Publications

@misc{nascimbeni2024k224planetaryrevisitedcheops,
title={The K2-24 planetary system revisited by CHEOPS},
author={V. Nascimbeni and L. Borsato and P. Leonardi and S. G. Sousa and T. G. Wilson and A. Fortier and A. Heitzmann and G. Mantovan and R. Luque and T. Zingales and G. Piotto and Y. Alibert and R. Alonso and T. Bárczy and D. Barrado Navascues and S. C. Barros and W. Baumjohann and T. Beck and W. Benz and N. Billot and F. Biondi and A. Brandeker and C. Broeg and M. -D. Busch and A. Collier Cameron and A. C. M. Correia and Sz. Csizmadia and P. E. Cubillos and M. B. Davies and M. Deleuil and A. Deline and L. Delrez and O. D. S. Demangeon and B. -O. Demory and A. Derekas and B. Edwards and D. Ehrenreich and A. Erikson and L. Fossati and M. Fridlund and D. Gandolfi and K. Gazeas and M. Gillon and M. Güdel and M. N. Günther and Ch. Helling and K. G. Isaak and F. Kerschbaum and L. Kiss and J. Korth and K. W. F. Lam and J. Laskar and A. Lecavelier des Etangs and A. Leleu and M. Lendl and D. Magrin and P. F. L. Maxted and B. Merín and C. Mordasini and G. Olofsson and R. Ottensamer and I. Pagano and E. Pallé and G. Peter and D. Pollacco and D. Queloz and R. Ragazzoni and N. Rando and H. Rauer and I. Ribas and N. C. Santos and G. Scandariato and D. Ségransan and A. E. Simon and A. M. S. Smith and R. Southworth and M. Stalport and S. Sulis and M. Gy. Szabó and S. Udry and B. Ulmer and V. Van Grootel and J. Venturini and E. Villaver and N. A. Walton},
year={2024},
eprint={2409.02995},
archivePrefix={arXiv},
primaryClass={astro-ph.EP},
url={https://arxiv.org/abs/2409.02995},
}

@misc{pfeil2024tripodtripopulationsizedistributions,
title={TriPoD: Tri-Population size distributions for Dust evolution. Coagulation in vertically integrated hydrodynamic simulations of protoplanetary disks},
author={Thomas Pfeil and Til Birnstiel and Hubert Klahr},
year={2024},
eprint={2409.03816},
archivePrefix={arXiv},
primaryClass={astro-ph.EP},
url={https://arxiv.org/abs/2409.03816},
}

@misc{liebing2024reddotslimitshabitableundetected,
title={RedDots: Limits on habitable and undetected planets orbiting nearby stars GJ 832, GJ 674, and Ross 128},
author={F. Liebing and S. V. Jeffers and P. Gorrini and C. A. Haswell and S. Dreizler and J. R. Barnes and C. Hartogh and V. Koseleva and F. Del Sordo and P. J. Amado and J. A. Caballero and M. J. López-González and N. Morales and A. Reiners and I. Ribas and A. Quirrenbach and E. Rodríguez and L. Tal-Or and Y. Tsapras},
year={2024},
eprint={2409.01173},
archivePrefix={arXiv},
primaryClass={astro-ph.EP},
url={https://arxiv.org/abs/2409.01173},
}

@misc{wu2024influenceplanetsdebrisdiscs,
title={Influence of planets on debris discs in star clusters -- II. The impact of stellar density},
author={Kai Wu and M. B. N. Kouwenhoven and Francesco Flammini Dotti and Rainer Spurzem},
year={2024},
eprint={2409.00996},
archivePrefix={arXiv},
primaryClass={astro-ph.EP},
url={https://arxiv.org/abs/2409.00996},
}

@article{Heller_2024,
title={A False Positive Transit Candidate for EPIC 211101996 from K2 and TESS Data Identified as Background Eclipsing Binary Gaia DR3 66767847894609792},
volume={8},
ISSN={2515-5172},
url={http://dx.doi.org/10.3847/2515-5172/ad73bb},
DOI={10.3847/2515-5172/ad73bb},
number={8},
journal={Research Notes of the AAS},
publisher={American Astronomical Society},
author={Heller, René and Hüschen, Milena and Harre, Jan-Vincent and Dreizler, Stefan},
year={2024},
month=aug, pages={212} }

@misc{muley2024gapedgeilluminationexcitespirals,
title={Can gap-edge illumination excite spirals in protoplanetary disks? Three-temperature radiation hydrodynamics and NIR image modelling},
author={Dhruv Muley and Julio David Melon Fuksman and Hubert Klahr},
year={2024},
eprint={2408.16461},
archivePrefix={arXiv},
primaryClass={astro-ph.EP},
url={https://arxiv.org/abs/2408.16461},
}

@misc{plunkett2024accretingcompanionoccurrencerates,
title={Accreting companion occurrence rates using a new method to compute emission-line survey sensitivity: Application to the H-alpha Giant Accreting Protoplanet Survey (GAPlanetS)},
author={Cailin Plunkett and Katherine B. Follette and Gabriel-Dominique Marleau and Eric Nielsen},
year={2024},
eprint={2408.01491},
archivePrefix={arXiv},
primaryClass={astro-ph.EP},
url={https://arxiv.org/abs/2408.01491},
}

@article{Spaeth_2024,
title={Non-radial oscillations mimicking a brown dwarf orbiting the cluster giant NGC 4349 No. 127},
volume={689},
ISSN={1432-0746},
url={http://dx.doi.org/10.1051/0004-6361/202450163},
DOI={10.1051/0004-6361/202450163},
journal={Astronomy & Astrophysics},
publisher={EDP Sciences},
author={Spaeth, Dane and Reffert, Sabine and Hunt, Emily L. and Kaminski, Adrian and Quirrenbach, Andreas},
year={2024},
month=sep, pages={A91} }

@article{Aoyama_2024,
title={Analyzing JWST/NIRSpec Hydrogen Line Detections at TWA 27B: Constraining Accretion Properties and Geometry},
volume={168},
ISSN={1538-3881},
url={http://dx.doi.org/10.3847/1538-3881/ad67df},
DOI={10.3847/1538-3881/ad67df},
number={4},
journal={The Astronomical Journal},
publisher={American Astronomical Society},
author={Aoyama, Yuhiko and Marleau, Gabriel-Dominique and Hashimoto, Jun},
year={2024},
month=sep, pages={155} }

@misc{böning2024commonlawdifferentialrotation,
title={A common law for the differential rotation of planets and stars},
author={Vincent G. A. Böning and Johannes Wicht},
year={2024},
eprint={2407.13484},
archivePrefix={arXiv},
primaryClass={astro-ph.SR},
url={https://arxiv.org/abs/2407.13484},
}

@article{Borsato_2024,
title={Characterisation of the warm-Jupiter TOI-1130 system with CHEOPS and a photo-dynamical approach},
volume={689},
ISSN={1432-0746},
url={http://dx.doi.org/10.1051/0004-6361/202450974},
DOI={10.1051/0004-6361/202450974},
journal={Astronomy & Astrophysics},
publisher={EDP Sciences},
author={Borsato, L. and Degen, D. and Leleu, A. and Hooton, M. J. and Egger, J. A. and Bekkelien, A. and Brandeker, A. and Collier Cameron, A. and Günther, M. N. and Nascimbeni, V. and Persson, C. M. and Bonfanti, A. and Wilson, T. G. and Correia, A. C. M. and Zingales, T. and Guillot, T. and Triaud, A. H. M. J. and Piotto, G. and Gandolfi, D. and Abe, L. and Alibert, Y. and Alonso, R. and Bárczy, T. and Navascues, D. Barrado and Barros, S. C. C. and Baumjohann, W. and Beck, T. and Bendjoya, P. and Benz, W. and Billot, N. and Broeg, C. and Busch, M.-D. 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 Fridlund, M. and Gazeas, K. and Gillon, M. and Güdel, M. and Heitzmann, A. 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 Lendl, M. and Magrin, D. and Marafatto, L. and Maxted, P. F. L. and Mecina, M. and Mékarnia, D. and Mordasini, C. and Mura, D. and Olofsson, G. and Ottensamer, R. and Pagano, I. and Pallé, E. and Peter, G. and Pollacco, D. and Queloz, D. and Ragazzoni, R. and Rando, N. and Ratti, F. and Rauer, H. and Ribas, I. and Salmon, S. 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 Suarez, O. and Sulis, S. and Szabó, Gy. M. and Udry, S. and Van Grootel, V. and Venturini, J. and Villaver, E. and Walton, N. A. and Wolter, D.},
year={2024},
month=sep, pages={A52} }

@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},
}

@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},
}

@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} }

@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} }

@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},
}

@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 }

@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},
}

@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} }

@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}
}

@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} }

@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}
}

@article{Leleu_2024,
title={Photo-dynamical characterisation of the TOI-178 resonant chain: Exploring the robustness of transit-timing variations and radial velocity mass characterisations},
volume={688},
ISSN={1432-0746},
url={http://dx.doi.org/10.1051/0004-6361/202450212},
DOI={10.1051/0004-6361/202450212},
journal={Astronomy & Astrophysics},
publisher={EDP Sciences},
author={Leleu, A. and Delisle, J.-B. and Delrez, L. and Bryant, E. M. and Brandeker, A. and Osborn, H. P. and Hara, N. and Wilson, T. G. and Billot, N. and Lendl, M. and Ehrenreich, D. and Chakraborty, H. and Günther, M. N. and Hooton, M. J. and Alibert, Y. and Alonso, R. and Alves, D. R. and Anderson, D. R. and Apergis, I. and Armstrong, D. and Bárczy, T. and Barrado Navascues, D. and Barros, S. C. C. and Battley, M. P. and Baumjohann, W. and Bayliss, D. and Beck, T. and Benz, W. and Borsato, L. and Broeg, C. and Burleigh, M. R. and Casewell, S. L. and Collier Cameron, A. and Correia, A. C. M. and Csizmadia, Sz. and Cubillos, P. E. and Davies, M. B. and Deleuil, M. and Deline, A. and Demangeon, O. D. S. and Demory, B.-O. and Derekas, A. and Edwards, B. and Erikson, A. and Fortier, A. and Fossati, L. and Fridlund, M. and Gandolfi, D. and Gazeas, K. and Gillen, E. and Gillon, M. and Goad, M. R. and Güdel, M. and Hawthorn, F. and Heitzmann, A. and Helling, Ch. and Isaak, K. G. and Jenkins, J. S. and Jenkins, J. M. and Kendall, A. and Kiss, L. L. and Korth, J. and Lam, K. W. F. and Laskar, J. and Latham, D. W. and Lecavelier des Etangs, A. and Magrin, D. and Maxted, P. F. L. and McCormac, J. and Mordasini, C. and Moyano, M. and Nascimbeni, V. and Olofsson, G. and Osborn, A. and Ottensamer, R. and Pagano, I. and Pallé, E. and Peter, G. and Piotto, G. and Pollacco, D. and Queloz, D. and Ragazzoni, R. and Rando, N. and Rauer, H. and Ribas, I. and Ricker, G. and Saha, S. and Santos, N. C. and Scandariato, G. and Seager, S. and Ségransan, D. and Simon, A. E. and Smith, A. M. S. and Sousa, S. G. and Stalport, M. and Sulis, S. and Szabó, Gy. M. and Udry, S. and Ulmer-Moll, S. and Van Grootel, V. and Vanderspek, R. and Venturini, J. and Villaver, E. and Vinés, J. I. and Walton, N. A. and West, R. G. and Wheatley, P. J. and Winn, J. and Zivave, T.},
year={2024},
month=aug, pages={A211} }

@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}
}

@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} }

@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},
}

@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}
}

@misc{keles2024pepsi,
title={The PEPSI Exoplanet Transit Survey (PETS). V: New Na D transmission spectra indicate a quieter atmosphere on HD 189733b},
author={E. Keles and S. Czesla and K. Poppenhaeger and P. Hauschildt and T. A. Carroll and I. Ilyin and M. Baratella and M. Steffen and K. G. Strassmeier and A. S. Bonomo and B. S. Gaudi and T. Henning and M. C. Johnson and K. Molaverdikhani and V. Nascimbeni and J. Patience and A. Reiners and G. Scandariato and E. Schlawin and E. Shkolnik and D. Sicilia and A. Sozzetti and M. Mallonn and C. Veillet and J. Wang and F. Yan},
year={2024},
eprint={2404.13586},
archivePrefix={arXiv},
primaryClass={astro-ph.EP}
}

@misc{yan2024possibly,
title={A possibly solar metallicity atmosphere escaping from HAT-P-32b revealed by H$\alpha$ and He absorption},
author={Dongdong Yan and Jianheng Guo and Kwang-il Seon and Manuel López-Puertas and Stefan Czesla and Manuel Lampón},
year={2024},
eprint={2403.17325},
archivePrefix={arXiv},
primaryClass={astro-ph.EP}
}

@misc{street2024romerea,
title={ROME/REA: Three-year, Tri-color Timeseries Photometry of the Galactic Bulge},
author={R. A. Street and E. Bachelet and Y. Tsapras and M. P. G. Hundertmark and V. Bozza and D. M. Bramich and A. Cassan and M. Dominik and R. Figuera Jaimes and K. Horne and S. Mao and A. Saha and J. Wambsganss and Weicheng Zang},
year={2024},
eprint={2403.05987},
archivePrefix={arXiv},
primaryClass={astro-ph.GA}
}

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

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

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

@article{Bernab__2024,
title={Evidence of apsidal motion and a possible co-moving companion star detected in the WASP-19 system},
volume={684},
ISSN={1432-0746},
url={http://dx.doi.org/10.1051/0004-6361/202346852},
DOI={10.1051/0004-6361/202346852},
journal={Astronomy & Astrophysics},
publisher={EDP Sciences},
author={Bernabò, L. M. and Csizmadia, Sz. and Smith, A. M. S. and Rauer, H. and Hatzes, A. and Esposito, M. and Gandolfi, D. and Cabrera, J.},
year={2024},
month=apr, pages={A78} }

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

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

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

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

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

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

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

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

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

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

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

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

@misc{swayne2023eblm,
title={The EBLM Project XI. Mass, radius and effective temperature measurements for 23 M-dwarf companions to solar-type stars observed with CHEOPS},
author={M. I. Swayne and P. F. L. Maxted and A. H. M. J. Triaud and S. G. Sousa and A. Deline and D. Ehrenreich and S. Hoyer and G. Olofsson and I. Boisse and A. Duck and S. Gill and D. Martin and J. McCormac and C. M. Persson and A. Santerne and D. Sebastian and M. R. Standing and L. Acuña and Y. Alibert and R. Alonso and G. Anglada and T. Bárczy and D. Barrado Navascues and S. C. C. Barros and W. Baumjohann and T. A. Baycroft and M. Beck and T. Beck and W. Benz and N. Billot and X. Bonfils and L. Borsato and V. Bourrier and A. Brandeker and C. Broeg and A. Carmona and S. Charnoz and A. Collier Cameron and P. Cortés-Zuleta and Sz. Csizmadia and P. E. Cubillos and M. B. Davies and M. Deleuil and X. Delfosse and L. Delrez and O. D. S. Demangeon and B. -O. Demory and G. Dransfield and A. Erikson and A. Fortier and T. Forveille and L. Fossati and M. Fridlund and D. Gandolfi and M. Gillon and M. Güdel and M. N. Günther and N. Hara and G. Hébrard and N. Heidari and C. Hellier and Ch. Helling and K. G. Isaak and F. Kerschbaum and F. Kiefer and L. L. Kiss and V. Kunovac and S. Lalitha and K. W. F. Lam and J. Laskar and A. Lecavelier des Etangs and M. Lendl and D. Magrin and L. Marafatto and E. Martioli and N. J. Miller and C. Mordasini and C. Moutou and V. Nascimbeni and R. Ottensamer and I. Pagano and E. Pallé and G. Peter and D. Piazza and G. Piotto and D. Pollacco and D. Queloz and R. Ragazzoni and N. Rando and H. Rauer and I. Ribas and N. C. Santos and G. Scandariato and D. Ségransan and A. E. Simon and A. M. S. Smith and R. Southworth and M. Stalport and Gy. M. Szabó and N. Thomas and S. Udry and B. Ulmer and V. Van Grootel and J. Venturini and N. A. Walton and E. Willett and T. G. Wilson},
year={2023},
eprint={2312.11339},
archivePrefix={arXiv},
primaryClass={astro-ph.SR}
}

