|
other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
| TOI-125c , the SIMBAD biblio (21 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST05:54:53 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2019AJ....158..177Q |
879 | A | X C | 21 | 19 | 43 | Near-resonance in a system of sub-Neptunes from TESS. | QUINN S.N., BECKER J.C., RODRIGUEZ J.E., et al. | |
| 2020MNRAS.492.5399N | 1277 | A | D | X C F | 30 | 21 | 27 | Mass determinations of the three mini-Neptunes transiting TOI-125. | NIELSEN L.D., GANDOLFI D., ARMSTRONG D.J., et al. |
|
2020AJ....159..239G |
16 | D | 2 | 1408 | ~ | Updated parameters and a new transmission spectrum of HD 97658b. | GUO X., CROSSFIELD I.J.M., DRAGOMIR D., et al. | ||
| 2020AJ....160..113B | 16 | D | 1 | 38 | 14 | HD 191939: three sub-Neptunes transiting a Sun-like star only 54 pc away. | BADENAS-AGUSTI M., GUNTHER M.N., DAYLAN T., et al. | ||
|
2021ApJS..254...39G |
17 | D | 1 | 2206 | 165 | The TESS Objects of Interest Catalog from the TESS Prime Mission. | GUERRERO N.M., SEAGER S., HUANG C.X., 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. | ||
| 2021A&A...653A.105O | 42 | X | 1 | 11 | 4 | TESS and HARPS reveal two sub-Neptunes around TOI 1062. | OTEGI J.F., BOUCHY F., HELLED R., 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. | ||
| 2021AJ....162..242B | 84 | C | 1 | 7 | ~ | A general origin for multiplanetary systems with significantly misaligned USP planets. | BREFKA L. and BECKER J.C. | ||
|
2022MNRAS.511.1043W |
43 | X | 1 | 32 | 22 | A pair of sub-Neptunes transiting the bright K-dwarf TOI-1064 characterized with CHEOPS. | WILSON T.G., GOFFO E., ALIBERT Y., et al. | ||
|
2022AJ....164...15E |
17 | D | 1 | 514 | 13 | The Ariel Target List: The Impact of TESS and the Potential for Characterizing Multiple Planets within a System. | EDWARDS B. and TINETTI G. | ||
| 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. | ||
|
2023ApJS..265....4K |
17 | D | 1 | 454 | 2 | ExoClock Project. III. 450 New Exoplanet Ephemerides from Ground and Space Observations. | KOKORI A., TSIARAS A., EDWARDS B., et al. | ||
|
2023A&A...676A.106B |
17 | D | 1 | 76 | ~ | ExoMDN: Rapid characterization of exoplanet interior structures with mixture density networks. | BAUMEISTER P. and TOSI N. | ||
| 2024ApJ...966..185C | 18 | D | 1 | 140 | ~ | Where Are the Water Worlds? Identifying Exo-water-worlds Using Models of Planet Formation and Atmospheric Evolution. | CHAKRABARTY A. and MULDERS G.D. | ||
|
2024A&A...685A.143M |
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 |
18 | D | 2 | 140 | ~ | Resonant sub-Neptunes are puffier. | LELEU A., DELISLE J.-B., BURN R., et al. | ||
| 2025MNRAS.537.3175A | 19 | D | 1 | 68 | ~ | The NCORES programme: precise planetary masses, null results, and insight into the planet mass distribution near the radius gap. | ARMSTRONG D.J., OSBORN A., BURN R., et al. | ||
| 2025ApJ...987...85R | 19 | D | 1 | 241 | ~ | Characterizing Exoplanets for Assessing Their Potential Habitability. | RODRIGUEZ-MOZOS J.M. and MOYA A. | ||
| 2026ApJS..282...37S | 20 | D | 1 | 94 | ~ | JWST Exoplanetary Worlds and Elemental Survey (JEWELS). I. High-precision Chemical Abundances of 20 FGK Planet-hosting Stars from JWST Cycle 2. | SUN Q. |