KOI-2384 , the SIMBAD biblio

KOI-2384 , the SIMBAD biblio (16 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST06:21:18

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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
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.
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.
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.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.
2018AJ....155..144K 458       D     X         12 23 22 Discovery of three self-lensing binaries from Kepler. KAWAHARA H., MASUDA K., MacLEOD M., et al.
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.
2019ApJ...881L...3M 84               F     1 8 28 Self-lensing discovery of a 0.2 M☉ white dwarf in an unusually wide orbit around a Sun-like star. MASUDA K., KAWAHARA H., LATHAM D.W., et al.
2020ApJ...890...23L viz 16       D               1 4936 35 Current population statistics do not favor photoevaporation over core-powered mass loss as the dominant cause of the exoplanet radius gap. LOYD R.O.P., SHKOLNIK E.L., SCHNEIDER A.C., et al.
2020AJ....160..108B viz 16       D               1 6855 109 The Gaia-Kepler stellar properties catalog. II. Planet radius demographics as a function of stellar mass and age. BERGER T.A., HUBER D., GAIDOS E., 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.
2022MNRAS.512.1843H 17       D               1 15 13 The white dwarf binary pathways survey - VI. Two close post-common envelope binaries with TESS light curves. HERNANDEZ M.S., SCHREIBER M.R., PARSONS S.G., et al.
2024ApJ...961L..45S 833 T   A     X C       17 1 ~ The First TESS Self-lensing Pulses: Revisiting
KIC 12254688. 		SORABELLA N.M., LAYCOCK S.G.T., CHRISTODOULOU D.M., et al.
2024AJ....168..298S 45           X         1 2 ~ Simulating Self-lensing and Eclipsing Signals due to Detached Compact Objects in the TESS Light Curves. SAJADIAN S. and AFSHORDI N.
2025AJ....169....3S 47           X         1 5 ~ Finite-lens Effect on Self-lensing in Detached White Dwarfs-main Sequence Binary Systems. SAJADIAN S. and FATHEDDIN H.

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