UCAC4 680-076231 , the SIMBAD biblio

UCAC4 680-076231 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST02:19:41


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Title First 3 Authors
2016AJ....151...68K viz 16       D               1 2915 316 Kepler eclipsing binary stars. VII. The catalog of eclipsing binaries found in the entire Kepler data set. KIRK B., CONROY K., PRSA A., et al.
2016ApJS..224...12C viz 16       D               1 1111 211 Planetary candidates observed by Kepler VII. The first fully uniform catalog based on the entire 48-month data set (Q1-Q17 DR24). COUGHLIN J.L., MULLALLY F., THOMPSON S.E., et al.
2016AJ....152..158T viz 16       D               1 4388 37 Detection of potential transit signals in 17 quarters of Kepler data: results of the final Kepler mission transiting planet search (DR25). TWICKEN J.D., JENKINS J.M., SEADER S.E., et al.
2017AJ....154..250L viz 16       D               1 2281 72 Tidal synchronization and differential rotation of Kepler eclipsing binaries. LURIE J.C., VYHMEISTER K., HAWLEY S.L., et al.
2018MNRAS.479..183B viz 16       D               1 2598 17 Gaia luminosities of pulsating A-F stars in the Kepler field. BALONA L.A.
2019A&A...630A.106G viz 16       D               1 308 39 Systematic search for stellar pulsators in the eclipsing binaries observed by Kepler. GAULME P. and GUZIK J.A.
2019ApJS..244...43Z viz 16       D               1 1328 22 Unbiased distribution of binary parameters from LAMOST and Kepler observations. ZHANG J., QIAN S.-B., WU Y., et al.
2022ApJS..262...12K viz 17       D               1 792 7 A Bayesian Analysis of Physical Parameters for 783 Kepler Close Binaries: Extreme-mass-ratio Systems and a New Mass Ratio versus Period Lower Limit. KOBULNICKY H.A., MOLNAR L.A., COOK E.M., et al.
2023A&A...672A.176P viz 17       D               1 2155 2 Mass-ratio distribution of contact binary stars. PESTA M. and PEJCHA O.
2024A&A...685A..62I viz 18       D               1 2906 ~ Automated eccentricity measurement from raw eclipsing binary light curves with intrinsic variability. IJSPEERT L.W., TKACHENKO A., JOHNSTON C., et al.

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