2MASS J18460190+4218461 , the SIMBAD biblio

2MASS J18460190+4218461 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST23:03:41

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		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.
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.
2016MNRAS.463.1624D 94       D         F     5 17 3 New Suns in the Cosmos II: differential rotation in Kepler Sun-like stars. DAS CHAGAS M.L., BRAVO J.P., COSTA A.D., et al.
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.
2019MNRAS.488.3274D viz 16       D               2 142 ~ Multifractal detrended moving average analysis of Kepler stars with surface differential rotation traces. DE FREITAS D.B., NEPOMUCENO M.M.F., CORDEIRO J.G., 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.
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.

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