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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: 424

Year
  • 2018
  • 2019
  • 2020
  • 2021
  • 2022
  • 2023
  • 2024
  1. J. Müller, B. Bitsch, A. D. Schneider

    A formation pathway for terrestrial planets with moderate water content involving atmospheric-volatile recycling

    bib

    @misc{müller2024formationpathwayterrestrialplanets,
    title={A formation pathway for terrestrial planets with moderate water content involving atmospheric-volatile recycling},
    author={Jonas Müller and Bertram Bitsch and Aaron David Schneider},
    year={2024},
    eprint={2406.09186},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP},
    url={https://arxiv.org/abs/2406.09186},
    }

    arXiv
  2. J. A. Egger, H. P. Osborn, D. Kubyshkina, C. Mordasini, Y. Alibert, M. N. Günther, M. Lendl, A. Brandeker, A. Heitzmann, A. Leleu, M. Damasso, A. Bonfanti, T. G. Wilson, S. G. Sousa, J. Haldemann, L. Delrez, M. J. Hooton, T. Zingales, R. Luque, R. Alonso, J. Asquier,, T. Bárczy, D. Barrado Navascues, S. C. C. Barros, W. Baumjohann, W. Benz, N. Billot, L. Borsato, C. Broeg, M. Buder, A. Castro-Gonzáles, A. Collier Cameron, A. C. M. Correia, D. Cortes, Sz. Csizmadia, P. E. Cubillos, M. B. Davies, M. Deleuil, A. Deline, O. D. S. Demangeon, B. O. Demory, A. Derekas, B. Edwards, D. Ehrenreich, A. Erikson, A. Fortier, L. Fossati, M. C. V. Fridlund, D. Gandolfi, K. Gazeas, M. Gillon, M. Guedel, Ch. Helling, K. G. Isaak, L. Kiss, J. Korth, K. W. F. Lam, J. Laskar, B. Lavie, A. Lecavelier des Etangs, C. Lovis, A. Luntzer, D. Magrin, P. F. L. Maxted, B. Merin, M. Munari, 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, J. Rodrigues, N. C. Santos, G. Scandariato, D. Ségransan, A. E. Simon, A. M. S. Smith, M. Stalport, S. Sulis, G. M. Szabó, S. Udry, V. Van Grootel, J. Venturini, E. Villaver, N. A. Walton

    Unveiling the internal structure and formation history of the three planets transiting HIP 29442 (TOI-469) with CHEOPS

    bib

    @misc{egger2024unveilinginternalstructureformation,
    title={Unveiling the internal structure and formation history of the three planets transiting HIP 29442 (TOI-469) with CHEOPS},
    author={J. A. Egger and H. P. Osborn and D. Kubyshkina and C. Mordasini and Y. Alibert and M. N. Günther and M. Lendl and A. Brandeker and A. Heitzmann and A. Leleu and M. Damasso and A. Bonfanti and T. G. Wilson and S. G. Sousa and J. Haldemann and L. Delrez and M. J. Hooton and T. Zingales and R. Luque and R. Alonso and J. Asquier and T. Bárczy and D. Barrado Navascues and S. C. C. Barros and W. Baumjohann and W. Benz and N. Billot and L. Borsato and C. Broeg and M. Buder and A. Castro-González and A. Collier Cameron and A. C. M. Correia and D. Cortes and Sz. Csizmadia and P. E. Cubillos and M. B. Davies and M. Deleuil and A. Deline and O. D. S. Demangeon and B. -O. Demory and A. Derekas and B. Edwards and D. Ehrenreich and A. Erikson and A. Fortier and L. Fossati and M. Fridlund and D. Gandolfi and K. Gazeas and M. Gillon and M. Güdel and Ch. Helling and K. G. Isaak and L. L. Kiss and J. Korth and K. W. F. Lam and J. Laskar and B. Lavie and A. Lecavelier des Etangs and C. Lovis and A. Luntzer and D. Magrin and P. F. L. Maxted and B. Merín and M. Munari 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 J. Rodrigues and N. C. Santos and G. Scandariato and D. Ségransan and A. E. Simon and A. M. S. Smith and M. Stalport and S. Sulis and Gy. M. Szabó and S. Udry and V. Van Grootel and J. Venturini and E. Villaver and N. A. Walton},
    year={2024},
    eprint={2406.18653},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP},
    url={https://arxiv.org/abs/2406.18653},
    }

    arXiv
  3. J. Mah, S. Savvidou, B. Bitsch

    Mind the gap: Distinguishing disc substructures and their impact on the inner disc composition

    bib

    @article{Mah_2024,
    title={Mind the gap: Distinguishing disc substructures and their impact on the inner disc composition},
    volume={686},
    ISSN={1432-0746},
    url={http://dx.doi.org/10.1051/0004-6361/202450322},
    DOI={10.1051/0004-6361/202450322},
    journal={Astronomy & Astrophysics},
    publisher={EDP Sciences},
    author={Mah, Jingyi and Savvidou, Sofia and Bitsch, Bertram},
    year={2024},
    month=jun, pages={L17} }

    DOI arXiv
  4. T. Pfeil, T. Birnstiel, H. Klahr

    Vertical shear instability with dust evolution and consistent cooling times. On the importance of the initial dust distribution

    bib

    @article{Pfeil_2024,
    title={Vertical shear instability with dust evolution and consistent cooling times: On the importance of the initial dust distribution},
    volume={687},
    ISSN={1432-0746},
    url={http://dx.doi.org/10.1051/0004-6361/202449323},
    DOI={10.1051/0004-6361/202449323},
    journal={Astronomy & Astrophysics},
    publisher={EDP Sciences},
    author={Pfeil, Thomas and Birnstiel, Til and Klahr, Hubert},
    year={2024},
    month=jun, pages={L5} }

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

    Exploring the ultra-hot Jupiter WASP-178b. Constraints on atmospheric chemistry and dynamics from a joint retrieval of VLT/CRIRES+ and space photometric data

    bib

    @misc{cont2024exploringultrahotjupiterwasp178b,
    title={Exploring the ultra-hot Jupiter WASP-178b. Constraints on atmospheric chemistry and dynamics from a joint retrieval of VLT/CRIRES$^+$ and space photometric data},
    author={D. Cont and L. Nortmann and F. Yan and F. Lesjak and S. Czesla and A. Lavail and A. Reiners and N. Piskunov and A. Hatzes and L. Boldt-Christmas and O. Kochukhov and T. Marquart and E. Nagel and A. D. Rains and M. Rengel and U. Seemann and D. Shulyak},
    year={2024},
    eprint={2406.08166},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP},
    url={https://arxiv.org/abs/2406.08166},
    }

    arXiv
  6. J. Mah, S. Savvidou, B. Bitsch

    Mind the gap: Distinguishing disc substructures and their impact on the composition of the inner disc

    bib

    @misc{mah2024mind,
    title={Mind the gap: Distinguishing disc substructures and their impact on the composition of the inner disc},
    author={Jingyi Mah and Sofia Savvidou and Bertram Bitsch},
    year={2024},
    eprint={2406.06219},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP}
    }

    arXiv
  7. C. Gapp, M. Rengel, P. Hartogh, H. Sagawa, H. Feuchtgruber, E. Lellouch, G. L. Villanueva

