Kepler-1542 , the SIMBAD biblio

Kepler-1542 , the SIMBAD biblio (66 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST14:00:57


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Title First 3 Authors
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.
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.
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               5 156 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...813..130W viz 16       D               1 211 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               4 2846 162 An increase in the mass of planetary systems around lower-mass stars. MULDERS G.D., PASCUCCI I. and APAI D.
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....8K viz 16       D               3 389 203 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.
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               4 471 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.
2017MNRAS.465.2634A viz 16       D               3 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.
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.
2017A&A...603A..30S viz 16       D               8 2500 58 Observational evidence for two distinct giant planet populations. SANTOS N.C., ADIBEKYAN V., FIGUEIRA P., 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...872...72C 97       D     X         3 15 ~ On the 9:7 mean motion resonance capture in a system of two equal-mass super-Earths. CUI Z., PAPALOIZOU J.C.B. and SZUSZKIEWICZ E.
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.
2019ApJS..241...29Y viz 16       D               1 3420 70 The flare catalog and the flare activity in the Kepler mission. YANG H. and LIU J.
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....159..207B 16       D               1 150 ~ Transit duration variations in multiplanet systems. BOLEY A.C., VAN LAERHOVEN C. and GRANADOS CONTRERAS A.P.
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.
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.
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.
2021ApJ...919..138T viz 17       D               1 531 12 Further evidence for tidal spin-up of hot Jupiter host stars. TEJADA AREVALO R.A., WINN J.N. and ANDERSON K.R.
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.
2022ApJ...926..120V 17       D               1 645 13 ExoMiner: A Highly Accurate and Explainable Deep Learning Classifier That Validates 301 New Exoplanets. VALIZADEGAN H., MARTINHO M.J.S., WILKENS L.S., et al.
2022A&A...661A..23F viz 17       D               4 267 15 Exoplanet X-ray irradiation and evaporation rates with eROSITA. FOSTER G., POPPENHAEGER K., ILIC N., 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               32 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.
2022A&A...664A..78F viz 17       D               1 7452 7 Characterization of Kepler targets based on medium-resolution LAMOST spectra analyzed with ROTFIT,. FRASCA A., MOLENDA-ZAKOWICZ J., ALONSO-SANTIAGO J., et al.
2023AJ....165..177S viz 17       D               6 131 ~ Revising Properties of Planet-Host Binary Systems. III. There Is No Observed Radius Gap for Kepler Planets in Binary Star Systems. SULLIVAN K., KRAUS A.L., HUBER D., et al.
2023ApJ...946...61L viz 61       D     X         2 257 ~ A Spectroscopic Analysis of a Sample of K2 Planet-host Stars: Stellar Parameters, Metallicities and Planetary Radii. LOAIZA-TACURI V., CUNHA K., SMITH V.V., et al.
2023AJ....166...58Q 435     A D     X C       10 25 ~ Confirming Resonance in Three Transiting Systems. QUINN T. and MacDONALD M.G.
2023AJ....166...94M viz 17       D               3 105 ~ 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.
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..122H 18       D               1 4 ~ Automated Scheduling of Doppler Exoplanet Observations at Keck Observatory. HANDLEY L.B., PETIGURA E.A., MISIC V.V., et al.
2024AJ....167..271V viz 242       D     X         6 165 ~ 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.
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..129S viz 18       D               2 350 ~ 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.
2024ApJ...973L...4R 134           X         3 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.
2025MNRAS.536.3123J 19       D               4 37 ~ FCN4Flare: fully convolution neural networks for flare detection. JIA M., LUO A.-L. and QIU B.
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.
2025ApJS..277...15J 19       D               2 136 ~ Half a Million Binary Stars Identified from the Low-resolution Spectra of LAMOST. JING Y., MAO T.-X., WANG J., 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.
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.
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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