TYC 3162-509-1 , the SIMBAD biblio

TYC 3162-509-1 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST08:05:26


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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.
2016ApJ...822L..34S 17       D               1 14 39 KIC 8462852 faded at an average rate of 0.164 ± 0.013 magnitudes Per century from 1890 to 1989. SCHAEFER B.E.
2017ApJ...834..207M viz 16       D               1 4096 4 Magnetic activity analysis for a sample of G-type main sequence Kepler targets. MEHRABI A., HE H. and KHOSROSHAHI H.
2018A&A...615A..49C viz 16       D               1 224763 54 Characterising open clusters in the solar neighbourhood with the Tycho-Gaia Astrometric Solution. CANTAT-GAUDIN T., VALLENARI A., SORDO R., et al.
2018JAVSO..46...33C         O           9 ~ KIC 8462852: Maria Mitchell Observatory Photographic Photometry 1922 to 1991. CASTELAZ M. and BARKER T.
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.
2022AJ....163..152S viz 17       D               1 583193 11 APOGEE Net: An Expanded Spectral Model of Both Low-mass and High-mass Stars. SPRAGUE D., CULHANE C., KOUNKEL M., et al.
2022ApJS..259...35A viz 17       D               1 611005 320 The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data. ABDURRO'UF, ACCETTA K., AERTS C., et al.
2022ApJ...930....7A viz 17       D               1 4216 14 Rotation Distributions around the Kraft Break with TESS and Kepler: The Influences of Age, Metallicity, and Binarity. AVALLONE E.A., TAYAR J.N., VAN SADERS J.L., et al.

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