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| K2-231b , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.23CEST23:55:34 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
2018AJ....155..173C 
|
724 | T A | X C | 16 | 62 | 17 |
K2-231 b: a sub-Neptune exoplanet transiting a solar twin in Ruprecht 147. |
CURTIS J.L., VANDERBURG A., TORRES G., et al. | |
| 2019A&A...624A.110F | 42 | X | 1 | 64 | 34 | Survival rates of planets in open clusters: the Pleiades, Hyades, and Praesepe clusters. | FUJII M.S. and HORI Y. | ||
|
2019ApJS..244...11K
|
17 | D | 1 | 2120 | 48 | Detection of hundreds of new planet candidates and eclipsing binaries in K2 campaigns 0-8. | KRUSE E., AGOL E., LUGER R., et al. | ||
| 2019MNRAS.489.4311C | 18 | D | 1 | 43 | 49 | On the survivability of planets in young massive clusters and its implication of planet orbital architectures in globular clusters. | CAI M.X., PORTEGIES ZWART S., KOUWENHOVEN M.B.N., et al. | ||
|
2020AJ....159..239G
|
17 | D | 1 | 1408 | ~ | Updated parameters and a new transmission spectrum of HD 97658b. | GUO X., CROSSFIELD I.J.M., DRAGOMIR D., et al. | ||
|
2020ApJ...904..140C
|
43 | X | 1 | 1402 | 77 | When do stalled stars resume spinning down? Advancing gyrochronology with Ruprecht 147. | CURTIS J.L., AGUEROS M.A., MATT S.P., et al. | ||
| 2021MNRAS.505.3767N | 17 | D | 1 | 134 | 15 | A PSF-based Approach to TESS High quality data Of Stellar clusters (PATHOS) - IV. Candidate exoplanets around stars in open clusters: frequency and age-planetary radius distribution. | NARDIELLO D., DELEUIL M., MANTOVAN G., et al. | ||
|
2022A&A...664A.163N
|
18 | D | 1 | 148 | 11 | The GAPS Programme at TNG. XXXVII. A precise density measurement of the young ultra-short period planet TOI-1807 b,. | NARDIELLO D., MALAVOLTA L., DESIDERA S., et al. | ||
| 2022AJ....164..209M | 18 | D | 1 | 71 | 1 | Color Dependence of the Transit Detectability of Young Active M Dwarfs. | MIYAKAWA K., HIRANO T., SATO B., et al. |
