sciencedirect.com/science/article/pii/S0967064521000369},
    author = {Qingmiao Li and Wenshen Xiao and Rujian Wang and Zhihua Chen},
    keywords = {Southern Ocean, Antarctic Ice Sheet, Deglaciation, Diatoms},
    abstract = {Diatom composition has been studied in two cores retrieved from the Cosmonaut Sea, East Antarctica, during the 36th Chinese Antarctic Research Expedition. The resulting diatom data are compared to other records from the Southern Ocean and the deglaciation history of the Antarctic ice sheet to reveal the climatic response of the ice-proximal environment to the melting of the ice sheet from the Last Glacial Maximum (LGM) to Holocene. The LGM is marked by low productivity and extensive sea ice cover that resulted in poor preservation of diatom frustules. The last deglacial warming process is facilitated by the “bipolar seesaw” effect. The environment in the Cosmonaut Sea is primarily influenced by the melting of the West Antarctic Ice Sheet (WAIS) during the last deglaciation, while the East Antarctic Ice Sheet (EAIS) remained relatively stable. Maximum sea ice retreat and southward intrusion of the warm Circumpolar Deep Water facilitate the melting of the EAIS during the early Holocene. The developing cavity under the WAIS is suggested to be responsible for the mid-late Holocene cooling in the Cosmonaut Sea. This indicates that the deglaciation of the WAIS is a primary control of environmental changes in the Cosmonaut Sea, despite its ice proximal location adjacent to the EAIS.}
    }

    DOI
  199. Ó. Carrión-González, A. García Muñoz, N. C. Santos, J. Cabrera, Sz. Csizmadia, H. Rauer

    Constraining the radius and atmospheric properties of directly imaged exoplanets through multi-phase observations

  200. N. Nettelmann, D. Valencia

    Exoplanetary Interiors

    bib

    @incollection{Nettelmann_2021,
    doi = {10.1088/2514-3433/abfa8fch16},

    url = {https://doi.org/10.1088%2F2514-3433%2Fabfa8fch16},

    year = 2021,
    month = {oct},

    publisher = {{IOP} Publishing},

    author = {Nadine Nettelmann and Diana Valencia},

    title = {Exoplanetary Interiors},

    booktitle = {{ExoFrontiers}
    }
    }

    DOI arXiv
  201. K. Herbst, J. L. Grenfell, M. Sinnhuber, F. Wunderlich

    INCREASE: An updated model suite to study the INfluence of Cosmic Rays on Exoplanetary AtmoSpherEs

    bib

    @article{https://doi.org/10.1002/asna.20210072,
    author = {Herbst, Konstantin and Grenfell, John Lee and Sinnhuber, Miriam and Wunderlich, Fabian},
    title = {INCREASE: An updated model suite to study the INfluence of Cosmic Rays on Exoplanetary AtmoSpherEs},
    journal = {Astronomische Nachrichten},
    volume = {n/a},
    number = {n/a},
    pages = {},
    keywords = {atmospheres, biosignatures, cosmic rays, habitability},
    doi = {https://doi.org/10.1002/asna.20210072},
    url = {https://onlinelibrary.wiley.com/doi/abs/10.1002/asna.20210072},
    eprint = {https://onlinelibrary.wiley.com/doi/pdf/10.1002/asna.20210072},
    abstract = {Abstract Exoplanets are as diverse as they are fascinating. They vary from ultrahot Jupiter-like low-density planets to presumed gas-ice-rock mixture worlds such as GJ 1214b or worlds as LHS 1140b, which features twice the Earth's bulk density. Regarding the great diversity of exoplanetary atmospheres, much remains to be explored. For a few selected objects such as GJ1214b, Proxima Centauri b, and the TRAPPIST-1 planets, the first observations of their atmospheres have already been achieved or are expected in the near future with the launch of the James Webb Space Telescope envisaged in October 2021. However, in order to interpret these observations, model studies of planetary atmospheres that account for various processes—such as atmospheric escape, outgassing, climate, photochemistry, as well as the physics of air showers and the transport of stellar energetic particles and galactic cosmic rays through the stellar astrospheres and planetary magnetic fields—are necessary. Here, we present our model suite INCREASE, a planned extension of the model suite discussed in Herbst, Grenfell, et al. (2019).}
    }

    DOI
  202. F. Liebing, S. V. Jeffers, A. Reiners, M. Zechmeister

    Convective blueshift strengths of 810 F to M solar-type stars

  203. Y. Shan, A. Reiners, D. Fabbian, E. Marfil, D. Montes, H. M. Tabernero, I. Ribas, J. A. Caballero, A. Quirrenbach, P. J. Amado, J. Aceituno, V. J. S. Béjar, M. Cortés-Contreras, S. Dreizler, A. P. Hatzes, Th. Henning, S. V. Jeffers, A. Kaminski, M. Kürster, M. Lafarga, J. C. Morales, E. Nagel, E. Pallé, V. M. Passegger, C. Rodríguez López, A. Schweitzer, M. Zechmeister

    The CARMENES search for exoplanets around M dwarfs. Not-so-fine hyperfine-split vanadium lines in cool star spectra

  204. M. Stangret, E. Pallé, N. Casasayas-Barris, M. Oshagh, A. Bello-Arufe, R. Luque, V. Nascimbeni, F. Yan, J. Orell-Miquel, D. Sicilia, L. Malavolta, B. C. Addison, L. A. Buchhave, A. S. Bonomo, F. Borsa, S. H. C. Cabot, M. Cecconi, D. A. Fischer, A. Harutyunyan, J. M. Mendonça, G. Nowak, H. Parviainen, A. Sozzetti, R. Tronsgaard

    The obliquity and atmosphere of the ultra-hot Jupiter TOI-1431b (MASCARA-5b): A misaligned orbit and no signs of atomic or molecular absorptions

  205. T. Willamo, J. J. Lehtinen, T. Hackman, M. J. Käpylä, O. Kochukhov, S. V. Jeffers, H. Korhonen, S. C. Marsden

    Zeeman-Doppler imaging of five young solar-type stars

    bib

    @article{Willamo_2022,
    doi = {10.1051/0004-6361/202141649},

    url = {https://doi.org/10.1051%2F0004-6361%2F202141649},

    year = 2022,
    month = {mar},

    publisher = {{EDP} Sciences},

    volume = {659},

    pages = {A71},

    author = {T. Willamo and J. J. Lehtinen and T. Hackman and M. J. Käpylä and O. Kochukhov and S. V. Jeffers and H. Korhonen and S. C. Marsden},

    title = {Zeeman-Doppler imaging of five young solar-type stars},

    journal = {Astronomy {\&}amp$\mathsemicolon$ Astrophysics}
    }

    DOI arXiv
  206. J. C. Yee, W. Zang, A. Udalski, Y. H. Ryu, J. Green, S. Hennerley, A. Marmont, T. Sumi, S. Mao, M. Gromadzki, P. Mróz, J. Skowron, R. Poleski, M. K. Szymański, I. Soszyński, P. Pietrukowicz, S. Kozlowski, K. Ulaczyk, K. A. Rybicki, P. Iwanek, M. Wrona, M. D. Albrow, S. J. Chung, A. Gould, C. Han, K. H. Hwang, Y. K. Jung, H. W. Kim, I. G. Shin, Y. Shvartzvald, S. M. Cha, D. J. Kim, S. L. Kim, C. U. Lee, Y. Lee, B. G. Park, R. W. Pogge, E. Bachelet, G. Christie, M. P. G. Hundertmark, D. Maoz, J. McCormick, T. Natusch, M. T. Penny, R. A. Street, Y. Tsapras, C. A. Beichman, G. Bryden, S. Calchi Novati, S. Carey, B. S. Gaudi, C. B. Henderson, S. Johnson, W. Zhu, I. A. Bond, F. Abe, R. Barry, D. P. Bennett, A. Bhattacharya, M. Donachie, H. Fujii, A. Fukui, Y. Hirao, S. Ishitani Silva, Y. Itow, R. Kirikawa, I. Kondo, N. Koshimoto, M. C. Alex Li, Y. Matsubara, Y. Muraki, S. Miyazaki, G. Olmschenk, C. Ranc, N. J. Rattenbury, Y. Satoh, H. Shoji, D. Suzuki, Y. Tanaka, P. J. Tristram, T. Yamawaki, A. Yonehara, MOA Collaboration

    OGLE-2019-BLG-0960 Lb: the Smallest Microlensing Planet

  207. S. Brown Sevilla, M. Keppler, M. Barraza-Alfaro, J. D. Melon Fuksman, N. T. Kurtovic, P. Pinilla, M. Feldt, W. Brandner, C. Ginski, Th. Henning, H. Klahr, R. Asensio-Torres, F. Cantalloube, A. Garufi, R. G. van Holstein, M. Langlois, F. Menard, E. Rickman, M. Benisty, G. Chauvin, A. Zurlo, L. Weber, A. Pavlov, J. Ramos, S. Rochat, R. Roelfsema

    A multiwavelength analysis of the spiral arms in the protoplanetary disk around WaOph 6

  208. B. Ercolano, G. Picogna, K. Monsch, J. J. Drake, T. Preibisch

    The dispersal of protoplanetary discs – II: photoevaporation models with observationally derived irradiating spectra

    bib

    @article{10.1093/mnras/stab2590,
    author = {Ercolano, Barbara and Picogna, Giovanni and Monsch, Kristina and Drake, Jeremy J and Preibisch, Thomas},
    title = "{The dispersal of protoplanetary discs – II: photoevaporation models with observationally derived irradiating spectra}",
    journal = {Monthly Notices of the Royal Astronomical Society},
    volume = {508},
    number = {2},
    pages = {1675-1685},
    year = {2021},
    month = {09},
    abstract = "{Young solar-type stars are known to be strong X-ray emitters and their X-ray spectra have been widely studied. X-rays from the central star may play a crucial role in the thermodynamics and chemistry of the circumstellar material as well as in the atmospheric evolution of young planets. In this paper, we present model spectra based on spectral parameters derived from the observations of young stars in the Orion nebula cluster from the Chandra Orion Ultradeep Project (COUP). The spectra are then used to calculate new photoevaporation prescriptions that can be used in disc and planet population synthesis models. Our models clearly show that disc wind mass loss rates are controlled by the stellar luminosity in the soft (\\$100\\, \\mathrm\\{eV\\}\\$ to \\$1\\, \\mathrm\\{keV\\}\\$) X-ray band. New analytical relations are provided for the mass loss rates and profiles of photoevaporative winds as a function of the luminosity in the soft X-ray band. The agreement between observed and predicted transition disc statistics moderately improved using the new spectra, but the observed population of strongly accreting large cavity discs can still not be reproduced by these models. Furthermore, our models predict a population of non-accreting transition discs that are not observed. This highlights the importance of considering the depletion of millimetre-sized dust grains from the outer disc, which is a likely reason why such discs have not been detected yet.}",
    issn = {0035-8711},
    doi = {10.1093/mnras/stab2590},
    url = {https://doi.org/10.1093/mnras/stab2590},
    eprint = {https://academic.oup.com/mnras/article-pdf/508/2/1675/40513968/stab2590.pdf},
    }

    DOI arXiv
  209. D. Höning, P. Baumeister, J. L. Grenfell, N. Tosi, M. J. Way

    Early Habitability and Crustal Decarbonation of a Stagnant-Lid Venus

    bib

    @article{https://doi.org/10.1029/2021JE006895,
    author = {Höning, Dennis and Baumeister, Philipp and Grenfell, John Lee and Tosi, Nicola and Way, Michael J.},
    title = {Early Habitability and Crustal Decarbonation of a Stagnant-Lid Venus},
    journal = {Journal of Geophysical Research: Planets},
    volume = {126},
    number = {10},
    pages = {e2021JE006895},
    keywords = {carbon cycle, exoplanets, habitability, planetary evolution, stagnant-lid, Venus},
    doi = {https://doi.org/10.1029/2021JE006895},
    url = {https://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/2021JE006895},
    eprint = {https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2021JE006895},
    note = {e2021JE006895 2021JE006895},
    abstract = {Abstract Little is known about the early evolution of Venus and a potential habitable period during the first 1 billion years. In particular, it remains unclear whether or not plate tectonics and an active carbonate-silicate cycle were present. In the presence of liquid water but without plate tectonics, weathering would have been limited to freshly produced basaltic crust, with an early carbon cycle restricted to the crust and atmosphere. With the evaporation of surface water, weathering would cease. With ongoing volcanism, carbonate sediments would be buried and sink downwards. Thereby, carbonates would heat up until they become unstable and the crust would become depleted in carbonates. With supply to the atmosphere the surface temperature rises further, the depth below which decarbonation occurs decreases, causing the release of even more . We assess the habitable period of an early stagnant-lid Venus by employing a coupled interior-atmosphere evolution model accounting for degassing, weathering, carbonate burial, and crustal decarbonation. We find that if initial surface conditions allow for liquid water, weathering can keep the planet habitable for up to 900 Myr, followed by evaporation of water and rapid crustal carbonate depletion. For the atmospheric of stagnant-lid exoplanets, we predict a bimodal distribution, depending on whether or not these planets experienced a runaway greenhouse in their history. Planets with high atmospheric could be associated with crustal carbonate depletion as a consequence of a runaway greenhouse, whereas planets with low atmospheric would indicate active silicate weathering and thereby a habitable climate.},
    year = {2021}
    }

    DOI arXiv
  210. S. Sabotta, M. Schlecker, P. Chaturvedi, E. W. Guenther, I. Muñoz Rodríguez, J. C. Muñoz Sánchez, J. A. Caballero, Y. Shan, S. Reffert, I. Ribas, A. Reiners, A. P. Hatzes, P. J. Amado, H. Klahr, J. C. Morales, A. Quirrenbach, Th. Henning, S. Dreizler, E. Pallé, M. Perger, M. Azzaro, S. V. Jeffers, A. Kaminski, M. Kürster, M. Lafarga, D. Montes, V. M. Passegger, M. Zechmeister

    The CARMENES search for exoplanets around M dwarfs. Planet occurrence rates from a subsample of 71 stars

  211. N. Manger, T. Pfeil, H. Klahr

    High-resolution parameter study of the vertical shear instability – II: dependence on temperature gradient and cooling time

    bib

    @article{10.1093/mnras/stab2599,
    author = {Manger, Natascha and Pfeil, Thomas and Klahr, Hubert},
    title = "{High-resolution parameter study of the vertical shear instability – II: dependence on temperature gradient and cooling time}",
    journal = {Monthly Notices of the Royal Astronomical Society},
    volume = {508},
    number = {4},
    pages = {5402-5409},
    year = {2021},
    month = {09},
    abstract = "{A certain appeal to the alpha model for turbulence and related viscosity in accretion discs was that one scales the Reynolds stresses simply on the thermal pressure, assuming that turbulence driven by a certain mechanism will attain a characteristic Mach number in its velocity fluctuations. Besides the notion that there are different mechanism driving turbulence and angular momentum transport in a disc, we also find that within a single instability mechanism, here the vertical shear instability, stresses do not linearly scale with thermal pressure. Here, we demonstrate in numerical simulations the effect of the gas temperature gradient and the thermal relaxation time on the average stresses generated in the non-linear stage of the instability. We find that the stresses scale with the square of the exponent of the radial temperature profile at least for a range of dlog T/dlog R = [−0.5, −1], beyond which the pressure scale height varies too much over the simulation domain, to provide clear results. Stresses are also dependent on thermal relaxation times, provided they are longer than 10−3 orbital periods. The strong dependence of viscous transport of angular momentum on the local conditions in the disc (especially temperature, temperature gradient, and surface density/optical depth) challenges the ideas of viscosity leading to smooth density distributions, opening a route for structure (ring) formation and time variable mass accretion.}",
    issn = {0035-8711},
    doi = {10.1093/mnras/stab2599},
    url = {https://doi.org/10.1093/mnras/stab2599},
    eprint = {https://academic.oup.com/mnras/article-pdf/508/4/5402/40979724/stab2599.pdf},
    }

