KOI-263 , the SIMBAD biblio

KOI-263 , the SIMBAD biblio (48 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.16CEST16:11:10


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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               1 997 230 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.
2012ApJS..199...24T viz 15       D               1 5394 66 Detection of potential transit signals in the first three quarters of Kepler mission data. TENENBAUM P., CHRISTIANSEN J.L., JENKINS J.M., et al.
2012Natur.486..375B viz 15       D               1 378 520 An abundance of small exoplanets around stars with a wide range of metallicities. BUCHHAVE L.A., LATHAM D.W., JOHANSEN A., et al.
2012AJ....144...42A viz 15       D               11 90 89 Adaptive optics images of Kepler Objects of Interest. ADAMS E.R., CIARDI D.R., DUPREE A.K., et al.
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.
2012ApJ...756..186S viz 15       D               1 811 35 Transit timing observations from Kepler. VI. Potentially interesting candidate systems from fourier-based statistical tests. STEFFEN J.H., FORD E.B., ROWE J.F., et al.
2012A&A...547A..36A viz 15       D               1 87 98 Exploring the α-enhancement of metal-poor planet-hosting stars. The Kepler and HARPS samples. ADIBEKYAN V.Zh., DELGADO MENA E., SOUSA S.G., et al.
2013ApJ...767..127H viz 16       D               1 189 246 Fundamental properties of Kepler planet-candidate host stars using asteroseismology. HUBER D., CHAPLIN W.J., CHRISTENSEN-DALSGAARD J., et al.
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.
2013A&A...560A...4R viz 16       D               1 24132 291 Rotation and differential rotation of active Kepler stars. REINHOLD T., REINERS A. and BASRI G.
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               2 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.
2014ApJ...788L...9B viz 16       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.
2014ApJ...791..111W 16       D               4 56 105 Influence of stellar multiplicity on planet formation. II. Planets are less common in multiple-star systems with separations smaller than 1500 AU. WANG J., FISCHER D.A., XIE J.-W., 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               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...808..187B viz 16       D               1 540 73 The metallicities of stars with and without transiting planets. BUCHHAVE L.A. and LATHAM D.W.
2015MNRAS.452.2127S viz 20       D               2 35 283 Ages and fundamental properties of Kepler exoplanet host stars from asteroseismology. SILVA AGUIRRE V., DAVIES G.R., BASU S., et al.
2016MNRAS.456.2183D 18       D               2 35 101 Oscillation frequencies for 35 Kepler solar-type planet-hosting stars using Bayesian techniques and machine learning. DAVIES G.R., SILVA AGUIRRE V., BEDDING T.R., 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.
2016ApJS..225....9H viz 16       D               2 2132 124 Transit timing observations from Kepler. IX. Catalog of the full long-cadence data set. HOLCZER T., MAZEH T., NACHMANI G., et al.
2016ApJS..225...32B viz 16       D               1 1473 266 Spectral properties of cool stars: extended abundance analysis of 1,617 planet-search stars. BREWER J.M., FISCHER D.A., VALENTI J.A., et al.
2016ApJ...830...31B 17       D               2 37 63 Fundamental parameters of main-sequence stars in an instant with machine learning. BELLINGER E.P., ANGELOU G.C., HEKKER S., 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.
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.
2017MNRAS.467..971B 16       D               1 56 38 ZASPE: a code to measure stellar atmospheric parameters and their covariance from spectra. BRAHM R., JORDAN A., HARTMAN J., et al.
2017ApJ...844..102H viz 16       D               1 2236 180 Asteroseismology and Gaia: testing scaling relations using 2200 Kepler stars with TGAS parallaxes. HUBER D., ZINN J., BOJSEN-HANSEN M., et al.
2017AJ....154..107P viz 16       D               1 1306 226 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 137 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.
2018AJ....155...68W viz 16       D               1 509 18 Elemental abundances of Kepler Objects of Interest in APOGEE. I. Two distinct orbital period regimes inferred from host star iron abundances. WILSON R.F., TESKE J., MAJEWSKI S.R., et al.
2018ApJ...855..115B viz 16       D               1 1305 5 Identifying young Kepler planet host stars from Keck-HIRES spectra of lithium. BERGER T.A., HOWARD A.W. and BOESGAARD A.M.
2018AJ....155..161Z viz 140       D     X         4 1274 24 Robo-AO Kepler survey. IV. The effect of nearby stars on 3857 planetary candidate systems. ZIEGLER C., LAW N.M., BARANEC C., et al.
2018ApJ...861..149F viz 16       D               2 2261 6 The Kepler Follow-up Observation Program. II. Stellar parameters from medium- and high-resolution spectroscopy. FURLAN E., CIARDI D.R., COCHRAN W.D., et al.
2018ApJS..237...38B viz 16       D               1 1111 42 Spectral properties of cool stars: extended abundance analysis of Kepler Objects of Interest. BREWER J.M. and FISCHER D.A.
2018MNRAS.481.3244G viz 16       D               1 3079 24 Chemo-kinematics of the Milky Way from the SDSS-III MARVELS survey. GRIEVES N., GE J., THOMAS N., et al.
2019A&A...622A.130B 59       D     X         2 97 34 Stellar ages, masses, and radii from asteroseismic modeling are robust to systematic errors in spectroscopy. BELLINGER E.P., HEKKER S., ANGELOU G.C., et al.
2019ApJ...875...29M viz 17       D               1 2918 72 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.
2019ApJ...879...69T viz 17       D               1 222609 141 The Payne: self-consistent ab initio fitting of stellar spectra. TING Y.-S., CONROY C., RIX H.-W., et al.
2019MNRAS.490.1509K 17       D               4 54 ~ Asteroseismic investigation of 20 planet and planet-candidate host stars. KAYHAN C., YILDIZ M. and CELIK ORHAN Z.
2020A&A...636A..85S viz 17       D               1 3696 ~ Derivation of parameters for 3748 FGK stars using H-band spectra from APOGEE Data Release 14. SARMENTO P., DELGADO MENA E., ROJAS-AYALA B., 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.
2021NatAs...5..707H viz 17       D               1 95 38 Weakened magnetic braking supported by asteroseismic rotation rates of Kepler dwarfs. HALL O.J., DAVIES G.R., VAN SADERS J., et al.
2024ApJ...962..138S 20       D               1 56 ~ Stellar Cruise Control: Weakened Magnetic Braking Leads to Sustained Rapid Rotation of Old Stars. SAUNDERS N., VAN SADERS J.L., LYTTLE A.J., et al.

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