KIC 10959566 , the SIMBAD biblio

KIC 10959566 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.16CEST07:28:54


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Title First 3 Authors
2014ApJS..211...24M viz 16       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...807...45D viz 16       D               1 2707 726 The occurrence of potentially habitable planets orbiting M dwarfs estimated from the full Kepler dataset and an empirical measurement of the detection sensitivity. DRESSING C.D. and CHARBONNEAU D.
2016MNRAS.457.2877G viz 16       D               1 4245 141 They are small worlds after all: revised properties of Kepler M dwarf stars and their planets. GAIDOS E., MANN A.W., KRAUS A.L., et al.
2019ApJ...883..175Y viz 17       D               1 3032 66 SDSS-IV MaStar: a large and comprehensive empirical stellar spectral library-first release. YAN R., CHEN Y., LAZARZ D., et al.
2020ApJ...892...31B viz 17       D               1 14873 35 Temperatures and metallicities of M dwarfs in the APOGEE Survey. BIRKY J., HOGG D.W., MANN A.W., et al.
2020ApJ...899...62C viz 17       D               1 3001 ~ Stellar parameters for the first release of the MaSTar library: an empirical approach. CHEN Y.-P., YAN R., MARASTON C., et al.
2020AJ....160..120J viz 17       D               1 365761 238 APOGEE data and spectral analysis from SDSS Data Release 16: seven years of observations including first results from APOGEE-South. JONSSON H., HOLTZMAN J.A., ALLENDE PRIETO C., et al.
2020MNRAS.499.3481A viz 17       D               1 28505 24 Evidence for metallicity-dependent spin evolution in the Kepler field. AMARD L., ROQUETTE J. and MATT S.P.
2020AJ....160..253L viz 17       D               1 3432 12 An increase in small-planet occurrence with metallicity for late-type dwarf stars in the Kepler field and its implications for planet formation. LU C.X., SCHLAUFMAN K.C. and CHENG S.
2021AJ....161..189L viz 17       D               1 29956 19 Gyro-kinematic ages for around 30,000 Kepler stars. LU Y., ANGUS R., CURTIS J.L., et al.

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