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| UCAC4 705-066565 , the SIMBAD biblio (12 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST23:20:06 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2013A&A...560A...4R |
15 | D | 1 | 24132 | 291 | Rotation and differential rotation of active Kepler stars. | REINHOLD T., REINERS A. and BASRI G. | ||
|
2014ApJS..211...24M |
15 | D | 1 | 34022 | 573 | Rotation periods of 34,030 Kepler main-sequence stars: the full autocorrelation sample. | McQUILLAN A., MAZEH T. and AIGRAIN S. | ||
|
2015ApJ...809....8B |
16 | D | 1 | 112329 | 282 | Terrestrial planet occurrence rates for the Kepler GK dwarf sample. | BURKE C.J., CHRISTIANSEN J.L., MULLALLY F., et al. | ||
|
2015A&A...583A..65R |
16 | D | 2 | 20938 | 134 | Rotation, differential rotation, and gyrochronology of active Kepler stars. | REINHOLD T. and GIZON L. | ||
|
2019AJ....157..143B |
16 | D | 1 | 423 | 5 | Re-evaluating small long-period confirmed planets from Kepler. | BURKE C.J., MULLALLY F., THOMPSON S.E., et al. | ||
|
2020ApJ...890...23L |
16 | D | 1 | 4936 | 35 | Current population statistics do not favor photoevaporation over core-powered mass loss as the dominant cause of the exoplanet radius gap. | LOYD R.O.P., SHKOLNIK E.L., SCHNEIDER A.C., et al. | ||
|
2020MNRAS.499.3481A |
16 | D | 1 | 28505 | 24 | Evidence for metallicity-dependent spin evolution in the Kepler field. | AMARD L., ROQUETTE J. and MATT S.P. | ||
|
2021AJ....161..189L |
17 | D | 1 | 29956 | 19 | Gyro-kinematic ages for around 30,000 Kepler stars. | LU Y., ANGUS R., CURTIS J.L., et al. | ||
| 2021MNRAS.504.5327A | 17 | D | 1 | 7000 | 19 | Exoplanet validation with machine learning: 50 new validated Kepler planets. | ARMSTRONG D.J., GAMPER J. and DAMOULAS T. | ||
|
2024AJ....168..129S |
18 | D | 3 | 350 | ~ | Revising Properties of Planet-Host Binary Systems. IV. The Radius Distribution of Small Planets in Binary Star Systems Is Dependent on Stellar Separation. | SULLIVAN K., KRAUS A.L., BERGER T.A., et al. | ||
|
2024A&A...689A.250C |
18 | D | 1 | 3075 | ~ | Mapping the exo-Neptunian landscape A ridge between the desert and savanna. | CASTRO-GONZALEZ A., BOURRIER V., LILLO-BOX J., et al. | ||
| 2025NatAs...9.1007K | 47 | X | 1 | 127 | ~ | Near-circular orbits for planets with Earth-like sizes and instellations around M and K dwarf stars. | KIPPING D., SOLANO-OROPEZA D., YAHALOMI D.A., et al. |