KOI-268.01 , the SIMBAD biblio

KOI-268.01 , the SIMBAD biblio (32 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST07:03:55


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Title First 3 Authors
2011PASP..123..412W viz 15       D               1 2897 398 The Exoplanet Orbit Database. WRIGHT J.T., KAKHOURI O., MARCY G.W., et al.
2013ApJS..204...24B viz 15       D               1 3274 922 Planetary candidates observed by Kepler. III. Analysis of the first 16 months of data. BATALHA N.M., ROWE J.F., BRYSON S.T., et al.
2013ApJ...767..127H viz 15       D               1 189 246 Fundamental properties of Kepler planet-candidate host stars using asteroseismology. HUBER D., CHAPLIN W.J., CHRISTENSEN-DALSGAARD J., et al.
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.
2014MNRAS.441..983D 81             C       1 15 141 PASTIS: Bayesian extrasolar planet validation - I. General framework, models, and performance. DIAZ R.F., ALMENARA J.M., SANTERNE A., et al.
2014ApJ...791...35L viz 15       D               2 800 137 Robotic laser adaptive optics imaging of 715 Kepler exoplanet candidates using Robo-AO. LAW N.M., MORTON T., BARANEC C., et al.
2015AJ....149...55E 172       D     X         5 48 34 High-resolution multi-band imaging for validation and characterization of small Kepler planets. EVERETT M.E., BARCLAY T., CIARDI D.R., 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.
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.
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.
2016AJ....152..158T viz 16       D               1 4388 37 Detection of potential transit signals in 17 quarters of Kepler data: results of the final Kepler mission transiting planet search (DR25). TWICKEN J.D., JENKINS J.M., SEADER S.E., et al.
2017AJ....153...25A viz 119           X         3 179 7 Probability of the physical association of 104 blended companions to Kepler Objects of Interest using visible and near-infrared adaptive optics photometry. ATKINSON D., BARANEC C., ZIEGLER C., et al.
2017AJ....154..108J viz 16       D               1 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.
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.
2018AJ....156...83Z viz 16       D               2 337 14 Robo-AO Kepler Survey. V. The effect of physically associated stellar companions on planetary systems. ZIEGLER C., LAW N.M., BARANEC C., et al.
2018MNRAS.479.4786V 18       D               1 117 318 An asteroseismic view of the radius valley: stripped cores, not born rocky. VAN EYLEN V., AGENTOFT C., LUNDKVIST M.S., et al.
2018ApJ...866...99B viz 16       D               1 7129 233 Revised radii of Kepler stars and planet's using Gaia Data Release 2. BERGER T.A., HUBER D., GAIDOS E., et al.
2018AJ....156..254W viz 16       D               1 1269 42 The California-Kepler Survey. VI. Kepler multis and singles have similar planet and stellar properties indicating a common origin. WEISS L.M., ISAACSON H.T., MARCY G.W., et al.
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.
2018ApJ...869...66H viz 16       D               1 99 ~ The application of autocorrelation SETI search techniques in an ATA survey. HARP G.R., ACKERMANN R.F., ASTORGA A., et al.
2019AJ....157...61V 17       D               2 110 147 The orbital eccentricity of small planet systems. VAN EYLEN V., ALBRECHT S., HUANG X., 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.
2019AJ....157..171K viz 16       D               1 4069 2 Visual analysis and demographics of Kepler transit timing variations. KANE M., RAGOZZINE D., FLOWERS X., 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.
2020ApJ...900L..44K viz 659     A D     X C       16 8 ~ An independent analysis of the six recently claimed exomoon candidates. KIPPING D.
2020ApJ...902L..20Q 66     A     X         2 7 ~ Application of orbital stability and tidal migration constraints for exomoon candidates. QUARLES B., LI G. and ROSARIO-FRANCO M.
2021MNRAS.501.2378F 184       D       C F     7 27 ~ Exomoon candidates from transit timing variations: eightKeplersystems with TTVs explainable by photometrically unseen exomoons. FOX C. and WIEGERT P.
2021A&A...645A.128Z 42           X         1 7 ~ Classification of orbits in three-dimensional exoplanetary systems. ZOTOS E.E., ERDI B. and SAEED T.
2021MNRAS.502.5292Z 42           X         1 15 ~ Mapping exomoon trajectories around Earth-like exoplanets. ZOTOS E.E., PAPADAKIS K.E. and WAGEH S.
2021MNRAS.505.1293S viz 17       D               1 573 7 Systematic search for long-term transit duration changes in Kepler transiting planets. SHAHAF S., MAZEH T., ZUCKER S., et al.
2025A&A...699A.166D 19       D               1 22 ~ Grand theft moons Formation of habitable moons around giant planets. DENCS Z., DOBOS V. and REGALY Z.
2026AJ....171...28H 20       D               2 28 ~ Detection of Exoplanets with Machine Learning Techniques Through Transit Light-curve Analysis. HOSSAIN M.S. and SADMAN M.

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