2MASS J19360237+4639506 , the SIMBAD biblio

2MASS J19360237+4639506 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.05.06CEST12:08:17


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Title First 3 Authors
2013A&A...560A...4R viz 16       D               1 24132 291 Rotation and differential rotation of active Kepler stars. REINHOLD T., REINERS A. and BASRI G.
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...809....8B viz 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 viz 16       D               1 20938 134 Rotation, differential rotation, and gyrochronology of active Kepler stars. REINHOLD T. and GIZON L.
2017MNRAS.469.4578H viz 16       D               1 8666 48 Deep learning classification in asteroseismology. HON M., STELLO D. and YU J.
2017A&A...605A.111C viz 16       D               1 531 81 Surface rotation of Kepler red giant stars. CEILLIER T., TAYAR J., MATHUR S., et al.
2018MNRAS.476.3233H viz 16       D               1 15009 17 Deep learning classification in asteroseismology using an improved neural network: results on 15 000 Kepler red giants and applications to K2 and TESS data. HON M., STELLO D. and YU J.
2020ApJS..247....9Z viz 17       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 viz 17       D               1 13200 33 Exploring the evolution of stellar rotation using galactic kinematics. ANGUS R., BEANE A., PRICE-WHELAN A.M., et al.
2020A&A...642A.225A viz 17       D               1 1044 ~ Inflection point in the power spectrum of stellar brightness variations. III. Facular versus spot dominance on stars with known rotation periods. AMAZO-GOMEZ E.M., SHAPIRO A.I., SOLANKI S.K., 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.

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