K2-285c , the SIMBAD biblio

K2-285c , the SIMBAD biblio (18 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST19:40:09

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2019A&A...623A..41P 147     A     X         4 6 9 Detection and Doppler monitoring of K2-285 (EPIC 246471491), a system of four transiting planets smaller than Neptune. PALLE E., NOWAK G., LUQUE R., et al.
2019A&A...623A.165E 163             C F     2 19 29 HD 219666 b: a hot-Neptune from TESS Sector 1. ESPOSITO M., ARMSTRONG D.J., GANDOLFI D., et al.
2019ApJ...880L...1A viz 16       D               1 146 ~ A gap in the mass distribution for warm Neptune and terrestrial planets. ARMSTRONG D.J., MERU F., BAYLISS D., et al.
2020A&A...634A..43O 16       D               1 141 104 Revisited mass-radius relations for exoplanets below 120 M⊕. OTEGI J.F., BOUCHY F. and HELLED R.
2020AJ....159..239G viz 16       D               1 1408 ~ Updated parameters and a new transmission spectrum of HD 97658b. GUO X., CROSSFIELD I.J.M., DRAGOMIR D., et al.
2020PASP..132e4401Z 16       D               1 81 38 Utilizing small telescopes operated by citizen scientists for transiting Exoplanet follow-up. ZELLEM R.T., PEARSON K.A., BLASER E., et al.
2021MNRAS.503.2825H 17       D               1 79 ~ Implications of an improved water equation of state for water-rich planets. HUANG C., RICE D.R., GRANDE Z.M., et al.
2021A&A...652A.110L 17       D               1 82 7 Why do more massive stars host larger planets? LOZOVSKY M., HELLED R., PASCUCCI I., et al.
2021ApJ...921...24S viz 17       D               1 328 1 The occurrence-weighted median planets discovered by transit surveys orbiting solar-type stars and their implications for planet formation and evolution. SCHLAUFMAN K.C. and HALPERN N.D.
2021A&A...656A.157B 17       D               1 48 9 Constraining stellar rotation and planetary atmospheric evolution of a dozen systems hosting sub-Neptunes and super-Earths. BONFANTI A., FOSSATI L., KUBYSHKINA D., et al.
2023MNRAS.519.6028R 17       D               1 86 7 Exoplanet atmosphere evolution: emulation with neural networks. ROGERS J.G., JANO MUNOZ C., OWEN J.E., et al.
2023A&A...676A.106B viz 17       D               1 76 ~ ExoMDN: Rapid characterization of exoplanet interior structures with mixture density networks. BAUMEISTER P. and TOSI N.
2024A&A...685A.143M viz 18       D               1 535 ~ Planets similar in size are often dissimilar in interior. MAMONOVA E., SHAN Y., HATALOVA P., et al.
2024MNRAS.531.3698H 206 ~ Shallower radius valley around low-mass hosts: evidence for icy planets, collisions, or high-energy radiation scatter. HO C.S.K., ROGERS J.G., VAN EYLEN V., et al.
2024A&A...687L...1L viz 18       D               1 140 ~ Resonant sub-Neptunes are puffier. LELEU A., DELISLE J.-B., BURN R., et al.
2024MNRAS.532.4752D 90           X         2 130 ~ The SHERLOCK pipeline: new exoplanet candidates in the WASP-16, HAT-P-27, HAT-P-26, and TOI-2411 systems. DEVORA-PAJARES M., POZUELOS F.J., THUILLIER A., et al.
2025ApJ...987...85R 19       D               1 241 ~ Characterizing Exoplanets for Assessing Their Potential Habitability. RODRIGUEZ-MOZOS J.M. and MOYA A.
2025A&A...701A.230M 93               F     1 33 ~ The Hot Neptune Initiative (HONEI) II. TOI-5795 b: A hot super-Neptune orbiting a metal-poor star. MANNI F., NAPONIELLO L., MANCINI L., et al.

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