KOI-5900 , the SIMBAD biblio

KOI-5900 , the SIMBAD biblio (18 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST04:19:54

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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
2014ApJ...787...47S viz 15       D               1 222 160 A study of the shortest-period planets found with Kepler. SANCHIS-OJEDA R., RAPPAPORT S., WINN J.N., et al.
2015ApJ...801....3M viz 16       D               1 3357 109 Photometric amplitude distribution of stellar rotation of KOIs–Indication for spin-orbit alignment of cool stars and high obliquity for hot stars. MAZEH T., PERETS H.B., McQUILLAN A., et al.
2015ApJS..217...31M viz 16       D               1 2033 213 Planetary candidates observed by Kepler. VI. Planet sample from Q1–Q16 (47 months). MULLALLY F., COUGHLIN J.L., THOMPSON S.E., 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               2 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..107P viz 16       D               1 1306 226 The California-Kepler Survey. I. High-resolution spectroscopy of 1305 stars hosting Kepler transiting planets. PETIGURA E.A., HOWARD A.W., MARCY G.W., et al.
2017AJ....154..108J viz 16       D               2 3237 137 The California-Kepler Survey. II. Precise physical properties of 2025 Kepler planets and their host stars. JOHNSON J.A., PETIGURA E.A., FULTON B.J., et al.
2018ApJ...855..115B viz 16       D               1 1305 5 Identifying young Kepler planet host stars from Keck-HIRES spectra of lithium. BERGER T.A., HOWARD A.W. and BOESGAARD A.M.
2018ApJS..237...38B viz 16       D               1 1111 42 Spectral properties of cool stars: extended abundance analysis of Kepler Objects of Interest. BREWER J.M. and FISCHER D.A.
2018AJ....156..264F viz 16       D               1 1909 365 The California-Kepler Survey. VII. Precise planet radii leveraging Gaia DR2 reveal the stellar mass dependence of the Planet radius gap. FULTON B.J. and PETIGURA E.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.
2019ApJ...875...29M viz 16       D               1 2918 72 A spectroscopic analysis of the California-Kepler Survey sample. I. Stellar parameters, planetary radii, and a slope in the radius gap. MARTINEZ C.F., CUNHA K., GHEZZI L., 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.
2020AJ....160..138H viz 16       D               1 72 17 Ultra-short-period planets are stable against tidal inspiral. HAMER J.H. and SCHLAUFMAN K.C.
2022AJ....163..179P viz 17       D               1 2962 39 The California-Kepler Survey. X. The Radius Gap as a Function of Stellar Mass, Metallicity, and Age. PETIGURA E.A., ROGERS J.G., ISAACSON H., et al.
2022A&A...663A...4S viz 17       D               1 14206 7 Assessment of [Fe/H] determinations for FGK stars in spectroscopic surveys. SOUBIRAN C., BROUILLET N. and CASAMIQUELA L.
2024AJ....168..109S viz 18       D               2 702 ~ Resonant and Ultra-short-period Planet Systems Are at Opposite Ends of the Exoplanet Age Distribution. SCHMIDT S.P., SCHLAUFMAN K.C. and HAMER J.H.

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