    Abundances of trace constituents in Jupiter’s atmosphere inferred from Herschel/PACS observations

    bib

    @article{Gapp_2024,
    title={Abundances of trace constituents in Jupiter’s atmosphere inferred from Herschel/PACS observations},
    ISSN={1432-0746},
    url={http://dx.doi.org/10.1051/0004-6361/202347345},
    DOI={10.1051/0004-6361/202347345},
    journal={Astronomy & Astrophysics},
    publisher={EDP Sciences},
    author={Gapp, C. and Rengel, M. and Hartogh, P. and Sagawa, H. and Feuchtgruber, H. and Lellouch, E. and Villanueva, G.L.},
    year={2024},
    month=jun }

    arXiv
  8. A. Fortier, A. E. Simon, C. Broeg, G. Olofsson, A. Deline, T. G. Wilson, P. F. L. Maxted, A. Brandeker, A. Collier Cameron, M. Beck, A. Bekkelien, N. Billot, A. Bonfanti, G. Bruno, J. Cabrera, L. Delrez, B. O. Demory, D. Futyan, H. -G. Florén, M. N. Günther, A. Heitzmann, S. Hoyer, K. G. Isaak, S. G. Sousa, M. Stalport, A. Turin, P. Verhoeve, B. Akinsanmi, Y. Alibert, R. Alonso, D. Banhidi, T. Bárczy, D. Barrado, S. C. C. Barros, W. Baumjohann, T. A. Baycroft, T. Beck, W. Benz, B. I. Biro, A. Bódi, X. Bonfils, L. Borsato, S. Charnoz, B. Cseh, Sz. Csizmadia, I. Csanyi, P. E. Cubillos, M. B. Davies, Y. T. Davis, M. Deleuil, O. D. S. Demangeon, A. Derekas, G. Dransfield, E. Ducrot, D. Ehrenreich, A. Erikson, C. Farina, L. Fossati, M. C. V. Fridlund, D. Gandolfi, Z. Garai, L. Garcia, M. Gillon, Y. Gómez Maqueo Chew, M. A. Gómez-Muñoz, V. Granata, M. Guedel, P. Guterman, T. Hegedüs, Ch. Helling, E. Jehin, C. Kalup, D. Kilkenny, L. Kiss, L. Kriskovics, K. W. F. Lam, J. Laskar, A. Lecavelier des Etangs, M. Lendl, A. Lopez Pina, A. Luntzer, D. Magrin, N. J. Miller, D. Modrego Contreras, C. Mordasini, M. Munari, C. Murray, V. Nascimbeni, H. Ottacher, R. Ottensamer, I. Pagano, A. Pál, E. Pallé, A. Pasetti, P. Pihlmann Pedersen, G. Peter, R. Petrucci, G. Piotto, A. Pizarro-Rubio, D. Pollacco, T. Pribulla, D. Queloz, R. Ragazzoni, N. Rando, H. Rauer, I. Ribas, L. Sabin, N. C. Santos, G. Scandariato, N. Schanche, U. Schroffenegger, O. J. Scutt, D. Sebastian, D. Ségransan, B. Seli, A. M. S. Smith, J. Southworth, M. R. Standing, G. M. Szabó, R. Szakáts, N. Thomas, M. Timmermans, A. Triaud, S. Udry, V. Van Grootel, J. Venturini, E. Villaver, J. Vinko, N. A. Walton, R. Wells, D. Wolter

    CHEOPS in-flight performance: A comprehensive look at the first 3.5 years of operations

    bib

    @misc{fortier2024cheopsinflightperformancecomprehensive,
    title={CHEOPS in-flight performance: A comprehensive look at the first 3.5 years of operations},
    author={A. Fortier and A. E. Simon and C. Broeg and G. Olofsson and A. Deline and T. G. Wilson and P. F. L. Maxted and A. Brandeker and A. Collier Cameron and M. Beck and A. Bekkelien and N. Billot and A. Bonfanti and G. Bruno and J. Cabrera and L. Delrez and B. -O. Demory and D. Futyan and H. -G. Florén and M. N. Günther and A. Heitzmann and S. Hoyer and K. G. Isaak and S. G. Sousa and M. Stalport and A. Turin and P. Verhoeve and B. Akinsanmi and Y. Alibert and R. Alonso and D. Bánhidi and T. Bárczy and D. Barrado and S. C. Barros and W. Baumjohann and T. Baycroft and T. Beck and W. Benz and B. I. Bíró and A. Bódi and X. Bonfils and L. Borsato and S. Charnoz and B. Cseh and Sz. Csizmadia and I. Csányi and P. E. Cubillos and M. B. Davies and Y. T. Davis and M. Deleuil and O. D. S. Demangeon and A. Derekas and G. Dransfield and E. Ducrot and D. Ehrenreich and A. Erikson and C. Fariña and L. Fossati and M. Fridlund and D. Gandolfi and Z. Garai and L. Garcia and M. Gillon and Y. Gómez Maqueo Chew and M. A. Gómez-Muñoz and V. Granata and M. Güdel and P. Guterman and T. Hegedüs and Ch. Helling and E. Jehin and Cs. Kalup and D. Kilkenny and L. Kiss and L. Kriskovics and K. W. F. Lam and J. Laskar and A. Lecavelier des Etangs and M. Lendl and A. Lopez Pina and A. Luntzer and D. Magrin and N. J. Miller and D. Modrego Contreras and C. Mordasini and M. Munari and C. A. Murray and V. Nascimbeni and H. Ottacher and R. Ottensamer and I. Pagano and A. Pál and E. Pallé and A. Pasetti and P. Pedersen and G. Peter and R. Petrucci and G. Piotto and A. Pizarro-Rubio and D. Pollacco and T. Pribulla and D. Queloz and R. Ragazzoni and N. Rando and H. Rauer and I. Ribas and L. Sabin and N. C. Santos and G. Scandariato and N. Schanche and U. Schroffenegger and O. J. Scutt and D. Sebastian and D. Ségransan and B. Seli and A. M. S. Smith and R. Southworth and M. R. Standing and M. Gy. Szabó and R. Szakáts and N. Thomas and M. Timmermans and A. H. M. J. Triaud and S. Udry and V. Van Grootel and J. Venturini and E. Villaver and J. Vinkó and N. A. Walton and R. Wells and D. Wolter},
    year={2024},
    eprint={2406.01716},
    archivePrefix={arXiv},
    primaryClass={astro-ph.IM},
    url={https://arxiv.org/abs/2406.01716},
    }

    arXiv
  9. S. Sulis, L. Borsato, S. Grouffal, H. P. Osborn, A. Santerne, A. Brandeker, M. N. Günther, A. Heitzmann, M. Lendl, M. Fridlund, D. Gandolfi, Y. Alibert, R. Alonso, T. Bárczy, D. Barrado Navascues, S. C. C. Barros, W. Baumjohann, T. Beck, W. Benz, M. Bergomi, N. Billot, A. Bonfanti, C. Broeg, A. Collier Cameron, C. Corral Van Damme, A. C. M. Correia, Sz. Csizmadia, P. E. Cubillos, M. B. Davies, M. Deleuil, A. Deline, L. Delrez, O. D. S. Demangeon, B. O. Demory, A. Derekas, B. Edwards, D. Ehrenreich, A. Erikson, A. Fortier, L. Fossati, K. Gazeas, M. Gillon, M. Guedel, Ch. Helling, S. Hoyer, K. G. Isaak, L. Kiss, J. Korth, K. W. F. Lam, J. Laskar, A. Lecavelier des Etangs, D. Magrin, P. F. L. Maxted, 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, G. Scandariato, D. Ségransan, A. E. Simon, A. M. S. Smith, S. G. Sousa, M. Stalport, M. Steinberger, G. M. Szabó, A. Tuson, S. Udry, S. Ulmer-Moll, V. Van Grootel, J. Venturini, E. Villaver, N. A. Walton, T. G. Wilson, D. Wolter, T. Zingales

