Kepler-1652 , the SIMBAD biblio

Kepler-1652 , the SIMBAD biblio (43 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.20CEST02:24:19

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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
2013ApJS..204...24B viz 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...95D viz 56       D     X         2 164 581 The occurrence rate of small planets around small stars. DRESSING C.D. and CHARBONNEAU D.
2013ApJ...770...43M viz 16       D               1 202 41 Testing the metal of late-type Kepler planet hosts with iron-clad methods. MANN A.W., GAIDOS E., KRAUS A., et al.
2013ApJ...770...90G viz 16       D               1 74 60 Candidate planets in the habitable zones of Kepler stars. GAIDOS E.
2013ApJ...775L..11M viz 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 viz 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.
2013MNRAS.436.1883W viz 16       D               1 961 136 Rotation periods, variability properties and ages for Kepler exoplanet candidate host stars. WALKOWICZ L.M. and BASRI G.S.
2013ApJ...779..188M viz 16       D               1 342 155 Spectro-thermometry of M dwarfs and their candidate planets: too hot, too cool, or just right? MANN A.W., GAIDOS E. and ANSDELL M.
2014ApJS..210...19B viz 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 viz 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.
2014ApJS..213....5M viz 16       D               1 111 51 Characterizing the cool KOIs. VI. H- and K-band spectra of Kepler M dwarf planet-candidate hosts. MUIRHEAD P.S., BECKER J., FEIDEN G.A., et al.
2014ApJ...790...57C 47           X         1 6 102 Magnetospheric structure and atmospheric joule heating of habitable planets orbiting M-dwarf stars. COHEN O., DRAKE J.J., GLOCER A., et al.
2014ApJ...794L...5K 118           X C       2 51 18 On the frequency of potential Venus analogs from Kepler data. KANE S.R., KOPPARAPU R.K. and DOMAGAL-GOLDMAN S.D.
2014ApJ...795...60H 90           X         2 3 71 Most sub-arcsecond companions of Kepler exoplanet candidate host stars are gravitationally bound. HORCH E.P., HOWELL S.B., EVERETT M.E., et al.
2015AJ....149...24G 453       D     X         12 26 29 Hubble Space Telescope high-resolution imaging of Kepler small and cool exoplanet host stars. GILLILAND R.L., CARTIER K.M.S., ADAMS E.R., et al.
2015AJ....149...55E 40           X         1 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 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 viz 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...804...97C 2184   K A D S   X C       54 31 20 Revision of earth-sized Kepler planet candidate properties with high-resolution imaging by the Hubble Space Telescope. CARTIER K.M.S., GILLILAND R.L., WRIGHT J.T., et al.
2015ApJS..218...26S viz 16       D               1 275 13 Characterizing the cool KOIs. VIII. Parameters of the planets orbiting Kepler's coolest dwarfs. SWIFT J.J., MONTET B.T., VANDERBURG A., et al.
2015ApJ...807..170H viz 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.
2015ApJ...807...45D viz 175       D     X C       4 2707 726 The occurrence of potentially habitable planets orbiting M dwarfs estimated from the full Kepler dataset and an empirical measurement of the detection sensitivity. DRESSING C.D. and CHARBONNEAU D.
2015ApJ...814...91B viz 16       D               1 524 24 Comparative habitability of transiting exoplanets. BARNES R., MEADOWS V.S. and EVANS N.
2015ApJ...814..130M viz 16       D               1 2846 162 An increase in the mass of planetary systems around lower-mass stars. MULDERS G.D., PASCUCCI I. and APAI D.
2016ApJ...816...66B 49           X         1 15 145 The Kepler dichotomy among the M dwarfs: half of systems contain five or more coplanar planets. BALLARD S. and JOHNSON J.A.
2016ApJ...822...86M viz 16       D               1 6130 337 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..224...12C viz 16       D               1 1110 211 Planetary candidates observed by Kepler VII. The first fully uniform catalog based on the entire 48-month data set (Q1-Q17 DR24). COUGHLIN J.L., MULLALLY F., THOMPSON S.E., et al.
2016MNRAS.457.2877G viz 136       D     X         4 4245 141 They are small worlds after all: revised properties of Kepler M dwarf stars and their planets. GAIDOS E., MANN A.W., KRAUS A.L., et al.
2016AJ....152....8K viz 136       D     X         4 389 203 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 viz 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.
2016ApJ...830....1K 44           X         1 30 122 A catalog of Kepler habitable zone exoplanet candidates. KANE S.R., HILL M.L., KASTING J.F., et al.
2017AJ....153...71F viz 57       D     X         2 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....153..117H viz 16       D               2 170 51 Assessing the effect of stellar companions from high-resolution imaging of Kepler Objects of Interest. HIRSCH L.A., CIARDI D.R., HOWARD A.W., et al.
2017MNRAS.465.2634A viz 16       D               1 5400 21 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..264T 382       D     X C       9 51 17 Validation of small Kepler transiting planet candidates in or near the habitable zone. TORRES G., KANE S.R., ROWE J.F., et al.
2020ApJ...890...23L viz 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.
2020AJ....160..120J viz 17       D               1 365761 238 APOGEE data and spectral analysis from SDSS Data Release 16: seven years of observations including first results from APOGEE-South. JONSSON H., HOLTZMAN J.A., ALLENDE PRIETO C., et al.
2020AJ....160..253L viz 17       D               1 3432 12 An increase in small-planet occurrence with metallicity for late-type dwarf stars in the Kepler field and its implications for planet formation. LU C.X., SCHLAUFMAN K.C. and CHENG S.
2022MNRAS.512..648D 45           X         1 40 9 Orbital architectures of planet-hosting binaries - II. Low mutual inclinations between planetary and stellar orbits. DUPUY T.J., KRAUS A.L., KRATTER K.M., et al.
2022AJ....164..138S 90           X         2 32 1 Revising Properties of Planet-Host Binary Systems. II. Apparent Near-Earth-analog Planets in Binaries Are Often Sub-Neptunes. SULLIVAN K. and KRAUS A.L.
2023MNRAS.525.5168M 19       D               1 68 ~ Impact of M-dwarf stellar wind and photoevaporation on the atmospheric evolution of small planets. MODI A., ESTRELA R. and VALIO A.
2023ApJ...954L..50E 19       D               1 205 ~ Living with a Red Dwarf: The Rotation-Age Relationships of M Dwarfs. ENGLE S.G. and GUINAN E.F.
2023ApJ...956...29Q 19       D               1 40 ~ Prospects for Cryovolcanic Activity on Cold Ocean Planets. QUICK L.C., ROBERGE A., MENDOZA G.T., et al.

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