    DOI arXiv
  212. L. Fossati, M. E. Young, D. Shulyak, T. Koskinen, C. Huang, P. E. Cubillos, K. France, A. G. Sreejith

    Non-local thermodynamic equilibrium effects determine the upper atmospheric temperature structure of the ultra-hot Jupiter KELT-9b

  213. M. P. Döllinger, M. Hartmann

    A sanity check for planets around evolved Stars

    DOI
  214. G. Cugno, P. Patapis, T. Stolker, S. P. Quanz, A. Boehle, H. J. Hoeijmakers, G.-D. Marleau, P. Mollière, E. Nasedkin, I. A. G. Snellen

    Molecular mapping of the PDS70 system. No molecular absorption signatures from the forming planet PDS70 b

  215. Sz. Csizmadia, A. M. S. Smith, J. Cabrera, P. Klagyivik, A. Chaushev, K. W. F. Lam

    The power of wavelets in analysis of transit and phase curves in presence of stellar variability and instrumental noise I. Method and validation

    bib

    @misc{https://doi.org/10.48550/arxiv.2108.11822,
    doi = {10.48550/ARXIV.2108.11822},

    url = {https://arxiv.org/abs/2108.11822},

    author = {Csizmadia, Sz. and Smith, A. M. S. and Cabrera, J. and Klagyivik, P. and Chaushev, A. and Lam, K. W. F.},

    keywords = {Earth and Planetary Astrophysics (astro-ph.EP), Instrumentation and Methods for Astrophysics (astro-ph.IM), Solar and Stellar Astrophysics (astro-ph.SR), FOS: Physical sciences, FOS: Physical sciences},

    title = {The power of wavelets in analysis of transit and phase curves in presence of stellar variability and instrumental noise I. Method and validation},

    publisher = {arXiv},

    year = {2021},

    copyright = {arXiv.org perpetual, non-exclusive license}
    }

    arXiv
  216. V. Van Eylen, N. Astudillo-Defru, X. Bonfils, J. Livingston, T. Hirano, R. Luque, K. W. F. Lam, A. B. Justesen, J. N. Winn, D. Gandolfi, G. Nowak, E. Pallé, S. Albrecht, F. Dai, B. Campos Estrada, J. E. Owen, D. Foreman-Mackey, M. Fridlund, J. Korth, S. Mathur, T. Forveille, T. Mikal-Evans, H. L. M. Osborne, J. M. Almenara, C. S. K. Ho, E. Artigau, O. Barragán, S. C. C. Barros, F. Bouchy, J. Cabrera, D. Caldwell, D. Charbonneau, P. Chaturvedi, W. D. Cochran, S. Csizmadia, M. Damasso, X. Delfosse, J. De Medeiros, R. F. Díaz, R. Doyon, M. Esposito, G. Fűrész, P. Figueira, I. Georgieva, E. Goffo, S. Grziwa, E. W. Guenther, A. P. Hatzes, J. M. Jenkins, P. Kabáth, E. Knudstrup, D. W. Latham, B. Lavie, C. Lovis, R. Mennickent, S. E. Mullally, F. Murgas, N. Narita, F. A. Pepe, C. M. Persson, S. Redfield, G. R. Ricker, N. C. Santos, S. Seager, L. M. Serrano, A. M. S. Smith, A. Suárez Mascareño, J. Subjak, J. D. Twicken, S. Udry, R. Vanderspek, M. R. Zapatero Osorio

    Masses and compositions of three small planets orbiting the nearby M dwarf L231-32 (TOI-270) and the M dwarf radius valley

    bib

    @article{10.1093/mnras/stab2143,
    author = {Van Eylen, V and Astudillo-Defru, N and Bonfils, X and Livingston, J and Hirano, T and Luque, R and Lam, K W F and Justesen, A B and Winn, J N and Gandolfi, D and Nowak, G and Palle, E and Albrecht, S and Dai, F and Campos Estrada, B and Owen, J E and Foreman-Mackey, D and Fridlund, M and Korth, J and Mathur, S and Forveille, T and Mikal-Evans, T and Osborne, H L M and Ho, C S K and Almenara, J M and Artigau, E and Barragán, O and Barros, S C C and Bouchy, F and Cabrera, J and Caldwell, D A and Charbonneau, D and Chaturvedi, P and Cochran, W D and Csizmadia, S and Damasso, M and Delfosse, X and De Medeiros, J R and Díaz, R F and Doyon, R and Esposito, M and Fűrész, G and Figueira, P and Georgieva, I and Goffo, E and Grziwa, S and Guenther, E and Hatzes, A P and Jenkins, J M and Kabath, P and Knudstrup, E and Latham, D W and Lavie, B and Lovis, C and Mennickent, R E and Mullally, S E and Murgas, F and Narita, N and Pepe, F A and Persson, C M and Redfield, S and Ricker, G R and Santos, N C and Seager, S and Serrano, L M and Smith, A M S and Mascareño, A Suárez and Subjak, J and Twicken, J D and Udry, S and Vanderspek, R and Zapatero Osorio, M R},
    title = "{Masses and compositions of three small planets orbiting the nearby M dwarf L231-32 (TOI-270) and the M dwarf radius valley}",
    journal = {Monthly Notices of the Royal Astronomical Society},
    volume = {507},
    number = {2},
    pages = {2154-2173},
    year = {2021},
    month = {08},
    abstract = "{We report on precise Doppler measurements of L231-32 (TOI-270), a nearby M dwarf (d = 22 pc, M⋆ = 0.39 M⊙, R⋆ = 0.38 R⊙), which hosts three transiting planets that were recently discovered using data from the Transiting Exoplanet Survey Satellite (TESS). The three planets are 1.2, 2.4, and 2.1 times the size of Earth and have orbital periods of 3.4, 5.7, and 11.4 d. We obtained 29 high-resolution optical spectra with the newly commissioned Echelle Spectrograph for Rocky Exoplanet and Stable Spectroscopic Observations (ESPRESSO) and 58 spectra using the High Accuracy Radial velocity Planet Searcher (HARPS). From these observations, we find the masses of the planets to be 1.58 ± 0.26, 6.15 ± 0.37, and 4.78 ± 0.43 M⊕, respectively. The combination of radius and mass measurements suggests that the innermost planet has a rocky composition similar to that of Earth, while the outer two planets have lower densities. Thus, the inner planet and the outer planets are on opposite sides of the ‘radius valley’ – a region in the radius-period diagram with relatively few members – which has been interpreted as a consequence of atmospheric photoevaporation. We place these findings into the context of other small close-in planets orbiting M dwarf stars, and use support vector machines to determine the location and slope of the M dwarf (Teff \\< 4000 K) radius valley as a function of orbital period. We compare the location of the M dwarf radius valley to the radius valley observed for FGK stars, and find that its location is a good match to photoevaporation and core-powered mass-loss models. Finally, we show that planets below the M dwarf radius valley have compositions consistent with stripped rocky cores, whereas most planets above have a lower density consistent with the presence of a H-He atmosphere.}",
    issn = {0035-8711},
    doi = {10.1093/mnras/stab2143},
    url = {https://doi.org/10.1093/mnras/stab2143},
    eprint = {https://academic.oup.com/mnras/article-pdf/507/2/2154/40141388/stab2143.pdf},
    }

    DOI arXiv
  217. Y. Aoyama, G.-D. Marleau, M. Ikoma, C. Mordasini

    Comparison of Planetary Hα-emission Models: A New Correlation with Accretion Luminosity

  218. J. P. de Leon, J. H. Livingston, M. Endl, W. D. Cochran, T. Hirano, R. A. García, S. Mathur, K. W. F. Lam, J. Korth, A. A. Trani, F. Dai, E. Díez Alonso, A. Castro-Gonzáles, M. Fridlund, A. Fukui, D. Gandolfi, P. Kabáth, M. Kuzuhara, R. Luque, A. B. Savel, H. Gill, C. Dressing, S. Giacalone, N. Narita, E. Pallé, V. Van Eylen, M. Tamura

    37 new validated planets in overlapping K2 campaigns

    bib

    @article{10.1093/mnras/stab2305,
    author = {de Leon, J P and Livingston, J and Endl, M and Cochran, W D and Hirano, T and García, R A and Mathur, S and Lam, K W F and Korth, J and Trani, A A and Dai, F and Díez Alonso, E and Castro-González, A and Fridlund, M and Fukui, A and Gandolfi, D and Kabath, P and Kuzuhara, M and Luque, R and Savel, A B and Gill, H and Dressing, C and Giacalone, S and Narita, N and Palle, E and Van Eylen, V and Tamura, M},
    title = "{37 new validated planets in overlapping K2 campaigns}",
    journal = {Monthly Notices of the Royal Astronomical Society},
    volume = {508},
    number = {1},
    pages = {195-218},
    year = {2021},
    month = {08},
    abstract = "{We analysed 68 candidate planetary systems first identified during Campaigns 5 and 6 (C5 and C6) of the NASA K2 mission. We set out to validate these systems by using a suite of follow-up observations, including adaptive optics, speckle imaging, and reconnaissance spectroscopy. The overlap between C5 with C16 and C18, and C6 with C17, yields light curves with long baselines that allow us to measure the transit ephemeris very precisely, revisit single transit candidates identified in earlier campaigns, and search for additional transiting planets with longer periods not detectable in previous works. Using vespa, we compute false positive probabilities of less than 1 per cent for 37 candidates orbiting 29 unique host stars and hence statistically validate them as planets. These planets have a typical size of 2.2 R⊕ and orbital periods between 1.99 and 52.71 d. We highlight interesting systems including a sub-Neptune with the longest period detected by K2, sub-Saturns around F stars, several multiplanetary systems in a variety of architectures. These results show that a wealth of planetary systems still remains in the K2 data, some of which can be validated using minimal follow-up observations and taking advantage of analyses presented in previous catalogues.}",
    issn = {0035-8711},
    doi = {10.1093/mnras/stab2305},
    url = {https://doi.org/10.1093/mnras/stab2305},
    eprint = {https://academic.oup.com/mnras/article-pdf/508/1/195/40435487/stab2305.pdf},
    }

    DOI arXiv
  219. M. Lafarga, I. Ribas, A. Reiners, A. Quirrenbach, P. J. Amado, J. A. Caballero, M. Azzaro, V. J. S. Béjar, M. Cortés-Contreras, S. Dreizler, A. P. Hatzes, Th. Henning, S. V. Jeffers, A. Kaminski, M. Kürster, D. Montes, J. C. Morales, M. Oshagh, C. Rodríguez López, P. Schöfer, A. Schweitzer, M. Zechmeister

    The CARMENES search for exoplanets around M dwarfs. Mapping stellar activity indicators across the M dwarf domain

  220. M. Bergemann, R. Hoppe, E. Semenova, M. Carlsson, S. A. Yakovleva, Y. V. Voronov, M. Bautista, A. Nemer, A. K. Belyaev, J. Leenaarts, L. Mashonkina, A. Reiners, M. Ellwarth

    Solar oxygen abundance

    bib

    @article{10.1093/mnras/stab2160,
    author = {Bergemann, Maria and Hoppe, Richard and Semenova, Ekaterina and Carlsson, Mats and Yakovleva, Svetlana A and Voronov, Yaroslav V and Bautista, Manuel and Nemer, Ahmad and Belyaev, Andrey K and Leenaarts, Jorrit and Mashonkina, Lyudmila and Reiners, Ansgar and Ellwarth, Monika},
    title = "{Solar oxygen abundance}",
    journal = {Monthly Notices of the Royal Astronomical Society},
    volume = {508},
    number = {2},
    pages = {2236-2253},
    year = {2021},
    month = {07},
    abstract = "{Motivated by the controversy over the surface metallicity of the Sun, we present a re-analysis of the solar photospheric oxygen (O) abundance. New atomic models of O and Ni are used to perform non-local thermodynamic equilibrium (NLTE) calculations with 1D hydrostatic (MARCS) and 3D hydrodynamical (Stagger and Bifrost) models. The Bifrost 3D MHD simulations are used to quantify the influence of the chromosphere. We compare the 3D NLTE line profiles with new high-resolution, R\\$\\approx 700\\, 000\\$, spatially resolved spectra of the Sun obtained using the IAG FTS instrument. We find that the O i lines at 777 nm yield the abundance of log A(O) = 8.74 ± 0.03 dex, which depends on the choice of the H-impact collisional data and oscillator strengths. The forbidden [O i] line at 630 nm is less model dependent, as it forms nearly in LTE and is only weakly sensitive to convection. However, the oscillator strength for this transition is more uncertain than for the 777 nm lines. Modelled in 3D NLTE with the Ni i blend, the 630 nm line yields an abundance of log A(O) = 8.77 ± 0.05 dex. We compare our results with previous estimates in the literature and draw a conclusion on the most likely value of the solar photospheric O abundance, which we estimate at log A(O) = 8.75 ± 0.03 dex.}",
    issn = {0035-8711},
    doi = {10.1093/mnras/stab2160},
    url = {https://doi.org/10.1093/mnras/stab2160},
    eprint = {https://academic.oup.com/mnras/article-pdf/508/2/2236/40587625/stab2160.pdf},
    }

    DOI arXiv
  221. F. Mekhaldi, F. Adolphi, K. Herbst, R. Muscheler

    The Signal of Solar Storms Embedded in Cosmogenic Radionuclides: Detectability and Uncertainties

    bib

    @article{https://doi.org/10.1029/2021JA029351,
    author = {Mekhaldi, F. and Adolphi, F. and Herbst, K. and Muscheler, R.},
    title = {The Signal of Solar Storms Embedded in Cosmogenic Radionuclides: Detectability and Uncertainties},
    journal = {Journal of Geophysical Research: Space Physics},
    volume = {126},
    number = {8},
    pages = {e2021JA029351},
    keywords = {solar storms, cosmogenic radionuclides, ice cores, solar particle events},
    doi = {https://doi.org/10.1029/2021JA029351},
    url = {https://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/2021JA029351},
    eprint = {https://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2021JA029351},
    note = {e2021JA029351 2021JA029351},
    abstract = {Abstract The threat that solar storms pose to our ever-modernizing society has gathered significant interest in the recent past. This is partly due to the discoveries of large peaks in the content of cosmogenic radionuclides such as radiocarbon (14C) in tree rings and beryllium-10 (10Be) and chlorine-36 (36Cl) in ice cores that were linked to extreme solar storms dated to the past millennia. To better assess the threat that they represent, we need to better quantify the relationship between their energy spectrum and their magnitude with respect to the content of the radionuclides that we measure in environmental archives such as ice cores. Here, we model the global production rate that the 59 largest particle storms coming from the Sun have induced for 10Be, 14C, and 36Cl during the past 70 years. We also consider the deposition flux in 10Be and 36Cl over the high latitudes where all Greenland ice cores are located. Our analysis shows that it is unlikely that any recent solar particle event can be detected in 10Be from ice cores. By relating these values to empirical data from ice cores, we are able to quantify different detection limits and uncertainties for 10Be and 36Cl. Due to different sensitivities to solar energetic particles, we assess that 10Be may only be suitable to detect a limited number of extreme solar storms, while 36Cl is suitable to detect any extreme particle event. This implies that the occurrence-rate estimates of extreme solar storms, based mainly on 14C and 10Be, relate to a small population of potential events.},
    year = {2021}
    }