@misc{balmer2023vltigravity,
title={VLTI/GRAVITY Provides Evidence the Young, Substellar Companion HD 136164 Ab formed like a "Failed Star"},
author={William O. Balmer and L. Pueyo and S. Lacour and J. J. Wang and T. Stolker and J. Kammerer and N. Pourré and M. Nowak and E. Rickman and S. Blunt and A. Sivaramakrishnan and D. Sing and K. Wagner and G. -D. Marleau and A. -M. Lagrange and R. Abuter and A. Amorim and R. Asensio-Torres and J. -P. Berger and H. Beust and A. Boccaletti and A. Bohn and M. Bonnefoy and H. Bonnet and M. S. Bordoni and G. Bourdarot and W. Brandner and F. Cantalloube and P. Caselli and B. Charnay and G. Chauvin and A. Chavez and E. Choquet and V. Christiaens and Y. Clénet and V. Coudé du Foresto and A. Cridland and R. Davies and R. Dembet and A. Drescher and G. Duvert and A. Eckart and F. Eisenhauer and N. M. F"orster Schreiber and P. Garcia and R. Garcia Lopez and E. Gendron and R. Genzel and S. Gillessen and J. H. Girard and S. Grant and X. Haubois and G. Heißel and Th. Henning and S. Hinkley and S. Hippler and M. Houllé and Z. Hubert and L. Jocou and M. Keppler and P. Kervella and L. Kreidberg and N. T. Kurtovic and V. Lapeyrère and J. -B. Le Bouquin and P. Léna and D. Lutz and A. -L. Maire and F. Mang and A. Mérand and P. Mollière and C. Mordasini and D. Mouillet and E. Nasedkin and T. Ott and G. P. P. L. Otten and C. Paladini and T. Paumard and K. Perraut and G. Perrin and O. Pfuhl and D. C. Ribeiro and L. Rodet and Z. Rustamkulov and J. Shangguan and T. Shimizu and C. Straubmeier and E. Sturm and L. J. Tacconi and A. Vigan and F. Vincent and K. Ward-Duong and F. Widmann and T. Winterhalder and J. Woillez and S. Yazici},
year={2023},
eprint={2312.08283},
archivePrefix={arXiv},
primaryClass={astro-ph.SR}
}

@misc{fuksman2023vertical,
title={Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks II. Secondary instabilities and stability regions},
author={Julio David Melon Fuksman and Mario Flock and Hubert Klahr},
year={2023},
eprint={2312.06890},
archivePrefix={arXiv},
primaryClass={astro-ph.EP}
}

@misc{dominik2023bouncing,
title={The bouncing barrier revisited: Impact on key planet formation processes and observational signatures},
author={Carsten Dominik and Cornelis Dullemond},
year={2023},
eprint={2312.06000},
archivePrefix={arXiv},
primaryClass={astro-ph.EP}
}

@misc{bonfanti2023characterising,
title={Characterising TOI-732 b and c: New insights into the M-dwarf radius and density valley},
author={A. Bonfanti and M. Brady and T. G. Wilson and J. Venturini and J. A. Egger and A. Brandeker and S. G. Sousa and M. Lendl and A. E. Simon and D. Queloz and G. Olofsson and V. Adibekyan and Y. Alibert and L. Fossati and M. J. Hooton and D. Kubyshkina and R. Luque and F. Murgas and A. J. Mustill and N. C. Santos and V. Van Grootel and R. Alonso and J. Asquier and T. Bandy and T. Bárczy and D. Barrado Navascues and S. C. C. Barros and W. Baumjohann and J. Bean and M. Beck and T. Beck and W. Benz and M. Bergomi and N. Billot and L. Borsato and C. Broeg and A. Collier Cameron and Sz. Csizmadia and P. E. Cubillos and M. B. Davies and M. Deleuil and A. Deline and L. Delrez and O. D. S. Demangeon and B. -O. Demory and D. Ehrenreich and A. Erikson and A. Fortier and M. Fridlund and D. Gandolfi and M. Gillon and M. Güdel and M. N. Günther and A. Heitzmann and Ch. Helling and S. Hoyer and K. G. Isaak and D. Kasper and L. L. Kiss and K. W. F. Lam and J. Laskar and A. Lecavelier des Etangs and D. Magrin and P. F. L. Maxted and C. Mordasini and V. Nascimbeni and R. Ottensamer and I. Pagano and E. Pallé and G. Peter and G. Piotto and D. Pollacco and R. Ragazzoni and N. Rando and H. Rauer and I. Ribas and G. Scandariato and D. Ségransan and A. Seifahrt and A. M. S. Smith and M. Stalport and G. Stefánsson and M. Steinberger and J. Stürmer and Gy. M. Szabó and N. Thomas and S. Udry and E. Villaver and N. A. Walton and K. Westerdorff and T. Zingales},
year={2023},
eprint={2311.12577},
archivePrefix={arXiv},
primaryClass={astro-ph.EP}
}

@misc{palle2023groundbreaking,
title={Ground-breaking Exoplanet Science with the ANDES spectrograph at the ELT},
author={Enric Palle and Katia Biazzo and Emeline Bolmont and Paul Molliere and Katja Poppenhaeger and Jayne Birkby and Matteo Brogi and Gael Chauvin and Andrea Chiavassa and Jens Hoeijmakers and Emmanuel Lellouch and Christophe Lovis and Roberto Maiolino and Lisa Nortmann and Hannu Parviainen and Lorenzo Pino and Martin Turbet and Jesse Wender and Simon Albrecht and Simone Antoniucci and Susana C. Barros and Andre Beaudoin and Bjorn Benneke and Isabelle Boisse and Aldo S. Bonomo and Francesco Borsa and Alexis Brandeker and Wolfgang Brandner and Lars A. Buchhave and Anne-Laure Cheffot and Robin Deborde and Florian Debras and Rene Doyon and Paolo Di Marcantonio and Paolo Giacobbe and Jonay I. Gonzalez Hernandez and Ravit Helled and Laura Kreidberg and Pedro Machado and Jesus Maldonado and Alessandro Marconi and B. L. Canto Martins and Adriano Miceli and Christoph Mordasini and Mamadou N'Diaye and Andrezj Niedzielski and Brunella Nisini and Livia Origlia and Celine Peroux and Alex G. M. Pietrow and Enrico Pinna and Emily Rauscher and Sabine Reffert and Philippe Rousselot and Nicoletta Sanna and Adrien Simonnin and Alejandro Suarez Mascareno and Alessio Zanutta and Mathias Zechmeister},
year={2023},
eprint={2311.17075},
archivePrefix={arXiv},
primaryClass={astro-ph.IM}
}

@misc{krieger2023improving,
title={Improving Monte Carlo radiative transfer in the regime of high optical depths: The minimum scattering order},
author={Anton Krieger and Sebastian Wolf},
year={2023},
eprint={2311.13252},
archivePrefix={arXiv},
primaryClass={astro-ph.IM}
}

@article{Harre_2023,
title={The Apparent Tidal Decay of WASP-4 b Can Be Explained by the Rømer Effect},
volume={9},
ISSN={2218-1997},
url={http://dx.doi.org/10.3390/universe9120506},
DOI={10.3390/universe9120506},
number={12},
journal={Universe},
publisher={MDPI AG},
author={Harre, Jan-Vincent and Smith, Alexis M. S.},
year={2023},
month=dec, pages={506} }

@misc{herbst2023impact,
title={Impact of Cosmic Rays on Atmospheric Ion Chemistry and Spectral Transmission Features of TRAPPIST-1e},
author={Konstantin Herbst and Andreas Bartenschlager and John Lee Grenfell and Nicolas Iro and Miriam Sinnhuber and Benjamin Taysum and Fabian Wunderlich and N. Eugene Engelbrecht and Juandre Light and Katlego D. Moloto and Jan-Vincent Harre and Heike Rauer and Franz Schreier},
year={2023},
eprint={2311.04684},
archivePrefix={arXiv},
primaryClass={astro-ph.EP}
}

@misc{kálmán2023modelling,
title={Modelling the Light Curves of Transiting Exomoons: a Zero-order Photodynamic Agent Added to the Transit and Light Curve Modeller},
author={Sz. Kálmán and Sz. Csizmadia and A. E. Simon and K. W. F. Lam and A. Deline and J. -V. Harre and Gy. M. Szabó},
year={2023},
eprint={2311.04647},
archivePrefix={arXiv},
primaryClass={astro-ph.EP}
}

@misc{singh2023cheops,
title={CHEOPS observations of KELT-20 b/MASCARA-2 b: an aligned orbit and signs of variability from a reflective dayside},
author={V. Singh and G. Scandariato and A. M. S. Smith and P. E. Cubillos and M. Lendl and N. Billot and A. Fortier and D. Queloz and S. G. Sousa and Sz. Csizmadia and A. Brandeker and L. Carone and T. G. Wilson and B. Akinsanmi and J. A. Patel and A. Krenn and O. D. S. Demangeon and G. Bruno and I. Pagano and M. J. Hooton and J. Cabrera and N. C. Santos and Y. Alibert and R. Alonso and J. Asquier and T. Bárczy and D. Barrado Navascues and S. C. C. Barros and W. Baumjohann and M. Beck and T. Beck and W. Benz and M. Bergomi and A. Bonfanti and X. Bonfils and L. Borsato and C. Broeg and S. Charnoz and A. Collier Cameron and M. B. Davies and M. Deleuil and A. Deline and L. Delrez and B. -O. Demory and D. Ehrenreich and A. Erikson and L. Fossati and M. Fridlund and D. Gandolfi and M. Gillon and M. Güdel and M. N. Günther and J. -V. Harre and A. Heitzmann and Ch. Helling and S. Hoyer and K. G. Isaak and L. L. Kiss and K. W. F. Lam and J. Laskar and A. Lecavelier des Etangs and D. Magrin and P. F. L. Maxted and H. Mischler and C. Mordasini and V. Nascimbeni and G. Olofsson and R. Ottensamer and E. Pallé and G. Peter and G. Piotto and D. Pollacco and R. Ragazzoni and N. Rando and H. Rauer and I. Ribas and S. Salmon and D. Ségransan and A. E. Simon and M. Stalport and M. Steinberger and Gy. M. Szabó and N. Thomas and S. Udry and B. Ulmer and V. Van Grootel and J. Venturini and E. Villaver and N. A. Walton and T. Zingales},
year={2023},
eprint={2311.03264},
archivePrefix={arXiv},
primaryClass={astro-ph.EP}
}

@article{Rengel_2023,
doi = {10.3389/fspas.2023.1176740},

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

year = 2023,
month = {may},

publisher = {Frontiers Media {SA}
},

volume = {10},

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

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

journal = {Frontiers in Astronomy and Space Sciences}
}

@misc{krieger2023improving,
title={Improving Monte Carlo radiative transfer simulations: A shift of framework},
author={Anton Krieger and Sebastian Wolf},
year={2023},
eprint={2310.18429},
archivePrefix={arXiv},
primaryClass={astro-ph.IM}
}

@misc{osborne2023toi544,
title={TOI-544 b: a potential water-world inside the radius valley in a two-planet system},
author={H. L. M. Osborne and V. Van Eylen and E. Goffo and D. Gandolfi and G. Nowak and C. M. Persson and J. Livingston and A. Weeks and E. Pallé and R. Luque and C. Hellier and I. Carleo and S. Redfield and T. Hirano and M. Garbaccio Gili and J. Alarcon and O. Barragán and N. Casasayas-Barris and M. R. Díaz and M. Esposito and J. S. Jenkins and E. Knudstrup and F. Murgas and J. Orell-Miquel and F. Rodler and L. Serrano and M. Stangret and S. H. Albrecht and A. Alqasim and W. D. Cochran and H. J. Deeg and M. Fridlund and A. Hatzes and J. Korth and K. W. F. Lam},
year={2023},
eprint={2310.14908},
archivePrefix={arXiv},
primaryClass={astro-ph.EP}
}

@misc{nagel2023carmenes,
title={The CARMENES search for exoplanets around M dwarfs. Telluric absorption corrected high S/N optical and near-infrared template spectra of 382 M dwarf stars},
author={E. Nagel and S. Czesla and A. Kaminski and M. Zechmeister and L. Tal-Or and J. H. M. M. Schmitt and A. Reiners and A. Quirrenbach and A. García López and J. A. Caballero and I. Ribas and P. J. Amado and V. J. S. Béjar and M. Cortés-Contreras and S. Dreizler and A. P. Hatzes and Th. Henning and S. V. Jeffers and M. Kürster and M. Lafarga and M. López-Puertas and D. Montes and J. C. Morales and S. Pedraz and A. Schweitzer},
year={2023},
eprint={2310.14715},
archivePrefix={arXiv},
primaryClass={astro-ph.SR}
}

@misc{alonso2023random,
title={No random transits in CHEOPS observations of HD 139139},
author={R. Alonso and S. Hoyer and M. Deleuil and A. E. Simon and M. Beck and W. Benz and H. -G. Florén and P. Guterman and L. Borsato and A. Brandeker and D. Gandolfi and T. G. Wilson and T. Zingales and Y. Alibert and G. Anglada and T. Bárczy and D. Barrado Navascues and S. C. C. Barros and W. Baumjohann and T. Beck and N. Billot and X. Bonfils and Ch. Broeg and S. Charnoz and A. Collier Cameron and C. Corral van Damme and Sz. and Csizmadia and P. E. Cubillos and M. B. Davies and A. Deline and L. Delrez and O. D. S. Demangeon and B. -O. Demory and D- Ehrenreich and A. Erikson and A. Fortier and L. Fossati and M. Fridlund and M. Gillon and M. Güdel and M. N. Günther and A. Heitzmann and Ch. Helling and K. G. Isaak and L. L. Kiss and E. Kopp and K. W. F. Lam and J. Laskar and A. Lecavelier des Etangs and M. Lendl and D. Magrin and P. F. L. Maxted and Ch. Mordasini and V. Nascimbeni and G. Olofsson and R. Ottensamer and I. Pagano and E. Pallé and G. Peter and G. Piotto and D. Pollacco and D. Queloz and R. Ragazzoni and N. Rando and H. Rauer and I. Ribas and N. C. Santos and G. Scandariato and D. Ségransan and A. M. S. Smith and S. G. Sousa and M. Stalport and Gy. M. Szabó and N. Thomas and S. Udry and B. Ulmer and V. Van grootel and J. Venturini and F. Verrecchia and N. A. Walton},
year={2023},
eprint={2310.10332},
archivePrefix={arXiv},
primaryClass={astro-ph.EP}
}

@misc{pfeil2023dust,
title={Dust Coagulation Reconciles Protoplanetary Disk Observations with the Vertical Shear Instability -- Part I: Dust Coagulation and the VSI Dead Zone},
author={Thomas Pfeil and Til Birnstiel and Hubert Klahr},
year={2023},
eprint={2310.07332},
archivePrefix={arXiv},
primaryClass={astro-ph.EP}
}

@misc{blunt2023vltigravity,
title={First VLTI/GRAVITY Observations of HIP 65426 b: Evidence for a Low or Moderate Orbital Eccentricity},
author={S. Blunt and W. O. Balmer and J. J. Wang and S. Lacour and S. Petrus and G. Bourdarot and J. Kammerer and N. Pourré and E. Rickman and J. Shangguan and T. Winterhalder and R. Abuter and A. Amorim and R. Asensio-Torres and M. Benisty and J. -P. Berger and H. Beust and A. Boccaletti and A. Bohn and M. Bonnefoy and H. Bonnet and W. Brandner and F. Cantalloube and P. Caselli and B. Charnay and G. Chauvin and A. Chavez and E. Choquet and V. Christiaens and Y. Clénet and V. Coudé du Foresto and A. Cridland and R. Dembet and A. Drescher and G. Duvert and A. Eckart and F. Eisenhauer and H. Feuchtgruber and P. Garcia and R. Garcia Lopez and E. Gendron and R. Genzel and S. Gillessen and J. H. Girard and X. Haubois and G. Heißel and Th. Henning and S. Hinkley and S. Hippler and M. Horrobin and M. Houllé and Z. Hubert and L. Jocou and M. Keppler and P. Kervella and L. Kreidberg and A. -M. Lagrange and V. Lapeyrère and J. -B. Le Bouquin and P. Léna and D. Lutz and A. -L. Maire and F. Mang and G. -D. Marleau and A. Mérand and P. Mollière and J. D. Monnier and C. Mordasini and D. Mouillet and E. Nasedkin and M. Nowak and T. Ott and G. P. P. L. Otten and C. Paladini and T. Paumard and K. Perraut and G. Perrin and O. Pfuhl and L. Pueyo and J. Rameau and L. Rodet and Z. Rustamkulov and T. Shimizu and D. Sing and T. Stolker and C. Straubmeier and E. Sturm and L. J. Tacconi and E. F. van Dishoeck and A. Vigan and F. Vincent and K. Ward-Duong and F. Widmann and E. Wieprecht and E. Wiezorrek and J. Woillez and S. Yazici and A. Young},
year={2023},
eprint={2310.00148},
archivePrefix={arXiv},
primaryClass={astro-ph.EP}
}

@misc{danti2023composition,
title={Composition of giant planets: the roles of pebbles and planetesimals},
author={Claudia Danti and Bertram Bitsch and Jingyi Mah},
year={2023},
eprint={2310.02886},
archivePrefix={arXiv},
primaryClass={astro-ph.EP}
}

@misc{betti2023comprehensive,
title={The Comprehensive Archive of Substellar and Planetary Accretion Rates},
author={S. K. Betti and K. B. Follette and K. Ward-Duong and A. E. Peck and Y. Aoyama and J. Bary and B. Dacus and S. Edwards and G. -D. Marleau and K. Mohamed and J. Palmo and C. Plunkett and C. Robinson and H. Wang},
year={2023},
eprint={2310.00072},
archivePrefix={arXiv},
primaryClass={astro-ph.SR}
}

@misc{abrams2023microlensing,
title={Microlensing Discovery and Characterization Efficiency in the Vera C. Rubin Legacy Survey of Space and Time},
author={Natasha S. Abrams and Markus P. G. Hundertmark and Somayeh Khakpash and Rachel A. Street and R. Lynne Jones and Jessica R. Lu and Etienne Bachelet and Yiannis Tsapras and Marc Moniez and Tristan Blaineauu and Rosanne Di Stefano and Martin Makler and Anibal Varela and Markus Rabus},
year={2023},
eprint={2309.15310},
archivePrefix={arXiv},
primaryClass={astro-ph.IM}
}

