TYC 3142-221-1 , the SIMBAD biblio

TYC 3142-221-1 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST05:37:21


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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.
2015AJ....150..126S 133       D     X C       3 80 4 KSwAGS: a Swift X-ray and UV survey of the Kepler field. I. SMITH K.L., BOYD P.T., MUSHOTZKY R.F., et al.
2016ApJ...829...23D viz 16       D               1 4045 212 The Kepler catalog of stellar flares. DAVENPORT J.R.A.
2016ApJ...831...27H 27 1 Rapidly rotating, X-ray bright stars in the Kepler field. HOWELL S.B., MASON E., BOYD P., et al.
2017ApJ...851..116M viz 16       D               1 472 73 Long-term photometric variability in Kepler full-frame images: magnetic cycles of Sun-like stars. MONTET B.T., TOVAR G. and FOREMAN-MACKEY D.
2019ApJS..241...29Y viz 16       D               1 3420 70 The flare catalog and the flare activity in the Kepler mission. YANG H. and LIU 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.
2020ApJS..251...15Z viz 16       D               1 20886 38 Phase II of the LAMOST-Kepler/K2 survey. I. Time series of medium-resolution Spectroscopic observations. ZONG W., FU J.-N., DE CAT P., et al.
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.
2022A&A...664A..78F viz 17       D               1 7452 7 Characterization of Kepler targets based on medium-resolution LAMOST spectra analyzed with ROTFIT,. FRASCA A., MOLENDA-ZAKOWICZ J., ALONSO-SANTIAGO J., et al.

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