USNO-A2.0 1275-13156506 , the SIMBAD biblio

USNO-A2.0 1275-13156506 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST01:23:24


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Title First 3 Authors
2010AstL...36..338F viz 15       D               1 1150 6 Proper motions and CCD photometry of stars in the region of the open cluster NGC 6866. FROLOV V.N., ANANJEVSKAJA Y.K., GORSHANOV D.L., et al.
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.
2017ApJ...834..207M viz 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.
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 17       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.
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.
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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