TYC 3542-328-1 , the SIMBAD biblio

TYC 3542-328-1 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST21:49:41


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Title First 3 Authors
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.
2016A&A...594A..39F viz 16       D               1 51408 86 Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra. FRASCA A., MOLENDA-ZAKOWICZ J., DE CAT P., et al.
2017ApJ...835...75J viz 16       D               1 211 3 Rotation periods of wide binaries in the Kepler field. JANES K.A.
2017MNRAS.472..675A viz 16       D               1 13582 89 Wide binaries in Tycho-Gaia: search method and the distribution of orbital separations. ANDREWS J.J., CHANAME J. and AGUEROS M.A.
2018MNRAS.479.4440G 16       D               2 129 3 On the identification of wide binaries in the Kepler field. GODOY-RIVERA D. and CHANAME J.
2020ApJS..247....9Z viz 16       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.
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.
2022MNRAS.514.1071M viz 17       D               1 2315 ~ A measurement of stellar surface gravity hidden in radial velocity differences of comoving stars. MOSCHELLA M., SLONE O., DROR J.A., 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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