    DOI
  222. E. W. Guenther, D. Woeckel, P. Chaturvedi, S. Kumar, M. K. Srivastava

    The flare-activity of 2MASS J16111534-1757214 in the upper Scorpius association

    bib

    @article{10.1093/mnras/stab1973,
    author = {Guenther, E W and Wöckel, D and Chaturvedi, P and Kumar, V and Srivastava, M K and Muheki, P},
    title = "{The flare-activity of 2MASS J16111534–1757214 in the upper Scorpius association}",
    journal = {Monthly Notices of the Royal Astronomical Society},
    volume = {507},
    number = {2},
    pages = {2103-2114},
    year = {2021},
    month = {07},
    abstract = "{Flares are known to play an important role for the evolution of the atmospheres of young planets. In order to understand the evolution of planets, it is thus important to study the flare-activity of young stars. This is particularly the case for young M‐stars, because they are very active. We study photometrically and spectroscopically the highly active M‐star 2MASS J16111534–1757214. We show that it is a member of the Upper Sco OB association, which has an age of 5–10 Myrs. We also re-evaluate the status of other bona-fide M‐stars in this region and identify 42 members. Analyzing the K2-light curves, we find that 2MASS J16111534–1757214 has, on average, one super-flare with \\$\\rm E\\ge 10^\\{35\\}\\$ erg every 620 h, and one with \\$\\rm E\\ge 10^\\{34\\}\\$ erg every 52 h. Although this is the most active M‐star in the Upper Sco association, the power-law index of its flare-distribution is similar to that of other M‐stars in this region. 2MASS J16111534–1757214 as well as other M‐stars in this region show a broken power-law distribution in the flare-frequency diagram. Flares larger than \\$\\rm E \\ge 3\\, 10^\\{34\\}\\$ erg have a power-law index \\$\\rm \\beta =-1.3\\pm 0.1\\$ and flares smaller than that \\$\\rm \\beta =-0.8\\pm 0.1\\$. We furthermore conclude that the flare-energy distribution for young M‐stars is not that different from solar-like stars.}",
    issn = {0035-8711},
    doi = {10.1093/mnras/stab1973},
    url = {https://doi.org/10.1093/mnras/stab1973},
    eprint = {https://academic.oup.com/mnras/article-pdf/507/2/2103/40205335/stab1973.pdf},
    }

    DOI arXiv
  223. G. M. Brandt, T. D. Brandt, T. J. Dupuy, D. Michalik, G.-D. Marleau

    The First Dynamical Mass Measurement in the HR 8799 System

  224. S. Kumar, A. J. Poser, M. Schöttler, U. Kleinschmidt, W. Dietrich, J. Wicht, M. French, R. Redmer

    Ionization and transport in partially ionized multicomponent plasmas: Application to atmospheres of hot Jupiters

    bib

    @article{2021PhRvE.103f3203K,
    author = {{Kumar}, Sandeep and {Poser}, Anna Julia and {Sch{\"o}ttler}, Manuel and {Kleinschmidt}, Uwe and {Dietrich}, Wieland and {Wicht}, Johannes and {French}, Martin and {Redmer}, Ronald},
    title = {{Ionization and transport in partially ionized multicomponent plasmas: Application to atmospheres of hot Jupiters}},
    journal = {\pre},
    keywords = {Physics - Plasma Physics, Astrophysics - Earth and Planetary Astrophysics},
    year = 2021,
    month = jun,
    volume = {103},
    number = {6},
    eid = {063203},
    pages = {063203},
    doi = {10.1103/PhysRevE.103.063203},
    archiveprefix = {arXiv},
    eprint = {2106.03092},
    primaryclass = {physics.plasm-ph},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021PhRvE.103f3203K},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

    DOI arXiv
  225. I. Georgieva, C. M. Persson, O. Barragán, G. Nowak, M. Fridlund, E. Pallé, D. Locci, R. Luque, I. Carleo, D. Gandolfi, S. R. Kane, J. Korth, K. G. Stassun, J. Livingston, E. Matthews, K. A. Collins, S. B. Howell, L. M. Serrano, S. Albrecht, A. Bieryla, C. E. Brasseur, D. R. Ciardi, W. D. Cochran, K. Colòn, I. Crossfield, Sz. Csizmadia, H. J. Deeg, M. Esposito, E. Furlan, T. Gan, E. Goffo, E. Gonzales, S. Grziwa, E. W. Guenther, P. Guerra, T. Hirano, J. M. Jenkins, E. L. N. Jensen, P. Kabáth, E. Knudstrup, K. W. F. Lam, D. W. Latham, A. Levine, R. A. Matson, S. McDermott, H. L. M. Osborne, M. Paegert, S. N. Quinn, S. Redfield, G. R. Ricker, J. E. Schlieder, N. Scott, S. Seager, A. M. S. Smith, P. Tenenbaum, J. D. Twicken, R. Vanderspek, V. Van Eylen, J. N. Winn

    Hot planets around cool stars – two short-period mini-Neptunes transiting the late K-dwarf TOI-1260

    bib

    @article{10.1093/mnras/stab1464,
    author = {Georgieva, I Y and Persson, C M and Barragán, O and Nowak, G and Fridlund, M and Locci, D and Palle, E and Luque, R and Carleo, I and Gandolfi, D and Kane, S R and Korth, J and Stassun, K G and Livingston, J and Matthews, E C and Collins, K A and Howell, S B and Serrano, L M and Albrecht, S and Bieryla, A and Brasseur, C E and Ciardi, D and Cochran, W D and Colon, K D and Crossfield, I J M and Csizmadia, Sz and Deeg, H J and Esposito, M and Furlan, E and Gan, T and Goffo, E and Gonzales, E and Grziwa, S and Guenther, E W and Guerra, P and Hirano, T and Jenkins, J M and Jensen, E L N and Kabáth, P and Knudstrup, E and Lam, K W F and Latham, D W and Levine, A M and Matson, R A and McDermott, S and Osborne, H L M and Paegert, M and Quinn, S N and Redfield, S and Ricker, G R and Schlieder, J E and Scott, N J and Seager, S and Smith, A M S and Tenenbaum, P and Twicken, J D and Vanderspek, R and Van Eylen, V and Winn, J N},
    title = "{Hot planets around cool stars – two short-period mini-Neptunes transiting the late K-dwarf TOI-1260}",
    journal = {Monthly Notices of the Royal Astronomical Society},
    volume = {505},
    number = {4},
    pages = {4684-4701},
    year = {2021},
    month = {05},
    abstract = "{We present the discovery and characterization of two sub-Neptunes in close orbits, as well as a tentative outer planet of a similar size, orbiting TOI-1260 – a low metallicity K6 V dwarf star. Photometry from Transiting Exoplanet Survey Satellite(TESS) yields radii of Rb = 2.33 ± 0.10 and Rc = 2.82 ± 0.15 R⊕, and periods of 3.13 and 7.49 d for TOI-1260 b and TOI-1260 c, respectively. We combined the TESS data with a series of ground-based follow-up observations to characterize the planetary system. From HARPS-N high-precision radial velocities we obtain Mb = \\$8.6 \_\\{ - 1.5 \\} ^ \\{ + 1.4 \\}\\$ and Mc = \\$11.8 \_\\{ - 3.2 \\} ^ \\{ + 3.4 \\}\\$ M⊕. The star is moderately active with a complex activity pattern, which necessitated the use of Gaussian process regression for both the light-curve detrending and the radial velocity modelling, in the latter case guided by suitable activity indicators. We successfully disentangle the stellar-induced signal from the planetary signals, underlining the importance and usefulness of the Gaussian process approach. We test the system’s stability against atmospheric photoevaporation and find that the TOI-1260 planets are classic examples of the structure and composition ambiguity typical for the 2–3 R⊕ range.}",
    issn = {0035-8711},
    doi = {10.1093/mnras/stab1464},
    url = {https://doi.org/10.1093/mnras/stab1464},
    eprint = {https://academic.oup.com/mnras/article-pdf/505/4/4684/38824317/stab1464.pdf},
    }

    DOI arXiv
  226. D. Cont, F. Yan, A. Reiners, N. Casasayas-Barris, P. Mollière, E. Pallé, Th. Henning, L. Nortmann, M. Stangret, S. Czesla, M. López-Puertas, A. Sánchez-López, F. Rodler, I. Ribas, A. Quirrenbach, J. A. Caballero, P. J. Amado, L. Carone, J. Khaimova, L. Kreidberg, K. Molaverdikhani, D. Montes, G. Morello, E. Nagel, M. Oshagh, M. Zechmeister

    Detection of Fe and evidence for TiO in the dayside emission spectrum of WASP-33b

    bib

    @article{Cont_2021,
    doi = {10.1051/0004-6361/202140732},

    url = {https://doi.org/10.1051%2F0004-6361%2F202140732},

    year = 2021,
    month = {may},

    publisher = {{EDP} Sciences},

    author = {D. Cont and F. Yan and A. Reiners and N. Casasayas-Barris and P. Molli{\`{e}
    }re and E. Pall{\'{e}} and Th. Henning and L. Nortmann and M. Stangret and S. Czesla and M. L{\'{o}}pez-Puertas and A. S{\'{a}}nchez-L{\'{o}}pez and F. Rodler and I. Ribas and A. Quirrenbach and J. A. Caballero and P. J. Amado and L. Carone and J. Khaimova and et al},

    title = {Detection of Fe and evidence for {TiO} in the dayside emission spectrum of {WASP}-33b},

    journal = {Astronomy {\&}amp$\mathsemicolon$ Astrophysics}
    }

    DOI arXiv
  227. K. Monsch, G. Picogna, B. Ercolano, T. Preibisch

    The imprint of X-ray photoevaporation of planet-forming discs on the orbital distribution of giant planets. II. Theoretical predictions

    bib

    @article{Monsch_2021,
    doi = {10.1051/0004-6361/202140647},

    url = {https://doi.org/10.1051%2F0004-6361%2F202140647},

    year = 2021,
    month = {jun},

    publisher = {{EDP} Sciences},

    volume = {650},

    pages = {A199},

    author = {Kristina Monsch and Giovanni Picogna and Barbara Ercolano and Thomas Preibisch},

    title = {The imprint of X-ray photoevaporation of planet-forming discs on the orbital distribution of giant planets},

    journal = {Astronomy {\&}amp$\mathsemicolon$ Astrophysics}
    }

    DOI arXiv
  228. Ó. Carrión-González, A. García Muñoz, J. Cabrera, S. Czismadia, N. C. Santos, H. Rauer

    Catalogue of exoplanets accessible in reflected starlight to the Nancy Grace Roman Space Telescope. A population study and prospects for phase-curve measurements

  229. R. Dawson, C. Huang, R. Brahm, K. A. Collins, M. J. Hobson, A. Jordán, J. Dong, J. Korth, T. Trifonov, L. Abe, A. Agabi, I. Bruni, R. P. Butler, M. Barbieri, K. I. Collins, D. Conti, J. D. Crane, N. Crouzet, G. Dransfield, P. Evans, N. Espinoza, T. Gan, T. Guillot, T. Henning, J. J. Lissauer, E. Jensen, W. Sainte, D. Mékarnia, G. Myers, S. Nandakumar, H. Relles, P. Sarkis, P. Torres, S. Shectman, F. X. Schmider, A. Shporer, C. Stockdale, J. Teske, A. Triaud, S. Wang, C. Ziegler, G. Ricker, R. Vanderspek, D. W. Latham, S. Seager, J. N. Winn, J. M. Jenkins, L. Bouma, J. A. Burt, D. Charbonneau, A. Levine, S. McDermott, B. McLean, M. Rose, B. Wohler

    Precise Transit and Radial-velocity Characterization of a Resonant Pair: The Warm Jupiter TOI-216c and Eccentric Warm Neptune TOI-216b.

    bib

    @ARTICLE{2021AJ....161..161D,
    author = {{Dawson}, Rebekah I. and {Huang}, Chelsea X. and {Brahm}, Rafael and {Collins}, Karen A. and {Hobson}, Melissa J. and {Jord{\'a}n}, Andr{\'e}s and {Dong}, Jiayin and {Korth}, Judith and {Trifonov}, Trifon and {Abe}, Lyu and {Agabi}, Abdelkrim and {Bruni}, Ivan and {Butler}, R. Paul and {Barbieri}, Mauro and {Collins}, Kevin I. and {Conti}, Dennis M. and {Crane}, Jeffrey D. and {Crouzet}, Nicolas and {Dransfield}, Georgina and {Evans}, Phil and {Espinoza}, N{\'e}stor and {Gan}, Tianjun and {Guillot}, Tristan and {Henning}, Thomas and {Lissauer}, Jack J. and {Jensen}, Eric L.~N. and {Sainte}, Wenceslas Marie and {M{\'e}karnia}, Djamel and {Myers}, Gordon and {Nandakumar}, Sangeetha and {Relles}, Howard M. and {Sarkis}, Paula and {Torres}, Pascal and {Shectman}, Stephen and {Schmider}, Fran{\c{c}}ois-Xavier and {Shporer}, Avi and {Stockdale}, Chris and {Teske}, Johanna and {Triaud}, Amaury H.~M.~J. and {Wang}, Sharon Xuesong and {Ziegler}, Carl and {Ricker}, G. and {Vanderspek}, R. and {Latham}, David W. and {Seager}, S. and {Winn}, J. and {Jenkins}, Jon M. and {Bouma}, L.~G. and {Burt}, Jennifer A. and {Charbonneau}, David and {Levine}, Alan M. and {McDermott}, Scott and {McLean}, Brian and {Rose}, Mark E. and {Vanderburg}, Andrew and {Wohler}, Bill},
    title = "{Precise Transit and Radial-velocity Characterization of a Resonant Pair: The Warm Jupiter TOI-216c and Eccentric Warm Neptune TOI-216b}",
    journal = {\aj},
    keywords = {Exoplanet astronomy, Exoplanet dynamics, Transit timing variation method, Radial velocity, 486, 490, 1710, 1332, Astrophysics - Earth and Planetary Astrophysics},
    year = 2021,
    month = apr,
    volume = {161},
    number = {4},
    eid = {161},
    pages = {161},
    doi = {10.3847/1538-3881/abd8d0},
    archivePrefix = {arXiv},
    eprint = {2102.06754},
    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021AJ....161..161D},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

