2MASS J19353106+4944009 , the SIMBAD biblio

2MASS J19353106+4944009 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST00:47:16

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2011A&A...529A..89D viz 15       D               1 3298 98 Global stellar variability study in the field-of-view of the Kepler satellite. DEBOSSCHER J., BLOMME J., AERTS C., et al.
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.
2015MNRAS.447.2714B viz 16       D               1 209 133 Flare stars across the H-R diagram. BALONA L.A.
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.
2016MNRAS.459.3659P 16       D               2 30 31 Statistical properties of quasi-periodic pulsations in white-light flares observed with Kepler. PUGH C.E., ARMSTRONG D.J., NAKARIAKOV V.M., et al.
2016ApJ...829...23D viz 16       D               1 4045 212 The Kepler catalog of stellar flares. DAVENPORT J.R.A.
2019ApJS..244...37G viz 16       D               1 1744 ~ Flare activity and magnetic feature analysis of the flare stars. GOODARZI H., MEHRABI A., KHOSROSHAHI H.G., 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.
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.
2024ApJS..274...31B 18       D               2 71 ~ Detecting Quasiperiodic Pulsations in Solar and Stellar Flares with a Neural Network. BELOV S.A., KOLOTKOV D.Y., NAKARIAKOV V.M., et al.

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