TYC 3143-1140-1 , the SIMBAD biblio

TYC 3143-1140-1 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST04:58:56


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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.
2013MNRAS.431.2240B viz 15       D               1 899 128 Activity in A-type stars. BALONA L.A.
2016ApJ...829...23D viz 16       D               1 4045 212 The Kepler catalog of stellar flares. DAVENPORT J.R.A.
2016A&A...594A..39F viz 16       D               1 51408 86 Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra. FRASCA A., MOLENDA-ZAKOWICZ J., DE CAT P., et al.
2017MNRAS.467.1830B viz 16       D               1 642 26 Starspots on A stars. BALONA L.A.
2018MNRAS.479..183B viz 16       D               1 2598 17 Gaia luminosities of pulsating A-F stars in the Kepler field. BALONA L.A.
2019MNRAS.485.2380M viz 16       D               1 14330 108 Gaia-derived luminosities of Kepler A/F stars and the pulsator fraction across the δ Scuti instability strip. MURPHY S.J., HEY D., VAN REETH T., 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.
2023ApJS..264...17Z viz 17       D               3 31380 1 Stellar Parameters and Spectroscopic Properties of TESS Objects Observed in the LAMOST Low- and Medium-resolution Spectral Survey. ZHANG L.-Y., SU T., MISRA P., et al.
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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