KOI-3568 , the SIMBAD biblio

KOI-3568 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST11:06:35

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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....142..160S viz 15       D               1 2325 365 Kepler eclipsing binary stars. II. 2165 eclipsing binaries in the second data release. SLAWSON R.W., PRSA A., WELSH W.F., et al.
2014MNRAS.437.3473A viz 16       D               1 2614 45 A catalogue of temperatures for Kepler eclipsing binary stars. ARMSTRONG D.J., GOMEZ MAQUEO CHEW Y., FAEDI F., et al.
2014AJ....147..119C viz 16       D               2 8010 91 Contamination in the Kepler field. Identification of 685 KOIs as false positives via ephemeris matching based on Q1-Q12 data. COUGHLIN J.L., THOMPSON S.E., BRYSON S.T., et al.
2015ApJS..217...16R viz 16       D               1 8625 149 Planetary candidates observed by Kepler. V. Planet sample from Q1-Q12 (36 months). ROWE J.F., COUGHLIN J.L., ANTOCI V., et al.
2016ApJ...822...86M viz 16       D               1 6130 337 False positive probabilities for all Kepler objects of interest: 1284 newly validated planets and 428 likely false positives. MORTON T.D., BRYSON S.T., COUGHLIN J.L., et al.
2016ApJ...824...15V viz 16       D               1 982 20 Orbital circularization of hot and cool Kepler eclipsing binaries. VAN EYLEN V., WINN J.N. and ALBRECHT S.
2017MNRAS.465.2634A viz 16       D               1 5400 21 Transit shapes and self-organizing maps as a tool for ranking planetary candidates: application to Kepler and K2. ARMSTRONG D.J., POLLACCO D. and SANTERNE A.
2017AJ....154..105K viz 16       D               1 532 5 Orbital parameters of the eclipsing detached Kepler binaries with eccentric orbits. KJURKCHIEVA D., VASILEVA D. and ATANASOVA T.
2018ApJS..235....5Q viz 16       D               1 2048 72 Physical properties and evolutionary states of EA-type eclipsing binaries observed by LAMOST. QIAN S.-B., ZHANG J., HE J.-J., et al.

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