KOI-2119 , the SIMBAD biblio

KOI-2119 , the SIMBAD biblio (20 results) C.D.S. - SIMBAD4 rel 1.7 - 2019.10.22CEST12:04:37


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Bibcode/DOI Score in Title|Abstract|
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Title First 3 Authors
2018ApJ...855..115B viz 19       D               1 1305 2 Identifying young Kepler planet host stars from Keck-HIRES spectra of lithium. BERGER T.A., HOWARD A.W. and BOESGAARD A.M.
2017A&A...603A..30S viz 18       D               2 2500 14 Observational evidence for two distinct giant planet populations. SANTOS N.C., ADIBEKYAN V., FIGUEIRA P., et al.
2017AJ....153...71F viz 18       D               1 3575 46 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...60W 18       D               1 95 16 Absence of a metallicity effect for ultra-short-period planets. WINN J.N., SANCHIS-OJEDA R., ROGERS L., et al.
2017AJ....154..107P viz 18       D               1 1306 56 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 18       D               1 3237 46 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.465.2634A viz 18       D               1 5400 9 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.
2016ApJ...822...86M viz 17       D               1 6129 125 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.
2015ApJ...801....3M viz 17       D               1 3357 52 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.
2015ApJ...809....8B viz 17       D               1 112329 139 Terrestrial planet occurrence rates for the Kepler GK dwarf sample. BURKE C.J., CHRISTIANSEN J.L., MULLALLY F., et al.
2015ApJ...814..130M viz 17       D               1 2846 46 An increase in the mass of planetary systems around lower-mass stars. MULDERS G.D., PASCUCCI I. and APAI D.
2015ApJS..217...16R viz 17       D               1 8625 84 Planetary candidates observed by Kepler. V. Planet sample from Q1-Q12 (36 months). ROWE J.F., COUGHLIN J.L., ANTOCI V., et al.
2014AJ....147..119C viz 17       D               1 8005 55 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.
2014ApJ...787...47S viz 17       D               1 222 68 A study of the shortest-period planets found with Kepler. SANCHIS-OJEDA R., RAPPAPORT S., WINN J.N., et al.
2014ApJS..210...19B viz 17       D               1 5860 162 Planetary candidates observed by Kepler IV: planet sample from Q1-Q8 (22 months). BURKE C.J., BRYSON S.T., MULLALLY F., et al.
2013A&A...560A...4R viz 16       D               1 24132 153 Rotation and differential rotation of active Kepler stars. REINHOLD T., REINERS A. and BASRI G.
2013ApJ...775L..11M viz 16       D               1 2010 107 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..204...24B viz 16       D               1 3274 701 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.
2013MNRAS.436.1883W viz 16       D               1 961 86 Rotation periods, variability properties and ages for Kepler exoplanet candidate host stars. WALKOWICZ L.M. and BASRI G.S.
2012ApJS..199...24T viz 16       D               1 5393 51 Detection of potential transit signals in the first three quarters of Kepler mission data. TENENBAUM P., CHRISTIANSEN J.L., JENKINS J.M., et al.

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2019.10.22-12:04:37

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