    HIP 41378 observed by CHEOPS: Where is planet d?

    bib

    @article{Sulis_2024,
    title={HIP 41378 observed by CHEOPS: Where is planet d?},
    volume={686},
    ISSN={1432-0746},
    url={http://dx.doi.org/10.1051/0004-6361/202449689},
    DOI={10.1051/0004-6361/202449689},
    journal={Astronomy & Astrophysics},
    publisher={EDP Sciences},
    author={Sulis, S. and Borsato, L. and Grouffal, S. and Osborn, H. P. and Santerne, A. and Brandeker, A. and Günther, M. N. and Heitzmann, A. and Lendl, M. and Fridlund, M. and Gandolfi, D. and Alibert, Y. and Alonso, R. and Bárczy, T. and Barrado Navascues, D. and Barros, S. C. C. and Baumjohann, W. and Beck, T. and Benz, W. and Bergomi, M. and Billot, N. and Bonfanti, A. and Broeg, C. and Collier Cameron, A. and Corral van Damme, C. and Correia, A. C. M. and Csizmadia, Sz. and Cubillos, P. E. and Davies, M. B. and Deleuil, M. and Deline, A. and Delrez, L. and Demangeon, O. D. S. and Demory, B.-O. and Derekas, A. and Edwards, B. and Ehrenreich, D. and Erikson, A. and Fortier, A. and Fossati, L. and Gazeas, K. and Gillon, M. and Güdel, M. and Helling, Ch. and Hoyer, S. and Isaak, K. G. and Kiss, L. L. and Korth, J. and Lam, K. W. F. and Laskar, J. and Lecavelier des Etangs, A. and Magrin, D. and Maxted, P. F. L. and Mordasini, C. and Nascimbeni, V. and Olofsson, G. and Ottensamer, R. and Pagano, I. and Pallé, E. and Peter, G. and Piazza, D. and Piotto, G. and Pollacco, D. and Queloz, D. and Ragazzoni, R. and Rando, N. 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 Sousa, S. G. and Stalport, M. and Steinberger, M. and Szabó, Gy. M. and Tuson, A. and Udry, S. and Ulmer-Moll, S. and Van Grootel, V. and Venturini, J. and Villaver, E. and Walton, N. A. and Wilson, T. G. and Wolter, D. and Zingales, T.},
    year={2024},
    month=jun, pages={L18} }

    DOI arXiv
  10. O. Kochukhov, A. M. Amarsi, A. Lavail, H. L. Ruh, A. Hahlin, A. P. Hatzes, E. Nagel, N. Piskunov, K. Pouilly, A. Reiners, M. Rengel, U. Seemann, D. Shulyak

    A conclusive non-detection of magnetic field in the Am star o Peg with high-precision near-infrared spectroscopy

    bib

    @misc{kochukhov2024conclusive,
    title={A conclusive non-detection of magnetic field in the Am star o Peg with high-precision near-infrared spectroscopy},
    author={O. Kochukhov and A. M. Amarsi and A. Lavail and H. L. Ruh and A. Hahlin and A. Hatzes and E. Nagel and N. Piskunov and K. Pouilly and A. Reiners and M. Rengel and U. Seemann and D. Shulyak},
    year={2024},
    eprint={2405.12778},
    archivePrefix={arXiv},
    primaryClass={astro-ph.SR}
    }

    arXiv
  11. A. Krieger, M. Küffmeier, S. Reissl, C. P. Dullemond, C. Ginski, S. Wolf

    Feasibility of detecting shadows in disks induced by infall

    bib

    @article{Krieger_2024,
    title={Feasibility of detecting shadows in disks induced by infall},
    volume={686},
    ISSN={1432-0746},
    url={http://dx.doi.org/10.1051/0004-6361/202348354},
    DOI={10.1051/0004-6361/202348354},
    journal={Astronomy & Astrophysics},
    publisher={EDP Sciences},
    author={Krieger, A. and Kuffmeier, M. and Reissl, S. and Dullemond, C. P. and Ginski, C. and Wolf, S.},
    year={2024},
    month=jun, pages={A111} }

    DOI arXiv
  12. A. Bhandare, B. Commerçon, G. Laibe, M. Flock, R. Kuiper, Th. Henning, A. Mignone, G.-D. Marleau

    Mixing is easy: New insights for cosmochemical evolution from pre-stellar core collapse

    bib

    @misc{bhandare2024mixing,
    title={Mixing is easy: New insights for cosmochemical evolution from pre-stellar core collapse},
    author={Asmita Bhandare and Benoît Commerçon and Guillaume Laibe and Mario Flock and Rolf Kuiper and Thomas Henning and Andrea Mignone and Gabriel-Dominique Marleau},
    year={2024},
    eprint={2404.09257},
    archivePrefix={arXiv},
    primaryClass={astro-ph.SR}
    }

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

    Three-temperature radiation hydrodynamics with PLUTO: Thermal and kinematic signatures of accreting protoplanets

    bib

    @misc{muley2024threetemperature,
    title={Three-temperature radiation hydrodynamics with PLUTO: Thermal and kinematic signatures of accreting protoplanets},
    author={Dhruv Muley and Julio David Melon Fuksman and Hubert Klahr},
    year={2024},
    eprint={2405.03375},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP}
    }

    arXiv
  14. L. Thomas, R. Saglia, L. Pasquini, A. Brucalassi, P. Bonifacio, J. De Medeiros, I. de Castro Leão, B. L. Canto Martins, H. Lukas Ruh, L. R. Bedin, M. Libralato, K. Biazzo

    Search for giant planets in M 67 V: A warm Jupiter orbiting the turn-off star S1429

    bib

    @article{Thomas_2024,
    title={Search for giant planets in M 67 V: A warm Jupiter orbiting the turn-off star S1429},
    volume={686},
    ISSN={1432-0746},
    url={http://dx.doi.org/10.1051/0004-6361/202449233},
    DOI={10.1051/0004-6361/202449233},
    journal={Astronomy & Astrophysics},
    publisher={EDP Sciences},
    author={Thomas, Luis and Saglia, Roberto and Pasquini, Luca and Brucalassi, Anna and Bonifacio, Piercarlo and de Medeiros, José Renan and de Castro Leão, Izan and Canto Martins, Bruno Leonardo and Lukas Ruh, Henrik and Bedin, Luigi Rolly and Libralato, Mattia and Biazzo, Katia},
    year={2024},
    month=may, pages={A19} }