@misc{jeffers2023stellar,
title={Stellar Activity Cycles},
author={Sandra V. Jeffers and Rene Kiefer and Travis S. Metcalfe},
year={2023},
eprint={2309.14138},
archivePrefix={arXiv},
primaryClass={astro-ph.SR}
}

@misc{pagano2023constraining,
title={Constraining the reflective properties of WASP-178b using Cheops photometry},
author={I. Pagano and G. Scandariato and V. Singh and M. Lendl and D. Queloz and A. E. Simon and S. G. Sousa and A. Brandeker and A. Collier Cameron and S. Sulis and V. Van Grootel and T. G. Wilson and Y. Alibert and R. Alonso and G. Anglada and T. Bárczy and D. Barrado Navascues and S. C. C. Barros and W. Baumjohann and M. Beck and T. Beck and W. Benz and N. Billot and X. Bonfils and L. Borsato and C. Broeg and G. Bruno and L. Carone and S. Charnoz and C. Corral van Damme and Sz. Csizmadia and P. E. Cubillos and M. B. Davies and M. Deleuil and A. Deline and L. Delrez and O. D. S. Demangeon and B. -O. Demory and D. Ehrenreich and A. Erikson and A. Fortier and L. Fossati and M. Fridlund and D. Gandolfi and M. Gillon and M. Güdel and M. N. Günther and Ch. Helling and S. Hoyer and K. G. Isaak and L. L. Kiss and E. Kopp and K. W. F. Lam and J. Laskar and A. Lecavelier des Etangs and D. Magrin and P. F. L. Maxted and C. Mordasini and M. Munari and V. Nascimbeni and G. Olofsson and R. Ottensamer and E. Pallé and G. Peter and G. Piotto and D. Pollacco and R. Ragazzoni and N. Rando and H. Rauer and C. Reimers and I. Ribas and M. Rieder and N. C. Santos and D. Ségransan and A. M. S. Smith and M. Stalport and M. Steller and Gy. M. Szabó and N. Thomas and S. Udry and J. Venturini and N. A. Walton},
year={2023},
eprint={2309.09037},
archivePrefix={arXiv},
primaryClass={astro-ph.EP}
}

@misc{dotti2023dynamical,
title={The dynamical evolution of protoplanetary disks and planets in dense star clusters},
author={Francesco Flammini Dotti and Roberto Capuzzo-Dolcetta and M. B. N. Kouwenhoven},
year={2023},
eprint={2309.06812},
archivePrefix={arXiv},
primaryClass={astro-ph.EP}
}

@misc{dotti2023dynamical,
title={The dynamical evolution of protoplanetary disks and planets in dense star clusters},
author={Francesco Flammini Dotti and Roberto Capuzzo-Dolcetta and M. B. N. Kouwenhoven},
year={2023},
eprint={2309.06812},
archivePrefix={arXiv},
primaryClass={astro-ph.EP}
}

@misc{maskoliūnas2023lens,
title={Lens mass estimate in the Galactic disk extreme parallax microlensing event Gaia19dke},
author={M. Maskoliūnas and Ł. Wyrzykowski and K. Howil and K. A. Rybicki and P. Zieliński and Z. Kaczmarek and K. Kruszyńska and M. Jabłońska and J. Zdanavičius and E. Pakštienė and V. Čepas and P. J. Mikołajczyk and R. Janulis and M. Gromadzki and N. Ihanec and R. Adomavičienė and K. Šiškauskaitė and M. Bronikowski and P. Sivak and A. Stankevičiūtė and M. Sitek and M. Ratajczak and U. Pylypenko and I. Gezer and S. Awiphan and E. Bachelet and K. Bąkowska and R. P. Boyle and V. Bozza and S. M. Brincat and U. Burgaz and T. Butterley and J. M. Carrasco and A. Cassan and F. Cusano and G. Damljanovic and J. W. Davidson and V. S. Dhillon and M. Dominik and F. Dubois and H. H. Esenoglu and R. Figuera Jaimes and A. Fukui and C. Galdies and A. Garofalo and V. Godunova and T. Güver and J. Heidt and M. Hundertmark and I. Izviekova and B. Joachimczyk and M. K. Kamińska and K. Kamiński and S. Kaptan and T. Kvernadze and O. Kvaratskhelia and S. Littlefair and O. Michniewicz and N. Nakhatutai and W. Ogłoza and R. Ohsawa and J. M. Olszewska and M. Polińska and A. Popowicz and J. K. T. Qvam and M. Radziwonowicz and D. E. Reichart and A. Słowikowska and A. Simon and E. Sonbas and M. Stojanovic and Y. Tsapras and S. Vanaverbeke and J. Wambsganss and R. W. Wilson and M. Żejmo and S. Zola},
year={2023},
eprint={2309.03324},
archivePrefix={arXiv},
primaryClass={astro-ph.SR}
}

@misc{bitsch2023enriching,
title={Enriching inner discs and giant planets with heavy elements},
author={Bertram Bitsch and Jingyi Mah},
year={2023},
eprint={2309.00509},
archivePrefix={arXiv},
primaryClass={astro-ph.EP}
}

@misc{mah2023closein,
title={Close-in ice lines and the super-stellar C/O ratio in discs around very low-mass stars},
author={J. Mah and B. Bitsch and I. Pascucci and T. Henning},
year={2023},
eprint={2308.15128},
archivePrefix={arXiv},
primaryClass={astro-ph.EP}
}

@article{Wunderlich2023,
author = {Wunderlich, Fabian and Grenfell, John Lee and Rauer, Heike},
year = {2023},
language = {eng},
copyright = {https://creativecommons.org/licenses/by/4.0/},
title = {Uncertainty in phosphine photochemistry in the Venus atmosphere prevents a firm biosignature attribution},
volume = {676},
url = "http://dx.doi.org/10.17169/refubium-40848",
}

@article{Sterken_2023,
doi = {10.1093/rasti/rzad034},

url = {https://doi.org/10.1093%2Frasti%2Frzad034},

year = 2023,
month = {aug},

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

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},

title = {Synergies between interstellar dust and heliospheric science with an Interstellar Probe},

journal = {{RAS} Techniques and Instruments}
}

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

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

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

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

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

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

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

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

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

year = 2023,
month = {jul},

publisher = {American Astronomical Society},

volume = {952},

number = {1},

pages = {89},

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

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

journal = {The Astrophysical Journal}
}

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

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

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

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

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

year = 2023,
month = {jun},

publisher = {{EDP} Sciences},

volume = {674},

pages = {A164},

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

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

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

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

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

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

year = 2023,
month = {jul},

publisher = {{EDP} Sciences},

volume = {675},

pages = {A122},

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

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

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

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

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

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

year = 2023,
month = {jun},

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

volume = {523},

number = {4},

pages = {4801--4817},

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

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

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

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

@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}
}

@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}
}

@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}
}

@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}
}

@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}
}

@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}
}

@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}
}

@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}
}

@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}
}

@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}
}

@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}
}

@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}
}

@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}
}

@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}
}

@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}
}

@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},

volume = {670},

pages = {A84},

author = {D. Kossakowski and M. Kürster and T. Trifonov and Th. Henning and J. Kemmer and J. A. Caballero and R. Burn and S. Sabotta and J. S. Crouse and T. J. Fauchez and E. Nagel and A. Kaminski and E. Herrero and E. Rodr{\'{\i}
}guez and E. Gonz{\'{a}}lez-{\'{A}}lvarez and A. Quirrenbach and P. J. Amado and I. Ribas and A. Reiners and J. Aceituno and V. J. S. B{\'{e}}jar and D. Baroch and S. T. Bastelberger and P. Chaturvedi and C. Cifuentes and S. Dreizler and S. V. Jeffers and R. Kopparapu and M. Lafarga and M. J. L{\'{o}}pez-Gonz{\'{a}}lez and S. Mart{\'{\i}}n-Ruiz and D. Montes and J. C. Morales and E. Pall{\'{e}} and A. Pavlov and S. Pedraz and V. Perdelwitz and M. P{\'{e}}rez-Torres and M. Perger and S. Reffert and C. Rodr{\'{\i}}guez L{\'{o}}pez and M. Schlecker and P. Schöfer and A. Schweitzer and Y. Shan and A. Shields and S. Stock and E. Wolf and M. R. Zapatero Osorio and M. Zechmeister},

title = {The {CARMENES} search for exoplanets around M dwarfs},

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

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

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

year = 2023,
month = {feb},

publisher = {{EDP} Sciences},

author = {E. Knudstrup and S. H. Albrecht and D. Gandolfi and M. L. Marcussen and E. Goffo and L. M. Serrano and F. Dai and S. Redfield and T. Hirano and Sz. Csizmadia and H. J. Deeg and M. Fridlund and K. W. F. Lam and J. H. Livingston and R. Luque and N. Narita and E. Palle and C. M. Persson and V. Van Eylen},

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

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

@misc{https://doi.org/10.48550/arxiv.2302.00699,
doi = {10.48550/ARXIV.2302.00699},

url = {https://arxiv.org/abs/2302.00699},

author = {Hirano, Teruyuki and Dai, Fei and Livingston, John H. and Kasagi, Yui and Narita, Norio and Ishikawa, Hiroyuki Tako and Grziwa, Sascha and Lam, Kristine W. F. and Miyakawa, Kohei and Serrano, Luisa M. and Matsumoto, Yuji and Kokubo, Eiichiro and Kimura, Tadahiro and Ikoma, Masahiro and Winn, Joshua N. and Wisniewski, John P. and Harakawa, Hiroki and Teng, Huan-Yu and Cochran, William D. and Fukui, Akihiko and Gandolfi, Davide and Guenther, Eike W. and Hori, Yasunori and Ikuta, Kai and Kawauchi, Kiyoe and Knudstrup, Emil and Korth, Judith and Kotani, Takayuki and Krishnamurthy, Vigneshwaran and Kudo, Tomoyuki and Kurokawa, Takashi and Kuzuhara, Masayuki and Luque, Rafael and Mori, Mayuko and Nishikawa, Jun and Omiya, Masashi and Orell-Miquel, Jaume and Palle, Enric and Persson, Carina M. and Redfield, Seth and Serabyn, Eugene and Smith, Alexis M. S. and Takahashi, Aoi and Takarada, Takuya and Ueda, Akitoshi and Van Eylen, Vincent and Vievard, Sebastien and Tamura, Motohide and Sato, Bun'ei},

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

title = {An Earth-sized Planet around an M5 Dwarf Star at 22 pc},

publisher = {arXiv},

year = {2023},

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

@misc{https://doi.org/10.48550/arxiv.2302.00056,
doi = {10.48550/ARXIV.2302.00056},

url = {https://arxiv.org/abs/2302.00056},

author = {Marvin, C. J. and Reiners, A. and Anglada-Escudé, G. and Jeffers, S. V. and Saikia, S. Boro},

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

title = {Absolute Ca II H & K and H-alpha flux measurements of low-mass stars: Extending $R'_\mathrm{HK}$ to M dwarfs},

publisher = {arXiv},

year = {2023},

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

@article{Petrus_2023,
doi = {10.1051/0004-6361/202244494},

url = {https://doi.org/10.1051%2F0004-6361%2F202244494},

year = 2023,
month = {jan},

publisher = {{EDP} Sciences},

volume = {670},

pages = {L9},

author = {S. Petrus and G. Chauvin and M. Bonnefoy and P. Tremblin and B. Charnay and P. Delorme and G.-D. Marleau and A. Bayo and E. Manjavacas and A.-M. Lagrange and P. Molli{\`{e}
}re and P. Palma-Bifani and B. Biller and J.-S. Jenkins and J.-M. Goyal and K. Hoch},

title = {X-{SHYNE}: X-shooter spectra of young exoplanet analogs},

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

@misc{https://doi.org/10.48550/arxiv.2301.12872,
doi = {10.48550/ARXIV.2301.12872},

url = {https://arxiv.org/abs/2301.12872},

author = {Perger, M. and Anglada-Escudé, G. and Baroch, D. and Lafarga, M. and Ribas, I. and Morales, J. C. and Herrero, E. and Amado, P. J. and Barnes, J. R. and Caballero, J. A. and Jeffers, S. V. and Quirrenbach, A. and Reiners, A.},

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

title = {A Machine Learning approach for correcting radial velocities using physical observables},

publisher = {arXiv},

year = {2023},

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

@article{Papaioannou_2023,
doi = {10.1051/0004-6361/202243407},

url = {https://doi.org/10.1051%2F0004-6361%2F202243407},

year = 2023,
month = {mar},

publisher = {{EDP} Sciences},

volume = {671},

pages = {A66},

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

title = {Revisiting empirical solar energetic particle scaling relations},

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

@misc{https://doi.org/10.48550/arxiv.2301.06873,
doi = {10.48550/ARXIV.2301.06873},

url = {https://arxiv.org/abs/2301.06873},

author = {Palle, E. and Orell-Miquel, J. and Brady, M. and Bean, J. and Hatzes, A. P. and Morello, G. and Morales, J. C. and Murgas, F. and Molaverdikhani, K. and Parviainen, H. and Sanz-Forcada, J. and Béjar, V. J. S. and Caballero, J. A. and Sreenivas, K. R. and Schlecker, M. and Ribas, I. and Perdelwitz, V. and Tal-Or, L. and Pérez-Torres, M. and Luque, R. and Dreizler, S. and Fuhrmeister, B. and Aceituno, F. and Amado, P. J. and Anglada-Escudé, G. and Caldwell, D. A. and Charbonneau, D. and Cifuentes, C. and de Leon, J. P. and Collins, K. A. and Dufoer, S. and Espinoza, N. and Essack, Z. and Fukui, A. and Chew, Y. Gómez Maqueo and Gómez-Muñoz, M. A. and Henning, Th. and Herrero, E. and Jeffers, S. V. and Jenkins, J. and Kaminski, A. and Kasper, J. and Kunimoto, M. and Latham, D. and Lillo-Box, J. and López-González, M. J. and Montes, D. and Mori, M. and Narita, N. and Quirrenbach, A. and Pedraz, S. and Reiners, A. and Rodríguez, E. and Rodríguez-López, C. and Sabin, L. and Schanche, N. and Schwarz, R-P. and Schweitzer, A. and Seifahrt, A. and Stefansson, G. and Sturmer, J. and Trifonov, T. and Vanaverbeke, S. and Wells, R. D. and Zapatero-Osorio, M. R. and Zechmeister, M.},

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

title = {GJ 806 (TOI-4481): A bright nearby multi-planetary system with a transiting hot, low-density super-Earth},

publisher = {arXiv},

year = {2023},

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

@misc{https://doi.org/10.48550/arxiv.2301.05034,
doi = {10.48550/ARXIV.2301.05034},

url = {https://arxiv.org/abs/2301.05034},

author = {Cabral, N. and Guilbert-Lepoutre, A. and Bitsch, B. and Lagarde, N. and Diakite, S.},

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

title = {How the origin of stars in the Galaxy impacts the composition of planetary building blocks},

publisher = {arXiv},

year = {2023},

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

@misc{blancopozo2023carmenes,
title={The CARMENES search for exoplanets around M dwarfs. A long-period planet around GJ 1151 measured with CARMENES and HARPS-N data},
author={J. Blanco-Pozo and M. Perger and M. Damasso and G. Anglada Escudé and I. Ribas and D. Baroch and J. A. Caballero and C. Cifuentes and S. V. Jeffers and M. Lafarga and A. Kaminski and S. Kaur and E. Nagel and V. Perdelwitz and M. Pérez-Torres and A. Sozzetti and D. Viganò and P. J. Amado and G. Andreuzzi and E. L. Brown and F. Del Sordo and S. Dreizler and D. Galadí-Enríquez and A. P. Hatzes and M. Kürster and A. F. Lanza and A. Melis and E. Molinari and D. Montes and M. Murgia and E. Pallé and L. Peña-Moñino and D. Perrodin and M. Pilia and E. Poretti and A. Quirrenbach and A. Reiners and A. Schweitzer and M. R. Zapatero Osorio and M. Zechmeister},
year={2023},
eprint={2301.04442},
archivePrefix={arXiv},
primaryClass={astro-ph.EP}
}

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

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

year = 2023,
month = {jan},

publisher = {{EDP} Sciences},

author = {D. Kossakowski and M. Kürster and T. Trifonov and Th. Henning and J. Kemmer and J. A. Caballero and R. Burn and S. Sabotta and J. S. Crouse and T. J. Fauchez and E. Nagel and A. Kaminski and E. Herrero and E. Rodr{\'{\i}
}guez and E. Gonz{\'{a}}lez-{\'{A}}lvarez and A. Quirrenbach and P. J. Amado and I. Ribas and et al},

title = {The {CARMENES} search for exoplanets around M dwarfs. Wolf 1069 b: Earth-mass planet in the habitable zone of a nearby, very low-mass starr},

