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KOI-7589 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.05.04CEST11:31:55 |
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...557L..10N | 16 | D | 1 | 12151 | 189 | Rotation periods of 12000 main-sequence Kepler stars: dependence on stellar spectral type and comparison with v sin i observations. | NIELSEN M.B., GIZON L., SCHUNKER H., et al. | ||
2016ApJ...822...86M | 16 | D | 1 | 6130 | 337 | False positive probabilities for all Kepler objects of interest: 1284 newly validated planets and 428 likely false positives. | MORTON T.D., BRYSON S.T., COUGHLIN J.L., et al. | ||
2016PASP..128g4502M | 16 | D | 1 | 305 | 14 | Identifying false alarms in the Kepler planet candidate catalog. | MULLALLY F., COUGHLIN J.L., THOMPSON S.E., et al. | ||
2018AJ....155..161Z | 16 | D | 1 | 1274 | 24 | Robo-AO Kepler survey. IV. The effect of nearby stars on 3857 planetary candidate systems. | ZIEGLER C., LAW N.M., BARANEC C., et al. | ||
2018ApJ...866...99B | 16 | D | 1 | 7129 | 233 | Revised radii of Kepler stars and planet's using Gaia Data Release 2. | BERGER T.A., HUBER D., GAIDOS E., et al. | ||
2019MNRAS.485.2380M | 17 | D | 1 | 14330 | 108 | Gaia-derived luminosities of Kepler A/F stars and the pulsator fraction across the δ Scuti instability strip. | MURPHY S.J., HEY D., VAN REETH T., et al. | ||
2020ApJ...890...23L | 17 | D | 1 | 4935 | 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. | ||
2020AJ....160..108B | 17 | D | 1 | 6855 | 109 | The Gaia-Kepler stellar properties catalog. II. Planet radius demographics as a function of stellar mass and age. | BERGER T.A., HUBER D., GAIDOS E., et al. | ||
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. |