KOI-2743 , the SIMBAD biblio

KOI-2743 , the SIMBAD biblio (19 results) C.D.S. - SIMBAD4 rel 1.7 - 2019.11.17CET17:26:38


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Title First 3 Authors
2018ApJ...855..115B viz 18       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 17       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 17       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..107P viz 17       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 17       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 17       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.
2016A&A...594A..39F viz 17       D               2 51408 21 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.
2016AJ....152...18B viz 17       D               2 1167 34 Robo-AO Kepler planetary candidate survey. II. Adaptive optics imaging of 969 Kepler exoplanet candidate host stars. BARANEC C., ZIEGLER C., LAW N.M., et al.
2016AJ....152..187M viz 17       D               1 471 33 A super-solar metallicity for stars with hot rocky exoplanets. MULDERS G.D., PASCUCCI I., APAI D., et al.
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.
2016ApJS..225....9H viz 17       D               1 2132 33 Transit timing observations from Kepler. IX. Catalog of the full long-cadence data set. HOLCZER T., MAZEH T., NACHMANI G., 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...807..170H viz 17       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.
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 16       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.
2014ApJS..210...19B viz 16       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.
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.

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2019.11.17-17:26:38

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