Kepler-402 , the SIMBAD biblio

Kepler-402 , the SIMBAD biblio (75 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST09:12:44

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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
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.429.2001H viz 54       D     X         2 140 33 150 new transiting planet candidates from Kepler Q1-Q6 data. HUANG X., BAKOS G.A. and HARTMAN J.D.
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.
2013MNRAS.435.1126B 15       D               1 72 20 Exoplanet predictions based on the generalized Titius-Bode relation. BOVAIRD T. and LINEWEAVER C.H.
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               4 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.
2014MNRAS.442..674H 54       D     X         2 40 10 Testing the Titius-Bode law predictions for Kepler multiplanet systems. HUANG C.X. and BAKOS G.A.
2014AJ....148...78D 248       D S   X         6 111 35 Adaptive optics images. III. 87 Kepler objects of interest. DRESSING C.D., ADAMS E.R., DUPREE A.K., 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.
2015MNRAS.448.3608B viz 16       D               6 156 6 Using the inclinations of Kepler systems to prioritize new Titius-Bode-based exoplanet predictions. BOVAIRD T., LINEWEAVER C.H. and JACOBSEN S.K.
2015ApJ...807..170H viz 16       D               3 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...813..100O viz 16       D               1 327 7 Deep GALEX UV survey of the Kepler field. I. Point source catalog. OLMEDO M., LLOYD J., MAMAJEK E.E., et al.
2015ApJ...814..130M viz 16       D               5 2846 162 An increase in the mass of planetary systems around lower-mass stars. MULDERS G.D., PASCUCCI I. and APAI D.
2016MNRAS.455.2980B 16       D               4 52 19 Oscillations of relative inclination angles in compact extrasolar planetary systems. BECKER J.C. and ADAMS F.C.
2016ApJ...821...47B viz 16       D               1 217 14 Efficient geometric probabilities of multi-transiting exoplanetary systems from CORBITS. BRAKENSIEK J. and RAGOZZINE D.
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...18B viz 16       D               4 1167 34 Robo-AO Kepler planetary candidate survey. II. Adaptive optics imaging of 969 Kepler exoplanet candidate host stars. BARANEC C., ZIEGLER C., LAW N.M., et al.
2016ApJS..225....9H viz 16       D               3 2132 124 Transit timing observations from Kepler. IX. Catalog of the full long-cadence data set. HOLCZER T., MAZEH T., NACHMANI G., et al.
2017AJ....153...25A viz 179 7 Probability of the physical association of 104 blended companions to Kepler Objects of Interest using visible and near-infrared adaptive optics photometry. ATKINSON D., BARANEC C., ZIEGLER C., 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..180S 16       D               2 119 3 A search for lost planets in the Kepler multi-planet systems and the discovery of the long-period, Neptune-sized exoplanet Kepler-150 f. SCHMITT J.R., JENKINS J.M. and FISCHER D.A.
2017MNRAS.465.2634A viz 16       D               5 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...602A.101R 40           X         1 69 10 Planetary migration and the origin of the 2:1 and 3:2 (near)-resonant population of close-in exoplanets. RAMOS X.S., CHARALAMBOUS C., BENITEZ-LLAMBAY P., et al.
2017MNRAS.468..549B 56       D     X         2 28 20 Effects of unseen additional planetary perturbers on compact extrasolar planetary systems. BECKER J.C. and ADAMS F.C.
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.
2017AJ....154..270W 16       D               2 70 21 Constraints on the obliquities of Kepler planet-hosting stars. WINN J.N., PETIGURA E.A., MORTON T.D., et al.
2018AJ....155...57C 41           X         1 34 51 The K2-138 system: a near-resonant chain of five sub-Neptune planets discovered by citizen scientists. CHRISTIANSEN J.L., CROSSFIELD I.J.M., BARENTSEN G., 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.
2018MNRAS.474.2094A viz 16       D               1 1073 143 Inferring probabilistic stellar rotation periods using Gaussian processes. ANGUS R., MORTON T., AIGRAIN S., 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               2 1111 42 Spectral properties of cool stars: extended abundance analysis of Kepler Objects of Interest. BREWER J.M. and FISCHER D.A.
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.
2018AJ....156..292T viz 16       D               1 647 8 The effects of stellar companions on the observed transiting exoplanet radius distribution. TESKE J.K., CIARDI D.R., HOWELL S.B., et al.
2019ApJ...875...29M viz 16       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.
2020ApJ...890...23L viz 16       D               5 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.
