Kepler-1582 , the SIMBAD biblio

Kepler-1582 , the SIMBAD biblio (22 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.16CEST20:29:39

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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
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.
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.
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...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 89             C       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.
2016MNRAS.457.2877G viz 16       D               1 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.
2017AJ....153...66Z viz 16       D               1 1663 45 Robo-AO Kepler Planetary Candidate Survey. III. Adaptive optics imaging of 1629 Kepler exoplanet candidate host stars. ZIEGLER C., LAW N.M., MORTON T., et al.
2017AJ....153...71F viz 16       D               1 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.
2017ApJS..229...30M viz 51           X         1 23 251 Revised stellar properties of Kepler targets for the Q1-17 (DR25) transit detection run. MATHUR S., HUBER D., BATALHA N.M., et al.
2017AJ....153..267M 81           X         2 42 16 The gold standard: accurate stellar and planetary parameters for eight Kepler M dwarf systems enabled by parallaxes. MANN A.W., DUPUY T., MUIRHEAD P.S., 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.
2017A&A...603A..30S viz 16       D               2 2500 58 Observational evidence for two distinct giant planet populations. SANTOS N.C., ADIBEKYAN V., FIGUEIRA P., et al.
2018ApJ...866...99B viz 16       D               1 7129 233 Revised radii of Kepler stars and planet's using Gaia Data Release 2. BERGER T.A., HUBER D., GAIDOS E., et al.
2019AJ....158...75H viz 184       D     X C       4 581 108 Kepler planet occurrence rates for mid-type M dwarfs as a function of spectral type. HARDEGREE-ULLMAN K.K., CUSHING M.C., MUIRHEAD P.S., et al.
2019ApJ...883..175Y viz 17       D               1 3032 66 SDSS-IV MaStar: a large and comprehensive empirical stellar spectral library-first release. YAN R., CHEN Y., LAZARZ D., 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..108B viz 17       D               1 6855 109 The Gaia-Kepler stellar properties catalog. II. Planet radius demographics as a function of stellar mass and age. BERGER T.A., HUBER D., GAIDOS E., et al.
2022ApJS..261...26S viz 18       D               2 1893 2 Magnetic Activity and Physical Parameters of Exoplanet Host Stars Based on LAMOST DR7, TESS, Kepler, and K2 Surveys. SU T., ZHANG L.-Y., LONG L., et al.

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