Kepler-462 , the SIMBAD biblio

Kepler-462 , the SIMBAD biblio (61 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST10:22:22

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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
2011ApJ...736...19B viz 15       D               1 1507 867 Characteristics of planetary candidates observed by Kepler. II. Analysis of the first four months of data. BORUCKI W.J., KOCH D.G., BASRI G., et al.
2011ApJ...738..170M viz 15       D               2 997 230 On the low false positive probabilities of Kepler planet candidates. MORTON T.D. and JOHNSON J.A.
2011ApJS..197....2F viz 15       D               1 980 66 Transit timing observations from Kepler. I. Statistical analysis of the first four months. FORD E.B., ROWE J.F., FABRYCKY D.C., et al.
2011ApJS..197....8L viz 16       D               1 177 608 Architecture and dynamics of Kepler's candidate multiple transiting planet systems. LISSAUER J.J., RAGOZZINE D., FABRYCKY D.C., et al.
2012MNRAS.420L..23V viz 38           X         1 94 22 Identifying non-resonant Kepler planetary systems. VERAS D. and FORD E.B.
2012ApJ...752...72D viz 15       D               1 229 7 A correlation between the eclipse depths of Kepler gas giant candidates and the metallicities of their parent stars. DODSON-ROBINSON S.E.
2012ApJ...756..185F viz 15       D               1 1856 44 Transit timing observations from Kepler. V. Transit timing variation candidates in the first sixteen months from polynomial models. FORD E.B., RAGOZZINE D., ROWE J.F., et al.
2013ApJ...774L..12S viz 15       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 15       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 15       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.
2014ApJS..210...19B viz 15       D               2 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.
2014ApJ...783....4W viz 15       D               1 487 103 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...784...45R viz 15       D               1 1691 388 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 15       D               1 8013 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.
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...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...67A 1544 T   A     X C       38 11 9 Spin-orbit misalignment of two-planet-system
KOI-89 via gravity darkening. 		AHLERS J.P., BARNES J.W. and BARNES R.
2015ApJ...814..130M viz 16       D               2 2846 162 An increase in the mass of planetary systems around lower-mass stars. MULDERS G.D., PASCUCCI I. and APAI D.
2015AJ....150..197H viz 78           X         2 24 32 HAT-P-57b: a short-period giant planet transiting a bright rapidly rotating A8V star confirmed via Doppler tomography. HARTMAN J.D., BAKOS G.A., BUCHHAVE L.A., et al.
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.
2016AJ....152....8K viz 16       D               1 389 203 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.
2016ApJ...827L..17M 39           X         1 26 22 A planet in an 840 day orbit around a Kepler main-sequence a star found from phase modulation of its pulsations. MURPHY S.J., BEDDING T.R. and SHIBAHASHI H.
2016ApJS..225....9H viz 16       D               4 2132 124 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               1 51408 86 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.
2017AJ....153...60M 80             C       1 5 16 The gravitational interaction between planets on inclined orbits and protoplanetary disks as the origin of primordial spin-orbit misalignments. MATSAKOS T. and KONIGL A.
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.
2017MNRAS.464.1709G 42           X         1 4 16 Outer-planet scattering can gently tilt an inner planetary system. GRATIA P. and FABRYCKY D.
2017MNRAS.465.2634A viz 16       D               2 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.
2016PASP..128g4502M viz 16       D               1 305 14 Identifying false alarms in the Kepler planet candidate catalog. MULLALLY F., COUGHLIN J.L., THOMPSON S.E., et al.
2017MNRAS.470..932H 40           X         1 10 5 Rapid rotators revisited: absolute dimensions of KOI-13. HOWARTH I.D. and MORELLO G.
2018ApJS..234....9O viz 177       D S     C       4 436 14 A spectral approach to transit timing variations. OFIR A., XIE J.-W., JIANG C.-F., 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.
2019MNRAS.485.2380M viz 16       D               1 14330 108 Gaia-derived luminosities of Kepler A/F stars and the pulsator fraction across the δ Scuti instability strip. MURPHY S.J., HEY D., VAN REETH T., et al.