    DOI arXiv
  230. V. Christiaens, M. G. Ubeira-Gabellini, H. Cánovas, P. Delorme, B. Pairet, O. Absil, S. Casassus, J. Girard, A. Zurlo, Y. Aoyama, G.-D. Marleau, L. Spina, N. Marel, L. Cieza, G. Lodato, S. Pérez, C. Pinte, D. Price, M. Reggiani

    A faint companion around CrA-9: protoplanet or obscured binary?

    bib

    @ARTICLE{2021MNRAS.502.6117C,
    author = {{Christiaens}, V. and {Ubeira-Gabellini}, M. -G. and {C{\'a}novas}, H. and {Delorme}, P. and {Pairet}, B. and {Absil}, O. and {Casassus}, S. and {Girard}, J.~H. and {Zurlo}, A. and {Aoyama}, Y. and {Marleau}, G. -D. and {Spina}, L. and {van der Marel}, N. and {Cieza}, L. and {Lodato}, G. and {P{\'e}rez}, S. and {Pinte}, C. and {Price}, D.~J. and {Reggiani}, M.},
    title = "{A faint companion around CrA-9: protoplanet or obscured binary?}",
    journal = {\mnras},
    keywords = {techniques: image processing, planets and satellites: formation, planet-disc interactions, protoplanetary discs, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
    year = 2021,
    month = apr,
    volume = {502},
    number = {4},
    pages = {6117-6139},
    doi = {10.1093/mnras/stab480},
    archivePrefix = {arXiv},
    eprint = {2102.10288},
    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021MNRAS.502.6117C},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

    DOI arXiv
  231. I. Kondo, J. C. Yee, D. P. Bennett, T. Sumi, N. Koshimoto, I. A. Bond, A. Gould, A. Udalski, Y. Shvartzvald, Y. K. Jung, W. Zang, V. Bozza, E. Bachelet, M. Hundertmark, N. J. Rattenbury, F. Abe, R. K. Barry, A. Bhattacharya, M. Donachie, A. Fukui, H. Fujii, Y. Hirao, S. Ishitani Silva, Y. Itow, R. Kirikawa, J. Li, Y. Matsubara, S. Miyazaki, Y. Muraki, G. Olmschenk, C. Ranc, Y. Satoh, H. Shoji, D. Suzuki, Y. Tanaka, P. J. Tristram, T. Yamawaki, A. Yonehara, P. Mróz, R. Poleski, J. Skowron, M. K. Szymański, I. Szymański, K. Ulaczyk, K. A. Rybicki, P. Iwanek, M. Wrona, M. Albrow, S. J. Chung, C. Han, K. H. Hwang, H. W. Kim, I. G. Shin, S. M. Cha, D. J. Kim, S. L. Kim, C. U. Lee, D. J. Lee, Y. Lee, S.L. Lee, B. G. Park, R. W. Pogge, Y. H. Ryu, C. A. Beichman, G. Bryden, S. Calchi Novati, S. Carey, B. S. Gaudi, C. B. Henderson, W. Zhu, D. Maoz, M. T. Penny, M. Dominik, U. G. Jørgensen, P. Longa-Peña, N. Peixinho, S. Sajadian, J. Skottfelt, C. Snodgrass, J. Tregloan-Reed, M. J. Burgdorf, J. Campbell-White, Y. I. Fujii, T. C. Hinse, E. Khalouei, S. Rahvar, M. Rabus, J. Southworth, Y. Tsapras, R. A. Street, D. M. Bramich, A. Cassan, K. Horne, S. Mao, A. Saha

    OGLE-2018-BLG-1185b : A Low-Mass Microlensing Planet Orbiting a Low-Mass Dwarf.

    bib

    @ARTICLE{2021arXiv210402157K,
    author = {{Kondo}, Iona and {Yee}, Jennifer C. and {Bennett}, David P. and {Sumi}, Takahiro and {Koshimoto}, Naoki and {Bond}, Ian A. and {Gould}, Andrew and {Udalski}, Andrzej and {Shvartzvald}, Yossi and {Jung}, Youn Kil and {Zang}, Weicheng and {Bozza}, Valerio and {Bachelet}, Etienne and {Hundertmark}, Markus P.~G. and {Rattenbury}, Nicholas J. and {Abe}, F. and {Barry}, R. and {Bhattacharya}, A. and {Donachie}, M. and {Fukui}, A. and {Fujii}, H. and {Hirao}, Y. and {Ishitani Silva}, S. and {Itow}, Y. and {Kirikawa}, R. and {Li}, M.~C.~A. and {Matsubara}, Y. and {Miyazaki}, S. and {Muraki}, Y. and {Olmschenk}, G. and {Ranc}, C. and {Satoh}, Y. and {Shoji}, H. and {Suzuki}, D. and {Tanaka}, Y. and {Tristram}, P.~J. and {Yamawaki}, T. and {Yonehara}, A. and {Mr{\'o}z}, P. and {Poleski}, R. and {Skowron}, J. and {Szyma{\'n}ski}, M.~K. and {Soszy{\'n}ski}, I. and {Koz{\l}owski}, S. and {Ulaczyk}, P. Pietrukowicz K. and {Rybicki}, K.~A. and {Iwanek}, P. and {Wrona}, M. and {Albrow}, M.~D. and {Chung}, S. -J. and {Han}, C. and {Hwang}, K. -H. and {Kim}, H. -W. and {Shin}, I. -G. and {Cha}, S. -M. and {Kim}, D. -J. and {Kim}, S. -L. and {Lee}, C. -U. and {Lee}, D. -J. and {Lee}, Y. and {Park}, B. -G. and {Pogge}, R.~W. and {Ryu}, Y. -H. and {Beichman}, C.~A. and {Bryden}, G. and {Calchi Novati}, S. and {Carey}, S. and {Gaudi}, B.~S. and {Henderson}, C.~B. and {Zhu}, W. and {Maoz}, D. and {Penny}, M.~T. and {Dominik}, M. and {J{\o}rgensen}, U.~G. and {Longa-Pe\{\textbackslash\raisebox{-0.5ex}\textasciitilde\{ n\}\}a}, P. and {Peixinho}, N. and {Sajadian}, S. and {Skottfelt}, J. and {Snodgrass}, C. and {Tregloan-Reed}, J. and {Burgdorf}, M.~J. and {Campbell-White}, J. and {Dib}, S. and {Fujii}, Y.~I. and {Hinse}, T.~C. and {Khalouei}, E. and {Rahvar}, S. and {Rabus}, M. and {Southworth}, J. and {Tsapras}, Y. and {Street}, R.~A. and {Bramich}, D.~M. and {Cassan}, A. and {Horne}, K. and {Wambsganss}, J. and {Mao}, S. and {Saha}, A.},
    title = "{OGLE-2018-BLG-1185b : A Low-Mass Microlensing Planet Orbiting a Low-Mass Dwarf}",
    journal = {arXiv e-prints},
    keywords = {Astrophysics - Earth and Planetary Astrophysics},
    year = 2021,
    month = apr,
    eid = {arXiv:2104.02157},
    pages = {arXiv:2104.02157},
    archivePrefix = {arXiv},
    eprint = {2104.02157},
    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021arXiv210402157K},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

    DOI arXiv
  232. S. Ataiee, W. Kley

    Pushing planets into an inner cavity by a resonant chain

    bib

    @article{2021A&A...648A..69A,
    author = {{Ataiee}, S. and {Kley}, W.},
    title = {{Pushing planets into an inner cavity by a resonant chain}},
    journal = {\aap},
    keywords = {methods: numerical, hydrodynamics, planets and satellites: dynamical evolution and stability, protoplanetary disks, Astrophysics - Earth and Planetary Astrophysics},
    year = 2021,
    month = apr,
    volume = {648},
    eid = {A69},
    pages = {A69},
    doi = {10.1051/0004-6361/202038772},
    archiveprefix = {arXiv},
    eprint = {2102.08612},
    primaryclass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...648A..69A},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

    DOI arXiv
  233. N. Casasayas-Barris, M. Stangret, V. Bourrier, H. M. Tabernero, F. Yan, F. Borsa, R. Allart, M. R. Zapatero Osorio, C. Lovis, S. G. Sousa, G. Chen, M. Oshagh, N. C. Santos, F. Pepe, R. Rebolo, P. Molaro, S. Cristiani, V. Adibekyan, Y. Alibert, C. Allende Prieto, F. Bouchy, O. Demangeon, P. Di Marcantonio, V. D'Odorico, D. Ehrenreich, P. Figueira, R. Génova Santos, J. I. González Hernández, B. Lavie, J. Lillo-Box, G. Lo Curto, C. Martins, A. Mehner, G. Micela, N. Nunes, E. Poretti, A. Sozzetti, A. Suárez Mascareño, S. Udry

    The atmosphere of HD 209458b seen with ESPRESSO. No detectable planetary absorptions at high resolution

    bib

    @ARTICLE{2021A&A...647A..26C,
    author = {{Casasayas-Barris}, N. and {Palle}, E. and {Stangret}, M. and {Bourrier}, V. and {Tabernero}, H.~M. and {Yan}, F. and {Borsa}, F. and {Allart}, R. and {Zapatero Osorio}, M.~R. and {Lovis}, C. and {Sousa}, S.~G. and {Chen}, G. and {Oshagh}, M. and {Santos}, N.~C. and {Pepe}, F. and {Rebolo}, R. and {Molaro}, P. and {Cristiani}, S. and {Adibekyan}, V. and {Alibert}, Y. and {Allende Prieto}, C. and {Bouchy}, F. and {Demangeon}, O.~D.~S. and {Di Marcantonio}, P. and {D'Odorico}, V. and {Ehrenreich}, D. and {Figueira}, P. and {G{\'e}nova Santos}, R. and {Gonz{\'a}lez Hern{\'a}ndez}, J.~I. and {Lavie}, B. and {Lillo-Box}, J. and {Lo Curto}, G. and {Martins}, C.~J.~A.~P. and {Mehner}, A. and {Micela}, G. and {Nunes}, N.~J. and {Poretti}, E. and {Sozzetti}, A. and {Su{\'a}rez Mascare{\~n}o}, A. and {Udry}, S.},
    title = "{The atmosphere of HD 209458b seen with ESPRESSO. No detectable planetary absorptions at high resolution}",
    journal = {\aap},
    keywords = {planets and satellites: individual: HD 209458b, planets and satellites: atmospheres, methods: observational, techniques: spectroscopic, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
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    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...647A..26C},
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    DOI arXiv
  234. E. Brown, S. C. Marsden, M. Mengel, S. V. Jeffers, I. Millburn, M. Mittag, P. Petit, A. Vidotto, J. Morin, V. See, M. M. Jardine, J. González-Pérez, BCool Collaboration

    Magnetic field and chromospheric activity evolution of HD 75332: a rapid magnetic cycle in an F star without a hot Jupiter

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    DOI arXiv
  235. R. Asensio-Torres, T. Henning, F. Cantalloube, P. Pinilla, D. Mesa, A. Garufi, S. Jorquera, R. Gratton, G. Chauvin, J. Szulagyi, R. van Boekel, R. Dong, G.-D. Marleau, M. Benisty, M. Villenave, C. Bergez-Casalou, C. Desgrange, M. Janson, M. Keppler, M. Langlois, F. Menard, E. Rickman, T. Stolker, M. Feldt, T. Fusco, L. Gluck, A. Pavlov, J. Ramos

    Perturbers: SPHERE detection limits to planetary-mass companions in protoplanetary disks

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    keywords = {Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
    year = 2021,
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    eprint = {2103.05377},
    primaryClass = {astro-ph.EP},
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    DOI arXiv
  236. F. Wunderlich, M. Scheucher, J. L. Grenfell, F. Schreier, C. Sousa-Silva, M. Godolt, H. Rauer

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    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...647A..48W},
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    DOI arXiv
  237. R. H. Tilbrook, M. R. Burleigh, J. C. Costes, S. Gill, L. D. Nielsen, J. I. Vines, D. Queloz, S. T. Hodgkin, H. L. Worters, M. R. Goad, J. S. Acton, B. A. Henderson, D. J. Armstrong, D. R. Anderson, D. Bayliss, F. Bouchy, J. T. Briegal, E. M. Bryant, S. L. Casewell, A. Chaushev, B. F. Cooke, P. Eigmüller, E. Gillen, M. N. Günther, A. Hogan, J. S. Jenkins, M. Lendl, J. McCormac, M. Moyano, L. Raynard, A. M. S. Smith, S. Udry, C. A. Watson, R. G. West, P. J. Wheatley, H. Breytenbach, R. R. Sefako, J. K. Thomas, D. R. Alves

    NGTS 15b, 16b, 17b and 18b: four hot Jupiters from the Next Generation Transit Survey

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    archiveprefix = {arXiv},
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    primaryclass = {astro-ph.EP},
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    DOI arXiv
  238. T.W. Moldenhauer, R. Kuiper, W. Kley

    Steady State by Recycling prevents Premature Collapse of Protoplanetary Atmospheres

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    keywords = {Astrophysics - Earth and Planetary Astrophysics},
    year = 2021,
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    pages = {arXiv:2102.00939},
    archivePrefix = {arXiv},
    eprint = {2102.00939},
    primaryClass = {astro-ph.EP},
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    DOI arXiv
  239. G. Scandariato, F. Borsa, D. Sicilia, L. Malavolta, K. Biazzo, A. S. Bonomo, G. Bruno, R. Claudi, E. Covino, P. Di Marcantonio, M. Esposito, G. Frustagli, A. F. Lanza, J. Maldonado, A. Maggio, L. Mancini, G. Micela, D. Nardiello, M. Rainer, V. Singh, A. Sozzetti, L. Affer, S. Benatti, A. Bignamini, V. Biliotti, R. Capuzzo-Dolcetta, I. Carleo, R. Cosentino, M. Damasso, S. Desidera, A. Gurtubai, A. Ghedina, P. Giacobbe, E. Giani, A. Harutyunyan, N. Hernandez, M. Hernandez Diaz, C. Knapic, G. Leto, A. F. Martinez Fiorenzano, E. Molinari, V. Nascimbeni, I. Pagano, M. Pedani, G. Piotto, E. Poretti, H. Stoev

    The GAPS Programme at TNG. XXIX. No detection of reflected light from 51 Peg b using optical high-resolution spectroscopy

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    keywords = {techniques: spectroscopic, planets and satellites: atmospheres, planets and satellites: detection, planets and satellites: gaseous planets, planets and satellites: individual: 51 Peg b, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
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    archivePrefix = {arXiv},
    eprint = {2012.10435},
    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...646A.159S},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

    DOI arXiv
  240. M. Janson, V. Squicciarini, P. Delorme, R. Gratton, M. Bonnefoy, S. Reffert, S. C. Eriksson, A. Vigan, M. Langlois, N. Engler, G. Chauvin, S. Desidera, L. Mayer, G.-D. Marleau, A. J. Bohn, M. Samland, M. Meyer, V. D'Orazi, T. Henning, S. P. Quanz, M. Kenworthy, J. C. Carson

