KOI-3097 , the SIMBAD biblio

KOI-3097 , the SIMBAD biblio (27 results) C.D.S. - SIMBAD4 rel 1.7 - 2019.09.22CEST00:25:26


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Title First 3 Authors
2019A&A...625A...7P 50           X         1 18 ~ The role of dissipative evolution for three-planet, near-resonant extrasolar systems. PICHIERRI G., BATYGIN K. and MORBIDELLI A.
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               6 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..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               3 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               1 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....8K viz 17       D               1 389 65 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.
2016AJ....152..187M viz 17       D               3 471 33 A super-solar metallicity for stars with hot rocky exoplanets. MULDERS G.D., PASCUCCI I., APAI D., et al.
2016ApJ...821...47B viz 17       D               1 217 14 Efficient geometric probabilities of multi-transiting exoplanetary systems from CORBITS. BRAKENSIEK J. and RAGOZZINE D.
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.
2016MNRAS.458.2051M 88           X         2 2 3 On the migration of three planets in a protoplanetary disc and the formation of chains of mean motion resonances. MIGASZEWSKI C.
2015AJ....149...55E 894     A D     X         22 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.
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...813..100O viz 17       D               1 327 7 Deep GALEX UV survey of the Kepler field. I. Point source catalog. OLMEDO M., LLOYD J., MAMAJEK E.E., et al.
2015ApJ...814..130M viz 17       D               3 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.
2015MNRAS.448.3608B viz 17       D               2 156 6 Using the inclinations of Kepler systems to prioritize new Titius-Bode-based exoplanet predictions. BOVAIRD T., LINEWEAVER C.H. and JACOBSEN S.K.
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.
2014AJ....148...78D 17       D               1 111 35 Adaptive optics images. III. 87 Kepler objects of interest. DRESSING C.D., ADAMS E.R., DUPREE A.K., et al.
2014ApJ...783....4W viz 17       D               1 487 55 Influence of stellar multiplicity on planet formation. I. Evidence of suppressed planet formation due to stellar companions within 20 AU and validation of four planets from the Kepler multiple planet candidates. WANG J., XIE J.-W., BARCLAY T., et al.
2014ApJ...788L...9B viz 17       D               1 293 26 Larger planet radii inferred from stellar "flicker" brightness variations of bright planet-host stars. BASTIEN F.A., STASSUN K.G. and PEPPER J.
2014ApJS..210...19B viz 17       D               3 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...770...69P viz 16       D               1 245 158 A plateau in the planet population below twice the size of Earth. PETIGURA E.A., MARCY G.W. and HOWARD A.W.
2013ApJ...774L..12S viz 16       D               1 469 25 A lack of short-period multiplanet systems with close-proximity pairs and the curious case of Kepler-42. STEFFEN J.H. and FARR W.M.
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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2019.09.22-00:25:26

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