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

@misc{https://doi.org/10.48550/arxiv.2212.09401,
doi = {10.48550/ARXIV.2212.09401},

url = {https://arxiv.org/abs/2212.09401},

author = {Böning, Vincent G. A. and Wulff, Paula and Dietrich, Wieland and Wicht, Johannes and Christensen, Ulrich R.},

keywords = {Earth and Planetary Astrophysics (astro-ph.EP), Solar and Stellar Astrophysics (astro-ph.SR), Chaotic Dynamics (nlin.CD), Fluid Dynamics (physics.flu-dyn), Geophysics (physics.geo-ph), FOS: Physical sciences, FOS: Physical sciences},

title = {Direct driving of simulated planetary jets by upscale energy transfer},

publisher = {arXiv},

year = {2022},

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

@article{Flores_Rivera_2023,
doi = {10.1051/0004-6361/202141664},

url = {https://doi.org/10.1051%2F0004-6361%2F202141664},

year = 2023,
month = {jan},

publisher = {{EDP} Sciences},

author = {L. Flores-Rivera and M. Flock and N. Kurtovic and B. Husemann and A. Banzatti and S. C. Ringqvist and},

title = {Forbidden emission lines in protostellar outflows and jets with {MUSE}
},

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

@article{Ringqvist_2023,
doi = {10.1051/0004-6361/202245424},

url = {https://doi.org/10.1051%2F0004-6361%2F202245424},

year = 2023,
month = {jan},

publisher = {{EDP} Sciences},

volume = {669},

pages = {L12},

author = {Simon C. Ringqvist and Gayathri Viswanath and Yuhiko Aoyama and Markus Janson and Gabriel-Dominique Marleau and Alexis Brandeker},

title = {Resolved near-{UV} hydrogen emission lines at 40-Myr super-Jovian protoplanet Delorme 1 ({AB})b},

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

@article{Lam_2022,
doi = {10.1093/mnras/stac3639},

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

year = 2022,
month = {dec},

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

author = {Kristine 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 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}
}

@article{Lam_2022,
doi = {10.1093/mnras/stac3639},

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}
}

@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}
}

@article{Marleau_2022,
doi = {10.3847/2515-5172/acaa34},
url = {https://dx.doi.org/10.3847/2515-5172/acaa34},
year = {2022},
month = {dec},
publisher = {The American Astronomical Society},
volume = {6},
number = {12},
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.}
}

@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}
}

@misc{https://doi.org/10.48550/arxiv.2211.15312,
doi = {10.48550/ARXIV.2211.15312},

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}
}

@article{Zakhozhay_2022,
doi = {10.1051/0004-6361/202244747},

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

year = 2022,
month = {nov},

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}
} I. Vin{\'{e}}s and Gabriel-Dominique Marleau and Jayshil A. Patel},

title = {Radial velocity survey for planets around young stars ({RVSPY})},

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

@misc{https://doi.org/10.48550/arxiv.2211.05646,
doi = {10.48550/ARXIV.2211.05646},

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

author = {Harre, J. -V. and Smith, A. M. S. and Barros, S. C. C. and Boué, G. and Csizmadia, Sz. and Ehrenreich, D. and Florén, H. -G. and Fortier, A. and Maxted, P. F. L. and Hooton, M. J. and Akinsanmi, B. and Serrano, L. M. and Rosário, N. M. and Demory, B. -O. and Jones, K. and Laskar, J. and Adibekyan, V. and Alibert, Y. and Alonso, R. and Anderson, D. R. and Anglada, G. and Asquier, J. and Bárczy, T. and Navascues, D. Barrado y and Baumjohann, W. and Beck, M. and Beck, T. and Benz, W. and Billot, N. and Biondi, F. and Bonfanti, A. and Bonfils, X. and Brandeker, A. and Broeg, C. and Cabrera, J. and Cessa, V. and Charnoz, S. and Cameron, A. Collier and Davies, M. B. and Deleuil, M. and Delrez, L. and Demangeon, O. D. S. and Erikson, A. and Fossati, L. and Fridlund, M. and Gandolfi, D. and Gillon, M. and Güdel, M. and Hellier, C. and Heng, K. and Hoyer, S. and Isaak, K. G. and Kiss, L. L. and Etangs, A. Lecavelier des and Lendl, M. and Lovis, C. and Luntzer, A. and Magrin, D. and Nascimbeni, V. and Olofsson, G. and Ottensamer, R. and Pagano, I. and Pallé, E. and Persson, C. M. and Peter, G. and Piotto, G. and Pollacco, D. and Queloz, D. and Ragazzoni, R. and Rando, N. and Rauer, H. and Ribas, I. and Ricker, G. R. and Salmon, S. and Santos, N. C. and Scandariato, G. and Seager, S. and Ségransan, D. and Simon, A. E. and Sousa, S. G. and Steller, M. and Szabó, Gy. M. and Thomas, N. and Udry, S. and Ulmer, B. and Van Grootel, V. and Walton, N. A. and Wilson, T. G. and Winn, J. N. and Wohler, B.},

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}
}

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

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

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

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

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

publisher = {arXiv},

year = {2022},

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

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

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

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

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

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

publisher = {arXiv},

year = {2022},

copyright = {Creative Commons Attribution 4.0 International}
}

@article{Orell_Miquel_2023,
doi = {10.1051/0004-6361/202244120},

url = {https://doi.org/10.1051%2F0004-6361%2F202244120},

year = 2023,
month = {jan},

publisher = {{EDP} Sciences},

volume = {669},

pages = {A40},

author = {J. Orell-Miquel and G. Nowak and F. Murgas and E. Palle and G. Morello and R. Luque and M. Badenas-Agusti and I. Ribas and M. Lafarga and N. Espinoza and J. C. Morales and M. Zechmeister and A. Alqasim and W. D. Cochran and D. Gandolfi and E. Goffo and P. Kab{\'{a}
}th and J. Korth and K. W. F. Lam and J. Livingston and A. Muresan and C. M. Persson and V. Van Eylen},

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

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

@article{Persson_2022,
doi = {10.1051/0004-6361/202244118},

url = {https://doi.org/10.1051%2F0004-6361%2F202244118},

year = 2022,
month = {oct},

publisher = {{EDP} Sciences},

volume = {666},

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}
}

@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}
}

@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},
}

@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}
}

@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}
}

@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}
}

@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}
}

@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}
}

@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}
}

@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}
}

@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},
}

@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}
}

@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}
}

@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}
}

@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},
}

@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}
}az and X. Bonfils and S. V. Jeffers and J. R. Barnes and F. Del Sordo and J.-M. Almenara and E. Artigau and F. Bouchy and D. Charbonneau and X. Delfosse and R. Doyon and P. Figueira and T. Forveille and C. A. Haswell and M. J. L{\'{o}}pez-Gonz{\'{a}}lez and C. Melo and R. E. Mennickent and G. Gaisn{\'{e}} and N. Morales Morales and F. Murgas and F. Pepe and E. Rodr{\'{\i}}guez and N. C. Santos and L. Tal-Or and Y. Tsapras and S. Udry},

title = {Detailed stellar activity analysis and modelling of {GJ} 832},

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

@misc{https://doi.org/10.48550/arxiv.2208.04867,
doi = {10.48550/ARXIV.2208.04867},

url = {https://arxiv.org/abs/2208.04867},

author = {Hinkley, S. and Lacour, S. and Marleau, G. -D. and Lagrange, A. M. and Wang, J. J. and Kammerer, J. and Cumming, A. and Nowak, M. and Rodet, L. and Stolker, T. and Balmer, W. -O. and Ray, S. and Bonnefoy, M. and Mollière, P. and Lazzoni, C. and Kennedy, G. and Mordasini, C. and Abuter, R. and Aigrain, S. and Amorim, A. and Asensio-Torres, R. and Babusiaux, C. and Benisty, M. and Berger, J. -P. and Beust, H. and Blunt, S. and Boccaletti, A. and Bohn, A. and Bonnet, H. and Bourdarot, G. and Brandner, W. and Cantalloube, F. and Caselli, P. and Charnay, B. and Chauvin, G. and Chomez, A. and Choquet, E. and Christiaens, V. and Clénet, Y. and Foresto, V. Coudé du and Cridland, A. and Delorme, P. and Dembet, R. and de Zeeuw, P. T. and Drescher, A. and Duvert, G. and Eckart, A. and Eisenhauer, F. and Feuchtgruber, H. and Galland, F. and Garcia, P. and Lopez, R. Garcia and Gardner, T. and Gendron, E. and Genzel, R. and Gillessen, S. and Girard, J. H. and Grandjean, A. and Haubois, X. and Heißel, G. and Henning, Th. and Hippler, S. and Horrobin, M. and Houllé, M. and Hubert, Z. and Jocou, L. and Keppler, M. and Kervella, P. and Kreidberg, L. and Lapeyrère, V. and Bouquin, J. -B. Le and Léna, P. and Lutz, D. and Maire, A. -L. and Mang, F. and Mérand, A. and Meunier, N. and Monnier, J. D. and Mordasini, C. and Mouillet, D. and Nasedkin, E. and Ott, T. and Otten, G. P. P. L. and Paladini, C. and Paumard, T. and Perraut, K. and Perrin, G. and Philipot, F. and Pfuhl, O. and Pourré, N. and Pueyo, L. and Rameau, J. and Rickman, E. and Rubini, P. and Rustamkulov, Z. and Samland, M. and Shangguan, J. and Shimizu, T. and Sing, D. and Straubmeier, C. and Sturm, E. and Tacconi, L. J. and van Dishoeck, E. F. and Vigan, A. and Vincent, F. and Ward-Duong, K. and Widmann, F. and Wieprecht, E. and Wiezorrek, E. and Woillez, J. and Yazici, S. and Young, A. and Zicher, N. and Collaboration, the GRAVITY},

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}
}

@article{Squicciarini_2022,
doi = {10.1051/0004-6361/202243675},

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},

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

@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}
}

@article{Tayar_2022,
doi = {10.3847/1538-4357/ac9312},

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}
}

@article{Bachelet_2022,
doi = {10.3847/1538-3881/ac78ed},

url = {https://doi.org/10.3847%2F1538-3881%2Fac78ed},

year = 2022,
month = {aug},

publisher = {American Astronomical Society},

volume = {164},

number = {3},

pages = {75},

author = {E. Bachelet and Y. Tsapras and Andrew Gould and R. A. Street and David P. Bennett and M. P. G. Hundertmark and V. Bozza and D. M. Bramich and A. Cassan and M. Dominik and K. Horne and S. Mao and A. Saha and J. Wambsganss and Weicheng Zang and Fumio Abe and Richard Barry and David P. Bennett and Aparna Bhattacharya and Ian A. Bond and Akihiko Fukui and Hirosane Fujii and Yuki Hirao and Yoshitaka Itow and Rintaro Kirikawa and Iona Kondo and Naoki Koshimoto and Yutaka Matsubara and Sho Matsumoto and Shota Miyazaki and Yasushi Muraki and Greg Olmschenk and Cl{\'{e}
}ment Ranc and Arisa Okamura and Nicholas J. Rattenbury and Yuki Satoh and Takahiro Sumi and Daisuke Suzuki and Stela Ishitani Silva and Taiga Toda and Paul . J. Tristram and Aikaterini Vandorou and Hibiki Yama 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 Yossi Shvartzvald and Jennifer C. Yee and Sang-Mok Cha and Dong-Jin 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 Andrzej Udalski and Przemek Mr{\'{o}}z and Rados{\l}aw Poleski and Jan Skowron 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 Mariusz Gromadzki},

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

journal = {The Astronomical Journal}
}

@misc{kálmán2022power,
title={The power of wavelets in analysis of transit and phase curves in presence of stellar variability and instrumental noise III.

@misc{https://doi.org/10.48550/arxiv.2208.00892,
doi = {10.48550/ARXIV.2208.00892},

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}
}

@misc{https://doi.org/10.48550/arxiv.2207.06622,
doi = {10.48550/ARXIV.2207.06622},

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}
}

@article{Godoy_2022,
doi = {10.1051/0004-6361/202040024},

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}
}gransan and T. Stolker},

title = {{ISPY} {\textendash} {NaCo} Imaging Survey for Planets around Young stars},

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

@article{Jeffers_2022,
doi = {10.1051/0004-6361/202141880},

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

year = 2022,
month = {jul},

publisher = {{EDP} Sciences},

volume = {663},

pages = {A27},

author = {S. V. Jeffers and J. R. Barnes and P. Schöfer and A. Quirrenbach and M. Zechmeister and P. J. Amado and J. A. Caballero and M. Fern{\'{a}
}ndez and E. Rodr{\'{\i}}guez and I. Ribas and A. Reiners and C. Cardona Guill{\'{e}}n and C. Cifuentes and S. Czesla and A. P. Hatzes and M. Kürster and D. Montes and J. C. Morales and S. Pedraz and S. Sadegi},

