KOI-1287 , the SIMBAD biblio

KOI-1287 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST07:59:55


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in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
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Title First 3 Authors
2014ApJS..210...19B viz 15       D               1 5860 211 Planetary candidates observed by Kepler IV: planet sample from Q1-Q8 (22 months). BURKE C.J., BRYSON S.T., MULLALLY F., et al.
2014AJ....147..119C viz 15       D               1 8013 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.
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.
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.
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.
2018ApJS..234....9O viz 16       D               1 436 14 A spectral approach to transit timing variations. OFIR A., XIE J.-W., JIANG C.-F., et al.
2018AJ....155..161Z viz 16       D               2 1274 24 Robo-AO Kepler survey. IV. The effect of nearby stars on 3857 planetary candidate systems. ZIEGLER C., LAW N.M., BARANEC C., et al.
2021MNRAS.504.5327A 17       D               1 7000 19 Exoplanet validation with machine learning: 50 new validated Kepler planets. ARMSTRONG D.J., GAMPER J. and DAMOULAS T.
2024AJ....168..129S viz 18       D               1 350 ~ Revising Properties of Planet-Host Binary Systems. IV. The Radius Distribution of Small Planets in Binary Star Systems Is Dependent on Stellar Separation. SULLIVAN K., KRAUS A.L., BERGER T.A., et al.

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