2MASS J19501488+4824401 , the SIMBAD biblio

2MASS J19501488+4824401 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST23:28:27


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Title First 3 Authors
2013A&A...560A...4R viz 15       D               1 24132 291 Rotation and differential rotation of active Kepler stars. REINHOLD T., REINERS A. and BASRI G.
2014ApJS..211...24M viz 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.
2015A&A...583A..65R viz 16       D               1 20938 134 Rotation, differential rotation, and gyrochronology of active Kepler stars. REINHOLD T. and GIZON L.
2017A&A...603A..52R viz 16       D               1 3204 51 Evidence for photometric activity cycles in 3203 Kepler stars. REINHOLD T., CAMERON R.H. and GIZON L.
2019A&A...622A..85N viz 16       D               1 3093 3 Starspot rotation rates versus activity cycle phase: Butterfly diagrams of Kepler stars are unlike that of the Sun. NIELSEN M.B., GIZON L., CAMERON R.H., et al.
2019AJ....157..143B viz 16       D               1 423 5 Re-evaluating small long-period confirmed planets from Kepler. BURKE C.J., MULLALLY F., THOMPSON S.E., et al.
2020AJ....160...90A viz 16       D               1 13200 33 Exploring the evolution of stellar rotation using galactic kinematics. ANGUS R., BEANE A., PRICE-WHELAN A.M., et al.
2020MNRAS.499.3481A viz 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 viz 17       D               1 29956 19 Gyro-kinematic ages for around 30,000 Kepler stars. LU Y., ANGUS R., CURTIS J.L., et al.
2021ApJS..255...17S viz 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 viz 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.

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