title = {The {CARMENES} search for exoplanets around M dwarfs},

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

@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}
}

@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}
}

@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}
}

@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}
}

@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}
}

@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}
}

@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}
}

@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}
}

@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.}
}

@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}
}

@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}
}

@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},
}

@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},
}

@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}
}

@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},
}

@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},
}

@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.}
}

@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} }

@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.}
}

@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},
}

@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. }
}

@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},
}

@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.}
}

@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}
}
}

@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).}
}

@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}
}

@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},
}

@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}
}

@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},
}

@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}
}

@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},
}

@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},
}

@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},
}

@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}
}

@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},
}

@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}
}

@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},
}

@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}
}

@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}
}

@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}
}

@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}
}

@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}
}

@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}
}

@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},
year = 2021,
month = mar,
volume = {647},
eid = {A26},
pages = {A26},
doi = {10.1051/0004-6361/202039539},
archivePrefix = {arXiv},
eprint = {2101.04094},
primaryClass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...647A..26C},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2021MNRAS.501.3981B,
author = {{Brown}, E.~L. and {Marsden}, S.~C. and {Mengel}, M.~W. and {Jeffers}, S.~V. and {Millburn}, I. and {Mittag}, M. and {Petit}, P. and {Vidotto}, A.~A. and {Morin}, J. and {See}, V. and {Jardine}, M. and {Gonz{\'a}lez-P{\'e}rez}, J.~N. and {BCool Collaboration}},
title = "{Magnetic field and chromospheric activity evolution of HD 75332: a rapid magnetic cycle in an F star without a hot Jupiter}",
journal = {\mnras},
keywords = {stars: activity, stars: magnetic field, stars: individual (HD 75332), Astrophysics - Solar and Stellar Astrophysics},
year = 2021,
month = mar,
volume = {501},
number = {3},
pages = {3981-4003},
doi = {10.1093/mnras/staa3878},
archivePrefix = {arXiv},
eprint = {2012.05407},
primaryClass = {astro-ph.SR},
adsurl = {https://ui.adsabs.harvard.edu/abs/2021MNRAS.501.3981B},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2021arXiv210305377A,
author = {{Asensio-Torres}, R. and {Henning}, Th. and {Cantalloube}, F. and {Pinilla}, P. and {Mesa}, D. and {Garufi}, A. and {Jorquera}, S. and {Gratton}, R. and {Chauvin}, G. and {Szulagyi}, J. and {van Boekel}, R. and {Dong}, R. and {Marleau}, G. -D. and {Benisty}, M. and {Villenave}, M. and {Bergez-Casalou}, C. and {Desgrange}, C. and {Janson}, M. and {Keppler}, M. and {Langlois}, M. and {Menard}, F. and {Rickman}, E. and {Stolker}, T. and {Feldt}, M. and {Fusco}, T. and {Gluck}, L. and {Pavlov}, A. and {Ramos}, J.},
title = "{Perturbers: SPHERE detection limits to planetary-mass companions in protoplanetary disks}",
journal = {arXiv e-prints},
keywords = {Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
year = 2021,
month = mar,
eid = {arXiv:2103.05377},
pages = {arXiv:2103.05377},
archivePrefix = {arXiv},
eprint = {2103.05377},
primaryClass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2021arXiv210305377A},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2021A&A...647A..48W,
author = {{Wunderlich}, Fabian and {Scheucher}, Markus and {Grenfell}, John Lee and {Schreier}, Franz and {Sousa-Silva}, Clara and {Godolt}, Mareike and {Rauer}, Heike},
title = "{Detectability of biosignatures on LHS 1140 b}",
journal = {\aap},
keywords = {planets and satellites: terrestrial planets, planets and satellites: detection, planets and satellites: composition, planets and satellites: atmospheres, techniques: spectroscopic, astrochemistry, Astrophysics - Earth and Planetary Astrophysics, Physics - Chemical Physics},
year = 2021,
month = mar,
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pages = {A48},
doi = {10.1051/0004-6361/202039663},
archivePrefix = {arXiv},
eprint = {2012.11426},
primaryClass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...647A..48W},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2021MNRAS.tmp..893T,
author = {{Tilbrook}, Rosanna H. and {Burleigh}, Matthew R. and {Costes}, Jean C. and {Gill}, Samuel and {Nielsen}, Louise Dyregaard and {Vines}, Jos{\'e} I. and {Queloz}, Didier and {Hodgkin}, Simon T. and {Worters}, Hannah L. and {Goad}, Michael R. and {Acton}, Jack S. and {Henderson}, Beth A. and {Armstrong}, David J. and {Anderson}, David R. and {Bayliss}, Daniel and {Bouchy}, Fran{\c{c}}ois and {Briegal}, Joshua T. and {Bryant}, Edward M. and {Casewell}, Sarah L. and {Chaushev}, Alexander and {Cooke}, Benjamin F. and {Eigm{\"u}ller}, Philipp and {Gillen}, Edward and {G{\"u}nther}, Maximilian N. and {Hogan}, Aleisha and {Jenkins}, James S. and {Lendl}, Monika and {McCormac}, James and {Moyano}, Maximiliano and {Raynard}, Liam and {Smith}, Alexis M.~S. and {Udry}, St{\'e}phane and {Watson}, Christopher A. and {West}, Richard G. and {Wheatley}, Peter J. and {Breytenbach}, Hannes and {Sefako}, Ramotholo R. and {Thomas}, Jessymol K. and {Alves}, Douglas R.},
title = {{NGTS 15b, 16b, 17b and 18b: four hot Jupiters from the Next Generation Transit Survey}},
journal = {\mnras},
keywords = {planetary systems, planets and satellites: detection, planets and satellites: gaseous planets, Astrophysics - Earth and Planetary Astrophysics},
year = 2021,
month = mar,
doi = {10.1093/mnras/stab815},
archiveprefix = {arXiv},
eprint = {2103.10302},
primaryclass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2021MNRAS.tmp..893T},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2021arXiv210200939M,
author = {{Moldenhauer}, T.~W. and {Kuiper}, R. and {Kley}, W. and {Ormel}, C.~W.},
title = "{Steady State by Recycling prevents Premature Collapse of Protoplanetary Atmospheres}",
journal = {arXiv e-prints},
keywords = {Astrophysics - Earth and Planetary Astrophysics},
year = 2021,
month = feb,
eid = {arXiv:2102.00939},
pages = {arXiv:2102.00939},
archivePrefix = {arXiv},
eprint = {2102.00939},
primaryClass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2021arXiv210200939M},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2021A&A...646A.159S,
author = {{Scandariato}, G. and {Borsa}, F. and {Sicilia}, D. and {Malavolta}, L. and {Biazzo}, K. and {Bonomo}, A.~S. and {Bruno}, G. and {Claudi}, R. and {Covino}, E. and {Di Marcantonio}, P. and {Esposito}, M. and {Frustagli}, G. and {Lanza}, A.~F. and {Maldonado}, J. and {Maggio}, A. and {Mancini}, L. and {Micela}, G. and {Nardiello}, D. and {Rainer}, M. and {Singh}, V. and {Sozzetti}, A. and {Affer}, L. and {Benatti}, S. and {Bignamini}, A. and {Biliotti}, V. and {Capuzzo-Dolcetta}, R. and {Carleo}, I. and {Cosentino}, R. and {Damasso}, M. and {Desidera}, S. and {Garcia de Gurtubai}, A. and {Ghedina}, A. and {Giacobbe}, P. and {Giani}, E. and {Harutyunyan}, A. and {Hernandez}, N. and {Hernandez Diaz}, M. and {Knapic}, C. and {Leto}, G. and {Mart{\'\i}nez Fiorenzano}, A.~F. and {Molinari}, E. and {Nascimbeni}, V. and {Pagano}, I. and {Pedani}, M. and {Piotto}, G. and {Poretti}, E. and {Stoev}, H.},
title = "{The GAPS Programme at TNG. XXIX. No detection of reflected light from 51 Peg b using optical high-resolution spectroscopy}",
journal = {\aap},
keywords = {techniques: spectroscopic, planets and satellites: atmospheres, planets and satellites: detection, planets and satellites: gaseous planets, planets and satellites: individual: 51 Peg b, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
year = 2021,
month = feb,
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pages = {A159},
doi = {10.1051/0004-6361/202039271},
archivePrefix = {arXiv},
eprint = {2012.10435},
primaryClass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...646A.159S},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2021A&A...646A.164J,
author = {{Janson}, Markus and {Squicciarini}, Vito and {Delorme}, Philippe and {Gratton}, Raffaele and {Bonnefoy}, Micka{\"e}l and {Reffert}, Sabine and {Mamajek}, Eric E. and {Eriksson}, Simon C. and {Vigan}, Arthur and {Langlois}, Maud and {Engler}, Natalia and {Chauvin}, Ga{\"e}l and {Desidera}, Silvano and {Mayer}, Lucio and {Marleau}, Gabriel-Dominique and {Bohn}, Alexander J. and {Samland}, Matthias and {Meyer}, Michael and {d'Orazi}, Valentina and {Henning}, Thomas and {Quanz}, Sascha and {Kenworthy}, Matthew and {Carson}, Joseph C.},
title = "{BEAST begins: sample characteristics and survey performance of the B-star Exoplanet Abundance Study}",
journal = {\aap},
keywords = {planets and satellites: detection, stars: early-type, brown dwarfs, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
year = 2021,
month = feb,
volume = {646},
eid = {A164},
pages = {A164},
doi = {10.1051/0004-6361/202039683},
archivePrefix = {arXiv},
eprint = {2101.02043},
primaryClass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...646A.164J},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2021A&A...646A.168C,
author = {{Carone}, Ludmila and {Molli{\`e}re}, Paul and {Zhou}, Yifan and {Bouwman}, Jeroen and {Yan}, Fei and {Baeyens}, Robin and {Apai}, D{\'a}niel and {Espinoza}, Nestor and {Rackham}, Benjamin V. and {Jord{\'a}n}, Andr{\'e}s and {Angerhausen}, Daniel and {Decin}, Leen and {Lendl}, Monika and {Venot}, Olivia and {Henning}, Thomas},
title = "{Indications for very high metallicity and absence of methane in the eccentric exo-Saturn WASP-117b}",
journal = {\aap},
keywords = {methods: observational, planets and satellites: atmospheres, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
year = 2021,
month = feb,
volume = {646},
eid = {A168},
pages = {A168},
doi = {10.1051/0004-6361/202038620},
archivePrefix = {arXiv},
eprint = {2006.05382},
primaryClass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...646A.168C},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2021A&A...646A.169M,
author = {{Monsch}, Kristina and {Picogna}, Giovanni and {Ercolano}, Barbara and {Kley}, Wilhelm},
title = "{Giant planet migration during the disc dispersal phase}",
journal = {\aap},
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},
year = 2021,
month = feb,
volume = {646},
eid = {A169},
pages = {A169},
doi = {10.1051/0004-6361/202039658},
archivePrefix = {arXiv},
eprint = {2101.01179},
primaryClass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...646A.169M},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2021A&A...646A.183S,
author = {{Smith}, A.~M.~S. and {Acton}, J.~S. and {Anderson}, D.~R. and {Armstrong}, D.~J. and {Bayliss}, D. and {Belardi}, C. and {Bouchy}, F. and {Brahm}, R. and {Briegal}, J.~T. and {Bryant}, E.~M. and {Burleigh}, M.~R. and {Cabrera}, J. and {Chaushev}, A. and {Cooke}, B.~F. and {Costes}, J.~C. and {Csizmadia}, Sz. and {Eigm{\"u}ller}, Ph. and {Erikson}, A. and {Gill}, S. and {Gillen}, E. and {Goad}, M.~R. and {G{\"u}nther}, M.~N. and {Henderson}, B.~A. and {Hogan}, A. and {Jord{\'a}n}, A. and {Lendl}, M. and {McCormac}, J. and {Moyano}, M. and {Nielsen}, L.~D. and {Rauer}, H. and {Raynard}, L. and {Tilbrook}, R.~H. and {Turner}, O. and {Udry}, S. and {Vines}, J.~I. and {Watson}, C.~A. and {West}, R.~G. and {Wheatley}, P.~J.},
title = "{NGTS-14Ab: a Neptune-sized transiting planet in the desert}",
journal = {\aap},
keywords = {planetary systems, planets and satellites: detection, planets and satellites: individual: NGTS-14Ab, binaries: general, Astrophysics - Earth and Planetary Astrophysics},
year = 2021,
month = feb,
volume = {646},
eid = {A183},
pages = {A183},
doi = {10.1051/0004-6361/202039712},
archivePrefix = {arXiv},
eprint = {2101.01470},
primaryClass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...646A.183S},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2021arXiv210203480G,
author = {{Gao}, Peter and {Wakeford}, Hannah R. and {Moran}, Sarah E. and {Parmentier}, Vivien},
title = "{Aerosols in Exoplanet Atmospheres}",
journal = {arXiv e-prints},
keywords = {Astrophysics - Earth and Planetary Astrophysics},
year = 2021,
month = feb,
eid = {arXiv:2102.03480},
pages = {arXiv:2102.03480},
archivePrefix = {arXiv},
eprint = {2102.03480},
primaryClass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2021arXiv210203480G},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2021arXiv210212854D,
author = {{Dietrich}, Wieland and {Wulff}, Paula and {Wicht}, Johannes and {Christensen}, Ulrich R.},
title = "{Linking Zonal Winds and Gravity II: explaining the equatorially antisymmetric gravity moments of Jupiter}",
journal = {arXiv e-prints},
keywords = {Astrophysics - Earth and Planetary Astrophysics},
year = 2021,
month = feb,
eid = {arXiv:2102.12854},
pages = {arXiv:2102.12854},
archivePrefix = {arXiv},
eprint = {2102.12854},
primaryClass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2021arXiv210212854D},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2021ApJ...906...78M,
author = {{Melon Fuksman}, Julio David and {Klahr}, Hubert and {Flock}, Mario and {Mignone}, Andrea},
title = "{A Two-moment Radiation Hydrodynamics Scheme Applicable to Simulations of Planet Formation in Circumstellar Disks}",
journal = {\apj},
keywords = {Radiative transfer, Protoplanetary disks, Planet formation, 1335, 1300, 1241, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
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doi = {10.3847/1538-4357/abc879},
archivePrefix = {arXiv},
eprint = {2005.01785},
primaryClass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2021ApJ...906...78M},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{Grenfell_2020,
doi = {10.1007/s11214-020-00716-4},

url = {https://doi.org/10.1007%2Fs11214-020-00716-4},

year = 2020,
month = {jul},

publisher = {Springer Science and Business Media {LLC}
},

volume = {216},

number = {5},

author = {John Lee Grenfell and Jeremy Leconte and Fran{\c{c}}ois Forget and Mareike Godolt and {\'{O}}scar Carri{\'{o}}n-Gonz{\'{a}}lez and Lena Noack and Feng Tian and Heike Rauer and Fabrice Gaillard and {\'{E}}meline Bolmont and Benjamin Charnay and Martin Turbet},

title = {Possible Atmospheric Diversity of Low Mass Exoplanets {\textendash} Some Central Aspects},

journal = {Space Science Reviews}
}

@ARTICLE{2020arXiv201202798P,
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title = "{A medium-resolution spectrum of the exoplanet HIP 65426 b}",
journal = {arXiv e-prints},
keywords = {Astrophysics - Earth and Planetary Astrophysics},
year = 2020,
month = dec,
eid = {arXiv:2012.02798},
pages = {arXiv:2012.02798},
archivePrefix = {arXiv},
eprint = {2012.02798},
primaryClass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020arXiv201202798P},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2021A&A...645A..16P,
author = {{Parviainen}, H. and {Palle}, E. and {Zapatero-Osorio}, M.~R. and {Nowak}, G. and {Fukui}, A. and {Murgas}, F. and {Narita}, N. and {Stassun}, K.~G. and {Livingston}, J.~H. and {Collins}, K.~A. and {Hidalgo Soto}, D. and {B{\'e}jar}, V.~J.~S. and {Korth}, J. and {Monelli}, M. and {Montanes Rodriguez}, P. and {Casasayas-Barris}, N. and {Chen}, G. and {Crouzet}, N. and {de Leon}, J.~P. and {Hernandez}, A. and {Kawauchi}, K. and {Klagyivik}, P. and {Kusakabe}, N. and {Luque}, R. and {Mori}, M. and {Nishiumi}, T. and {Prieto-Arranz}, J. and {Tamura}, M. and {Watanabe}, N. and {Gan}, T. and {Collins}, K.~I. and {Jensen}, E.~L.~N. and {Barclay}, T. and {Doty}, J.~P. and {Jenkins}, J.~M. and {Latham}, D.~W. and {Paegert}, M. and {Ricker}, G. and {Rodriguez}, D.~R. and {Seager}, S. and {Shporer}, A. and {Vanderspek}, R. and {Villase{\~n}or}, J. and {Winn}, J.~N. and {Wohler}, B. and {Wong}, I.},
title = "{TOI-519 b: A short-period substellar object around an M dwarf validated using multicolour photometry and phase curve analysis}",
journal = {\aap},
keywords = {stars: individual: TIC 218 795 833, planets and satellites: general, methods: statistical, techniques: photometric, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
year = 2021,
month = jan,
volume = {645},
eid = {A16},
pages = {A16},
doi = {10.1051/0004-6361/202038934},
archivePrefix = {arXiv},
eprint = {2011.11458},
primaryClass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...645A..16P},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2021A&A...645A..22Y,
author = {{Yan}, F. and {Wyttenbach}, A. and {Casasayas-Barris}, N. and {Reiners}, A. and {Pall{\'e}}, E. and {Henning}, Th. and {Molli{\`e}re}, P. and {Czesla}, S. and {Nortmann}, L. and {Molaverdikhani}, K. and {Chen}, G. and {Snellen}, I.~A.~G. and {Zechmeister}, M. and {Huang}, C. and {Ribas}, I. and {Quirrenbach}, A. and {Caballero}, J.~A. and {Amado}, P.~J. and {Cont}, D. and {Khalafinejad}, S. and {Khaimova}, J. and {L{\'o}pez-Puertas}, M. and {Montes}, D. and {Nagel}, E. and {Oshagh}, M. and {Pedraz}, S. and {Stangret}, M.},
title = "{Detection of the hydrogen Balmer lines in the ultra-hot Jupiter WASP-33b}",
journal = {\aap},
keywords = {planets and satellites: atmospheres, techniques: spectroscopic, planets and satellites: individual: WASP-33b, Astrophysics - Earth and Planetary Astrophysics},
year = 2021,
month = jan,
volume = {645},
eid = {A22},
pages = {A22},
doi = {10.1051/0004-6361/202039302},
archivePrefix = {arXiv},
eprint = {2011.07888},
primaryClass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...645A..22Y},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2021A&A...645A..41L,
author = {{Luque}, R. and {Serrano}, L.~M. and {Molaverdikhani}, K. and {Nixon}, M.~C. and {Livingston}, J.~H. and {Guenther}, E.~W. and {Pall{\'e}}, E. and {Madhusudhan}, N. and {Nowak}, G. and {Korth}, J. and {Cochran}, W.~D. and {Hirano}, T. and {Chaturvedi}, P. and {Goffo}, E. and {Albrecht}, S. and {Barrag{\'a}n}, O. and {Brice{\~n}o}, C. and {Cabrera}, J. and {Charbonneau}, D. and {Cloutier}, R. and {Collins}, K.~A. and {Collins}, K.~I. and {Col{\'o}n}, K.~D. and {Crossfield}, I.~J.~M. and {Csizmadia}, Sz. and {Dai}, F. and {Deeg}, H.~J. and {Esposito}, M. and {Fridlund}, M. and {Gandolfi}, D. and {Georgieva}, I. and {Glidden}, A. and {Goeke}, R.~F. and {Grziwa}, S. and {Hatzes}, A.~P. and {Henze}, C.~E. and {Howell}, S.~B. and {Irwin}, J. and {Jenkins}, J.~M. and {Jensen}, E.~L.~N. and {K{\'a}bath}, P. and {Kidwell}, R.~C. and {Kielkopf}, J.~F. and {Knudstrup}, E. and {Lam}, K.~W.~F. and {Latham}, D.~W. and {Lissauer}, J.~J. and {Mann}, A.~W. and {Matthews}, E.~C. and {Mireles}, I. and {Narita}, N. and {Paegert}, M. and {Persson}, C.~M. and {Redfield}, S. and {Ricker}, G.~R. and {Rodler}, F. and {Schlieder}, J.~E. and {Scott}, N.~J. and {Seager}, S. and {{\v{S}}ubjak}, J. and {Tan}, T.~G. and {Ting}, E.~B. and {Vanderspek}, R. and {Van Eylen}, V. and {Winn}, J.~N. and {Ziegler}, C.},
title = "{A planetary system with two transiting mini-Neptunes near the radius valley transition around the bright M dwarf TOI-776}",
journal = {\aap},
keywords = {planetary systems, techniques: photometric, techniques: radial velocities, stars: individual: LP 961-53, stars: low-mass, Astrophysics - Earth and Planetary Astrophysics},
year = 2021,
month = jan,
volume = {645},
eid = {A41},
pages = {A41},
doi = {10.1051/0004-6361/202039455},
archivePrefix = {arXiv},
eprint = {2009.08338},
primaryClass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...645A..41L},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2021A&A...645A..43S,
author = {{Schib}, O. and {Mordasini}, C. and {Wenger}, N. and {Marleau}, G. -D. and {Helled}, R.},
title = "{The influence of infall on the properties of protoplanetary discs. Statistics of masses, sizes, lifetimes, and fragmentation}",
journal = {\aap},
keywords = {instabilities, protoplanetary disks, accretion, accretion disks, planets and satellites: formation, stars: formation},
year = 2021,
month = jan,
volume = {645},
eid = {A43},
pages = {A43},
doi = {10.1051/0004-6361/202039154},
adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...645A..43S},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2021A&A...645A..79S,
author = {{Sarkis}, P. and {Mordasini}, C. and {Henning}, Th. and {Marleau}, G.~D. and {Molli{\`e}re}, P.},
title = "{Evidence of three mechanisms explaining the radius anomaly of hot Jupiters}",
journal = {\aap},
keywords = {planets and satellites: gaseous planets, planets and satellites: interiors, planets and satellites: physical evolution, Astrophysics - Earth and Planetary Astrophysics},
year = 2021,
month = jan,
volume = {645},
eid = {A79},
pages = {A79},
doi = {10.1051/0004-6361/202038361},
archivePrefix = {arXiv},
eprint = {2009.04291},
primaryClass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...645A..79S},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2021A&A...645A.131V,
author = {{Voelkel}, Oliver and {Deienno}, Rogerio and {Kretke}, Katherine and {Klahr}, Hubert},
title = "{Linking planetary embryo formation to planetesimal formation. I. The effect of the planetesimal surface density in the terrestrial planet zone}",
journal = {\aap},
keywords = {planets and satellites: terrestrial planets, Astrophysics - Earth and Planetary Astrophysics},
year = 2021,
month = jan,
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eid = {A131},
pages = {A131},
doi = {10.1051/0004-6361/202039214},
archivePrefix = {arXiv},
eprint = {2008.10442},
primaryClass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...645A.131V},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2021A&A...645A.132V,
author = {{Voelkel}, Oliver and {Deienno}, Rogerio and {Kretke}, Katherine and {Klahr}, Hubert},
title = "{Linking planetary embryo formation to planetesimal formation. II. The effect of pebble accretion in the terrestrial planet zone}",
journal = {\aap},
keywords = {planets and satellites: formation, planets and satellites: terrestrial planets, Astrophysics - Earth and Planetary Astrophysics},
year = 2021,
month = jan,
volume = {645},
eid = {A132},
pages = {A132},
doi = {10.1051/0004-6361/202039245},
archivePrefix = {arXiv},
eprint = {2008.10432},
primaryClass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...645A.132V},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@ARTICLE{2021A&A...645A.143K,
author = {{Krieger}, A. and {Wolf}, S.},
title = "{The scattering order problem in Monte Carlo radiative transfer}",
journal = {\aap},
keywords = {methods: numerical, radiative transfer, scattering, dust, extinction, opacity, polarization, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
year = 2021,
month = jan,
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pages = {A143},
doi = {10.1051/0004-6361/202039133},
archivePrefix = {arXiv},
eprint = {2011.14905},
primaryClass = {astro-ph.IM},
adsurl = {https://ui.adsabs.harvard.edu/abs/2021A&A...645A.143K},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020A&A...644A..13S,
author = {{Stolker}, T. and {Marleau}, G. -D. and {Cugno}, G. and {Molli{\`e}re}, P. and {Quanz}, S.~P. and {Todorov}, K.~O. and {K{\"u}hn}, J.},
title = {{MIRACLES: atmospheric characterization of directly imaged planets and substellar companions at 4-5 {\ensuremath{\mu}}m. II. Constraints on the mass and radius of the enshrouded planet PDS 70 b}},
journal = {\aap},
keywords = {stars: individual: PDS 70, planets and satellites: atmospheres, planets and satellites: formation, techniques: high angular resolution, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
year = 2020,
month = dec,
volume = {644},
eid = {A13},
pages = {A13},
doi = {10.1051/0004-6361/202038878},
archiveprefix = {arXiv},
eprint = {2009.04483},
primaryclass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...644A..13S},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020A&A...644A...1P,
author = {{Pinto}, Marcelo Tala and {Reffert}, Sabine and {Quirrenbach}, Andreas and {Stock}, Stephan and {Trifonov}, Trifon and {Mitchell}, David S.},
title = {{Precise radial velocities of giant stars. XIV. Evidence of planetary companions around HD 25723, 17 Sco, 3 Cnc, and 44 UMa}},
journal = {\aap},
keywords = {techniques: radial velocities, planetary systems, planets and satellites: detection, brown dwarfs, stars: evolution},
year = 2020,
month = dec,
volume = {644},
eid = {A1},
pages = {A1},
doi = {10.1051/0004-6361/202038285},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...644A...1P},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@misc{https://doi.org/10.48550/arxiv.2011.06608,
doi = {10.48550/ARXIV.2011.06608},