    BEAST begins: sample characteristics and survey performance of the B-star Exoplanet Abundance Study

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    year = 2021,
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    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...646A.164J},
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  241. L. Carone, P. Mollière, G. Zhou, J. Bouwman, F. Yan, R. Baeyens, D. Apai, N. Espinoza, B. V. Rackham, A. Jordán, D. Angerhausen, L. Decin, M. Lendl, O. Venot, T. Henning

    Indications for very high metallicity and absence of methane in the eccentric exo-Saturn WASP-117b

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  242. K. Monsch, G. Picogna, B. Ercolano, W. Kley

    Giant planet migration during the disc dispersal phase

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    keywords = {protoplanetary disks, planet-disk interactions, planets and satellites: gaseous planets, X-rays: stars, methods: numerical, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
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    month = feb,
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    archivePrefix = {arXiv},
    eprint = {2101.01179},
    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...646A.169M},
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    DOI arXiv
  243. A. Smith, J. S. Acton, D. R. Anderson, D. J. Armstrong, D. Bayliss, C. Belardi, F. Bouchy, R. Brahm, J. T. Briegal, E. Bryant, M. R. Burleigh, J. Cabrera, A. Chaushev, B. Cooke, J. C. Costes, S. Csizmadia, P. Eigmüller, A. Erikson, S. Gill, E. Gillen, M. R. Goad, M. N. Günther, C. B. Henderson, A. Hogan, A. Jordán, M. Lendl, J. McCormac, M. Moyano, L. D. Nielsen, H. Rauer, L. Raynard, R. H. Tilbrook, O. Turner, S. Udry, J. I. Vines, C. A. Watson, R. G. West, P. J. Wheatley

    NGTS-14Ab: a Neptune-sized transiting planet in the desert

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    year = 2021,
    month = feb,
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    archivePrefix = {arXiv},
    eprint = {2101.01470},
    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...646A.183S},
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    DOI arXiv
  244. P. Gao, H. R. Wakeford, S. Moran, V. Parmentier

    Aerosols in Exoplanet Atmospheres

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    keywords = {Astrophysics - Earth and Planetary Astrophysics},
    year = 2021,
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    pages = {arXiv:2102.03480},
    archivePrefix = {arXiv},
    eprint = {2102.03480},
    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021arXiv210203480G},
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  245. W. Dietrich, P. Wulff, J. Wicht, U. R. Christensen

    Linking Zonal Winds and Gravity II: explaining the equatorially antisymmetric gravity moments of Jupiter

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    journal = {arXiv e-prints},
    keywords = {Astrophysics - Earth and Planetary Astrophysics},
    year = 2021,
    month = feb,
    eid = {arXiv:2102.12854},
    pages = {arXiv:2102.12854},
    archivePrefix = {arXiv},
    eprint = {2102.12854},
    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021arXiv210212854D},
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  246. J. D. Melon Fuksman, H. Klahr, M. Flock, A. Mignone

    A Two-moment Radiation Hydrodynamics Scheme Applicable to Simulations of Planet Formation in Circumstellar Disks

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  247. J. L. Grenfell, J. Leconte, F. Forget, M. Godolt, Ó. Carrión-González, L. Noack, F. Tian, H. Rauer, F. Gaillard, E. Bolmont, B. Charnay, M. Turbet

    Possible Atmospheric Diversity of Low Mass Exoplanets – Some Central Aspects

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  248. S. Petrus, M. Bonnefoy, G. Chauvin, B. Charnay, G.-D. Marleau, R. Gratton, A. M. Lagrange, J. Rameau, C. Mordasini, M. Nowak, P. Delorme, A. Boccaletti, A. Carlotti, M. Houllé, A. Vigan, F. Allard, S. Desidera, V. D'Orazi, H. J. Hoeijmakers, A. Wyttenbach, B. Lavie

    A medium-resolution spectrum of the exoplanet HIP 65426 b

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  249. H. Parviainen, M. R. Zapatero Osorio, G. Nowak, A. Fukui, F. Murgas, N. Narita, K. G. Stassun, J. H. Livingston, K. A. Collins, D. Hidalgo Soto, V. J. S. Béjar, J. Korth, M. Monelli, P. Montañés-Rodríguez, N. Casasayas-Barris, G. Chen, N. Crouzet, J. de Leon, A. Hernandez, K. Kawauchi, P. Klagyivik, N. Kusakabe, R. Luque, M. Mori, T. Nishiumi, J. Prieto-Arranz, M. Tamura, N. Watanabe, T. Gan, E. Jensen, T. Barclay, J. Doty, J. M. Jenkins, D. W. Latham, M. Paegert, G. Ricker, D. Rodriguez, S. Seager, A. Shporer, R. Vanderspek, J. Noel Villaseñor, J. N. Winn, B. Wohler, I. Wong

    TOI-519 b: A short-period substellar object around an M dwarf validated using multicolour photometry and phase curve analysis

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    title = "{TOI-519 b: A short-period substellar object around an M dwarf validated using multicolour photometry and phase curve analysis}",
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    keywords = {stars: individual: TIC 218 795 833, planets and satellites: general, methods: statistical, techniques: photometric, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
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    pages = {A16},
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    archivePrefix = {arXiv},
    eprint = {2011.11458},
    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...645A..16P},
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    DOI arXiv
  250. F. Yan, A. Wyttenbach, N. Casasayas-Barris, A. Reiners, T. Henning, P. Mollière, S. Czesla, L. Nortmann, K. Molaverdikhani, G. Chen, I. A. G. Snellen, M. Zechmeister, C. Huang, I. Ribas, A. Quirrenbach, J. A. Caballero, P. J. Amado, D. Cont, S. Khalafinejad, J. Khaimova, M. López-Puertas, D. Montes, E. Nagel, M. Oshagh, S. Pedraz, M. Stangret

    Detection of the hydrogen Balmer lines in the ultra-hot Jupiter WASP-33b

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    title = "{Detection of the hydrogen Balmer lines in the ultra-hot Jupiter WASP-33b}",
    journal = {\aap},
    keywords = {planets and satellites: atmospheres, techniques: spectroscopic, planets and satellites: individual: WASP-33b, Astrophysics - Earth and Planetary Astrophysics},
    year = 2021,
    month = jan,
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    eid = {A22},
    pages = {A22},
    doi = {10.1051/0004-6361/202039302},
    archivePrefix = {arXiv},
    eprint = {2011.07888},
    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...645A..22Y},
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  251. R. Luque, L. M. Serrano, K. Molaverdikhani, M. Nixon, J. Livingston, E. Guenther, N. Madhusudhan, G. Nowak, J. Korth, W. D. Cochran, T. Hirano, P. Chaturvedi, E. Goffo, S. Albrecht, O. Barragán, C. Briceño, J. Cabrera, D. Charbonneau, R. Cloutier, K. A. Collins, K. I. Collins, K. Colòn, I. Crossfield, S. Csizmadia, F. Dai, H. Deeg, M. Esposito, M. Fridlund, D. Gandolfi, I. Georgieva, A. Glidden, R. Goeke, S. Grziwa, A. P. Hatzes, C. E. Henze, S. Howell, J. Irwin, J. M. Jenkins, E. Jensen, P. Kabáth, R. Kidwell, J. Kielkopf, E. Knudstrup, K. W. F. Lam, D. W. Latham, J. J. Lissauer, A. W. Mann, E. Matthews, I. Mireles, N. Narita, M. Paegert, C. M. Persson, S. Redfield, G. Ricker, F. Rodler, J. E. Schlieder, N. Scott, S. Seager, J. Subjak, T. Tan, E. B. Ting, R. Vanderspek, V. Van Eylen, J. N. Winn, C. Ziegler

    A planetary system with two transiting mini-Neptunes near the radius valley transition around the bright M dwarf TOI-776

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    archivePrefix = {arXiv},
    eprint = {2009.08338},
    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...645A..41L},
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    DOI arXiv
  252. O. Schib, C. Mordasini, N. Wenger, G.-D. Marleau, R. Helled

    The influence of infall on the properties of protoplanetary discs. Statistics of masses, sizes, lifetimes, and fragmentation

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    DOI arXiv
  253. P. Sarkis, C. Mordasini, T. Henning, G.-D. Marleau, P. Mollière

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    eprint = {2009.04291},
    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...645A..79S},
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    DOI arXiv
  254. O. Voelkel, R. Deienno, K. Kretke, H. Klahr

    Linking planetary embryo formation to planetesimal formation. I. The effect of the planetesimal surface density in the terrestrial planet zone

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    archivePrefix = {arXiv},
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    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...645A.131V},
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    DOI arXiv
  255. O. Voelkel, R. Deienno, K. Kretke, H. Klahr

    Linking planetary embryo formation to planetesimal formation. II. The effect of pebble accretion in the terrestrial planet zone

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    journal = {\aap},
    keywords = {planets and satellites: formation, planets and satellites: terrestrial planets, Astrophysics - Earth and Planetary Astrophysics},
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    month = jan,
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    archivePrefix = {arXiv},
    eprint = {2008.10432},
    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...645A.132V},
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    }

    DOI arXiv
  256. A. Krieger, S. Wolf

    The scattering order problem in Monte Carlo radiative transfer

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    month = jan,
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    archivePrefix = {arXiv},
    eprint = {2011.14905},
    primaryClass = {astro-ph.IM},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...645A.143K},
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  257. T. Stolker, G.-D. Marleau, G. Cugno, P. Mollière, S. P. Quanz, K. O. Todorov, J. Kühn

    MIRACLES: atmospheric characterization of directly imaged planets and substellar companions at 4-5 μm. II. Constraints on the mass and radius of the enshrouded planet PDS 70 b

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    eprint = {2009.04483},
    primaryclass = {astro-ph.EP},
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    DOI arXiv
  258. M. Tala-Pinto, S. Reffert, A. Quirrenbach, S. Stock, T. Trifonov, D. S. Mitchell

    Precise radial velocities of giant stars. XIV. Evidence of planetary companions around HD 25723

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    keywords = {techniques: radial velocities, planetary systems, planets and satellites: detection, brown dwarfs, stars: evolution},
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    Spectral appearance of the planetary-surface accretion shock: Global spectra and hydrogen-line profiles and fluxes

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    keywords = {Earth and Planetary Astrophysics (astro-ph.EP), FOS: Physical sciences, FOS: Physical sciences},

    title = {Spectral appearance of the planetary-surface accretion shock: Global spectra and hydrogen-line profiles and fluxes},

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    year = {2020},

    copyright = {Creative Commons Attribution 4.0 International}
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    arXiv
  260. L. Fossati, D. Shulyak, A. G. Sreejith, T. Koskinen, M. E. Young, P. E. Cubillos, L. M. Lara, K. France, M. Rengel, P. W. Cauley, J. D. Turner, A. Wyttenbach, F. Yan

    A data-driven approach to constraining the atmospheric temperature structure of the ultra-hot Jupiter KELT-9b

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    DOI arXiv
  261. M. Lendl, S. Csizmadia, A. Deline, L. Fossati, D. Kitzmann, K. Heng, S. Hoyer, S. Salmon, W. Benz, C. Broeg, D. Ehrenreich, A. Fortier, D. Queloz, A. Bonfanti, A. Brandeker, A. Collier Cameron, L. Delrez, A. García Muñoz, M. J. Hooton, P. F. L. Maxted, B. M. Morris, V. Van Grootel, T. G. Wilson, Y. Alibert, R. Alonso, J. Asquier,, T. Bandy, T. Bárczy, D. Barrado, S. C. C. Barros, W. Baumjohann, M. Beck, T. Beck, A. Bekkelien, M. Bergomi, N. Billot, F. Biondi, X. Bonfils, V. Bourrier, M. D. Busch, J. Cabrera, V. Cessa, S. Charnoz, B. Chazelas, C. Corral Van Damme, M. B. Davies, M. Deleuil, O. D. S. Demangeon, B. O. Demory, A. Erikson, J. Farinato, M. Fridlund, D. Futyan, D. Gandolfi, M. Gillon, P. Guterman, J. Hasiba, E. Hernandez, K. G. Isaak, L. Kiss, T. Kuntzer, A. Lecavelier des Etangs, T. Lüftinger, J. Laskar, C. Lovis, D. Magrin, L. Malvasio, L. Marafatto, H. Michaelis, M. Munari, V. Nascimbeni, G. Olofsson, H. Ottacher, R. Ottensamer, I. Pagano, G. Peter, D. Piazza, G. Piotto, D. Pollacco, F. Ratti, H. Rauer, R. Ragazzoni, N. Rando, I. Ribas, M. Rieder, R. Rohlfs, F. Safa, N. C. Santos, G. Scandariato, D. Ségransan, A. E. Simon, V. Singh, A. M. S. Smith, M. Sordet, S. G. Sousa, M. Steller, G. M. Szabó, N. Thomas, M. Tschentscher, S. Udry, V. Viotto, I. Walter, N. A. Walton, F. Wildi, D. Wolter

    The hot dayside and asymmetric transit of WASP-189 b seen by CHEOPS

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  263. F. Wunderlich, M. Scheucher, M. Godolt, J. L. Grenfell, F. Schreier, P. C. Schneider, D. J. Wilson, A. Sánchez-López, M. López-Puertas, H. Rauer

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  264. E. M. Amazo-Gómez, A. I. Shapiro, S. K. Solanki, G. Kopp, M. Oshagh, T. Reinhold, A. Reiners

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  266. O. Voelkel, H. Klahr, C. Mordasini, C. Lenz

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  267. M. Rengel, A. Reiners, D. Cont, C. Gapp, J. Khaimova, L. M. Lara, D. Shulyak, F. Yan

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  270. H. Parviainen, J. Korth

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    K2-280 b – a low density warm sub-Saturn around a mildly evolved star

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    title = {{K2-280 b - a low density warm sub-Saturn around a mildly evolved star}},
    journal = {\mnras},
    keywords = {techniques: photometric, techniques: radial velocities, techniques: spectroscopic, planets and satellites: detection, stars: individual: (EPIC 216494238, K2-280), Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
    year = 2020,
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    pages = {4423-4435},
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    archiveprefix = {arXiv},
    eprint = {2007.07939},
    primaryclass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2020MNRAS.497.4423N},
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    DOI arXiv
  285. M. Lisogorskyi, S. Boro Saikia, S. V. Jeffers, H. R. A. Jones, J. Morin, M. Mengel, A. Reiners, A. A. Vidotto, P. Petit

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    keywords = {techniques: radial velocities, stars: activity, stars: individual: HD22049, stars: magnetic field, starspots, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
    year = 2020,
    month = jul,
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    archiveprefix = {arXiv},
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    primaryclass = {astro-ph.EP},
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  286. F. Flammini Dotti, M. B. N. Kouwenhoven, Q. Shu, W. Hao, R. Spurzem

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    journal = {\mnras},
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    month = jul,
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    pages = {3623-3637},
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    archiveprefix = {arXiv},
    eprint = {2007.11999},
    primaryclass = {astro-ph.EP},
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  287. B. Akinsanmi, S. C. C. Barros, N. C. Santos, M. Oshagh, L. M. Serrano

