Kepler-48c , the SIMBAD biblio

Kepler-48c , the SIMBAD biblio (72 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST10:20:36


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Title First 3 Authors
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.
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.
2011PASP..123..412W viz 15       D               1 2897 398 The Exoplanet Orbit Database. WRIGHT J.T., KAKHOURI O., MARCY G.W., 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.
2013A&A...552A.119S viz 15       D               1 1487 118 Magnetic energy fluxes in sub-Alfvenic planet star and moon planet interactions. SAUR J., GRAMBUSCH T., DULING S., et al.
2013ApJ...770...69P viz 15       D               1 245 238 A plateau in the planet population below twice the size of Earth. PETIGURA E.A., MARCY G.W. and HOWARD A.W.
2013ApJ...775...34O 54       D     X         2 89 24 Condition for capture into first-order mean motion resonances and application to constraints on the origin of resonant systems. OGIHARA M. and KOBAYASHI H.
2013ApJ...775...53H 16       D               1 93 195 Testing in situ assembly with the Kepler planet candidate sample. HANSEN B.M.S. and MURRAY N.
2013ApJS..208...22X viz 15       D               3 29 51 Transit timing variation of near-resonance planetary pairs: confirmation of 12 multiple-planet systems. XIE J.-W.
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.
2014ApJS..210...20M viz 250       D     X C       6 94 394 Masses, radii, and orbits of small Kepler planets: the transition from gaseous to rocky planets. MARCY G.W., ISAACSON H., HOWARD A.W., et al.
2014ApJ...783L...6W 18       D               1 66 499 The mass-radius relation for 65 exoplanets smaller than 4 earth radii. WEISS L.M. and MARCY G.W.
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.
2014ApJ...787...80H viz 15       D               2 261 190 Densities and eccentricities of 139 Kepler planets from transit time variations. HADDEN S. and LITHWICK Y.
2014ApJ...787..173H 93       D     X         3 58 38 Mass-radius relations and core-envelope decompositions of super-earths and sub-neptunes. HOWE A.R., BURROWS A. and VERNE W.
2014ApJ...790..146F viz 15       D               1 918 579 Architecture of Kepler's multi-transiting systems. II. New investigations with twice as many candidates. FABRYCKY D.C., LISSAUER J.J., RAGOZZINE D., et al.
2014Natur.513..328M 25 38 Doppler spectroscopy as a path to the detection of Earth-like planets. MAYOR M., LOVIS C. and SANTOS N.C.
2014ApJ...796...48Z viz 15       D               1 199 11 The ground-based H-, K-, and L-band absolute emission spectra of HD 209458b. ZELLEM R.T., GRIFFITH C.A., DEROO P., et al.
2014A&A...572A..51F 93       D       C       2 111 15 Revisiting the correlation between stellar activity and planetary surface gravity. FIGUEIRA P., OSHAGH M., ADIBEKYAN V.Z., et al.
2015ApJ...801...41R 83           X         2 52 558 Most 1.6 Earth-radius planets are not rocky. ROGERS L.A.
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...806..183W viz 16       D               1 223 146 How rocky are they? the composition distribution of Kepler's Sub-Neptune planet candidates within 0.15 AU. WOLFGANG A. and LOPEZ E.
2015ApJ...809...77S viz 95             C       1 11 375 The Transiting Exoplanet Survey Satellite: simulations of planet detections and astrophysical false positives. SULLIVAN P.W., WINN J.N., BERTA-THOMPSON Z.K., et al.
2015MNRAS.453.4089S 16       D               1 103 3 Tides alone cannot explain Kepler planets close to 2:1 MMR. SILBURT A. and REIN H.
2016ApJ...816...95G 40           X         1 10 33 The Kepler-454 system: a small, not-rocky inner planet, a jovian world, and a distant companion. GETTEL S., CHARBONNEAU D., DRESSING C.D., et al.
2016ApJ...820...39J 16       D               1 107 126 Secure mass measurements from transit timing: 10 Kepler exoplanets between 3 and 8 M⊕ with diverse densities and incident fluxes. JONTOF-HUTTER D., FORD E.B., ROWE J.F., et al.