url = {https://arxiv.org/abs/2011.06608},

author = {Aoyama, Yuhiko and Marleau, Gabriel-Dominique and Mordasini, Christoph and Ikoma, Masahiro},

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},

publisher = {arXiv},

year = {2020},

copyright = {Creative Commons Attribution 4.0 International}
}

@article{2020A&A...643A.131F,
author = {{Fossati}, L. and {Shulyak}, D. and {Sreejith}, A.~G. and {Koskinen}, T. and {Young}, M.~E. and {Cubillos}, P.~E. and {Lara}, L.~M. and {France}, K. and {Rengel}, M. and {Cauley}, P.~W. and {Turner}, J.~D. and {Wyttenbach}, A. and {Yan}, F.},
title = {{A data-driven approach to constraining the atmospheric temperature structure of the ultra-hot Jupiter KELT-9b}},
journal = {\aap},
keywords = {radiative transfer, planets and satellites: atmospheres, planets and satellites: gaseous planets, planets and satellites: individual: KELT-9b, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
year = 2020,
month = nov,
volume = {643},
eid = {A131},
pages = {A131},
doi = {10.1051/0004-6361/202039061},
archiveprefix = {arXiv},
eprint = {2010.00997},
primaryclass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...643A.131F},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020A&A...643A..94L,
author = {{Lendl}, M. and {Csizmadia}, Sz. and {Deline}, A. and {Fossati}, L. and {Kitzmann}, D. and {Heng}, K. and {Hoyer}, S. and {Salmon}, S. and {Benz}, W. and {Broeg}, C. and {Ehrenreich}, D. and {Fortier}, A. and {Queloz}, D. and {Bonfanti}, A. and {Brandeker}, A. and {Collier Cameron}, A. and {Delrez}, L. and {Garcia Mu{\~n}oz}, A. and {Hooton}, M.~J. and {Maxted}, P.~F.~L. and {Morris}, B.~M. and {Van Grootel}, V. and {Wilson}, T.~G. and {Alibert}, Y. and {Alonso}, R. and {Asquier}, J. and {Bandy}, T. and {B{\'a}rczy}, T. and {Barrado}, D. and {Barros}, S.~C.~C. and {Baumjohann}, W. and {Beck}, M. and {Beck}, T. and {Bekkelien}, A. and {Bergomi}, M. and {Billot}, N. and {Biondi}, F. and {Bonfils}, X. and {Bourrier}, V. and {Busch}, M. -D. and {Cabrera}, J. and {Cessa}, V. and {Charnoz}, S. and {Chazelas}, B. and {Corral Van Damme}, C. and {Davies}, M.~B. and {Deleuil}, M. and {Demangeon}, O.~D.~S. and {Demory}, B. -O. and {Erikson}, A. and {Farinato}, J. and {Fridlund}, M. and {Futyan}, D. and {Gandolfi}, D. and {Gillon}, M. and {Guterman}, P. and {Hasiba}, J. and {Hernandez}, E. and {Isaak}, K.~G. and {Kiss}, L. and {Kuntzer}, T. and {Lecavelier des Etangs}, A. and {L{\"u}ftinger}, T. and {Laskar}, J. and {Lovis}, C. and {Magrin}, D. and {Malvasio}, L. and {Marafatto}, L. and {Michaelis}, H. and {Munari}, M. and {Nascimbeni}, V. and {Olofsson}, G. and {Ottacher}, H. and {Ottensamer}, R. and {Pagano}, I. and {Pall{\'e}}, E. and {Peter}, G. and {Piazza}, D. and {Piotto}, G. and {Pollacco}, D. and {Ratti}, F. and {Rauer}, H. and {Ragazzoni}, R. and {Rando}, N. and {Ribas}, I. and {Rieder}, M. and {Rohlfs}, R. and {Safa}, F. and {Santos}, N.~C. and {Scandariato}, G. and {S{\'e}gransan}, D. and {Simon}, A.~E. and {Singh}, V. and {Smith}, A.~M.~S. and {Sordet}, M. and {Sousa}, S.~G. and {Steller}, M. and {Szab{\'o}}, Gy. M. and {Thomas}, N. and {Tschentscher}, M. and {Udry}, S. and {Viotto}, V. and {Walter}, I. and {Walton}, N.~A. and {Wildi}, F. and {Wolter}, D.},
title = {{The hot dayside and asymmetric transit of WASP-189 b seen by CHEOPS}},
journal = {\aap},
keywords = {techniques: photometric, planets and satellites: atmospheres, planets and satellites: individual: WASP-189 b, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
year = 2020,
month = nov,
volume = {643},
eid = {A94},
pages = {A94},
doi = {10.1051/0004-6361/202038677},
archiveprefix = {arXiv},
eprint = {2009.13403},
primaryclass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...643A..94L},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020A&A...643A..64O,
author = {{Oshagh}, M. and {Bauer}, F.~F. and {Lafarga}, M. and {Molaverdikhani}, K. and {Amado}, P.~J. and {Nortmann}, L. and {Reiners}, A. and {Guzm{\'a}n-Mesa}, A. and {Pall{\'e}}, E. and {Nagel}, E. and {Caballero}, J.~A. and {Casasayas-Barris}, N. and {Claret}, A. and {Czesla}, S. and {Galad{\'\i}}, D. and {Henning}, Th. and {Khalafinejad}, S. and {L{\'o}pez-Puertas}, M. and {Montes}, D. and {Quirrenbach}, A. and {Ribas}, I. and {Stangret}, M. and {Yan}, F. and {Zapatero Osorio}, M.~R. and {Zechmeister}, M.},
title = {{The widest broadband transmission spectrum (0.38-1.71 {\ensuremath{\mu}}m) of HD 189733b from ground-based chromatic Rossiter-McLaughlin observations}},
journal = {\aap},
keywords = {techniques: radial velocities, techniques: spectroscopic, methods: numerical, planets and satellites: atmospheres, stars: activity, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
year = 2020,
month = nov,
volume = {643},
eid = {A64},
pages = {A64},
doi = {10.1051/0004-6361/202039213},
archiveprefix = {arXiv},
eprint = {2009.13823},
primaryclass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...643A..64O},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020ApJ...901..126W,
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title = {{Distinguishing between Wet and Dry Atmospheres of TRAPPIST-1 e and f}},
journal = {\apj},
keywords = {Exoplanet atmospheres, Exoplanet atmospheric composition, Planetary atmospheres, 487, 2021, 1244, Astrophysics - Earth and Planetary Astrophysics},
year = 2020,
month = oct,
volume = {901},
number = {2},
eid = {126},
pages = {126},
doi = {10.3847/1538-4357/aba59c},
archiveprefix = {arXiv},
eprint = {2006.11349},
primaryclass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020ApJ...901..126W},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020A&A...642A.225A,
author = {{Amazo-G{\'o}mez}, E.~M. and {Shapiro}, A.~I. and {Solanki}, S.~K. and {Kopp}, G. and {Oshagh}, M. and {Reinhold}, T. and {Reiners}, A.},
title = {{Inflection point in the power spectrum of stellar brightness variations. III. Facular versus spot dominance on stars with known rotation periods}},
journal = {\aap},
keywords = {stars: rotation, stars: solar-type, methods: observational, techniques: photometric, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Earth and Planetary Astrophysics},
year = 2020,
month = oct,
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eid = {A225},
pages = {A225},
doi = {10.1051/0004-6361/202038926},
archiveprefix = {arXiv},
eprint = {2008.11492},
primaryclass = {astro-ph.SR},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...642A.225A},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020A&A...642A..98Y,
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title = {{LBT transmission spectroscopy of HAT-P-12b. Confirmation of a cloudy atmosphere with no significant alkali features}},
journal = {\aap},
keywords = {planets and satellites: atmospheres, techniques: spectroscopic, stars: atmospheres, planets and satellites: individual: HAT-P-12b, Astrophysics - Earth and Planetary Astrophysics},
year = 2020,
month = oct,
volume = {642},
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pages = {A98},
doi = {10.1051/0004-6361/201937265},
archiveprefix = {arXiv},
eprint = {2007.15485},
primaryclass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...642A..98Y},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020A&A...642A..75V,
author = {{Voelkel}, Oliver and {Klahr}, Hubert and {Mordasini}, Christoph and {Emsenhuber}, Alexandre and {Lenz}, Christian},
title = {{Effect of pebble flux-regulated planetesimal formation on giant planet formation}},
journal = {\aap},
keywords = {protoplanetary disks, planets and satellites: formation, Astrophysics - Earth and Planetary Astrophysics},
year = 2020,
month = oct,
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pages = {A75},
doi = {10.1051/0004-6361/202038085},
archiveprefix = {arXiv},
eprint = {2004.03492},
primaryclass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...642A..75V},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020NatRP...2..562H,
author = {{Helled}, Ravit and {Mazzola}, Guglielmo and {Redmer}, Ronald},
title = {{Understanding dense hydrogen at planetary conditions}},
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keywords = {Astrophysics - Earth and Planetary Astrophysics},
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pages = {562-574},
doi = {10.1038/s42254-020-0223-3},
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eprint = {2006.12219},
primaryclass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020NatRP...2..562H},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020NatAs.tmp..180J,
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title = {{An ultrahot Neptune in the Neptune desert}},
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year = 2020,
month = sep,
doi = {10.1038/s41550-020-1142-z},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020NatAs.tmp..180J},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020MNRAS.499.3356P,
author = {{Parviainen}, H. and {Korth}, J.},
title = {{Going back to basics: accelerating exoplanet transit modelling using Taylor-series expansion of the orbital motion}},
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keywords = {methods: numerical, techniques: photometric, planets and satellites: general, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics},
year = 2020,
month = sep,
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number = {3},
pages = {3356-3361},
doi = {10.1093/mnras/staa2953},
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eprint = {2009.09965},
primaryclass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020MNRAS.499.3356P},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020ApJ...901...54K,
author = {{Klahr}, Hubert and {Schreiber}, Andreas},
title = {{Turbulence Sets the Length Scale for Planetesimal Formation: Local 2D Simulations of Streaming Instability and Planetesimal Formation}},
journal = {\apj},
keywords = {Solar system formation, Protoplanetary disks, Planet formation, Planetesimals, Asteroids, Small solar system bodies, Classical Kuiper Belt objects, Trans-Neptunian objects, Comets, Hydrodynamical simulations, 1530, 1300, 1241, 1259, 72, 1469, 250, 1705, 280, 767, Astrophysics - Earth and Planetary Astrophysics},
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pages = {54},
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archiveprefix = {arXiv},
eprint = {2007.10696},
primaryclass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020ApJ...901...54K},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020AJ....160..114C,
author = {{Carleo}, Ilaria and {Gandolfi}, Davide and {Barrag{\'a}n}, Oscar and {Livingston}, John H. and {Persson}, Carina M. and {Lam}, Kristine W.~F. and {Vidotto}, Aline and {Lund}, Michael B. and {D'Angelo}, Carolina Villarreal and {Collins}, Karen A. and {Fossati}, Luca and {Howard}, Andrew W. and {Kubyshkina}, Daria and {Brahm}, Rafael and {Oklop{\v{c}}i{\'c}}, Antonija and {Molli{\`e}re}, Paul and {Redfield}, Seth and {Serrano}, Luisa Maria and {Dai}, Fei and {Fridlund}, Malcolm and {Borsa}, Francesco and {Korth}, Judith and {Esposito}, Massimiliano and {D{\'\i}az}, Mat{\'\i}as R. and {Nielsen}, Louise Dyregaard and {Hellier}, Coel and {Mathur}, Savita and {Deeg}, Hans J. and {Hatzes}, Artie P. and {Benatti}, Serena and {Rodler}, Florian and {Alarcon}, Javier and {Spina}, Lorenzo and {Santos}, {\^A}ngela R.~G. and {Georgieva}, Iskra and {Garc{\'\i}a}, Rafael A. and {Gonz{\'a}lez-Cuesta}, Luc{\'\i}a and {Ricker}, George R. and {Vanderspek}, Roland and {Latham}, David W. and {Seager}, Sara and {Winn}, Joshua N. and {Jenkins}, Jon M. and {Albrecht}, Simon and {Batalha}, Natalie M. and {Beard}, Corey and {Boyd}, Patricia T. and {Bouchy}, Fran{\c{c}}ois and {Burt}, Jennifer A. and {Butler}, R. Paul and {Cabrera}, Juan and {Chontos}, Ashley and {Ciardi}, David R. and {Cochran}, William D. and {Collins}, Kevin I. and {Crane}, Jeffrey D. and {Crossfield}, Ian and {Csizmadia}, Szilard and {Dragomir}, Diana and {Dressing}, Courtney and {Eigm{\"u}ller}, Philipp and {Endl}, Michael and {Erikson}, Anders and {Espinoza}, Nestor and {Fausnaugh}, Michael and {Feng}, Fabo and {Flowers}, Erin and {Fulton}, Benjamin and {Gonzales}, Erica J. and {Grieves}, Nolan and {Grziwa}, Sascha and {Guenther}, Eike W. and {Guerrero}, Natalia M. and {Henning}, Thomas and {Hidalgo}, Diego and {Hirano}, Teruyuki and {Hjorth}, Maria and {Huber}, Daniel and {Isaacson}, Howard and {Jones}, Matias and {Jord{\'a}n}, Andr{\'e}s and {Kab{\'a}th}, Petr and {Kane}, Stephen R. and {Knudstrup}, Emil and {Lubin}, Jack and {Luque}, Rafael and {Mireles}, Ismael and {Narita}, Norio and {Nespral}, David and {Niraula}, Prajwal and {Nowak}, Grzegorz and {Palle}, Enric and {P{\"a}tzold}, Martin and {Petigura}, Erik A. and {Prieto-Arranz}, Jorge and {Rauer}, Heike and {Robertson}, Paul and {Rose}, Mark E. and {Roy}, Arpita and {Sarkis}, Paula and {Schlieder}, Joshua E. and {S{\'e}gransan}, Damien and {Shectman}, Stephen and {Skarka}, Marek and {Smith}, Alexis M.~S. and {Smith}, Jeffrey C. and {Stassun}, Keivan and {Teske}, Johanna and {Twicken}, Joseph D. and {Eylen}, Vincent Van and {Wang}, Sharon and {Weiss}, Lauren M. and {Wyttenbach}, Aur{\'e}lien},
title = {{The Multiplanet System TOI-421}},
journal = {\aj},
keywords = {Exoplanet astronomy, Exoplanet systems, Exoplanets, Mini Neptunes, Hot Neptunes, Fundamental parameters of stars, High resolution spectroscopy, Transit photometry, Radial velocity, 486, 484, 498, 1063, 754, 555, 2096, 1709, 1332, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
year = 2020,
month = sep,
volume = {160},
number = {3},
eid = {114},
pages = {114},
doi = {10.3847/1538-3881/aba124},
archiveprefix = {arXiv},
eprint = {2004.10095},
primaryclass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020AJ....160..114C},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{Pfeil_2021,
doi = {10.3847/1538-4357/ac0054},

