TYC 3142-35-1 , the SIMBAD biblio

TYC 3142-35-1 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST23:51:41


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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               2 20938 134 Rotation, differential rotation, and gyrochronology of active Kepler stars. REINHOLD T. and GIZON L.
2016AJ....152..181H viz 16       D               1 9279 22 SETI observations of exoplanets with the Allen Telescope Array. HARP G.R., RICHARDS J., TARTER J.C., et al.
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.510.5623M viz 17       D               1 144 9 Inferring the rotation period distribution of stars from their projected rotation velocities and radii: Application to late-F/early-G Kepler stars. MASUDA K., PETIGURA E.A. and HALL O.J.
2023A&A...674A..34G viz 17       D               1 307215 85 Gaia Data Release 3 Stellar multiplicity, a teaser for the hidden treasure. GAIA COLLABORATION, ARENOU F., BABUSIAUX C., 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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