    DOI arXiv
  15. E. Bachelet, P. Rota, V. Bozza, P. Zieliński, Y. Tsapras, M. P. G. Hundertmark, J. Wambsganss, L. Wyrzykowski, P. Mikolajczyk, R. A. Street, R. Figuera Jaimes, A. Cassan, M. Dominik, D. A. H. Buckley, S. Awiphan, N. Nakharutai, S. Zola, K. A. Rybicki, M. Gromadzki, K. Howil, N. Ihanec, M. Jabłońska, K. Kruszyńska, U. Pylypenko, M. Ratajczak, M. Sitek, M. Rabus

    A Close Binary Lens Revealed by the Microlensing Event Gaia20bof

    bib

    @misc{bachelet2024closebinarylensrevealed,
    title={A close binary lens revealed by the microlensing event Gaia20bof},
    author={E. Bachelet and P. Rota and V. Bozza and P. Zielinski and Y. Tsapras and M. Hundertmark and J. Wambsganss and L. Wyrzykowski and P. J. Mikolajczyk and R. A. Street and R. Figuera Jaimes and A. Cassan and M. Dominik and D. A. H. Buckley and S. Awiphan and N. Nakhaharutai and S. Zola and K. A. Rybicki and M. Gromadzki and K. Howil and N. Ihanec and M. Jablonska and K. Kruszynska and U. Pylypenko and M. Ratajczak and M. Sitek and M. Rabus},
    year={2024},
    eprint={2405.02223},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP},
    url={https://arxiv.org/abs/2405.02223},
    }

    DOI arXiv
  16. H. Klahr

    Thermal baroclinic instabilities in accretion disks I: Combined dispersion relation for Goldreich-Schubert-Fricke Instability and Convective Overstability in disks around young stars

    bib

    @misc{klahr2024thermal,
    title={Thermal baroclinic instabilities in accretion disks I: Combined dispersion relation for Goldreich-Schubert-Fricke Instability and Convective Overstability in disks around young stars},
    author={Hubert Klahr},
    year={2024},
    eprint={2404.15933},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP}
    }

    arXiv
  17. E. Keles, S. Czesla, K. Poppenhaeger, P. H. Hauschildt, T. A. Carroll, I. V. Ilyin, M. Baratella, M. Steffen, K. G. Strassmeier, A. S. Bonomo, B. S. Gaudi, T. Henning, M. C. Johnson, K. Molaverdikhani, V. Nascimbeni, J. Patience, A. Reiners, G. Scandariato, E. Schlawin, E. Shkolnik, D. Sicilia, A. Sozzetti, M. Mallonn, C. Veillet, J. Wang, F. Yan

    The PEPSI Exoplanet Transit Survey (PETS) – V. New Na D transmission spectra indicate a quieter atmosphere on HD 189733b

    bib

    @misc{keles2024pepsi,
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  18. D. Yan, J. Guo, K.-i. Seon, M. López-Puertas, S. Czesla, M. Lampón

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    arXiv
  19. N. Engelbrecht, K. Herbst, R. Du Toit Strauss, K. Scherer, J. Light, K. Moloto

    On the Comprehensive 3D Modeling of the Radiation Environment of Proxima Centauri b: A New Constraint on Habitability?

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    arXiv
  21. 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

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    arXiv
  22. 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

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    arXiv
  24. 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

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    DOI arXiv
  25. 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

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

    Which stars can form planets: Planetesimal formation at low metallicities

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    arXiv
  27. 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

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

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    arXiv
  29. 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

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

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

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

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

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    arXiv
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    arXiv
  35. 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

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    arXiv
  36. 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

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

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

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    DOI arXiv
  39. 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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    arXiv
  40. C. Dominik, C. P. Dullemond

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

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    arXiv
  41. 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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  42. 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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    arXiv
  43. A. Krieger, S. Wolf

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

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    arXiv
  44. 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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    arXiv
  45. 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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    arXiv
  46. 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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    DOI arXiv
  47. 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
  48. 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
  49. A. Krieger, S. Wolf

    Improving Monte Carlo radiative transfer simulations: A shift of framework

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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
  55. C. Danti, B. Bitsch, J. Mah

    Composition of giant planets: the roles of pebbles and planetesimals

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    arXiv
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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
  58. 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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    arXiv
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    arXiv
  65. 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
  66. F. Wunderlich, J. L. Grenfell, H. Rauer

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    Synergies between interstellar dust and heliospheric science with an Interstellar Probe

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    author = {Veerle J Sterken and S Hunziker and K Dialynas and J Leitner and M Sommer and R Srama and L R Baalmann and A Li and K Herbst and A Galli and P Brandt and M Riebe and W J Baggaley and M Blanc and A Czechowski and F Effenberger and B Fields and P Frisch and M Horanyi and H-W Hsu and N Khawaja and H Krüger and W S Kurth and N F W Ligterink and J L Linsky and C Lisse and D Malaspina and J A Miller and M Opher and A R Poppe and F Postberg and E Provornikova and S Redfield and J Richardson and M Rowan-Robinson and K Scherer and M M Shen and J D Slavin and Z Sternovsky and G Stober and P Strub and J Szalay and M Trieloff},

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    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},
    }

    DOI
  88. F. Schreier, J. L. Grenfell, F. Wunderlich, T. Trautmann

    Assessment of a physics-based retrieval of exoplanet atmospheric temperatures from infrared emission spectra

    bib

    @article{Schreier_2023,
    doi = {10.1093/mnras/stad1526},

    url = {https://doi.org/10.1093%2Fmnras%2Fstad1526},

    year = 2023,
    month = {may},

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

    author = {Franz Schreier and J Lee Grenfell and Fabian Wunderlich and Thomas Trautmann},

    title = {Assessment of a physics-based retrieval of exoplanet atmospheric temperatures from infrared emission spectra},

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

    DOI arXiv
  89. H. J. Deeg, I. Georgieva, G. Nowak, C. M. Persson, B. Cale, F. Murgas, E. Pallé, D. Godoy Rivera, F. Dai, D. R. Ciardi, J. M. Akana Murphy, P. G. Beck, C. J. Burke, J. Cabrera, I. Carleo, W. D. Cochran, K. A. Collins, Sz. Csizmadia, M. El Mufti, M. Fridlund, A. Fukui, D. Gandolfi, R. A. García, E. W. Guenther, P. Guerra, S. Grziwa, H. Isaacson, K. Isogai, J. M. Jenkins, P. Kabáth, J. Korth, K. W. F. Lam, D. W. Latham, R. Luque, M. B. Lund, J. H. Livingston, S. Mathis, S. Mathur, N. Narita, J. Orell-Miquel, H. L. M. Osborne, H. Parviainen, P. Plavchan, S. Redfield, D. Rodriguez, R. P. Schwarz, S. Seager, A. M. S. Smith, V. Van Eylen, J. Van Zandt, J. N. Winn, C. Ziegler