2019ApJ...879...69T viz 16       D               1 222610 141 The Payne: self-consistent ab initio fitting of stellar spectra. TING Y.-S., CONROY C., RIX H.-W., et al.
2020ApJ...890...23L viz 16       D               2 4936 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...88W 44           X         1 18 61 Exploring the atmospheric dynamics of the extreme ultrahot Jupiter KELT-9b using TESS photometry. WONG I., SHPORER A., KITZMANN D., et al.
2020AJ....160..108B viz 16       D               2 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.
2020AJ....160..120J viz 16       D               1 365763 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.
2020MNRAS.497.4091M 82           X         2 57 ~ Dynamical evolution of two-planet systems and its connection with white dwarf atmospheric pollution. MALDONADO R.F., VILLAVER E., MUSTILL A.J., et al.
2020AJ....160..224M 1095 T   A S   X C       24 8 ~ Revisiting the architecture of the
KOI-89 system. 		MASUDA K. and TAMAYO D.
2021ApJ...909..115C viz 17       D               1 2176 13 Planets Across Space and Time (PAST). I. Characterizing the memberships of Galactic components and stellar ages: revisiting the kinematic methods and applying to planet host stars. CHEN D.-C., XIE J.-W., ZHOU J.-L., et al.
2021MNRAS.503.4092B 17       D               1 124 ~ Revisiting the Kepler field with TESS: Improved ephemerides using TESS 2 min data. BATTLEY M.P., KUNIMOTO M., ARMSTRONG D.J., et al.
2021MNRAS.504.5327A 17       D               1 7000 19 Exoplanet validation with machine learning: 50 new validated Kepler planets. ARMSTRONG D.J., GAMPER J. and DAMOULAS T.
2021AJ....162...98B viz 17       D               1 2175 ~ Seeking echoes of circumstellar disks in Kepler light curves. BROMLEY B.C., LEONARD A., QUINTANILLA A., et al.
2022MNRAS.510.2041C viz 43           X         1 315 3 The GALAH Survey: improving our understanding of confirmed and candidate planetary systems with large stellar surveys. CLARK J.T., WRIGHT D.J., WITTENMYER R.A., et al.
2022AJ....163..152S viz 17       D               1 583193 11 APOGEE Net: An Expanded Spectral Model of Both Low-mass and High-mass Stars. SPRAGUE D., CULHANE C., KOUNKEL M., et al.
2022ApJS..259...35A viz 17       D               1 611005 320 The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data. ABDURRO'UF, ACCETTA K., AERTS C., et al.
2022ApJS..259...63S viz 17       D               1 10269 2 Objective Separation between CP1 and CP2 Based on Feature Extraction with Machine Learning. SHANG L.-H., LUO A.-L., WANG L., et al.
2022ApJS..261...26S viz 17       D               3 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.
2022ApJ...935L..10G 128           X C       2 9 1 HD 56414 b: A Warm Neptune Transiting an A-type Star. GIACALONE S., DRESSING C.D., GARCIA MUNOZ A., et al.
2022PASP..134h2001A viz 128           X C       2 366 39 Stellar Obliquities in Exoplanetary Systems. ALBRECHT S.H., DAWSON R.I. and WINN J.N.
2023MNRAS.518.2068G viz 17       D               1 179 2 Chaos in multiplanetary extrasolar systems. GAJDOS P. and VANKO M.
2023ApJS..264...17Z viz 17       D               1 31380 1 Stellar Parameters and Spectroscopic Properties of TESS Objects Observed in the LAMOST Low- and Medium-resolution Spectral Survey. ZHANG L.-Y., SU T., MISRA P., et al.
2024AJ....167...55H viz 18       D               2 586 ~ Kepler-discovered Multiple-planet Systems near Period Ratios Suggestive of Mean-motion Resonances Are Young. HAMER J.H. and SCHLAUFMAN K.C.
2024AJ....168..109S viz 18       D               2 702 ~ Resonant and Ultra-short-period Planet Systems Are at Opposite Ends of the Exoplanet Age Distribution. SCHMIDT S.P., SCHLAUFMAN K.C. and HAMER J.H.
2024AJ....168..177C viz 18       D               1 260 ~ Detecting Exoplanet Transits with the Next Generation of X-Ray Telescopes. CILLEY R., KING G.W. and CORRALES L.
2024A&A...689A.250C viz 18       D               2 3075 ~ Mapping the exo-Neptunian landscape A ridge between the desert and savanna. CASTRO-GONZALEZ A., BOURRIER V., LILLO-BOX J., et al.
2024A&A...691A..53S viz 18       D               1 4078 ~ SWEET-Cat: A view on the planetary mass-radius relation. SOUSA S.G., ADIBEKYAN V., DELGADO-MENA E., et al.
2025A&A...699A.100D viz 19       D               1 2580 ~ The Gaia spectroscopic catalogue of exoplanets and host stars. DE LAVERNY P., LIGI R., CRIDA A., et al.
2026A&A...706A.222B 420       D S   X C       7 6 ~ ExoNAMD: Leveraging the spin-orbit angle to constrain the dynamics of multi-planet systems. BOCCHIERI A., ZAK J. and TURRINI D.

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