KOI-5 , the SIMBAD biblio

KOI-5 , the SIMBAD biblio (91 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST14:06:23

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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               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.
2012AJ....143...39C viz 15       D               1 90 34 A uniform search for secondary eclipses of hot Jupiters in Kepler Q2 light curves. COUGHLIN J.L. and LOPEZ-MORALES M.
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.
2012ApJ...752...53L 15       D               1 320 18 Debris disks in Kepler exoplanet systems. LAWLER S.M. and GLADMAN 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.
2012AJ....144...42A viz 15       D               4 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.
2013ApJS..204...24B viz 15       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..127H viz 15       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...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.
2013A&A...560A.112M 15       D               3 60 34 High-precision stellar limb-darkening measurements. A transit study of 38 Kepler planetary candidates. MUELLER H.M., HUBER K.F., CZESLA S., 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.
2014PASP..126...34P 15       D               2 26 36 Investigation of Kepler Objects of Interest stellar parameters from observed transit durations. PLAVCHAN P., BILINSKI C. and CURRIE T.
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.
2014ApJ...788L...9B viz 15       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 696     A D S   X C       17 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.
2014ApJ...794..133S 15       D               1 41 21 Statistical eclipses of close-in Kepler sub-saturns. SHEETS H.A. and DEMING D.
2015AJ....149...18K 133       D     X C       3 97 61 Detection of stars within : ∼0.8 in of Kepler objects of interest. KOLBL R., MARCY G.W., ISAACSON H., 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 55       D     X         2 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...806..248W viz 133       D     X         4 143 44 Influence of stellar multiplicity on planet formation. III. Adaptive optics imaging of Kepler stars with gas giant planets. WANG J., FISCHER D.A., HORCH E.P., 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..126V 429       S   X         10 105 201 Eccentricity from transit photometry: small planets in Kepler multi-planet systems have low eccentricities. VAN EYLEN V. and ALBRECHT S.
2015AJ....150..144T 718       D     X C       18 12 13 A comparison of spectroscopic versus imaging techniques for detecting close companions to Kepler objects of interest. TESKE J.K., EVERETT M.E., HIRSCH L., et al.
2015ApJ...813..130W viz 211       D     X         6 211 27 Influence of stellar multiplicity on planet formation. IV. Adaptive optics imaging of Kepler stars with multiple transiting planet candidates. WANG J., FISCHER D.A., XIE J.-W., et al.
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.
2015MNRAS.452.2127S viz 371       D     X         10 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 17       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.
2016AJ....151...68K viz 16       D               1 2915 316 Kepler eclipsing binary stars. VII. The catalog of eclipsing binaries found in the entire Kepler data set. KIRK B., CONROY K., PRSA 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....6W viz 16       D               3 3060 13 Calibration of LAMOST stellar surface gravities using the Kepler asteroseismic data. WANG L., WANG W., WU Y., et al.
2016AJ....152....8K viz 448       D     X C       11 389 203 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 16       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.
2016ApJ...831...20B viz 16       D               1 798 55 C/O and Mg/Si ratios of stars in the solar neighborhood. BREWER J.M. and FISCHER D.A.
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.
2016AJ....152..187M viz 16       D               1 471 74 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 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 56       D     X         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.
2017RAA....17....5W 16       D               2 180 4 Stellar parameters of main sequence turn-off star candidates observed with LAMOST and Kepler. WU Y.-Q., XIANG M.-S., ZHANG X.-F., 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.
2016PASP..128i4502E 16       D               1 35 16 Kea: a new tool to obtain stellar parameters from low to moderate signal-to-noise and high-resolution echelle spectra. ENDL M. and COCHRAN W.D.
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.
2017AJ....154..250L viz 16       D               1 2281 72 Tidal synchronization and differential rotation of Kepler eclipsing binaries. LURIE J.C., VYHMEISTER K., HAWLEY S.L., 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...861..149F viz 16       D               1 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.479..391K 16       D               1 101 11 Reliability of stellar inclination estimated from asteroseismology: analytical criteria, mock simulations, and Kepler data analysis. KAMIAKA S., BENOMAR O. and SUTO Y.