2020ApJ...890L..31L viz 16       D               1 85 ~ Mutual inclination excitation by stellar oblateness. LI G., DAI F. and BECKER J.
2020ApJ...893L...1W 123           X   F     2 51 33 The Kepler peas in a pod pattern is astrophysical. WEISS L.M. and PETIGURA E.A.
2020AJ....160..108B viz 16       D               5 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.
2021AJ....161...68L viz 17       D               2 253 24 Hot stars with Kepler planets have high obliquities. LOUDEN E.M., WINN J.N., PETIGURA E.A., 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.
2020PASJ...72...24L 16       D               1 90 ~ The reliability of the Titius-Bode relation and its implications for the search for exoplanets. LARA P., CORDERO-TERCERO G. and ALLEN C.
2021ApJ...910L..19C 84               F     1 61 ~ When the peas jump around the pod: how stellar clustering affects the observed correlations between planet properties in multiplanet systems. CHEVANCE M., KRUIJSSEN J.M.D. and LONGMORE S.N.
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.
2021ApJS..255...17S viz 17       D               1 39591 57 Surface rotation and photometric activity for Kepler targets. II. G and F main-sequence stars and cool subgiant stars. SANTOS A.R.G., BRETON S.N., MATHUR S., et al.
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.
2021ApJ...920...19G viz 17       D               1 807 5 A spectroscopic analysis of the California-Kepler Survey sample. II. Correlations of stellar metallicities with planetary architectures. GHEZZI L., MARTINEZ C.F., WILSON R.F., et al.
2021ApJ...920L..34M 84               F     1 48 16 Split peas in a pod: intra-system uniformity of super-Earths and sub-Neptunes. MILLHOLLAND S.C. and WINN J.N.
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.
2022AJ....164...60S viz 17       D               4 854 2 Galactic Chemical Evolution of Exoplanet Hosting Stars: Are High-mass Planetary Systems Young? SWASTIK C., BANYAL R.K., NARANG M., et al.
2022AJ....164...72M 85               F     1 61 6 Edge-of-the-Multis: Evidence for a Transition in the Outer Architectures of Compact Multiplanet Systems. MILLHOLLAND S.C., HE M.Y. and ZINK J.K.
2022ApJS..261...26S viz 17       D               1 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....166...94M viz 17       D               5 105 ~ exoMMR: A New Python Package to Confirm and Characterize Mean Motion Resonances. MacDONALD M.G., POLANIA VIVAS M.S., D'ANGIOLILLO S., et al.
2023ApJ...954..137S 87               F     1 64 ~ Can Cold Jupiters Sculpt the Edge-of-the-multis? SOBSKI N. and MILLHOLLAND S.C.
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.
2024AJ....167...55H viz 18       D               20 586 ~ Kepler-discovered Multiple-planet Systems near Period Ratios Suggestive of Mean-motion Resonances Are Young. HAMER J.H. and SCHLAUFMAN K.C.
2024AJ....167..103J viz 18       D               2 190 ~ Kepler Multitransiting System Physical Properties and Impact Parameter Variations. JUDKOVSKY Y., OFIR A. and AHARONSON O.
2024AJ....167..271V viz 152       D     X         4 165 ~ Differences between Stable and Unstable Architectures of Compact Planetary Systems. VOLK K. and MALHOTRA R.
2024ApJ...968L...4G 90               F     1 48 ~ Peas-in-a-pod across the Radius Valley: Rocky Systems Are Less Uniform in Mass but More Uniform in Size and Spacing. GOYAL A.V. and WANG S.
2024MNRAS.533.1290S viz 18       D               1 7737 ~ The impact of stellar metallicity on rotation and activity evolution in the Kepler field using gyro-kinematic ages. SEE V., LU Y., AMARD L., et al.
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.
2024ApJ...973L...4R 90               F     1 49 ~ The Distribution of Planet Radius in Kepler Multiplanet Systems Depends on Gap Complexity. RICE D.R., STEFFEN J.H. and VAZAN A.
2024A&A...689A.250C viz 18       D               5 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.
2025ApJ...980L..46H 19       D               1 92 ~ Short-period Small Planets with High Mutual Inclinations are More Common around Metal-rich Stars. HUA X., WANG S.X., AN D., et al.
2025A&A...695A.191Y 355     A     X C       7 19 ~ The dynamical history of the Kepler-221 planet system. YI T., ORMEL C.W., HUANG S., et al.
2025A&A...696A.174C 187           X C       3 17 ~ Can metal-rich worlds form by giant impacts? CAMBIONI S., WEISS B.P., ASPHAUG E., et al.
2025ApJ...986..178Q 19       D               1 450 ~ Revisiting the Li Abundances of Stars with and without Detected Planets from High-resolution Spectroscopy. QIN J., YAN H.-L., CUI W., et al.
2026ApJ...998..301G 20       D               1 561 ~ A Comprehensive Study of the Relations between the Properties of Planetary Systems and the Chemical Compositions of Their Host Stars. GHEZZI L., COSTA-ALMEIDA E., LOAIZA-TACURI V., et al.

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