url = {https://doi.org/10.3847%2F1538-4357%2Fac0054},

year = 2021,
month = {jul},

publisher = {American Astronomical Society},

volume = {915},

number = {2},

pages = {130},

author = {Thomas Pfeil and Hubert Klahr},

title = {The Sandwich Mode for Vertical Shear Instability in Protoplanetary Disks},

journal = {The Astrophysical Journal}
}

@article{2020MNRAS.498.4503F,
author = {{Fridlund}, M. and {Livingston}, J. and {Gandolfi}, D. and {Persson}, C.~M. and {Lam}, K.~W.~F. and {Stassun}, K.~G. and {Hellier}, C. and {Korth}, J. and {Hatzes}, A.~P. and {Malavolta}, L. and {Luque}, R. and {Redfield}, S. and {Guenther}, E.~W. and {Albrecht}, S. and {Barragan}, O. and {Benatti}, S. and {Bouma}, L. and {Cabrera}, J. and {Cochran}, W.~D. and {Csizmadia}, S. and {Dai}, F. and {Deeg}, H.~J. and {Esposito}, M. and {Georgieva}, I. and {Grziwa}, S. and {Gonz{\'a}lez Cuesta}, L. and {Hirano}, T. and {Jenkins}, J.~M. and {Kabath}, P. and {Knudstrup}, E. and {Latham}, D.~W. and {Mathur}, S. and {Mullally}, S.~E. and {Narita}, N. and {Nowak}, G. and {Olofsson}, A.~O.~H. and {Palle}, E. and {P{\"a}tzold}, M. and {Pompei}, E. and {Rauer}, H. and {Ricker}, G. and {Rodler}, F. and {Seager}, S. and {Serrano}, L.~M. and {Smith}, A.~M.~S. and {Spina}, L. and {Subjak}, J. and {Tenenbaum}, P. and {Ting}, E.~B. and {Vanderburg}, A. and {Vanderspek}, R. and {Van Eylen}, V. and {Villanueva}, S. and {Winn}, J.~N.},
title = {{The TOI-763 system: sub-Neptunes orbiting a Sun-like star}},
journal = {\mnras},
keywords = {planets and satellites: detection, planets and satellites: individual: TOI-763, planets and satellites: individual: TIC 178819686, Astrophysics - Earth and Planetary Astrophysics},
year = 2020,
month = aug,
volume = {498},
number = {3},
pages = {4503-4517},
doi = {10.1093/mnras/staa2502},
archiveprefix = {arXiv},
eprint = {2008.12535},
primaryclass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020MNRAS.498.4503F},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020ApJ...899..130S,
author = {{Szegedi-Elek}, E. and {{\'A}brah{\'a}m}, P. and {Wyrzykowski}, {\L}. and {Kun}, M. and {K{\'o}sp{\'a}l}, {\'A}. and {Chen}, L. and {Marton}, G. and {Mo{\'o}r}, A. and {Kiss}, C. and {P{\'a}l}, A. and {Szabados}, L. and {Varga}, J. and {Varga-Vereb{\'e}lyi}, E. and {Andreas}, C. and {Bachelet}, E. and {Bischoff}, R. and {B{\'o}di}, A. and {Breedt}, E. and {Burgaz}, U. and {Butterley}, T. and {Carrasco}, J.~M. and {{\v{C}}epas}, V. and {Damljanovic}, G. and {Gezer}, I. and {Godunova}, V. and {Gromadzki}, M. and {Gurgul}, A. and {Hardy}, L. and {Hildebrandt}, F. and {Hoffmann}, S. and {Hundertmark}, M. and {Ihanec}, N. and {Janulis}, R. and {Kalup}, Cs. and {Kaczmarek}, Z. and {K{\"o}nyves-T{\'o}th}, R. and {Krezinger}, M. and {Kruszy{\'n}ska}, K. and {Littlefair}, S. and {Maskoli{\={u}}nas}, M. and {M{\'e}sz{\'a}ros}, L. and {Miko{\l}ajczyk}, P. and {Mugrauer}, M. and {Netzel}, H. and {Ordasi}, A. and {Pak{\v{s}}tien{\.{e}}}, E. and {Rybicki}, K.~A. and {S{\'a}rneczky}, K. and {Seli}, B. and {Simon}, A. and {{\v{S}}i{\v{s}}kauskait{\.{e}}}, K. and {S{\'o}dor}, {\'A}. and {Sokolovsky}, K.~V. and {Stenglein}, W. and {Street}, R. and {Szak{\'a}ts}, R. and {Tomasella}, L. and {Tsapras}, Y. and {Vida}, K. and {Zdanavi{\v{c}}ius}, J. and {Zieli{\'n}ski}, M. and {Zieli{\'n}ski}, P. and {Zi{\'o}{\l}kowska}, O.},
title = {{Gaia 18dvy: A New FUor in the Cygnus OB3 Association}},
journal = {\apj},
keywords = {Star formation, Accretion, Protoplanetary disks, Eruptive variable stars, 1569, 14, 1300, 476, Astrophysics - Solar and Stellar Astrophysics},
year = 2020,
month = aug,
volume = {899},
number = {2},
eid = {130},
pages = {130},
doi = {10.3847/1538-4357/aba129},
archiveprefix = {arXiv},
eprint = {2005.11537},
primaryclass = {astro-ph.SR},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020ApJ...899..130S},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020ApJ...899...54M,
author = {{Mai}, Chuhong and {Desch}, Steven J. and {Kuiper}, Rolf and {Marleau}, Gabriel-Dominique and {Dullemond}, Cornelis},
title = {{The Dynamic Proto-atmospheres around Low-mass Planets with Eccentric Orbits}},
journal = {\apj},
keywords = {Hydrodynamics, Planetary atmospheres, Planet formation, Elliptical orbits, 1963, 1244, 1241, 457, Astrophysics - Earth and Planetary Astrophysics},
year = 2020,
month = aug,
volume = {899},
number = {1},
eid = {54},
pages = {54},
doi = {10.3847/1538-4357/aba4a8},
archiveprefix = {arXiv},
eprint = {2007.04398},
primaryclass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020ApJ...899...54M},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020A&A...640L...5Y,
author = {{Yan}, F. and {Pall{\'e}}, E. and {Reiners}, A. and {Molaverdikhani}, K. and {Casasayas-Barris}, N. and {Nortmann}, L. and {Chen}, G. and {Molli{\`e}re}, P. and {Stangret}, M.},
title = {{A temperature inversion with atomic iron in the ultra-hot dayside atmosphere of WASP-189b}},
journal = {\aap},
keywords = {planets and satellites: atmospheres, techniques: spectroscopic, planets and satellites: individual: WASP-189b, Astrophysics - Earth and Planetary Astrophysics},
year = 2020,
month = aug,
volume = {640},
eid = {L5},
pages = {L5},
doi = {10.1051/0004-6361/202038294},
archiveprefix = {arXiv},
eprint = {2007.02716},
primaryclass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...640L...5Y},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020A&A...640A.136C,
author = {{Carri{\'o}n-Gonz{\'a}lez}, {\'O}. and {Garc{\'\i}a Mu{\~n}oz}, A. and {Cabrera}, J. and {Csizmadia}, Sz. and {Santos}, N.~C. and {Rauer}, H.},
title = {{Directly imaged exoplanets in reflected starlight: the importance of knowing the planet radius}},
journal = {\aap},
keywords = {planets and satellites: atmospheres, planets and satellites: gaseous planets, radiative transfer, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics},
year = 2020,
month = aug,
volume = {640},
eid = {A136},
pages = {A136},
doi = {10.1051/0004-6361/202038101},
archiveprefix = {arXiv},
eprint = {2006.08784},
primaryclass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...640A.136C},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020A&A...640A.131M,
author = {{Molli{\`e}re}, P. and {Stolker}, T. and {Lacour}, S. and {Otten}, G.~P.~P.~L. and {Shangguan}, J. and {Charnay}, B. and {Molyarova}, T. and {Nowak}, M. and {Henning}, Th. and {Marleau}, G. -D. and {Semenov}, D.~A. and {van Dishoeck}, E. and {Eisenhauer}, F. and {Garcia}, P. and {Garcia Lopez}, R. and {Girard}, J.~H. and {Greenbaum}, A.~Z. and {Hinkley}, S. and {Kervella}, P. and {Kreidberg}, L. and {Maire}, A. -L. and {Nasedkin}, E. and {Pueyo}, L. and {Snellen}, I.~A.~G. and {Vigan}, A. and {Wang}, J. and {de Zeeuw}, P.~T. and {Zurlo}, A.},
title = {{Retrieving scattering clouds and disequilibrium chemistry in the atmosphere of HR 8799e}},
journal = {\aap},
keywords = {methods: numerical, planets and satellites: atmospheres, radiative transfer, instrumentation: spectrographs, Astrophysics - Earth and Planetary Astrophysics},
year = 2020,
month = aug,
volume = {640},
eid = {A131},
pages = {A131},
doi = {10.1051/0004-6361/202038325},
archiveprefix = {arXiv},
eprint = {2006.09394},
primaryclass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...640A.131M},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020A&A...640A..61L,
author = {{Lenz}, Christian T. and {Klahr}, Hubert and {Birnstiel}, Tilman and {Kretke}, Katherine and {Stammler}, Sebastian},
title = {{Constraining the parameter space for the solar nebula. The effect of disk properties on planetesimal formation}},
journal = {\aap},
keywords = {accretion, accretion disks, protoplanetary disks, circumstellar matter, turbulence, methods: numerical, minor planets, asteroids: general},
year = 2020,
month = aug,
volume = {640},
eid = {A61},
pages = {A61},
doi = {10.1051/0004-6361/202037878},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...640A..61L},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020AJ....160...74H,
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title = {{OGLE-2017-BLG-0406: Spitzer Microlens Parallax Reveals Saturn-mass Planet Orbiting M-dwarf Host in the Inner Galactic Disk}},
journal = {\aj},
keywords = {Gravitational microlensing, Gravitational microlensing exoplanet detection, 672, 2147, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics},
year = 2020,
month = aug,
volume = {160},
number = {2},
eid = {74},
pages = {74},
doi = {10.3847/1538-3881/ab9ac3},
archiveprefix = {arXiv},
eprint = {2004.09067},
primaryclass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020AJ....160...74H},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{Vigan_2021,
doi = {10.1051/0004-6361/202038107},

url = {https://doi.org/10.1051%2F0004-6361%2F202038107},

year = 2021,
month = {jul},

publisher = {{EDP} Sciences},

volume = {651},

pages = {A72},

author = {A. Vigan and C. Fontanive and M. Meyer and B. Biller and M. Bonavita and M. Feldt and S. Desidera and G.-D. Marleau and A. Emsenhuber and R. Galicher and K. Rice and D. Forgan and C. Mordasini and R. Gratton and H. Le Coroller and A.-L. Maire and F. Cantalloube and G. Chauvin and A. Cheetham and J. Hagelberg and A.-M. Lagrange and M. Langlois and M. Bonnefoy and J.-L. Beuzit and A. Boccaletti and V. D'Orazi and P. Delorme and C. Dominik and Th. Henning and M. Janson and E. Lagadec and C. Lazzoni and R. Ligi and F. Menard and D. Mesa and S. Messina and C. Moutou and A. Müller and C. Perrot and M. Samland and H. M. Schmid and T. Schmidt and E. Sissa and M. Turatto and S. Udry and A. Zurlo and L. Abe and J. Antichi and R. Asensio-Torres and A. Baruffolo and P. Baudoz and J. Baudrand and A. Bazzon and P. Blanchard and A. J. Bohn and S. Brown Sevilla and M. Carbillet and M. Carle and E. Cascone and J. Charton and R. Claudi and A. Costille and V. De Caprio and A. Delboulb{\'{e}
} and K. Dohlen and N. Engler and D. Fantinel and P. Feautrier and T. Fusco and P. Gigan and J. H. Girard and E. Giro and D. Gisler and L. Gluck and C. Gry and N. Hubin and E. Hugot and M. Jaquet and M. Kasper and D. Le Mignant and M. Llored and F. Madec and Y. Magnard and P. Martinez and D. Maurel and O. Möller-Nilsson and D. Mouillet and T. Moulin and A. Orign{\'{e}} and A. Pavlov and D. Perret and C. Petit and J. Pragt and P. Puget and P. Rabou and J. Ramos and E. L. Rickman and F. Rigal and S. Rochat and R. Roelfsema and G. Rousset and A. Roux and B. Salasnich and J.-F. Sauvage and A. Sevin and C. Soenke and E. Stadler and M. Suarez and Z. Wahhaj and L. Weber and F. Wildi},