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    keywords = {techniques: photometric, techniques: spectroscopic, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics},
    year = 2020,
    month = jul,
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    number = {3},
    pages = {3484-3492},
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    archiveprefix = {arXiv},
    eprint = {2007.11221},
    primaryclass = {astro-ph.EP},
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  288. K. Stock, M. X. Cai, R. Spurzem, M. B. N. Kouwenhoven, S. Portegies Zwart

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    journal = {\mnras},
    keywords = {methods: numerical, planets and satellites: dynamical evolution and stability, galaxies: clusters: general, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics},
    year = 2020,
    month = jul,
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    number = {2},
    pages = {1807-1825},
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    archiveprefix = {arXiv},
    eprint = {2007.11601},
    primaryclass = {astro-ph.EP},
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  289. S. Gill, P. J. Wheatley, B. F. Cooke, A. Jordán, L. D. Nielsen, D. Bayliss, D. R. Anderson, J. I. Vines, M. Lendl, J. S. Acton, D. J. Armstrong, F. Bouchy, R. Brahm, E. M. Bryant, M. R. Burleigh, S. L. Casewell, P. Eigmüller, N. Espinoza, E. Gillen, M. R. Goad, N. Grieves, M. N. Günther, T. Henning, M. J. Hobson, A. Hogan, J. S. Jenkins, J. McCormac, M. Moyano, H. P. Osborn, D. Pollacco, D. Queloz, H. Rauer, L. Raynard, F. Rojas, P. Sarkis, A. M. S. Smith, M. Tala-Pinto, R. H. Tilbrook, S. Udry, C. A. Watson, R. G. West

    NGTS-11 b (TOI-1847 b): A Transiting Warm Saturn Recovered from a TESS Single-transit Event

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    keywords = {Exoplanet astronomy, Exoplanet detection methods, Exoplanets, Extrasolar gas giants, Photometry, High resolution spectroscopy, 486, 489, 498, 509, 1234, 2096, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
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  290. M. Scheucher, F. Wunderlich, J. L. Grenfell, M. Godolt, F. Schreier, D. Kappel, R. Haus, K. Herbst, H. Rauer

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    keywords = {Radiative transfer simulations, Radiative transfer, Computational methods, Exoplanets, Extrasolar rocky planets, Exoplanet atmospheres, Planetary atmospheres, Mini Neptunes, Super Earths, 1967, 1335, 1965, 498, 511, 487, 1244, 1063, 1655, Astrophysics - Earth and Planetary Astrophysics},
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    Precise mass and radius of a transiting super-Earth planet orbiting the M dwarf TOI-1235: a planet in the radius gap?

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    journal = {\aap},
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    primaryclass = {astro-ph.EP},
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    DOI arXiv
  292. M. Lombart, G. Chauvin, P. Rojo, E. Lagadec, P. Delorme, H. Beust, M. Bonnefoy, R. Galicher, R. Gratton, D. Mesa, M. Bonavita, F. Allard, A. Bayo, A. Boccaletti, S. Desidera, J. Girard, J. S. Jenkins, H. Klahr, G. Laibe, A. M. Lagrange, C. Lazzoni, G.-D. Marleau, D. Minniti, C. Mordasini

    VLT/SPHERE survey for exoplanets around young early-type stars, including systems with multi-belt architectures

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    title = {{VLT/SPHERE survey for exoplanets around young early-type stars, including systems with multi-belt architectures}},
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    keywords = {techniques: imaging spectroscopy, planets and satellites: detection, planets and satellites: fundamental parameters, planets and satellites: atmospheres, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
    year = 2020,
    month = jul,
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    archiveprefix = {arXiv},
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    primaryclass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...639A..54L},
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    The GAPS programme at TNG. XXII. The GIARPS view of the extended helium atmosphere of HD 189733 b accounting for stellar activity

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    title = {{The GAPS programme at TNG. XXII. The GIARPS view of the extended helium atmosphere of HD 189733 b accounting for stellar activity}},
    journal = {\aap},
    keywords = {planets and satellites: atmospheres, planets and satellites: fundamental parameters, techniques: spectroscopic, planets and satellites: individual: HD 189733 b, stars: activity, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
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    month = jul,
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    archiveprefix = {arXiv},
    eprint = {2005.05676},
    primaryclass = {astro-ph.EP},
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  294. D. Shulyak, L. M. Lara, M. Rengel, N. E. Nèmec

    Stellar impact on disequilibrium chemistry and observed spectra of hot Jupiter atmospheres

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    journal = {\aap},
    keywords = {planets and satellites: atmospheres, planets and satellites: composition, stars: activity, methods: numerical, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
    year = 2020,
    month = jul,
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    archiveprefix = {arXiv},
    eprint = {2005.01470},
    primaryclass = {astro-ph.EP},
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  295. S. Hojjatpanah, M. Oshagh, P. Figueira, N. C. Santos, E. M. Amazo-Gómez, S. G. Sousa, V. Adibekyan, B. Akinsanmi, O. Demangeon, J. Faria, J. Gomes da Silva, N. Meunier

    The correlation between photometric variability and radial velocity jitter. Based on TESS and HARPS observations

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  298. S. C. Eriksson, R. Asensio-Torres, M. Janson, Y. Aoyama, G.-D. Marleau, M. Bonnefoy, S. Petrus

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  301. M. Stangret, N. Casasayas-Barris, F. Yan, A. Sánchez-López, M. López-Puertas

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    Three planets transiting the evolved star EPIC 249893012: a hot 8.8-M super-Earth and two warm 14.7 and 10.2-M sub-Neptunes

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  312. S. Boldt, M. Oshagh, S. Dreizler, M. Mallonn, N. C. Santos, A. Claret, A. Reiners, E. Sedaghati

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    Is there Na I in the atmosphere of HD 209458b?. Effect of the centre-to-limb variation and Rossiter-McLaughlin effect in transmission spectroscopy studies

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    primaryclass = {astro-ph.EP},
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  314. G. Chen, N. Casasayas-Barris, F. Yan, M. Stangret, H. M. Cegla, R. Allart, C. Lovis

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    primaryclass = {astro-ph.EP},
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  335. F. Schreier, S. Städt, F. Wunderlich, M. Godolt, J. L. Grenfell

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  336. S. Petrus, M. Bonnefoy, G. Chauvin, C. Babusiaux, P. Delorme, A. M. Lagrange, N. Florent, A. Bayo, M. Janson, B. Biller, E. Manjavacas, G.-D. Marleau, T. Kopytova

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  338. A. Ziampras, S. Ataiee, W. Kley, C. P. Dullemond, C. Baruteau

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    MuSCAT2 multicolour validation of TESS candidates: an ultra-short-period substellar object around an M dwarf

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    DOI arXiv
  340. C. N. Kimmig, C. P. Dullemond, W. Kley

    Effect of wind-driven accretion on planetary migration

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  341. M. Küffmeier, F. G. Goicovic, C. P. Dullemond

    Late encounter events as source of disks and spiral structures. Forming second generation disks

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    DOI arXiv
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    ROME/REA: A Gravitational Microlensing Search for Exoplanets Beyond the Snow Line on a Global Network of Robotic Telescopes. PASP, 131(1006):124401

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  344. F. Yan, N. Casasayas-Barris, K. Molaverdikhani, F. J. Alonso-Floriano, A. Reiners, T. Henning, P. Mollière, G. Chen, L. Nortmann, I. A. G. Snellen, I. Ribas, A. Quirrenbach, J. A. Caballero, P. J. Amado, M. Azzaro, F. F. Bauer, M. Cortés-Contreras, S. Czesla, S. Khalafinejad, L. M. Lara, M. López-Puertas, D. Montes, E. Nagel, M. Oshagh, A. Sánchez-López, M. Stangret, M. Zechmeister

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  345. D. Mesa, M. Keppler, F. Cantalloube, L. Rodet, B. Charnay, R. Gratton, M. Langlois, A. Boccaletti, M. Bonnefoy, A. Vigan, O. Flasseur, J. Bae, M. Benisty, G. Chauvin, S. Desidera, T. Henning, A. M. Lagrange, M. Meyer, J. Milli, J. de Boer, A. Müller, B. Pairet, A. Zurlo, S. Antoniucci, J. L. Baudino, S. Brown Sevilla, E. Cascone, A. Cheetham, R. U. Claudi, P. Delorme, V. D'Orazi, M. Feldt, J. Hagelberg, M. Janson, Q. Kral, E. Lagadec, C. Lazzoni, R. Ligi, A. L. Maire, P. Martinez, F. Menard, N. Meunier, C. Perrot, S. Petrus, C. Pinte, E. L. Rickman, S. Rochat, D. Rouan, M. Samland, J. F. Sauvage, T. Schmidt, S. Udry, L. Weber, F. Wildi

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    Radial velocity confirmation of K2-100b: a young, highly irradiated, and low-density transiting hot Neptune

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  347. Grégoire Montavon, Jasmine MacKenzie, Nadine Nettelmann, Nicola Tosi, Philipp Baumeister, Sebastiano Padovan, Mareike Godolt

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  348. M. X. Cai, S. Portegies Zwart, M. B. N. Kouwenhoven, R. Spurzem

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  350. A. Fukui, D. Suzuki, N. Koshimoto, E. Bachelet, T. Vanmunster, D. Storey, H. Maehara, K. Yanagisawa, T. Yamada, A. Yonehara, T. Hirano, D. P. Bennett, V. Bozza, D. Mawet, M. T. Penny, S. Awiphan, A. Oksanen, T. M. Heintz, T. E. Oberst, V. J. S. Béjar, N. Casasayas-Barris, G. Chen, N. Crouzet, D. Hidalgo, P. Klagyivik, F. Murgas, N. Narita, H. Parviainen, N. Watanabe, N. Kusakabe, M. Mori, Y. Terada, J. P. de Leon, A. Hernandez, R. Luque, M. Monelli, P. Montañés-Rodríguez, J. Prieto-Arranz, K. L. Murata, S. Shugarov, Y. Kubota, C. Otsuki, A. Shionoya, T. Nishiumi, A. Nishide, M. Fukagawa, K. Onodera, Jr. Villanueva, S. R. A. Street, Y. Tsapras, M. Hundertmark, M. Kuzuhara, M. Fujita, C. Beichman, J. P. Beaulieu, R. Alonso, D. E. Reichart, N. Kawai, M. Tamura

    Kojima-1Lb Is a Mildly Cold Neptune around the Brightest Microlensing Host Star

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    NGTS-6b: an ultrashort period hot-Jupiter orbiting an old K dwarf

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    OGLE-2015-BLG-1649Lb: A Gas Giant Planet around a Low-mass Dwarf

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    title = {{A giant exoplanet orbiting a very-low-mass star challenges planet formation models}},
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    DOI arXiv
  364. S. S. Li, W. Zang, A. Udalski, Y. Shvartzvald, D. Huber, C. U. Lee, T. Sumi, A. Gould, S. Mao, P. Fouqué, T. Wang, S. Dong, U. G. Jørgensen, A. Cole, P. Mróz, M. K. Szymański, J. Skowron, R. Poleski, I. Soszyński, P. Pietrukowicz, K. Ulaczyk, K. A. Rybicki, P. Iwanek, J. C. Yee, S. Calchi Novati, C. A. Beichman, G. Bryden, S. Carey, B. S. Gaudi, C. B. Henderson, W. Zhu, M. D. Albrow, S. J. Chung, C. Han, K. H. Hwang, Y. K. Jung, Y. H. Ryu, I. G. Shin, S. M. Cha, D. J. Kim, H. W. Kim, S. L. Kim, D. J. Lee, Y. Lee, B. G. Park, R. W. Pogge, I. A. Bond, F. Abe, R. Barry, D. P. Bennett, A. Bhattacharya, M. Donachie, A. Fukui, Y. Hirao, Y. Itow, I. Kondo, N. Koshimoto, M. C. A. Li, Y. Matsubara, Y. Muraki, S. Miyazaki, M. Nagakane, C. Ranc, N. J. Rattenbury, H. Suematsu, D. J. Sullivan, D. Suzuki, P. J. Tristram, A. Yonehara, G. Christie, J. Drummond, J. Green, S. Hennerley, T. Natusch, I. Porritt, E. Bachelet, D. Maoz, R. A. Street, Y. Tsapras, V. Bozza, M. Dominik, M. Hundertmark, N. Peixinho, S. Sajadian, M. J. Burgdorf, D. F. Evans, R. Figuera Jaimes, Y. I. Fujii, L. K. Haikala, T. Henning, T. C. Hinse, L. Mancini, P. Longa-Peña, S. Rahvar, M. Rabus, J. Skottfelt, C. Snodgrass, J. Southworth, E. Unda-Sanzana, C. von Essen, J. P. Beaulieu, J. Blackman, K. Hill

    OGLE-2017-BLG-1186: first application of asteroseismology and Gaussian processes to microlensing

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    DOI arXiv
  365. J. Wicht, T. Gastine, L. D. V. Duarte, W. Dietrich

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    month = sep,
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    DOI arXiv
  366. D. Shulyak, M. Rengel, A. Reiners, U. Seemann, F. Yan

    Remote sensing of exoplanetary atmospheres with ground-based high-resolution near-infrared spectroscopy

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    keywords = {planets and satellites: atmospheres, planets and satellites: individual: HD 189733 b, radiative transfer, methods: numerical, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
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    DOI arXiv
  367. Y. Tsapras, A. Cassan, C. Ranc, E. Bachelet, R. Street, A. Udalski, M. Hundertmark, V. Bozza, J. P. Beaulieu, J. B. Marquette, E. Euteneuer, D. M. Bramich, M. Dominik, R. Figuera Jaimes, K. Horne, S. Mao, J. Menzies, R. Schmidt, C. Snodgrass, I. A. Steele, J. Wambsganss, P. Mróz, M. K. Szymański, I. Soszyński, J. Skowron, P. Pietrukowicz, R. Poleski, K. Ulaczyk, M. Pawlak, U. G. Jørgensen, J. Skottfelt, A. Popovas, S. Ciceri, H. Korhonen, M. Küffmeier, D. F. Evans, N. Peixinho, T. C. Hinse, M. J. Burgdorf, J. Southworth, R. Tronsgaard, E. Kerins, M. I. Andersen, S. Rahvar, Y. Wang, O. Wertz, M. Rabus, S. Calchi Novati, G. D'Ago, G. Scarpetta, L. Mancini, F. Abe, Y. Asakura, D. P. Bennett, A. Bhattacharya, M. Donachie, P. Evans, A. Fukui, Y. Hirao, Y. Itow, K. Kawasaki, N. Koshimoto, M. C. A. Li, C. H. Ling, K. Masuda, Y. Matsubara, Y. Muraki, S. Miyazaki, M. Nagakane, K. Ohnishi, N. Rattenbury, T. Saito, A. Sharan, H. Shibai, D. J. Sullivan, T. Sumi, D. Suzuki, P. J. Tristram, T. Yamada, A. Yonehara, Robonet Team, OGLE Collaboration