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.
2019A&A...622A.130B 16       D               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...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.
2019ApJS..244...43Z viz 16       D               1 1328 22 Unbiased distribution of binary parameters from LAMOST and Kepler observations. ZHANG J., QIAN S.-B., WU Y., et al.
2019A&A...631A.152A 16       D               2 121 ~ Dusty phenomena in the vicinity of giant exoplanets. ARKHYPOV O.V., KHODACHENKO M.L. and HANSLMEIER A.
2020ApJ...890...23L viz 16       D               1 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.
2020A&A...636A..85S viz 16       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 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.
2021AJ....161..164H viz 100       D       C       2 192 26 Speckle observations of TESS exoplanet host stars: understanding the binary exoplanet host star orbital period distribution. HOWELL S.B., MATSON R.A., CIARDI D.R., et al.
2021MNRAS.503.4092B 59       D     X         2 124 ~ 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...75L viz 17       D               1 517 28 Speckle observations of TESS exoplanet host stars. II. Stellar companions at 1-1000 au and implications for small planet detection. LESTER K.V., MATSON R.A., HOWELL S.B., et al.
2021AJ....162...98B viz 17       D               2 2175 ~ Seeking echoes of circumstellar disks in Kepler light curves. BROMLEY B.C., LEONARD A., QUINTANILLA A., 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.
2022ApJ...925L...5B 85           X         2 7 4 The Chaotic History of the Retrograde Multi-planet System in K2-290A Driven by Distant Stars. BEST S. and PETROVICH C.
2022AJ....163..128W viz 17       D               1 1570 6 The influence of 10 unique chemical elements in shaping the distribution of Kepler planets. WILSON R.F., CANAS C.I., MAJEWSKI S.R., 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.
2022MNRAS.512L..60H viz 17       D               1 1974 9 The flaring TESS Objects of Interest: flare rates for all two-minute cadence TESS planet candidates. HOWARD W.S.
2022MNRAS.512..648D 43           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.
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.
2022MNRAS.513..102C viz 17       D               1 961 6 The TESS Triple-9 Catalog: 999 uniformly vetted exoplanet candidates. CACCIAPUOTI L., KOSTOV V.B., KUCHNER M., et al.
2022A&A...663A...4S viz 17       D               1 14206 7 Assessment of [Fe/H] determinations for FGK stars in spectroscopic surveys. SOUBIRAN C., BROUILLET N. and CASAMIQUELA L.
2022ApJS..263...33C 783       D     X         19 85 2 An Early Catalog of Planet-hosting Multiple-star Systems of Order Three and Higher. CUNTZ M., LUKE G.E., MILLARD M.J., et al.
2022ApJ...941..175L 17       D               2 99 2 Meta-analysis of Photometric and Asteroseismic Measurements of Stellar Rotation Periods: The Lomb-Scargle Periodogram, Autocorrelation Function, and Wavelet and Rotational Splitting Analysis for 92 Kepler Asteroseismic Targets. LU Y., BENOMAR O., KAMIAKA S., et al.
2023ApJS..264...17Z viz 17       D               4 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.
2023A&A...672A.176P viz 17       D               1 2155 2 Mass-ratio distribution of contact binary stars. PESTA M. and PEJCHA O.
2024A&A...684A.113M 18       D               2 92 ~ Characterisation of FG-type stars with improved transport of chemical elements. MOEDAS N., BOSSINI D., DEAL M., et al.
2024A&A...685A..62I viz 18       D               1 2906 ~ Automated eccentricity measurement from raw eclipsing binary light curves with intrinsic variability. IJSPEERT L.W., TKACHENKO A., JOHNSTON C., et al.
2024AJ....168..129S viz 18       D               1 350 ~ Revising Properties of Planet-Host Binary Systems. IV. The Radius Distribution of Small Planets in Binary Star Systems Is Dependent on Stellar Separation. SULLIVAN K., KRAUS A.L., BERGER T.A., et al.
2024MNRAS.534..575E 1317       D     X C       29 51 ~ Orbital architectures of planet-hosting binaries - III. Testing mutual inclinations of stellar and planetary orbits in triple-star systems. EVANS E.L., DUPUY T.J., SULLIVAN K., et al.
2024A&A...689A.250C viz 18       D               1 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.
2025MNRAS.541.2553K 47           X         1 11 ~ Comprehensive analysis of CM Draconis: eclipse timing variations driven by either a third body or stellar magnetic activity. KALOMENI B. and YAKUT K.
2025AJ....170..212S 112       D     X         3 797 ~ A Homogeneous Catalog of Oscillating Solar-type Stars Observed by the Kepler Mission and a New Amplitude Scaling Relation Including Chromospheric Activity. SAYEED M., HUBER D., CHONTOS A., et al.
2026AJ....171...28H 20       D               1 28 ~ Detection of Exoplanets with Machine Learning Techniques Through Transit Light-curve Analysis. HOSSAIN M.S. and SADMAN M.

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