2MASS J19380130+4556452 , the SIMBAD biblio

2MASS J19380130+4556452 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST14:18:56

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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
2011AJ....141...83P viz 15       D               1 1893 430 Kepler eclipsing binary stars. I. Catalog and principal characterization of 1879 eclipsing binaries in the first data release. PRSA A., BATALHA N., SLAWSON R.W., et al.
2011AJ....142..160S viz 15       D               1 2328 365 Kepler eclipsing binary stars. II. 2165 eclipsing binaries in the second data release. SLAWSON R.W., PRSA A., WELSH W.F., et al.
2012Natur.485..478M viz 16       D               1 148 419 Superflares on solar-type stars. MAEHARA H., SHIBAYAMA T., NOTSU S., et al.
2013ApJS..209....5S viz 15       D               1 285 309 Superflares on solar-type stars observed with Kepler. I. Statistical properties of superflares. SHIBAYAMA T., MAEHARA H., NOTSU S., 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.
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.
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.
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.
2025A&A...697A..80H 19       D               1 48 ~ Comparing the Sun to Sun-like stars The importance of addressing facular and/or spot domination. HERBST K., AMAZO-GOMEZ E.M. and PAPAIOANNOU A.

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