Kepler-468 , the SIMBAD biblio

Kepler-468 , the SIMBAD biblio (41 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST06:07:40


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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.
2011AJ....142..160S viz 15       D               1 2328 365 Kepler eclipsing binary stars. II. 2165 eclipsing binaries in the second data release. SLAWSON R.W., PRSA A., WELSH W.F., 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.
2013MNRAS.436.1883W viz 15       D               1 961 136 Rotation periods, variability properties and ages for Kepler exoplanet candidate host stars. WALKOWICZ L.M. and BASRI G.S.
2014ApJS..210...19B viz 15       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.
2014MNRAS.437.3473A viz 15       D               1 2614 45 A catalogue of temperatures for Kepler eclipsing binary stars. ARMSTRONG D.J., GOMEZ MAQUEO CHEW Y., FAEDI F., et al.
2014AJ....147..119C viz 15       D               2 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.
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...809....8B viz 16       D               1 112329 282 Terrestrial planet occurrence rates for the Kepler GK dwarf sample. BURKE C.J., CHRISTIANSEN J.L., MULLALLY F., 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.
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.
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.
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.
2018ApJS..235....5Q viz 16       D               1 2048 72 Physical properties and evolutionary states of EA-type eclipsing binaries observed by LAMOST. QIAN S.-B., ZHANG J., HE J.-J., et al.
2018AJ....155..161Z viz 16       D               1 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               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.
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.
2018ApJ...869...66H viz 16       D               1 99 ~ The application of autocorrelation SETI search techniques in an ATA survey. HARP G.R., ACKERMANN R.F., ASTORGA A., et al.
2019AJ....158...59S viz 16       D               2 109 ~ Autoregressive planet search: feasibility study for irregular time series. STUHR A.M., FEIGELSON E.D., CACERES G.A., 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...638A.143A 16       D               1 193 ~ Variability of transit light curves of Kepler objects of interest. ARKHYPOV O.V., KHODACHENKO M.L. and HANSLMEIER A.
2020AJ....160..108B viz 99       D     X         3 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.
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.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.
2022AJ....163..179P viz 17       D               1 2962 39 The California-Kepler Survey. X. The Radius Gap as a Function of Stellar Mass, Metallicity, and Age. PETIGURA E.A., ROGERS J.G., ISAACSON H., et al.
2022ApJS..259...50S viz 17       D               1 1632 9 New Pulsating Stars Detected in EA-type Eclipsing-binary Systems Based on TESS Data. SHI X.-D., QIAN S.-B. and LI L.-J.
2022ApJS..261...26S viz 17       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.
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.
2023AJ....165...82J 17       D               1 167 3 Statistical Analysis of the Dearth of Super-eccentric Jupiters in the Kepler Sample. JACKSON J.M., DAWSON R.I., QUARLES B., et al.
2023A&A...672A.176P viz 17       D               1 2155 2 Mass-ratio distribution of contact binary stars. PESTA M. and PEJCHA O.
2023NatAs...7..900C viz 17       D               1 1054 ~ On the behaviour of spin-orbit connection of exoplanets. CANTO MARTINS B.L., MESSIAS Y.S., ARRUDA GONCALVES M.I., et al.
2023A&A...679L..12G viz 17       D               1 796 ~ Stellar spectral-type (mass) dependence of the dearth of close-in planets around fast-rotating stars Architecture of Kepler confirmed single-exoplanet systems compared to star-planet evolution models. GARCIA R.A., GOURVES C., SANTOS A.R.G., et al.
2024AJ....167...48M 108       D       C       5 72 ~ Signs of Similar Stellar Obliquity Distributions for Hot and Warm Jupiters Orbiting Cool Stars. MORGAN M., BOWLER B.P., TRAN Q.H., 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.
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...695A..81U 19       D               1 80 ~ Detection of oscillation-like patterns in eclipsing binary light curves using neural network-based object detection algorithms. ULAS B., SZKLENAR T. and SZABO R.

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