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| K2-285b , the SIMBAD biblio (12 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST05:48:26 |
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More on score
| 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 | 66 | A | X | 2 | 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. | |
2019ApJ...880L...1A 
|
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. | ||
| 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
|
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 | 100 | D | C | 2 | 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. | ||
|
2024A&A...685A.143M
|
18 | D | 2 | 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. | |||||
| 2025ApJ...987...85R | 19 | D | 1 | 241 | ~ | Characterizing Exoplanets for Assessing Their Potential Habitability. | RODRIGUEZ-MOZOS J.M. and MOYA A. |
