TYC 2666-23-1 , the SIMBAD biblio

TYC 2666-23-1 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST19:14:37


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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.
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.
2020AJ....160..120J viz 16       D               1 365763 238 APOGEE data and spectral analysis from SDSS Data Release 16: seven years of observations including first results from APOGEE-South. JONSSON H., HOLTZMAN J.A., ALLENDE PRIETO C., 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.
2021ApJ...906...40G viz 17       D               1 352 ~ Flare activity and magnetic feature analysis of the flare stars. II. Subgiant branch. GOODARZI H., MEHRABI A., KHOSROSHAHI H.G., et al.
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.
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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