2MASS J18564682+4412310 , the SIMBAD biblio

2MASS J18564682+4412310 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST00:30:04


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Title First 3 Authors
2011A&A...529A..89D viz 15       D               1 3298 98 Global stellar variability study in the field-of-view of the Kepler satellite. DEBOSSCHER J., BLOMME J., AERTS C., et al.
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.
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               2 20938 134 Rotation, differential rotation, and gyrochronology of active Kepler stars. REINHOLD T. and GIZON L.
2017PASJ...69...41M 161           X C       3 13 56 Starspot activity and superflares on solar-type stars. MAEHARA H., NOTSU Y., NOTSU S., et al.
2017MNRAS.472.1618G viz 16       D               2 1784 106 A Kepler study of starspot lifetimes with respect to light-curve amplitude and spectral type. GILES H.A.C., COLLIER CAMERON A. and HAYWOOD R.D.
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.
2022A&A...668A.167V viz 17       D               1 210 3 Superflares on solar-like stars A new method for identifying the true flare sources in photometric surveys. VASILYEV V., REINHOLD T., SHAPIRO A.I., 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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