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KOI-2640 , the SIMBAD biblio (25 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST19:22:18 |
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 |
---|---|---|---|---|---|---|---|---|---|
2012ApJ...756..185F | 15 | D | 1 | 1856 | 44 | Transit timing observations from Kepler. V. Transit timing variation candidates in the first sixteen months from polynomial models. | FORD E.B., RAGOZZINE D., ROWE J.F., et al. | ||
2013ApJS..204...24B | 16 | 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 | 16 | D | 1 | 189 | 246 | Fundamental properties of Kepler planet-candidate host stars using asteroseismology. | HUBER D., CHAPLIN W.J., CHRISTENSEN-DALSGAARD J., et al. | ||
2013ApJ...775L..11M | 16 | D | 1 | 2010 | 189 | Stellar rotation periods of the Kepler Objects of Interest: a dearth of close-in planets around fast rotators. | McQUILLAN A., MAZEH T. and AIGRAIN S. | ||
2013ApJS..208...16M | 16 | D | 1 | 1518 | 139 | Transit timing observations from Kepler. VIII. Catalog of transit timing measurements of the first twelve quarters. | MAZEH T., NACHMANI G., HOLCZER T., et al. | ||
2014ApJS..210...19B | 16 | 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 | 16 | D | 1 | 8010 | 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. | ||
2014A&A...566A.103L | 16 | D | 2 | 359 | 102 | High-resolution imaging of Kepler planet host candidates. A comprehensive comparison of different techniques. | LILLO-BOX J., BARRADO D. and BOUY H. | ||
2015ApJ...801....3M | 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...16R | 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...807..170H | 16 | D | 1 | 2117 | 10 | Time variation of Kepler transits induced by stellar Spots–A way to distinguish between prograde and retrograde motion. II. Application to KOIs. | HOLCZER T., SHPORER A., MAZEH T., et al. | ||
2016AJ....152....8K | 16 | D | 1 | 389 | 203 | The impact of stellar multiplicity on planetary systems. I. The ruinous influence of close binary companions. | KRAUS A.L., IRELAND M.J., HUBER D., et al. | ||
2016ApJS..225....9H | 16 | D | 1 | 2132 | 124 | Transit timing observations from Kepler. IX. Catalog of the full long-cadence data set. | HOLCZER T., MAZEH T., NACHMANI G., et al. | ||
2017AJ....153...71F | 16 | D | 1 | 3575 | 164 | The Kepler follow-up observation program. I. A catalog of companions to Kepler stars from high-resolution imaging. | FURLAN E., CIARDI D.R., EVERETT M.E., et al. | ||
2017AJ....154..107P | 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 | 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. | ||
2017MNRAS.469.4578H | 16 | D | 1 | 8666 | 48 | Deep learning classification in asteroseismology. | HON M., STELLO D. and YU J. | ||
2018ApJ...855..115B | 16 | D | 2 | 1305 | 5 | Identifying young Kepler planet host stars from Keck-HIRES spectra of lithium. | BERGER T.A., HOWARD A.W. and BOESGAARD A.M. | ||
2018MNRAS.474.2094A | 16 | D | 1 | 1073 | 143 | Inferring probabilistic stellar rotation periods using Gaussian processes. | ANGUS R., MORTON T., AIGRAIN S., et al. | ||
2018MNRAS.476.3233H | 16 | D | 1 | 15009 | 17 | Deep learning classification in asteroseismology using an improved neural network: results on 15 000 Kepler red giants and applications to K2 and TESS data. | HON M., STELLO D. and YU J. | ||
2018ApJ...861..149F | 16 | D | 1 | 2261 | 6 | The Kepler Follow-up Observation Program. II. Stellar parameters from medium- and high-resolution spectroscopy. | FURLAN E., CIARDI D.R., COCHRAN W.D., et al. | ||
2018ApJS..236...42Y | 16 | D | 1 | 16097 | 158 | Asteroseismology of 16,000 Kepler red giants: global oscillation parameters, masses, and radii. | YU J., HUBER D., BEDDING T.R., et al. | ||
2018ApJS..237...38B | 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. | ||
2019ApJ...875...29M | 17 | 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 | 17 | D | 1 | 4935 | 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. |