    An analysis of binary microlensing event OGLE-2015-BLG-0060

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    title = {{An analysis of binary microlensing event OGLE-2015-BLG-0060}},
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    month = aug,
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    pages = {4603-4614},
    doi = {10.1093/mnras/stz1404},
    archiveprefix = {arXiv},
    eprint = {1906.02630},
    primaryclass = {astro-ph.EP},
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    DOI arXiv
  368. N. Casasayas-Barris, F. Yan, G. Chen, S. Kohl, M. Stangret, H. Parviainen, Ch. Helling, N. Watanabe, S. Czesla, A. Fukui, P. Montañés-Rodríguez, E. Nagel, N. Narita, L. Nortmann, G. Nowak, J. H. M. M. Schmitt, M. R. Zapatero Osorio

    Atmospheric characterization of the ultra-hot Jupiter MASCARA-2b/KELT-20b. Detection of CaII, FeII, NaI, and the Balmer series of H (Hα, Hβ, and Hγ) with high-dispersion transit spectroscopy

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    title = {{Atmospheric characterization of the ultra-hot Jupiter MASCARA-2b/KELT-20b. Detection of CaII, FeII, NaI, and the Balmer series of H (H{\ensuremath{\alpha}}, H{\ensuremath{\beta}}, and H{\ensuremath{\gamma}}) with high-dispersion transit spectroscopy}},
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    keywords = {planets and satellites: atmospheres, planetary systems, methods: observational, techniques: spectroscopic, planets and satellites: individual: MASCARA-2b, planets and satellites: individual: KELT-20b, Astrophysics - Earth and Planetary Astrophysics},
    year = 2019,
    month = aug,
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    eid = {A9},
    pages = {A9},
    doi = {10.1051/0004-6361/201935623},
    archiveprefix = {arXiv},
    eprint = {1905.12491},
    primaryclass = {astro-ph.EP},
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    DOI arXiv
  369. C. P. Dullemond, M. Küffmeier, F. Goicovic, M. Fukagawa, V. Oehl, M. Kramer

    Cloudlet capture by transitional disk and FU Orionis stars

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    title = {{Cloudlet capture by transitional disk and FU Orionis stars}},
    journal = {\aap},
    keywords = {protoplanetary disks, stars: formation, ISM: clouds, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics},
    year = 2019,
    month = aug,
    volume = {628},
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    archiveprefix = {arXiv},
    eprint = {1911.05158},
    primaryclass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2019A&A...628A..20D},
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    }

    DOI arXiv
  370. G.-D. Marleau, C. Mordasini, R. Kuiper

    The Planetary Accretion Shock. II. Grid of Postshock Entropies and Radiative Shock Efficiencies for Nonequilibrium Radiation Transport

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    keywords = {accretion, accretion disks, methods: analytical, methods: numerical, planets and satellites: formation, planets and satellites: gaseous planets, radiative transfer, Astrophysics - Earth and Planetary Astrophysics},
    year = 2019,
    month = aug,
    volume = {881},
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    archiveprefix = {arXiv},
    eprint = {1906.05869},
    primaryclass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2019ApJ...881..144M},
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    }

    DOI arXiv
  371. D. K. Sing, P. Lavvas, G. E. Ballester, A. Lecavelier des Etangs, M. S. Marley, N. Nikolov, L. Ben-Jaffel, V. Bourrier, L. A. Buchhave, D. L. Deming, D. Ehrenreich, T. Mikal-Evans, T. Kataria, N. K. Lewis, M. López-Morales, A. García Muñoz, G. W. Henry, J. Sanz-Forcada, J. J. Spake, R. Wakeford, PanCET Collaboration

    The Hubble Space Telescope PanCET Program: Exospheric Mg II and Fe II in the Near-ultraviolet Transmission Spectrum of WASP-121b Using Jitter Decorrelation

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    title = {{The Hubble Space Telescope PanCET Program: Exospheric Mg II and Fe II in the Near-ultraviolet Transmission Spectrum of WASP-121b Using Jitter Decorrelation}},
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    keywords = {planets and satellites: atmospheres, stars: individual: WASP-121, techniques: photometric, techniques: spectroscopic, Astrophysics - Earth and Planetary Astrophysics},
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    primaryclass = {astro-ph.EP},
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    DOI arXiv
  372. C. M. Persson, S. Csizmadia, A. J. Mustill, M. Fridlund, A. P. Hatzes, G. Nowak, I. Georgieva, D. Gandolfi, M. B. Davies, J. H. Livingston, P. Montañés-Rodríguez, M. Endl, T. Hirano, J. Prieto-Arranz, J. Korth, S. Grziwa, M. Esposito, S. Albrecht, M. C. Johnson, O. Barragán, H. Parviainen, V. Van Eylen, R. Alonso Sobrino, P. G. Beck, J. Cabrera, I. Carleo, W. D. Cochran, F. Dai, H. J. Deeg, J. P. de Leon, P. Eigmüller, A. Erikson, A. Fukui, L. González-Cuesta, E. W. Guenther, D. Hidalgo, M. Hjorth, P. Kabáth, E. Knudstrup, N. Kusakabe, K. W. F. Lam, M. N. Lund, R. Luque, S. Mathur, F. Murgas, N. Narita, D. Nespral,, P. Niraula, A. O. Henrik Olofsson, M. Pätzold, H. Rauer, S. Redfield, I. Ribas, M. Skarka, A. M. S. Smith, J. Subjak, M. Tamura

    Greening of the brown-dwarf desert. EPIC 212036875b: a 51 MJ object in a 5-day orbit around an F7 V star

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    title = {{Greening of the brown-dwarf desert. EPIC 212036875b: a 51 M$_{J}$ object in a 5-day orbit around an F7 V star}},
    journal = {\aap},
    keywords = {planetary systems, stars: fundamental parameters, stars: individual: EPIC 212036875, techniques: photometric, techniques: radial velocities, Astrophysics - Earth and Planetary Astrophysics},
    year = 2019,
    month = aug,
    volume = {628},
    eid = {A64},
    pages = {A64},
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    archiveprefix = {arXiv},
    eprint = {1906.05048},
    primaryclass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2019A&A...628A..64P},
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    DOI arXiv
  373. D. Höning, N. Tosi, T. Spohn

    Carbon cycling and interior evolution of water-covered plate tectonics and stagnant-lid planets

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    primaryclass = {astro-ph.EP},
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    DOI arXiv
  374. R. G. West, E. Gillen, D. Bayliss, M. R. Burleigh, L. Delrez, M. N. Günther, S. T. Hodgkin, J. A. G. Jackman, J. S. Jenkins, G. W. King, J. McCormac, L. D. Nielsen, L. Raynard, A. M. S. Smith, M. Soto, O. Turner, P. J. Wheatley, Y. Almleaky, D. J. Armstrong, C. Belardi, F. Bouchy, J. T. Briegal, A. Burdanov, J. Cabrera, S. L. Casewell, A. Chaushev, B. Chazelas, P. Chote, B. F. Cooke, S. Csizmadia, E. Ducrot, P. Eigmüller, A. Erikson, E. Foxell, B. T. Gänsicke, M. Gillon, M. R. Goad, E. Jehin, G. Lambert, E. S. Longstaff, T. Louden, M. Moyano, C. Murray, D. Pollacco, D. Queloz, H. Rauer, S. Sohy, S. J. Thompson, S. Udry, S. R. Walker, C. A. Watson

    NGTS-4b: A sub-Neptune transiting in the desert

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    title = {{NGTS-4b: A sub-Neptune transiting in the desert}},
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    DOI arXiv
  375. D. Veras, M. Efroimsky, V. V. Makarov, G. Boué, V. Wolthoff, S. Reffert, A. Quirrenbach, E. P. Tremblay, B. T. Gänsicke

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    DOI arXiv
  376. A. Musso Barcucci, R. Launhardt, G. M. Kennedy, H. Avenhaus, S. S. Brems, R. van Boekel, F. Cantalloube, A. Cheetham, G. Cugno, J. Girard, N. Godoy, T. K. Henning, S. Metchev, A. Müller, J. Olofsson, F. Pepe, S. P. Quanz, A. Quirrenbach, S. Reffert, E. L. Rickman, M. Samland, D. Ségransan

    ISPY – NaCo Imaging Survey for Planets around Young stars. Discovery of an M dwarf in the gap between HD 193571 and its debris ring

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    DOI arXiv
  377. N. R. Deacon, T. Henning, D. E. Kossakowski

    Data-driven stellar parameters for southern TESS FGK targets

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    DOI arXiv
  378. M. Janson, R. Asensio-Torres, D. André, M. Bonnefoy, P. Delorme, S. Reffert, S. Desidera, M. Langlois, G. Chauvin, R. Gratton, A. J. Bohn, S. C. Eriksson, G.-D. Marleau, A. Vigan, J. C. Carson

    The B-Star Exoplanet Abundance Study: a co-moving 16-25 MJup companion to the young binary system HIP 79098

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    DOI arXiv
  379. P. Lavvas, T. Koskinen, M. E. Steinrueck, A. García Muñoz, A. P. Showman

    Photochemical Hazes in Sub-Neptunian Atmospheres with a Focus on GJ 1214bLavvas

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    DOI arXiv
  380. R. A. Street, E. Bachelet, Y. Tsapras, M. P. G. Hundertmark, V. Bozza, M. Dominik, ROME/REA, MiNDSTEp Teams, ROME/REA Team, D. M. Bramich, A. Cassan, K. Horne, S. Mao, A. Saha, J. Wambsganss, W. Zang, MiNDSTEp Team, U. G. Jørgensen, P. Longa-Peña, N. Peixinho, S. Sajadian, M. J. Burgdorf, J. Campbell-White, S. Dib, D. F. Evans, Y. I. Fujii, T. C. Hinse, E. Khalouei, S. Lowry, S. Rahvar, M. Rabus, J. Skottfelt, C. Snodgrass, J. Southworth, J. Tregloan-Reed

    OGLE-2018-BLG-0022: A Nearby M-dwarf Binary

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    DOI arXiv
  381. P. Eigmüller, A. Chaushev, E. Gillen, A. Smith, L. D. Nielsen, O. Turner, S. Csizmadia, B. Smalley, D. Bayliss, C. Belardi, F. Bouchy, M. R. Burleigh, J. Cabrera, S. L. Casewell, B. Chazelas, B. F. Cooke, A. Erikson, B. T. Gänsicke, M. N. Günther, M. R. Goad, A. Grange, J. A. G. Jackman, J. S. Jenkins, J. McCormac, M. Moyano, D. Pollacco, K. Poppenhaeger, D. Queloz, L. Raynard, H. Rauer, S. Udry, S. R. Walker, C. A. Watson, R. G. West, P. J. Wheatley

    NGTS-5b: a highly inflated planet offering insights into the sub-Jovian desert

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    DOI arXiv
  382. M. Godolt, N. Tosi, B. Stracke, J. Lee Grenfell, T. Ruedas, T. Spohn, H. Rauer

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    DOI arXiv
  383. J. A. G. Jackman, P. J. Wheatley, D. Bayliss, M. R. Burleigh, S. L. Casewell, P. Eigmüller, M. R. Goad, D. Pollacco, L. Raynard, C. A. Watson, R. G. West

    Detection of a giant white-light flare on an L2.5 dwarf with the Next Generation Transit Survey

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    DOI arXiv
  384. M. Keppler, R. Teague, J. Bae, M. Benisty, T. Henning, R. van Boekel, E. Chapillon, P. Pinilla, J. P. Williams, G. H. M. Bertrang, S. Facchini, M. Flock, C. Ginski, A. Juhasz, H. Klahr, Y. Liu, A. Müller, L. M. Pérez, A. Pohl, G. Rosotti, M. Samland, D. Semenov

    Highly structured disk around the planet host PDS 70 revealed by high-angular resolution observations with ALMA

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  385. M. Malik, D. Kitzmann, J. M. Mendonça, S. L. Grimm, G.-D. Marleau, E. F. Linder, S. M. Tsai, K. Heng

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  386. K. Reichert, S. Reffert, S. Stock, T. Trifonov, A. Quirrenbach

    Precise radial velocities of giant stars. XII. Evidence against the proposed planet Aldebaran b

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    DOI arXiv
  387. M. Hjorth, A. B. Justesen, T. Hirano, S. Albrecht, F. Dai, R. Alonso, O. Barragán, M. Esposito, M. Kuzuhara, K. W. F. Lam, J. H. Livingston, P. Montañés-Rodríguez, N. Narita, G. Nowak, J. Prieto-Arranz, S. Redfield, F. Rodler, V. Van Eylen, J. N. Winn, G. Antoniciello, J. Cabrera, W. D. Cochran, S. Csizmadia, J. de Leon, H. Deeg, Eigmüller, M. Endl, A. Erikson, M. Fridlund, S. Grziwa, E. Guenther, A. P. Hatzes, P. Heeren, D. Hidalgo, J. Korth, R. Luque, D. Nespral,, M. Pätzold, C. M. Persson, H. Rauer, A. M. S. Smith, T. Trifonov

    K2-290: a warm Jupiter and a mini-Neptune in a triple-star system

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    primaryclass = {astro-ph.EP},
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    DOI arXiv
  388. G. Cugno, S. P. Quanz, R. Launhardt, A. Musso Barcucci, S. S. Brems, A. Cheetham, T. Henning, A. Müller, J. Olofsson, F. Pepe, A. Quirrenbach, S. Reffert, E. L. Rickman, D. Ségransan

    ISPY – NaCo Imaging Survey for Planets around Young stars. A young companion candidate embedded in the R CrA cloud

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    journal = {\aap},
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    DOI arXiv
  389. F. Wunderlich, M. Godolt, J. Lee Grenfell, S. Städt, A. M. S. Smith, S. Gebauer, F. Schreier, P. Hedelt, H. Rauer

    Detectability of atmospheric features of Earth-like planets in the habitable zone around M dwarfs

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    title = {{Detectability of atmospheric features of Earth-like planets in the habitable zone around M dwarfs}},
    journal = {\aap},
    keywords = {planets and satellites: atmospheres, planets and satellites: detection, planets and satellites: surfaces, planets and satellites: terrestrial planets, techniques: spectroscopic, stars: low-mass, Astrophysics - Earth and Planetary Astrophysics},
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    month = apr,
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    archiveprefix = {arXiv},
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    primaryclass = {astro-ph.EP},
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    DOI arXiv
  390. G.-D. Marleau, G. A. L. Coleman, A. Leleu, C. Mordasini

    Exploring the formation by core accretion and the luminosity evolution of directly imaged planets. The case of HIP 65426 b

