TYC 3554-1762-1 , the SIMBAD biblio

TYC 3554-1762-1 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.17CEST00:06:55


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Title First 3 Authors
2013A&A...557L..10N viz 16       D               1 12151 189 Rotation periods of 12000 main-sequence Kepler stars: dependence on stellar spectral type and comparison with v sin i observations. NIELSEN M.B., GIZON L., SCHUNKER H., et al.
2014ApJS..210....1C viz 16       D               1 519 296 Asteroseismic fundamental properties of solar-type stars observed by the NASA Kepler mission. CHAPLIN W.J., BASU S., HUBER D., 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.
2014A&A...572A..34G viz 16       D               1 315 228 Rotation and magnetism of Kepler pulsating solar-like stars. Towards asteroseismically calibrated age-rotation relations. GARCIA R.A., CEILLIER T., SALABERT D., et al.
2015ApJ...808..187B viz 16       D               1 540 73 The metallicities of stars with and without transiting planets. BUCHHAVE L.A. and LATHAM D.W.
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...844..102H viz 16       D               1 2236 180 Asteroseismology and Gaia: testing scaling relations using 2200 Kepler stars with TGAS parallaxes. HUBER D., ZINN J., BOJSEN-HANSEN M., et al.
2018ApJ...861..149F viz 16       D               1 2261 6 The Kepler Follow-up Observation Program. II. Stellar parameters from medium- and high-resolution spectroscopy. FURLAN E., CIARDI D.R., COCHRAN W.D., et al.
2020ApJS..247....9Z viz 17       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 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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