Kepler-1093 , the SIMBAD biblio

Kepler-1093 , the SIMBAD biblio (29 results) C.D.S. - SIMBAD4 rel 1.8 - 2022.11.29CET02:12:26


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Title First 3 Authors
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.
2013ApJS..204...24B viz 16       D               1 3274 779 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.429.2001H viz 16       D               1 140 33 150 new transiting planet candidates from Kepler Q1-Q6 data. HUANG X., BAKOS G.A. and HARTMAN J.D.
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.
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.
2014ApJ...784...45R viz 16       D               1 1691 227 Validation of Kepler's multiple planet candidates. III. Light curve analysis and announcement of hundreds of new multi-planet systems. ROWE J.F., BRYSON S.T., MARCY G.W., et al.
2014AJ....147..119C viz 16       D               1 8008 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.
2015ApJ...801....3M viz 16       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.
2015ApJS..217...16R viz 16       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.
2015ApJ...807..170H viz 16       D               2 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...814..130M viz 16       D               2 2846 46 An increase in the mass of planetary systems around lower-mass stars. MULDERS G.D., PASCUCCI I. and APAI D.
2016ApJ...822...86M viz 16       D               1 6129 192 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.
2016AJ....152...18B viz 16       D               3 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.
2016ApJS..225....9H viz 16       D               2 2132 33 Transit timing observations from Kepler. IX. Catalog of the full long-cadence data set. HOLCZER T., MAZEH T., NACHMANI G., et al.
2016A&A...594A..39F viz 16       D               2 51409 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..187M viz 16       D               2 471 33 A super-solar metallicity for stars with hot rocky exoplanets. MULDERS G.D., PASCUCCI I., APAI D., et al.
2017AJ....153...71F viz 16       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.
2017MNRAS.465.2634A viz 16       D               2 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.
2017AJ....154..107P viz 16       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 16       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.
2017A&A...603A..30S viz 16       D               4 2500 14 Observational evidence for two distinct giant planet populations. SANTOS N.C., ADIBEKYAN V., FIGUEIRA P., et al.
2018ApJ...855..115B viz 17       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.
2018MNRAS.474.2094A viz 17       D               1 1073 17 Inferring probabilistic stellar rotation periods using Gaussian processes. ANGUS R., MORTON T., AIGRAIN S., et al.
2018AJ....156...83Z viz 17       D               2 337 1 Robo-AO Kepler Survey. V. The effect of physically associated stellar companions on planetary systems. ZIEGLER C., LAW N.M., BARANEC C., et al.
2018ApJS..237...38B viz 17       D               1 1111 ~ Spectral properties of cool stars: extended abundance analysis of Kepler Objects of Interest. BREWER J.M. and FISCHER D.A.
2018AJ....156..292T viz 17       D               1 647 ~ The effects of stellar companions on the observed transiting exoplanet radius distribution. TESKE J.K., CIARDI D.R., HOWELL S.B., et al.
2019ApJ...875...29M viz 17       D               1 2918 ~ 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 viz 17       D               2 4935 ~ 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.
2021AJ....161...68L viz 18       D               2 253 ~ Hot stars with Kepler planets have high obliquities. LOUDEN E.M., WINN J.N., PETIGURA E.A., et al.

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2022.11.29-02:12:26

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