    TOI-1416: A system with a super-Earth planet with a 1.07d period

    bib

    @misc{deeg2023toi1416,
    title={TOI-1416: A system with a super-Earth planet with a 1.07d period},
    author={H. J. Deeg and I. Y. Georgieva and G. Nowak and C. M. Persson and B. L. Cale and F. Murgas and E. Pallé and D. Godoy Rivera and F. Dai and D. R. Ciardi and J. M. Akana Murphy and P. G. Beck and C. J. Burke and J. Cabrera and I. Carleo and W. D. Cochran and K. A. Collins and Sz. Csizmadia and M. El Mufti and M. Fridlund and A. Fukui and D. Gandolfi and R. A. García and E. W. Guenther and P. Guerra and S. Grziwa and H. Isaacson and K. Isogai and J. M. Jenkins and P. Kábath and J. Korth and K. W. F. Lam and D. W. Latham and R. Luque and M. B. Lund and J. H. Livingston and S. Mathis and S. Mathur and N. Narita and J. Orell-Miquel and H. L. M. Osborne and H. Parviainen and P. P. Plavchan and S. Redfield and D. R. Rodriguez and R. P. Schwarz and S. Seager and A. M. S. Smith and V. Van Eylen and J. Van Zandt and J. N Winn and C. Ziegler},
    year={2023},
    eprint={2305.18542},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP}
    }

    arXiv
  90. J. Korth, D. Gandolfi, J. Subjak, S. Howard, S. Ataiee, K. A. Collins, S. N. Quinn, A. J. Mustill, T. Guillot, N. Lodieu, A. M. S. Smith, M. Esposito, F. Rodler, A. Muresan, L. Abe, S. H. Albrecht, A. Alqasim, K. Barkaoui, P. G. Beck, C. J. Burke, R. P. Butler, D. M. Conti, K. I. Collins, J. D. Crane, F. Dai, H. J. Deeg, P. Evans, S. Grziwa, A. P. Hatzes, T. Hirano, K. Horne, C. Huang, J. M. Jenkins, P. Kabáth, J. Kielkopf, E. Knudstrup, D. W. Latham, J. Livingston, R. Luque, S. Mathur, F. Murgas, H. L. M. Osborne, E. Pallé, C. M. Persson, J. E. Rodriguez, M. Rose, P. Rowden, R. P. Schwarz, S. Seager, L. M. Serrano, L. Sha, S. A. Shectman, A. Shporer, G. Srdoc, C. Stockdale, T. G. Tan, J. Teske, V. Van Eylen, A. Vanderburg, R. Vanderspek, S. Wang, J. N. Winn

    TOI-1130: A photodynamical analysis of a hot Jupiter in resonance with an inner low-mass planet

    bib

    @misc{korth2023toi1130,
    title={TOI-1130: A photodynamical analysis of a hot Jupiter in resonance with an inner low-mass planet},
    author={J. Korth and D. Gandolfi and J. Šubjak and S. Howard and S. Ataiee and K. A. Collins and S. N. Quinn and A. J. Mustill and T. Guillot and N. Lodieu and A. M. S. Smith and M. Esposito and F. Rodler and A. Muresan and L. Abe and S. H. Albrecht and A. Alqasim and K. Barkaoui and P. G. Beck and C. J. Burke and R. P. Butler and D. M. Conti and K. I. Collins and J. D. Crane and F. Dai and H. J. Deeg and P. Evans and S. Grziwa and A. P. Hatzes and T. Hirano and K. Horne and C. X. Huang and J. M. Jenkins and P. Kabáth and J. F. Kielkopf and E. Knudstrup and D. W. Latham and J. Livingston and R. Luque and S. Mathur and F. Murgas and H. L. M. Osborne and E. Pallé and C. M. Persson and J. E. Rodriguez and M. Rose and P. Rowden and R. P. Schwarz and S. Seager and L. M. Serrano and L. Sha and S. A. Shectman and A. Shporer and G. Srdoc and C. Stockdale and T. G. Tan and J. K. Teske and V. Van Eylen and A. Vanderburg and R. Vanderspek and S. X. Wang and J. N. Winn},
    year={2023},
    eprint={2305.15565},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP}
    }

    arXiv
  91. R. A. Street, X. Li, S. Khakpash, E. Bellm, L. Girardi, L. Jones, N. S. Abrams, Y. Tsapras, M. P. G. Hundertmark, E. Bachelet, P. Gandhi, P. Szkody, W. I. Clarkson, R. Szabo, L. Prisinzano, R. Bonito, D. A. H. Buckley, J. P. Marais, R. Di Stefano

    LSST Survey Strategy in the Galactic Plane and Magellanic Clouds

    bib

    @misc{street2023lsst,
    title={LSST Survey Strategy in the Galactic Plane and Magellanic Clouds},
    author={R. A. Street and X. Li and S. Khakpash and E. Bellm and L. Girardi and L. Jones and N. S. Abrams and Y. Tsapras and M. P. G. Hundertmark and E. Bachelet and P. Gandhi and P. Szkody and W. I. Clarkson and R. Szabo and L. Prisinzano and R. Bonito and D. A. H. Buckley and J. P. Marais and R. Di Stefano},
    year={2023},
    eprint={2305.11988},
    archivePrefix={arXiv},
    primaryClass={astro-ph.GA}
    }

    DOI arXiv
  92. D. Demars, M. Bonnefoy, C. Dougados, Y. Aoyama, T. Thanathibodee, G.-D. Marleau, P. Tremblin, P. Delorme, P. Palma-Bifani, S. Petrus, P. B. Bowler, G. Chauvin, A. M. Lagrange

    Emission line variability of young 10-30 Mjup companions : I. The case of GQ Lup b and GSC 06214-00210 b

    bib

    @misc{demars2023emission,
    title={Emission line variability of young 10-30 Mjup companions : I. The case of GQ Lup b and GSC 06214-00210 b},
    author={Dorian Demars and Mickael Bonnefoy and Catherine Dougados and Yuhiko Aoyama and Thanawuth Thanathibodee and Gabriel-Dominique Marleau and Pascal Tremblin and Philippe Delorme and Paulina Palma-Bifani and Simon Petrus and Brendan P. Bowler and Gael Chauvin and Anne-Marie Lagrange},
    year={2023},
    eprint={2305.09460},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP}
    }

    arXiv
  93. H. Klahr, H. Baehr, J. D. Melon Fuksman

    Thermal instabilities in accretion disks II: Numerical Experiments for the Goldreich-Schubert-Fricke Instability and the Convective Overstability in disks around young stars

    bib

    @misc{klahr2023thermal,
    title={Thermal instabilities in accretion disks II: Numerical Experiments for the Goldreich-Schubert-Fricke Instability and the Convective Overstability in disks around young stars},
    author={Hubert Klahr and Hans Baehr and Julio David Melon Fuksman},
    year={2023},
    eprint={2305.08165},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP}
    }

    arXiv
  94. G.-D. Marleau, R. Kuiper, W. Béthune, C. Mordasini

    The Planetary Accretion Shock. III. Smoothing-free 2.5D simulations and calculation of H alpha emission