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    journal = {\aap},
    keywords = {planets and satellites: formation, planet-disk interactions, planets and satellites: dynamical evolution and stability, planets and satellites: physical evolution, planets and satellites: individual: HIP 65426 b, Astrophysics - Earth and Planetary Astrophysics},
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    DOI arXiv
  391. M. Esposito, D. J. Armstrong, D. Gandolfi, V. Adibekyan, M. Fridlund, N. C. Santos, J. H. Livingston, E. Delgado Mena, L. Fossati, J. Lillo-Box, O. Barragán, D. Barrado, P. E. Cubillos, B. Cooke, A. B. Justesen, F. Meru, R. F. Díaz, F. Dai, L. D. Nielsen, C. M. Persson, P. J. Wheatley, A. P. Hatzes, V. Van Eylen, M. M. Musso, R. Alonso, P. G. Beck, S. C. C. Barros, D. Bayliss, A. S. Bonomo, F. Bouchy, D. J. A. Brown, E. Bryant, J. Cabrera, W. D. Cochran, S. Csizmadia, H. Deeg, O. Demangeon, M. Deleuil, X. Dumusque, P. Eigmüller, M. Endl, A. Erikson, F. Faedi, P. Figueira, A. Fukui, S. Grziwa, E. W. Guenther, D. Hidalgo, M. Hjorth, T. Hirano, S. Hojjatpanah, E. Knudstrup, J. Korth, K. W. F. Lam, J. de Leon, M. N. Lund, R. Luque, S. Mathur, P. Montañés-Rodríguez, N. Narita, D. Nespral,, P. Niraula, G. Nowak, H. P. Osborn, M. Pätzold, D. Pollacco, J. Prieto-Arranz, H. Rauer, S. Redfield, I. Ribas, S. G. Sousa, A. M. S. Smith, M. Tala-Pinto, S. Udry, J. N. Winn

    HD 219666 b: a hot-Neptune from TESS Sector 1

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    title = {{HD 219666 b: a hot-Neptune from TESS Sector 1}},
    journal = {\aap},
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    month = mar,
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    eprint = {1812.05881},
    primaryclass = {astro-ph.EP},
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    DOI arXiv
  392. J. H. Livingston, F. Dai, T. Hirano, D. Gandolfi, A. A. Trani, G. Nowak, W. D. Cochran, M. Endl, S. Albrecht, O. Barragán, J. Cabrera, S. Csizmadia, J. P. de Leon, H. Deeg, P. Eigmüller, A. Erikson, M. Fridlund, A. Fukui, S. Grziwa, E. W. Guenther, A. P. Hatzes, J. Korth, M. Kuzuhara, P. Montañes, N. Narita, D. Nespral,, M. Pätzold, C. M. Persson, J. Prieto-Arranz, H. Rauer, M. Tamura, V. Van Eylen, J. N. Winn

    K2-264: a transiting multiplanet system in the Praesepe open cluster

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    DOI arXiv
  393. K. Monsch, B. Ercolano, G. Picogna, T. Preibisch, M. M. Rau

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    DOI arXiv
  394. T. Trifonov, S. Stock, T. Henning, S. Reffert, M. Kürster, M. H. Lee, B. Bitsch, R. P. Butler, S. S. Vogt

    Two Jovian Planets around the Giant Star HD 202696: A Growing Population of Packed Massive Planetary Pairs around Massive Stars?

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    DOI arXiv
  395. R. Luque, G. Nowak, F. Dai, A. Kaminski, E. Nagel, D. Hidalgo, F. Bauer, M. Lafarga, J. Livingston, O. Barragán, T. Hirano, M. Fridlund, D. Gandolfi, A. B. Justesen, M. Hjorth, V. Van Eylen, J. N. Winn, M. Esposito, J. C. Morales, S. Albrecht, R. Alonso, P. J. Amado, P. Beck, J. A. Caballero, J. Cabrera, W. D. Cochran, S. Csizmadia, H. Deeg, P. Eigmüller, M. Endl, A. Erikson, A. Fukui, S. Grziwa, E. W. Guenther, A. P. Hatzes, E. Knudstrup, J. Korth, K. W. F. Lam, M. N. Lund, S. Mathur, P. Montañés-Rodríguez, N. Narita, D. Nespral,, P. Niraula, M. Pätzold, C. M. Persson, J. Prieto-Arranz, A. Quirrenbach, H. Rauer, S. Redfield, A. Reiners, I. Ribas, A. M. S. Smith

    Detection and characterization of an ultra-dense sub-Neptunian planet orbiting the Sun-like star K2-292

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    DOI arXiv
  396. E. F. Linder, C. Mordasini, P. Mollière, G.-D. Marleau, M. Malik, S. P. Quanz, M. R. Meyer

    Evolutionary models of cold and low-mass planets: cooling curves, magnitudes, and detectability

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    DOI arXiv
  397. D. Ó Fionnagáin, A. A. Vidotto, P. Petit, C. P. Folsom, S. V. Jeffers, S. C. Marsden, J. Morin, J. D. do Nascimento, BCool Collaboration

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    title = {{The solar wind in time - II. 3D stellar wind structure and radio emission}},
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    DOI arXiv
  398. J. Korth, S. Csizmadia, D. Gandolfi, M. Fridlund, M. Pätzold, T. Hirano, J. Livingston, C. M. Persson, H. J. Deeg, A. B. Justesen, O. Barragán, S. Grziwa, M. Endl, R. Tronsgaard, F. Dai, W. D. Cochran, S. Albrecht, R. Alonso, J. Cabrera, P. W. Cauley, F. Cusano, P. Eigmüller, A. Erikson, M. Esposito, E. W. Guenther, A. P. Hatzes, D. Hidalgo, M. Kuzuhara, P. Montañes, N. R. Napolitano, N. Narita, P. Niraula, D. Nespral,, G. Nowak, C. E. Petrillo, S. Redfield, J. Prieto-Arranz, H. Rauer, A. M. S. Smith, C. Tortora, V. Van Eylen, J. N. Winn

    K2-140b and K2-180b – Characterization of a hot Jupiter and a mini-Neptune from the K2 mission

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    DOI arXiv
  399. S. Boro Saikia, T. Lueftinger, S. V. Jeffers, C. P. Folsom, V. See, P. Petit, S. C. Marsden, A. A. Vidotto, J. Morin, A. Reiners, M. Guedel, BCool Collaboration

    Direct evidence of a full dipole flip during the magnetic cycle of a sun-like star

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    DOI arXiv
  400. N. R. Deacon

    Detecting free-floating planets using water-dependent colour terms in the next generation of infrared space-based surveys

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    DOI arXiv
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    DOI arXiv
  402. D. Gandolfi, O. Barragán, J. H. Livingston, M. Fridlund, A. B. Justesen, S. Redfield, L. Fossati, S. Mathur, S. Grziwa, J. Cabrera, R. A. García, C. M. Persson, V. Van Eylen, A. P. Hatzes, D. Hidalgo, S. Albrecht, L. Bugnet, W. D. Cochran, S. Csizmadia, H. Deeg, P. Eigmüller, M. Endl, A. Erikson, M. Esposito, E. Guenther, J. Korth, R. Luque, P. Montañés-Rodríguez, D. Nespral,, G. Nowak, M. Pätzold, J. Prieto-Arranz

    TESS’s first planet. A super-Earth transiting the naked-eye star π Mensae

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    DOI arXiv
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    DOI arXiv
  404. A. Bhandare, R. Kuiper, T. Henning, C. Fendt, G.-D. Marleau, A. Kölligan

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    DOI arXiv
  405. J. Prieto-Arranz, D. Gandolfi, O. Barragán, E. W. Guenther, F. Dai, M. Fridlund, T. Hirano, J. Livingston, R. Luque, P. Niraula, C. M. Persson, S. Redfield, S. Albrecht, R. Alonso, G. Antoniciello, J. Cabrera, W. D. Cochran, S. Csizmadia, H. Deeg, P. Eigmüller, M. Endl, A. Erikson, M. E. Everett, A. Fukui, S. Grziwa, A. P. Hatzes, D. Hidalgo, M. Hjorth, J. Korth, D. Lorenzo-Oliveira, F. Murgas, N. Narita, D. Nespral,, G. Nowak, M. Pätzold, P. Montañés-Rodríguez, H. Rauer, I. Ribas, A. M. S. Smith, T. Trifonov, V. Van Eylen, J. N. Winn

    Mass determination of the 1:3:5 near-resonant planets transiting GJ 9827 (K2-135)

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    primaryclass = {astro-ph.EP},
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    DOI arXiv
  406. J. Prieto-Arranz, D. Gandolfi, O. Barragán, E. W. Guenther, F. Dai, M. Fridlund, T. Hirano, J. Livingston, R. Luque, P. Niraula, C. M. Persson, S. Redfield, S. Albrecht, R. Alonso, G. Antoniciello, J. Cabrera, W. D. Cochran, S. Csizmadia, H. Deeg, P. Eigmüller, M. Endl, A. Erikson, M. E. Everett, A. Fukui, S. Grziwa, A. P. Hatzes, D. Hidalgo, M. Hjorth, J. Korth, D. Lorenzo-Oliveira, F. Murgas, N. Narita, D. Nespral,, G. Nowak, M. Pätzold, P. Montañés-Rodríguez, H. Rauer, I. Ribas, A. M. S. Smith, T. Trifonov, V. Van Eylen, J. N. Winn

    Mass determination of the 1:3:5 near-resonant planets transiting GJ 9827 (K2-135)Prieto-Arranz

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    month = oct,
    volume = {618},
    eid = {A116},
    pages = {A116},
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    archiveprefix = {arXiv},
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    primaryclass = {astro-ph.EP},
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    DOI arXiv
  407. C. M. Persson, M. Fridlund, O. Barragán, F. Dai, D. Gandolfi, A. P. Hatzes, T. Hirano, S. Grziwa, J. Korth, J. Prieto-Arranz, L. Fossati, V. Van Eylen, A. B. Justesen, J. Livingston, D. Kubyshkina, H. J. Deeg, E. W. Guenther, G. Nowak, J. Cabrera, P. Eigmüller, S. Csizmadia, A. M. S. Smith, A. Erikson, S. Albrecht, R. Alonso Sobrino, W. D. Cochran, M. Endl, M. Esposito, A. Fukui, P. Heeren, D. Hidalgo, M. Hjorth, M. Kuzuhara, N. Narita, D. Nespral,, M. Pätzold, H. Rauer, F. Rodler, J. N. Winn

    Super-Earth of 8 M⊕ in a 2.2-day orbit around the K5V star K2-216

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    DOI arXiv
  408. M. Keppler, M. Benisty, A. Müller, T. Henning, R. van Boekel, F. Cantalloube, C. Ginski, R. G. van Holstein, A. L. Maire, A. Pohl, M. Samland, H. Avenhaus, J. L. Baudino, A. Boccaletti, J. de Boer, M. Bonnefoy, G. Chauvin, S. Desidera, M. Langlois, C. Lazzoni, G.-D. Marleau, C. Mordasini, N. Pawellek, T. Stolker, A. Vigan, A. Zurlo, T. Birnstiel, W. Brandner, M. Feldt, M. Flock, J. Girard, R. Gratton, J. Hagelberg, A. Isella, M. Janson, A. Juhasz, J. Kemmer, Q. Kral, A. M. Lagrange, R. Launhardt, A. Matter, F. Menard, J. Milli, P. Mollière, J. Olofsson, L. Pérez, P. Pinilla, C. Pinte, S. P. Quanz, T. Schmidt, Z. Wahhaj, J. P. Williams, E. Buenzli, M. Cudel, C. Dominik, R. Galicher, M. Kasper, J. Lannier, D. Mesa, D. Mouillet, S. Peretti, C. Perrot, G. Salter, E. Sissa, F. Wildi, L. Abe, J. Antichi, J. C. Augereau, A. Baruffolo, P. Baudoz, A. Bazzon, J. L. Beuzit, P. Blanchard, S. S. Brems, T. Buey, V. De Caprio, M. Carbillet, M. Carle, E. Cascone, A. Cheetham, R. Claudi, A. Costille, A. Delboulbé, K. Dohlen, D. Fantinel, P. Feautrier, T. Fusco, E. Giro, L. Gluck, C. Gry, N. Hubin, E. Hugot, M. Jaquet, D. Le Mignant, M. Llored, F. Madec, Y. Magnard, P. Martinez, D. Maurel, M. Meyer, O. Möller-Nilsson, T. Moulin, L. Mugnier, A. Origné, A. Pavlov, D. Perret, C. Petit, J. Pragt, P. Puget, P. Rabou, J. Ramos, F. Rigal, S. Rochat, R. Roelfsema, G. Rousset, A. Roux, B. Salasnich, J. F. Sauvage, A. Sevin, C. Soenke, E. Stadler, M. Suarez, M. Turatto, L. Weber

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    primaryclass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2018Geosc...8..365T},
    adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

    DOI arXiv
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    @article{2018A&A...617L...2M,
    author = {{M{\"u}ller}, A. and {Keppler}, M. and {Henning}, Th. and {Samland}, M. and {Chauvin}, G. and {Beust}, H. and {Maire}, A. -L. and {Molaverdikhani}, K. and {van Boekel}, R. and {Benisty}, M. and {Boccaletti}, A. and {Bonnefoy}, M. and {Cantalloube}, F. and {Charnay}, B. and {Baudino}, J. -L. and {Gennaro}, M. and {Long}, Z.~C. and {Cheetham}, A. and {Desidera}, S. and {Feldt}, M. and {Fusco}, T. and {Girard}, J. and {Gratton}, R. and {Hagelberg}, J. and {Janson}, M. and {Lagrange}, A. -M. and {Langlois}, M. and {Lazzoni}, C. and {Ligi}, R. and {M{\'e}nard}, F. and {Mesa}, D. and {Meyer}, M. and {Molli{\`e}re}, P. and {Mordasini}, C. and {Moulin}, T. and {Pavlov}, A. and {Pawellek}, N. and {Quanz}, S.~P. and {Ramos}, J. and {Rouan}, D. and {Sissa}, E. and {Stadler}, E. and {Vigan}, A. and {Wahhaj}, Z. and {Weber}, L. and {Zurlo}, A.},
    title = {{Orbital and atmospheric characterization of the planet within the gap of the PDS 70 transition disk}},
    journal = {\aap},
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    month = sep,
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    eid = {L2},
    pages = {L2},
    doi = {10.1051/0004-6361/201833584},
    archiveprefix = {arXiv},
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    primaryclass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2018A&A...617L...2M},
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    }

    DOI arXiv
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    title = {{Magellan Adaptive Optics Imaging of PDS 70: Measuring the Mass Accretion Rate of a Young Giant Planet within a Gapped Disk}},
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    archiveprefix = {arXiv},
    eprint = {1807.10766},
    primaryclass = {astro-ph.EP},
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    }

    DOI arXiv
  412. A. C. Cheetham, M. Samland, S. S. Brems, R. Launhardt, G. Chauvin, D. Ségransan, T. Henning, A. Quirrenbach, H. Avenhaus, G. Cugno, J. Girard, N. Godoy, G. M. Kennedy, A. L. Maire, S. Metchev, A. Müller, A. Musso Barcucci, J. Olofsson, F. Pepe, S. P. Quanz, D. Queloz, S. Reffert, E. Rickman, R. van Boekel, A. Boccaletti, M. Bonnefoy, F. Cantalloube, B. Charnay, P. Delorme, M. Janson, M. Keppler, A. M. Lagrange, M. Langlois, C. Lazzoni, F. Menard, D. Mesa, M. Meyer, T. Schmidt, E. Sissa, S. Udry, A. Zurlo

    Spectral and orbital characterisation of the directly imaged giant planet HIP 65426 b

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    title = {{Spectral and orbital characterisation of the directly imaged giant planet HIP 65426 b}},
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    DOI arXiv
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