2MASS J19304741+4100044 , the SIMBAD biblio

2MASS J19304741+4100044 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST18:25:51


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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.
2015ApJ...809....8B viz 16       D               1 112329 282 Terrestrial planet occurrence rates for the Kepler GK dwarf sample. BURKE C.J., CHRISTIANSEN J.L., MULLALLY F., et al.
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.
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...90A viz 16       D               1 13200 33 Exploring the evolution of stellar rotation using galactic kinematics. ANGUS R., BEANE A., PRICE-WHELAN A.M., et al.
2020A&A...642A.225A viz 16       D               1 1044 ~ Inflection point in the power spectrum of stellar brightness variations. III. Facular versus spot dominance on stars with known rotation periods. AMAZO-GOMEZ E.M., SHAPIRO A.I., SOLANKI S.K., et al.
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.
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.
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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