    bib

    @misc{marleau2023planetary,
    title={The Planetary Accretion Shock. III. Smoothing-free 2.5D simulations and calculation of H alpha emission},
    author={Gabriel-Dominique Marleau and Rolf Kuiper and William Béthune and Christoph Mordasini},
    year={2023},
    eprint={2305.01679},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP}
    }

    arXiv
  95. S. Müller, R. Helled

    Warm giant exoplanet characterisation: current state, challenges and outlook

    bib

    @misc{müller2023warm,
    title={Warm giant exoplanet characterisation: current state, challenges and outlook},
    author={Simon Müller and Ravit Helled},
    year={2023},
    eprint={2304.12782},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP}
    }

    arXiv
  96. I. Georgieva, C. M. Persson, E. Goffo, L. Acuna, A. Aguichine, L. M. Serrano, K. W. F. Lam, D. Gandolfi, K. A. Collins, S. B. Howell, F. Dai, M. C. V. Fridlund, J. Korth, M. Deleuil, O. Barragán, W. D. Cochran, S. Csizmadia, H. J. Deeg, E. W. Guenther, A. P. Hatzes, J. M. Jenkins, J. H. Livingston, R. Luque, O. Mousis, H. L. M. Osborne, E. Pallé, S. Redfield, V. Van Eylen, J. D. Twicken, J. N. Winn, A. Alqasim, K. I. Collins, C. L. Gnilka, D. W. Latham, H. M. Lewis, H. M. Relles, G. R. Ricker, P. Rowden, S. Seager, A. Shporer, T. G. Tan, A. Vanderburg, R. Vanderspek

    TOI-733 b – a planet in the small-planet radius valley orbiting a Sun-like star

    bib

    @misc{georgieva2023toi733,
    title={TOI-733 b -- a planet in the small-planet radius valley orbiting a Sun-like star},
    author={Iskra Y. Georgieva and Carina M. Persson and Elisa Goffo and Lorena Acuña and Artyom Aguichine and Luisa M. Serrano and Kristine W. F. Lam and Davide Gandolfi and Karen A. Collins and Steven B. Howell and Fei Dai and Malcolm Fridlund and Judith Korth and Magali Deleuil and Oscar Barragán and William D. Cochran and Szilárd Csizmadia and Hans J. Deeg and Eike Guenther and Artie P. Hatzes and Jon M. Jenkins and John Livingston and Rafael Luque and Olivier Mousis and Hannah L. M. Osborne and Enric Palle and Seth Redfield and Vincent Van Eylen and Joseph D. Twicken and Joshua N. Winn and Ahlam Alqasim and Kevin I. Collins and Crystal L. Gnilka and David W. Latham and Hannah M. Lewis and Howard M. Relles and George R. Ricker and Pamela Rowden and Sara Seager and Avi Shporer and Thiam-Guan Tan and Andrew Vanderburg and Roland Vanderspek},
    year={2023},
    eprint={2304.06655},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP}
    }

    arXiv
  97. 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, MOA Collaboration, M. 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, KMTNet Collaboration, G. Christie, T. Cooper, J. Drummond, J. Green, S. Hennerley, J. McCormick, L. A. G. Monard, T. Natusch, I. Porritt, T. G. Tan, Microfun Collaboration, 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, Omega Collaboration, G. Rau

    MOA-2020-BLG-208Lb: Cool Sub-Saturn-mass Planet within Predicted Desert

    bib

    @article{Olmschenk_2023,
    doi = {10.3847/1538-3881/acbcc8},

    url = {https://doi.org/10.3847%2F1538-3881%2Facbcc8},

    year = 2023,
    month = {mar},

    publisher = {American Astronomical Society},

    volume = {165},

    number = {4},

    pages = {175},

    author = {Greg Olmschenk and David P. Bennett and Ian A. Bond and Weicheng Zang and Youn Kil Jung and Jennifer C. Yee and Etienne Bachelet and Fumio Abe and Richard K. Barry and Aparna Bhattacharya and Hirosane Fujii and Akihiko Fukui and Yuki Hirao and Stela Ishitani Silva and Yoshitaka Itow and Rintaro Kirikawa and Iona Kondo and Naoki Koshimoto and Yutaka Matsubara and Sho Matsumoto and Shota Miyazaki and Brandon Munford and Yasushi Muraki and Arisa Okamura and Cl{\'{e}
    }ment Ranc and Nicholas J. Rattenbury and Yuki Satoh and Takahiro Sumi and Daisuke Suzuki and Taiga Toda and Paul J. Tristram and Aikaterini Vandorou and Hibiki Yama and Michael D. Albrow and Sang-Mok Cha and Sun-Ju Chung and Andrew Gould and Cheongho Han and Kyu-Ha Hwang and Dong-Jin Kim and Hyoun-Woo Kim and Seung-Lee Kim and Chung-Uk Lee and Dong-Joo Lee and Yongseok Lee and Byeong-Gon Park and Richard W. Pogge and Yoon-Hyun Ryu and In-Gu Shin and Yossi Shvartzvald and Grant Christie and Tony Cooper and John Drummond and Jonathan Green and Steve Hennerley and Jennie McCormick and L. A. G. Monard and Tim Natusch and Ian Porritt and Thiam-Guan Tan and Shude Mao and Dan Maoz and Matthew T. Penny and Wei Zhu and V. Bozza and Arnaud Cassan and Martin Dominik and Markus Hundertmark and R. Figuera Jaimes and K. Kruszy{\'{n}}ska and K. A. Rybicki and R. A. Street and Y. Tsapras and Joachim Wambsganss and {\L}. Wyrzykowski and P. Zieli{\'{n}}ski and Gioia Rau},

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

    journal = {The Astronomical Journal}
    }

    DOI arXiv
  98. E. Knudstrup, S. H. Albrecht, D. Gandolfi, M. L. Marcussen, E. Goffo, L. M. Serrano, F. Dai, S. Redfield, T. Hirano, S. Csizmadia, W. D. Cochran, H. J. Deeg, M. C. V. Fridlund, K. W. F. Lam, J. H. Livingston, R. Luque, N. Narita, E. Pallé, C. M. Persson, V. Van Eylen

    A puffy polar planet. The low density, hot Jupiter TOI-640 b is on a polar orbit

    bib

    @article{Knudstrup_2023,
    doi = {10.1051/0004-6361/202245301},

    url = {https://doi.org/10.1051%2F0004-6361%2F202245301},

    year = 2023,
    month = {mar},

    publisher = {{EDP} Sciences},

    volume = {671},

    pages = {A164},

    author = {Emil Knudstrup and Simon H. Albrecht and Davide Gandolfi and Marcus L. Marcussen and Elisa Goffo and Luisa M. Serrano and Fei Dai and Seth Redfield and Teruyuki Hirano and Szil{\'{a}
    }rd Csizmadia and William D. Cochran and Hans J. Deeg and Malcolm Fridlund and Kristine W. F. Lam and John H. Livingston and Rafael Luque and Norio Narita and Enric Palle and Carina M. Persson and Vincent Van Eylen},

    title = {A puffy polar planet},

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

    DOI arXiv
  99. J. Mah, B. Bitsch

    Forming super-Mercuries: The role of stellar abundances

    bib

    @misc{mah2023forming,
    title={Forming super-Mercuries: The role of stellar abundances},
    author={J. Mah and B. Bitsch},
    year={2023},
    eprint={2303.11948},
    archivePrefix={arXiv},
    primaryClass={astro-ph.EP}
    }

    arXiv
  100. F. Liebing, S. V. Jeffers, M. Zechmeister, A. Reiners

    Convective blueshift strengths for 242 evolved stars

    bib

    @misc{https://doi.org/10.48550/arxiv.2303.04556,
    doi = {10.48550/ARXIV.2303.04556},

    url = {https://arxiv.org/abs/2303.04556},

    author = {Liebing, F. and Jeffers, S. V. and Zechmeister, M. and Reiners, A.},

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

    title = {Convective blueshift strengths for 242 evolved stars},

    publisher = {arXiv},

    year = {2023},

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

    arXiv
  101. J. MacKenzie, J. L. Grenfell, P. Baumeister, N. Tosi, J. Cabrera, H. Rauer