title = {The {SPHERE} infrared survey for exoplanets ({SHINE})},

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

@article{2020NatSR..1010907O,
author = {{Ortenzi}, G. and {Noack}, L. and {Sohl}, F. and {Guimond}, C.~M. and {Grenfell}, J.~L. and {Dorn}, C. and {Schmidt}, J.~M. and {Vulpius}, S. and {Katyal}, N. and {Kitzmann}, D. and {Rauer}, H.},
title = {{Mantle redox state drives outgassing chemistry and atmospheric composition of rocky planets}},
journal = {Scientific Reports},
year = 2020,
month = jul,
volume = {10},
eid = {10907},
pages = {10907},
doi = {10.1038/s41598-020-67751-7},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020NatSR..1010907O},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020MNRAS.497.4423N,
author = {{Nowak}, Grzegorz and {Palle}, Enric and {Gandolfi}, Davide and {Deeg}, Hans J. and {Hirano}, Teruyuki and {Barrag{\'a}n}, Oscar and {Kuzuhara}, Masayuki and {Dai}, Fei and {Luque}, Rafael and {Persson}, Carina M. and {Fridlund}, Malcolm and {Johnson}, Marshall C. and {Korth}, Judith and {Livingston}, John H. and {Grziwa}, Sascha and {Mathur}, Savita and {Hatzes}, Artie P. and {Prieto-Arranz}, Jorge and {Nespral}, David and {Hidalgo}, Diego and {Hjorth}, Maria and {Albrecht}, Simon and {Van Eylen}, Vincent and {Lam}, Kristine W.~F. and {Cochran}, William D. and {Esposito}, Massimiliano and {Csizmadia}, Szil{\'a}rd and {Guenther}, Eike W. and {Kabath}, Petr and {Blay}, Pere and {Brahm}, Rafael and {Jord{\'a}n}, Andr{\'e}s and {Espinoza}, N{\'e}stor and {Rojas}, Felipe and {Casasayas Barris}, N{\'u}ria and {Rodler}, Florian and {Alonso Sobrino}, Roi and {Cabrera}, Juan and {Carleo}, Ilaria and {Chaushev}, Alexander and {de Leon}, Jerome and {Eigm{\"u}ller}, Philipp and {Endl}, Michael and {Erikson}, Anders and {Fukui}, Akihiko and {Georgieva}, Iskra and {Gonz{\'a}lez-Cuesta}, Luc{\'\i}a and {Knudstrup}, Emil and {Lund}, Mikkel N. and {Monta{\~n}es Rodr{\'\i}guez}, Pilar and {Murgas}, Felipe and {Narita}, Norio and {Niraula}, Prajwal and {P{\"a}tzold}, Martin and {Rauer}, Heike and {Redfield}, Seth and {Ribas}, Ignasi and {Skarka}, Marek and {Smith}, Alexis M.~S. and {Subjak}, Jano},
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,
volume = {497},
number = {4},
pages = {4423-4435},
doi = {10.1093/mnras/staa2077},
archiveprefix = {arXiv},
eprint = {2007.07939},
primaryclass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020MNRAS.497.4423N},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020MNRAS.497.4009L,
author = {{Lisogorskyi}, M. and {Boro Saikia}, S. and {Jeffers}, S.~V. and {Jones}, H.~R.~A. and {Morin}, J. and {Mengel}, M. and {Reiners}, A. and {Vidotto}, A.~A. and {Petit}, P.},
title = {{The impact of unresolved magnetic spots on high-precision radial velocity measurements}},
journal = {\mnras},
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,
volume = {497},
number = {3},
pages = {4009-4021},
doi = {10.1093/mnras/staa2184},
archiveprefix = {arXiv},
eprint = {2007.12193},
primaryclass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020MNRAS.497.4009L},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020MNRAS.497.3623F,
author = {{Flammini Dotti}, Francesco and {Kouwenhoven}, M.~B.~N. and {Shu}, Qi and {Hao}, Wei and {Spurzem}, Rainer},
title = {{Planetary systems in a star cluster II: intermediate-mass black holes and planetary systems}},
journal = {\mnras},
keywords = {planets and satellites: dynamical evolution and stability, planetary systems, stars: solar-type, stars: statistics, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics},
year = 2020,
month = jul,
volume = {497},
number = {3},
pages = {3623-3637},
doi = {10.1093/mnras/staa2188},
archiveprefix = {arXiv},
eprint = {2007.11999},
primaryclass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020MNRAS.497.3623F},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020MNRAS.497.3484A,
author = {{Akinsanmi}, B. and {Barros}, S.~C.~C. and {Santos}, N.~C. and {Oshagh}, M. and {Serrano}, L.~M.},
title = {{Constraining the oblateness of transiting planets with photometry and spectroscopy}},
journal = {\mnras},
keywords = {techniques: photometric, techniques: spectroscopic, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics},
year = 2020,
month = jul,
volume = {497},
number = {3},
pages = {3484-3492},
doi = {10.1093/mnras/staa2164},
archiveprefix = {arXiv},
eprint = {2007.11221},
primaryclass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020MNRAS.497.3484A},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020MNRAS.497.1807S,
author = {{Stock}, Katja and {Cai}, Maxwell X. and {Spurzem}, Rainer and {Kouwenhoven}, M.~B.~N. and {Portegies Zwart}, Simon},
title = {{On the survival of resonant and non-resonant planetary systems in star clusters}},
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,
volume = {497},
number = {2},
pages = {1807-1825},
doi = {10.1093/mnras/staa2047},
archiveprefix = {arXiv},
eprint = {2007.11601},
primaryclass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020MNRAS.497.1807S},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020ApJ...898L..11G,
author = {{Gill}, Samuel and {Wheatley}, Peter J. and {Cooke}, Benjamin F. and {Jord{\'a}n}, Andr{\'e}s and {Nielsen}, Louise D. and {Bayliss}, Daniel and {Anderson}, David R. and {Vines}, Jose I. and {Lendl}, Monika and {Acton}, Jack S. and {Armstrong}, David J. and {Bouchy}, Fran{\c{c}}ois and {Brahm}, Rafael and {Bryant}, Edward M. and {Burleigh}, Matthew R. and {Casewell}, Sarah L. and {Eigm{\"u}ller}, Philipp and {Espinoza}, N{\'e}stor and {Gillen}, Edward and {Goad}, Michael R. and {Grieves}, Nolan and {G{\"u}nther}, Maximilian N. and {Henning}, Thomas and {Hobson}, Melissa J. and {Hogan}, Aleisha and {Jenkins}, James S. and {McCormac}, James and {Moyano}, Maximiliano and {Osborn}, Hugh P. and {Pollacco}, Don and {Queloz}, Didier and {Rauer}, Heike and {Raynard}, Liam and {Rojas}, Felipe and {Sarkis}, Paula and {Smith}, Alexis M.~S. and {Pinto}, Marcelo Tala and {Tilbrook}, Rosanna H. and {Udry}, St{\'e}phane and {Watson}, Christopher A. and {West}, Richard G.},
title = {{NGTS-11 b (TOI-1847 b): A Transiting Warm Saturn Recovered from a TESS Single-transit Event}},
journal = {\apjl},
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},
year = 2020,
month = jul,
volume = {898},
number = {1},
eid = {L11},
pages = {L11},
doi = {10.3847/2041-8213/ab9eb9},
archiveprefix = {arXiv},
eprint = {2005.00006},
primaryclass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020ApJ...898L..11G},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020ApJ...898...44S,
author = {{Scheucher}, Markus and {Wunderlich}, F. and {Grenfell}, J.~L. and {Godolt}, M. and {Schreier}, F. and {Kappel}, D. and {Haus}, R. and {Herbst}, K. and {Rauer}, H.},
title = {{Consistently Simulating a Wide Range of Atmospheric Scenarios for K2-18b with a Flexible Radiative Transfer Module}},
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},
year = 2020,
month = jul,
volume = {898},
number = {1},
eid = {44},
pages = {44},
doi = {10.3847/1538-4357/ab9084},
archiveprefix = {arXiv},
eprint = {2005.02114},
primaryclass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020ApJ...898...44S},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020A&A...639A.132B,
author = {{Bluhm}, P. and {Luque}, R. and {Espinoza}, N. and {Pall{\'e}}, E. and {Caballero}, J.~A. and {Dreizler}, S. and {Livingston}, J.~H. and {Mathur}, S. and {Quirrenbach}, A. and {Stock}, S. and {Van Eylen}, V. and {Nowak}, G. and {L{\'o}pez}, E.~D. and {Csizmadia}, Sz. and {Zapatero Osorio}, M.~R. and {Sch{\"o}fer}, P. and {Lillo-Box}, J. and {Oshagh}, M. and {Gonz{\'a}lez-{\'A}lvarez}, E. and {Amado}, P.~J. and {Barrado}, D. and {B{\'e}jar}, V.~J.~S. and {Cale}, B. and {Chaturvedi}, P. and {Cifuentes}, C. and {Cochran}, W.~D. and {Collins}, K.~A. and {Collins}, K.~I. and {Cort{\'e}s-Contreras}, M. and {D{\'\i}ez Alonso}, E. and {El Mufti}, M. and {Ercolino}, A. and {Fridlund}, M. and {Gaidos}, E. and {Garc{\'\i}a}, R.~A. and {Georgieva}, I. and {Gonz{\'a}lez-Cuesta}, L. and {Guerra}, P. and {Hatzes}, A.~P. and {Henning}, Th. and {Herrero}, E. and {Hidalgo}, D. and {Isopi}, G. and {Jeffers}, S.~V. and {Jenkins}, J.~M. and {Jensen}, E.~L.~N. and {K{\'a}bath}, P. and {Kaminski}, A. and {Kemmer}, J. and {Korth}, J. and {Kossakowski}, D. and {K{\"u}rster}, M. and {Lafarga}, M. and {Mallia}, F. and {Montes}, D. and {Morales}, J.~C. and {Morales-Calder{\'o}n}, M. and {Murgas}, F. and {Narita}, N. and {Passegger}, V.~M. and {Pedraz}, S. and {Persson}, C.~M. and {Plavchan}, P. and {Rauer}, H. and {Redfield}, S. and {Reffert}, S. and {Reiners}, A. and {Ribas}, I. and {Ricker}, G.~R. and {Rodr{\'\i}guez-L{\'o}pez}, C. and {Santos}, A.~R.~G. and {Seager}, S. and {Schlecker}, M. and {Schweitzer}, A. and {Shan}, Y. and {Soto}, M.~G. and {Subjak}, J. and {Tal-Or}, L. and {Trifonov}, T. and {Vanaverbeke}, S. and {Vanderspek}, R. and {Wittrock}, J. and {Zechmeister}, M. and {Zohrabi}, F.},
title = {{Precise mass and radius of a transiting super-Earth planet orbiting the M dwarf TOI-1235: a planet in the radius gap?}},
journal = {\aap},
keywords = {techniques: photometric, techniques: radial velocities, stars: individual: TOI-1235, stars: late-type, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
year = 2020,
month = jul,
volume = {639},
eid = {A132},
pages = {A132},
doi = {10.1051/0004-6361/202038160},
archiveprefix = {arXiv},
eprint = {2004.06218},
primaryclass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...639A.132B},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020A&A...639A..54L,
author = {{Lombart}, M. and {Chauvin}, G. and {Rojo}, P. and {Lagadec}, E. and {Delorme}, P. and {Beust}, H. and {Bonnefoy}, M. and {Galicher}, R. and {Gratton}, R. and {Mesa}, D. and {Bonavita}, M. and {Allard}, F. and {Bayo}, A. and {Boccaletti}, A. and {Desidera}, S. and {Girard}, J. and {Jenkins}, J.~S. and {Klahr}, H. and {Laibe}, G. and {Lagrange}, A. -M. and {Lazzoni}, C. and {Marleau}, G. -D. and {Minniti}, D. and {Mordasini}, C.},
title = {{VLT/SPHERE survey for exoplanets around young early-type stars, including systems with multi-belt architectures}},
journal = {\aap},
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,
volume = {639},
eid = {A54},
pages = {A54},
doi = {10.1051/0004-6361/202037961},
archiveprefix = {arXiv},
eprint = {2005.08850},
primaryclass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...639A..54L},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020A&A...639A..49G,
author = {{Guilluy}, G. and {Andretta}, V. and {Borsa}, F. and {Giacobbe}, P. and {Sozzetti}, A. and {Covino}, E. and {Bourrier}, V. and {Fossati}, L. and {Bonomo}, A.~S. and {Esposito}, M. and {Giampapa}, M.~S. and {Harutyunyan}, A. and {Rainer}, M. and {Brogi}, M. and {Bruno}, G. and {Claudi}, R. and {Frustagli}, G. and {Lanza}, A.~F. and {Mancini}, L. and {Pino}, L. and {Poretti}, E. and {Scandariato}, G. and {Affer}, L. and {Baffa}, C. and {Baruffolo}, A. and {Benatti}, S. and {Biazzo}, K. and {Bignamini}, A. and {Boschin}, W. and {Carleo}, I. and {Cecconi}, M. and {Cosentino}, R. and {Damasso}, M. and {Desidera}, S. and {Falcini}, G. and {Martinez Fiorenzano}, A.~F. and {Ghedina}, A. and {Gonz{\'a}lez-{\'A}lvarez}, E. and {Guerra}, J. and {Hernandez}, N. and {Leto}, G. and {Maggio}, A. and {Malavolta}, L. and {Maldonado}, J. and {Micela}, G. and {Molinari}, E. and {Nascimbeni}, V. and {Pagano}, I. and {Pedani}, M. and {Piotto}, G. and {Reiners}, A.},
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},
year = 2020,
month = jul,
volume = {639},
eid = {A49},
pages = {A49},
doi = {10.1051/0004-6361/202037644},
archiveprefix = {arXiv},
eprint = {2005.05676},
primaryclass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...639A..49G},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020A&A...639A..48S,
author = {{Shulyak}, D. and {Lara}, L.~M. and {Rengel}, M. and {N{\`e}mec}, N. -E.},
title = {{Stellar impact on disequilibrium chemistry and observed spectra of hot Jupiter atmospheres}},
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,
volume = {639},
eid = {A48},
pages = {A48},
doi = {10.1051/0004-6361/201937210},
archiveprefix = {arXiv},
eprint = {2005.01470},
primaryclass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...639A..48S},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020A&A...639A..35H,
author = {{Hojjatpanah}, S. and {Oshagh}, M. and {Figueira}, P. and {Santos}, N.~C. and {Amazo-G{\'o}mez}, E.~M. and {Sousa}, S.~G. and {Adibekyan}, V. and {Akinsanmi}, B. and {Demangeon}, O. and {Faria}, J. and {Gomes da Silva}, J. and {Meunier}, N.},
title = {{The correlation between photometric variability and radial velocity jitter. Based on TESS and HARPS observations}},
journal = {\aap},
keywords = {techniques: spectroscopic, planets and satellites: detection, techniques: radial velocities, techniques: photometric, stars: activity, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
year = 2020,
month = jul,
volume = {639},
eid = {A35},
pages = {A35},
doi = {10.1051/0004-6361/202038035},
archiveprefix = {arXiv},
eprint = {2005.10105},
primaryclass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...639A..35H},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020Sci...368.1477J,
author = {{Jeffers}, S.~V. and {Dreizler}, S. and {Barnes}, J.~R. and {Haswell}, C.~A. and {Nelson}, R.~P. and {Rodr{\'\i}guez}, E. and {L{\'o}pez-Gonz′lez}, M.~J. and {Morales}, N. and {Luque}, R. and {Zechmeister}, M. and {Vogt}, S.~S. and {Jenkins}, J.~S. and {Palle}, E. and {Berdi {\~n}as}, Z.~M. and {Coleman}, G.~A.~L. and {D{\'\i}az}, M.~R. and {Ribas}, I. and {Jones}, H.~R.~A. and {Butler}, R.~P. and {Tinney}, C.~G. and {Bailey}, J. and {Carter}, B.~D. and {O'Toole}, S. and {Wittenmyer}, R.~A. and {Crane}, J.~D. and {Feng}, F. and {Shectman}, S.~A. and {Teske}, J. and {Reiners}, A. and {Amado}, P.~J. and {Anglada-Escud{\'e}}, G.},
title = {{A multiplanet system of super-Earths orbiting the brightest red dwarf star GJ 887}},
journal = {Science},
keywords = {ASTRONOMY; PLANET SCI, Astrophysics - Earth and Planetary Astrophysics},
year = 2020,
month = jun,
volume = {368},
number = {6498},
pages = {1477-1481},
doi = {10.1126/science.aaz0795},
archiveprefix = {arXiv},
eprint = {2006.16372},
primaryclass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020Sci...368.1477J},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020MNRAS.496.5176D,
author = {{Deacon}, N.~R. and {Kraus}, A.~L.},
title = {{Wide binaries are rare in open clusters}},
journal = {\mnras},
keywords = {binaries: visual, stars: formation, open clusters and associations: individual, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Astrophysics of Galaxies},
year = 2020,
month = jun,
volume = {496},
number = {4},
pages = {5176-5200},
doi = {10.1093/mnras/staa1877},
archiveprefix = {arXiv},
eprint = {2006.06679},
primaryclass = {astro-ph.SR},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020MNRAS.496.5176D},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020A&A...638L...6E,
author = {{Eriksson}, Simon C. and {Asensio Torres}, Rub{\'e}n and {Janson}, Markus and {Aoyama}, Yuhiko and {Marleau}, Gabriel-Dominique and {Bonnefoy}, Mickael and {Petrus}, Simon},
title = {{Strong H{\ensuremath{\alpha}} emission and signs of accretion in a circumbinary planetary mass companion from MUSE}},
journal = {\aap},
keywords = {planets and satellites: individual: 2MASS J01033563-5515561 (AB)b (Delorme 1 (AB)b), planetary systems, accretion, accretion disks, stars: low-mass, techniques: imaging spectroscopy, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
year = 2020,
month = jun,
volume = {638},
eid = {L6},
pages = {L6},
doi = {10.1051/0004-6361/202038131},
archiveprefix = {arXiv},
eprint = {2005.11725},
primaryclass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...638L...6E},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020A&A...638A..86B,
author = {{Bhandare}, Asmita and {Kuiper}, Rolf and {Henning}, Thomas and {Fendt}, Christian and {Flock}, Mario and {Marleau}, Gabriel-Dominique},
title = {{Birth of convective low-mass to high-mass second Larson cores}},
journal = {\aap},
keywords = {stars: formation, methods: numerical, hydrodynamics, radiative transfer, equation of state, convection, Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Physics - Computational Physics},
year = 2020,
month = jun,
volume = {638},
eid = {A86},
pages = {A86},
doi = {10.1051/0004-6361/201937029},
archiveprefix = {arXiv},
eprint = {2004.12419},
primaryclass = {astro-ph.SR},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...638A..86B},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

@article{2020A&A...638A..61P,
author = {{Palle}, E. and {Nortmann}, L. and {Casasayas-Barris}, N. and {Lamp{\'o}n}, M. and {L{\'o}pez-Puertas}, M. and {Caballero}, J.~A. and {Sanz-Forcada}, J. and {Lara}, L.~M. and {Nagel}, E. and {Yan}, F. and {Alonso-Floriano}, F.~J. and {Amado}, P.~J. and {Chen}, G. and {Cifuentes}, C. and {Cort{\'e}s-Contreras}, M. and {Czesla}, S. and {Molaverdikhani}, K. and {Montes}, D. and {Passegger}, V.~M. and {Quirrenbach}, A. and {Reiners}, A. and {Ribas}, I. and {S{\'a}nchez-L{\'o}pez}, A. and {Schweitzer}, A. and {Stangret}, M. and {Zapatero Osorio}, M.~R. and {Zechmeister}, M.},
title = {{A He I upper atmosphere around the warm Neptune GJ 3470 b}},
journal = {\aap},
keywords = {planetary systems, planets and satellites: atmospheres, planet-star interactions, planets and satellites: general, planets and satellites: individual: GJ 3470b, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
year = 2020,
month = jun,
volume = {638},
eid = {A61},
pages = {A61},
doi = {10.1051/0004-6361/202037719},
archiveprefix = {arXiv},
eprint = {2004.12812},
primaryclass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020A&A...638A..61P},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}