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| KOI-8084 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST00:46:24 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
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. | ||
|
2017ApJ...834..207M |
16 | D | 1 | 4096 | 4 | Magnetic activity analysis for a sample of G-type main sequence Kepler targets. | MEHRABI A., HE H. and KHOSROSHAHI H. | ||
|
2020ApJS..247....9Z |
16 | D | 1 | 5575 | 26 | Magnetic activity of F-, G-, and K-type stars in the LAMOST-Kepler field. | ZHANG J., BI S., LI Y., et al. | ||
|
2020AJ....160...90A |
16 | D | 1 | 13200 | 33 | Exploring the evolution of stellar rotation using galactic kinematics. | ANGUS R., BEANE A., PRICE-WHELAN A.M., et al. | ||
| 2020AJ....160..200B | 16 | D | 1 | 96 | ~ | Reliability correction is key for robust Kepler occurrence rates. | BRYSON S., COUGHLIN J.L., KUNIMOTO M., 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. | ||
|
2021ApJS..255...17S |
17 | D | 1 | 39591 | 57 | Surface rotation and photometric activity for Kepler targets. II. G and F main-sequence stars and cool subgiant stars. | SANTOS A.R.G., BRETON S.N., MATHUR S., et al. | ||
|
2024MNRAS.533.1290S |
18 | D | 1 | 7737 | ~ | The impact of stellar metallicity on rotation and activity evolution in the Kepler field using gyro-kinematic ages. | SEE V., LU Y., AMARD L., et al. |