    Effect of improved atmospheric opacities in modelling sub-Neptunes. A case study for GJ 1214 b

    DOI
  102. 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, 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, M. Horrobin, M. Houllé, Z. Hubert, L. Jocou, M. Keppler, P. Kervella, L. Kreidberg, V. Lapeyrère, J. -B. Le Bouquin, P. Léna, D. Lutz, A. L. Maire, F. Mang, A. Mérand, N. Meunier, J. D. Monnier, D. Mouillet, E. Nasedkin, T. Ott, G. P. P. L. Otten, C. Paladini, T. Paumard, K. Perraut, G. Perrin, F. Philipot, O. Pfuhl, N. Pourré, L. Pueyo, J. Rameau, E. Rickman, P. Rubini, Z. Rustamkulov, M. Samland, J. Shangguan, T. Shimizu, D. K. Sing, C. Straubmeier, E. Sturm, L. J. Tacconi, E. van Dishoeck, A. Vigan, F. Vincent, K. Ward-Duong, F. Widmann, E. Wieprecht, E. Wiezorrek, J. Woillez, S. Yazici, A. Young, N. Zicher

    Direct discovery of the inner exoplanet in the HD 206893 system. Evidence for deuterium burning in a planetary-mass companion

    DOI
  103. F. Yan, L. Nortmann, A. Reiners, N. Piskunov, A. P. Hatzes, U. Seemann, D. Shulyak, A. Lavail, A. D. Rains, D. Cont, M. Rengel, F. Lesjak, E. Nagel, O. Kochukhov, S. Czesla, L. Boldt-Christmas, U. Heiter, J. V. Smoker, F. Rodler, P. Bristow, R. J. Dorn, Y. Jung, T. Marquart, E. Stempels

    CRIRES+ detection of CO emissions lines and temperature inversions on the dayside of WASP-18b and WASP-76b

    bib

    @misc{https://doi.org/10.48550/arxiv.2302.08736,
    doi = {10.48550/ARXIV.2302.08736},

    url = {https://arxiv.org/abs/2302.08736},

    author = {Yan, F. and Nortmann, L. and Reiners, A. and Piskunov, N. and Hatzes, A. and Seemann, U. and Shulyak, D. and Lavail, A. and Rains, A. D. and Cont, D. and Rengel, M. and Lesjak, F. and Nagel, E. and Kochukhov, O. and Czesla, S. and Boldt-Christmas, L. and Heiter, U. and Smoker, J. V. and Rodler, F. and Bristow, P. and Dorn, R. J. and Jung, Y. and Marquart, T. and Stempels, E.},

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

    title = {CRIRES+ detection of CO emissions lines and temperature inversions on the dayside of WASP-18b and WASP-76b},

    publisher = {arXiv},

    year = {2023},

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

    arXiv
  104. M. Rengel

    About the atomic and molecular databases in the planetary community — A contribution in the Laboratory Astrophysics Data WG IAU 2022 GA session

    bib

    @misc{https://doi.org/10.48550/arxiv.2302.05452,
    doi = {10.48550/ARXIV.2302.05452},

    url = {https://arxiv.org/abs/2302.05452},

    author = {Rengel, M.},

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

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

    publisher = {arXiv},

    year = {2023},

    copyright = {Creative Commons Attribution 4.0 International}
    }

    arXiv
  105. D. Kossakowski, M. Kürster, T. Trifonov, Th. Henning, J. Kemmer, J. A. Caballero, R. Burn, S. Sabotta, J. S. Crouse, T. J. Fauchez, E. Nagel, A. Kaminski, E. Herrero, E. Rodríguez, E. González-Álvarez, A. Quirrenbach, P. J. Amado, I. Ribas, A. Reiners, J. Aceituno, V. J. S. Béjar, D. Baroch, S. T. Bastelberger, P. Chaturvedi, C. Cifuentes, S. Dreizler, S. V. Jeffers, R. Kopparapu, M. Lafarga, M. J. López-González, S. Martín-Ruiz, D. Montes, J. C. Morales, E. Pallé, A. Pavlov, S. Pedraz, V. Perdelwitz, M. Pérez-Torres, M. Perger, S. Reffert, C. Rodríguez López, M. Schlecker, P. Schöfer, A. Schweitzer, Y. Shan, A. Shields, S. Stock, E. Wolf, M. R. Zapatero Osorio, M. Zechmeister

    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

    bib

    @article{Kossakowski_2023,
    doi = {10.1051/0004-6361/202245322},

    url = {https://doi.org/10.1051%2F0004-6361%2F202245322},

    year = 2023,
    month = {feb},

    publisher = {{EDP} Sciences},

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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
  124. 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}
    }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 Adibekyan and R Alonso and G A 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 C 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 characterization of the multiplanet system},

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

    DOI arXiv
  125. 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
  126. 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},
    month = {dec},
    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
  129. 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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    @misc{https://doi.org/10.48550/arxiv.2211.15312,
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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
  130. 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}
    }

    DOI arXiv
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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
  132. 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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    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
  133. 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,
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    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
  134. 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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    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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    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
  136. 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
  137. 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
  138. 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
  139. 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
  140. 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
  141. 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

  142. 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
  143. 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
  144. 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
  145. 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
  146. 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
  147. 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
  148. 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
  149. 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
  150. 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
  151. 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
  152. 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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    url = {https://arxiv.org/abs/2208.04867},

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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
  153. 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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  154. 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
  155. 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
  156. 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
  157. 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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    url = {https://doi.org/10.3847%2F1538-3881%2Fac78ed},

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

    volume = {164},

    number = {3},

    pages = {75},

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    journal = {The Astronomical Journal}
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  158. 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
  159. 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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    @misc{https://doi.org/10.48550/arxiv.2208.00892,
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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
  160. 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
  161. 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

  162. 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
  163. 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,
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    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
  164. 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
  165. 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
  166. 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
  167. 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
  168. 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
  169. 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
  170. 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
  171. 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
  172. 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

  173. 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

  174. 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

  175. 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
  176. 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
  177. 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
  178. 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

  179. 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

  180. 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
  181. A. Krieger, S. Wolf

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

  182. 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

  183. 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

  184. 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

  185. 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
  186. 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

