KOI-363 , the SIMBAD biblio

KOI-363 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.7 - 2019.09.22CEST15:23:23


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Bibcode/DOI Score in Title|Abstract|
Keywords
in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
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Title First 3 Authors
2017MNRAS.465.2634A viz 18       D               1 5400 9 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.
2016ApJ...822...86M viz 17       D               1 6129 125 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.
2015ApJS..217...16R viz 17       D               1 8625 84 Planetary candidates observed by Kepler. V. Planet sample from Q1-Q12 (36 months). ROWE J.F., COUGHLIN J.L., ANTOCI V., et al.
2014AJ....147..119C viz 17       D               2 8005 55 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.
2014AJ....148...61T viz 17       D               1 288 13 WIYN open cluster study. LIX. Radial velocity membership of the evolved population of the old open cluster NGC 6791. TOFFLEMIRE B.M., GOSNELL N.M., MATHIEU R.D., et al.
2014ApJS..210...19B viz 17       D               1 5860 162 Planetary candidates observed by Kepler IV: planet sample from Q1-Q8 (22 months). BURKE C.J., BRYSON S.T., MULLALLY F., et al.
2012ApJS..199...24T viz 16       D               1 5393 51 Detection of potential transit signals in the first three quarters of Kepler mission data. TENENBAUM P., CHRISTIANSEN J.L., JENKINS J.M., et al.
2011AJ....142..160S viz 16       D               1 2320 258 Kepler eclipsing binary stars. II. 2165 eclipsing binaries in the second data release. SLAWSON R.W., PRSA A., WELSH W.F., et al.
2011ApJ...736...19B viz 16       D               1 1507 682 Characteristics of planetary candidates observed by Kepler. II. Analysis of the first four months of data. BORUCKI W.J., KOCH D.G., BASRI G., et al.

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2019.09.22-15:23:23

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