  187. 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

  188. 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
  189. 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

  190. 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
  191. 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

  192. 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

  193. 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

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

    Steady-state accretion in magnetized protoplanetary disks

  195. 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

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

    On the multiple generations of planetary embryos

  197. 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
  198. 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

  199. 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
  200. 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

  201. 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
  202. 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

  203. 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

  204. 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
  205. 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

  206. 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

  207. 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

  208. 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

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

    Misaligned disks induced by infall

  210. 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

  211. 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

  212. 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

  213. 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
  214. 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
  215. 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
  216. 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
  217. 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
  218. 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
  219. 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

  220. 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
  221. 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
  222. F. Liebing, S. V. Jeffers, A. Reiners, M. Zechmeister

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

  223. 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

  224. 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

  225. 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
  226. 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

  227. 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

  228. 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
  229. 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
  230. 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

  231. 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
  232. 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

  233. M. P. Döllinger, M. Hartmann

    A sanity check for planets around evolved Stars

    DOI
  234. 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

  235. 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
  236. 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
  237. Y. Aoyama, G.-D. Marleau, M. Ikoma, C. Mordasini

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

  238. 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
  239. 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

  240. 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
  241. 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
  242. 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
  243. G. M. Brandt, T. D. Brandt, T. J. Dupuy, D. Michalik, G.-D. Marleau

    The First Dynamical Mass Measurement in the HR 8799 System

  244. 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
  245. 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
  246. 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
  247. 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
  248. 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

  249. 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
  250. 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
  251. 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
  252. 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
  253. 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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  254. 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
  255. 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},
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  256. F. Wunderlich, M. Scheucher, J. L. Grenfell, F. Schreier, C. Sousa-Silva, M. Godolt, H. Rauer

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    primaryClass = {astro-ph.EP},
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    DOI arXiv
  257. 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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    DOI arXiv
  258. 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},
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    pages = {arXiv:2102.00939},
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    eprint = {2102.00939},
    primaryClass = {astro-ph.EP},
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    DOI arXiv
  259. 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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    archivePrefix = {arXiv},
    eprint = {2012.10435},
    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...646A.159S},
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    DOI arXiv
  260. 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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  261. 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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  262. 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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    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
  263. 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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    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...646A.183S},
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    DOI arXiv
  264. P. Gao, H. R. Wakeford, S. Moran, V. Parmentier

    Aerosols in Exoplanet Atmospheres

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    primaryClass = {astro-ph.EP},
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  265. 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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    pages = {arXiv:2102.12854},
    archivePrefix = {arXiv},
    eprint = {2102.12854},
    primaryClass = {astro-ph.EP},
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  266. 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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  267. 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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  268. 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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  269. 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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    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
  270. 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}",
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    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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    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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  271. 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},
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    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...645A..41L},
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    DOI arXiv
  272. 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
  273. 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
  274. O. Voelkel, R. Deienno, K. Kretke, H. Klahr

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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
  275. 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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    keywords = {planets and satellites: formation, planets and satellites: terrestrial planets, Astrophysics - Earth and Planetary Astrophysics},
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    eprint = {2008.10432},
    primaryClass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...645A.132V},
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    DOI arXiv
  276. A. Krieger, S. Wolf

    The scattering order problem in Monte Carlo radiative transfer

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    eprint = {2011.14905},
    primaryClass = {astro-ph.IM},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...645A.143K},
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  277. 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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    DOI arXiv
  278. M. Tala-Pinto, S. Reffert, A. Quirrenbach, S. Stock, T. Trifonov, D. S. Mitchell

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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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    arXiv
  280. 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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  281. 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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  283. 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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  284. E. M. Amazo-Gómez, A. I. Shapiro, S. K. Solanki, G. Kopp, M. Oshagh, T. Reinhold, A. Reiners

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  285. F. Yan, N. Espinoza, K. Molaverdikhani, T. Henning, L. Mancini, M. Mallonn, B. V. Rackham, D. Apai, A. Jordán, P. Mollière, G. Chen, L. Carone, A. Reiners

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

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

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  290. 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,
    month = jul,
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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
  305. 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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  306. 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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    number = {3},
    pages = {3623-3637},
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    archiveprefix = {arXiv},
    eprint = {2007.11999},
    primaryclass = {astro-ph.EP},
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  307. 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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  308. 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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    DOI arXiv
  309. 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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    title = {{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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    eprint = {2005.00006},
    primaryclass = {astro-ph.EP},
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  310. M. Scheucher, F. Wunderlich, J. L. Grenfell, M. Godolt, F. Schreier, D. Kappel, R. Haus, K. Herbst, H. Rauer

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    journal = {\apj},
    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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    DOI arXiv
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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
  312. 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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    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},
    eprint = {2005.08850},
    primaryclass = {astro-ph.EP},
    adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...639A..54L},
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    DOI arXiv
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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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  314. D. Shulyak, L. M. Lara, M. Rengel, N. E. Nèmec

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

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

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  319. A. Bhandare, R. Kuiper, T. Henning, C. Fendt, M. Flock, G.-D. Marleau

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

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    keywords = {planetary systems, planets and satellites: individual: MASCARA2-b, planets and satellites: atmospheres, techniques: spectroscopic, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
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  323. P. Baumeister, S. Padovan, N. Tosi, G. Montavon, N. Nettelmann, J. MacKenzie, M. Godolt

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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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  332. 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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  334. 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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  353. A. García Muñoz, A. Youngblood, L. Fossati, D. Gandolfi, J. Cabrera, H. Rauer

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  355. F. Schreier, S. Städt, F. Wunderlich, M. Godolt, J. L. Grenfell

    SVEEEETIES: singular vector expansion to estimate Earth-like exoplanet temperatures from infrared emission spectra

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  356. 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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    DOI arXiv
  358. A. Ziampras, S. Ataiee, W. Kley, C. P. Dullemond, C. Baruteau

    The impact of planet wakes on the location and shape of the water ice line in a protoplanetary disk

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    month = jan,
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    DOI arXiv
  359. H. Parviainen, M. R. Zapatero Osorio, P. Montañés-Rodríguez, F. Murgas, N. Narita, D. Hidalgo Soto, V. J. S. Béjar, J. Korth, M. Monelli, N. Casasayas-Barris, N. Crouzet, J. P. de Leon, A. Fukui, A. Hernandez, P. Klagyivik, N. Kusakabe, R. Luque, M. Mori, T. Nishiumi, J. Prieto-Arranz, M. Tamura, N. Watanabe, C. Burke, D. Charbonneau, K. A. Collins, D. Conti, A. Garcia Soto, J. S. Jenkins, J. M. Jenkins, A. Levine, J. Li, S. Rinehart, S. Seager, P. Tenenbaum, E. B. Ting, R. Vanderspek, M. Vezie, J. N. Winn

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

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

    Effect of wind-driven accretion on planetary migration

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    DOI arXiv
  361. 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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  364. 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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  365. 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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  367. Grégoire Montavon, Jasmine MacKenzie, Nadine Nettelmann, Nicola Tosi, Philipp Baumeister, Sebastiano Padovan, Mareike Godolt

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  370. 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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