2016ApJ...824..103F 39           X         1 14 5 Solubility of rock in steam atmospheres of planets. FEGLEY B., JACOBSON N.S., WILLIAMS K.B., et al.
2016ApJ...825...19W viz 17       D               1 99 221 Probabilistic mass-radius relationship for sub-Neptune-sized planets. WOLFGANG A., ROGERS L.A. and FORD E.B.
2016MNRAS.461.1841C 16       D               1 150 9 An upper boundary in the mass-metallicity plane of exo-Neptunes. COURCOL B., BOUCHY F. and DELEUIL M.
2016AJ....152..158T viz 16       D               1 4388 37 Detection of potential transit signals in 17 quarters of Kepler data: results of the final Kepler mission transiting planet search (DR25). TWICKEN J.D., JENKINS J.M., SEADER S.E., et al.
2017ApJ...834...17C viz 16       D               1 290 454 Probabilistic forecasting of the masses and radii of other worlds. CHEN J. and KIPPING D.
2017MNRAS.466.1868C viz 16       D               1 176 21 An overabundance of low-density Neptune-like planets. CUBILLOS P., ERKAEV N.V., JUVAN I., et al.
2017AJ....154....5H viz 16       D               1 231 145 Kepler planet masses and eccentricities from TTV analysis. HADDEN S. and LITHWICK Y.
2017MNRAS.469..171R 79           X         2 12 5 Transit probabilities in secularly evolving planetary systems. READ M.J., WYATT M.C. and TRIAUD A.H.M.J.
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..109F viz 16       D               1 900 847 The California-Kepler Survey. III. A gap in the radius distribution of small planets. FULTON B.J., PETIGURA E.A., HOWARD A.W., et al.
2017AJ....154..236W 16       D               1 34 7 Near mean-motion resonances in the system observed by Kepler: affected by mass accretion and Type I migration. WANG S. and JI J.
2018AJ....155...48W viz 16       D               1 911 204 The California-Kepler survey. V. Peas in a pod: planets in a Kepler multi-planet system are similar in size and regularly spaced. WEISS L.M., MARCY G.W., PETIGURA E.A., et al.
2018ApJ...853..163J 19       D               1 57 202 Compositional imprints in Density-Distance-Time: a rocky composition for close-in low-mass exoplanets from the location of the valley of evaporation. JIN S. and MORDASINI C.
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.
2018AJ....155..206A viz 16       D               3 183 5 Systematic search for rings around Kepler planet candidates: constraints on ring size and occurrence rate. AIZAWA M., MASUDA K., KAWAHARA H., 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.
2018AJ....156..254W viz 16       D               2 1269 42 The California-Kepler Survey. VI. Kepler multis and singles have similar planet and stellar properties indicating a common origin. WEISS L.M., ISAACSON H.T., MARCY G.W., et al.
2018AJ....156..264F viz 16       D               1 1909 365 The California-Kepler Survey. VII. Precise planet radii leveraging Gaia DR2 reveal the stellar mass dependence of the Planet radius gap. FULTON B.J. and PETIGURA E.A.
2019A&A...623A.165E 163             C F     2 19 29 HD 219666 b: a hot-Neptune from TESS Sector 1. ESPOSITO M., ARMSTRONG D.J., GANDOLFI D., et al.
2019RAA....19...41G viz 16       D               1 1982 17 Transit timing variations and linear ephemerides of confirmed Kepler transiting exoplanets. GAJDOS P., VANKO M. and PARIMUCHA S.
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.
2019AJ....157..171K viz 16       D               1 4069 2 Visual analysis and demographics of Kepler transit timing variations. KANE M., RAGOZZINE D., FLOWERS X., et al.
2019AJ....157..174O viz 16       D               1 176 61 Discovery of a third transiting planet in the Kepler-47 circumbinary system. OROSZ J.A., WELSH W.F., HAGHIGHIPOUR N., et al.
2019ApJ...880L...1A viz 16       D               1 146 ~ A gap in the mass distribution for warm Neptune and terrestrial planets. ARMSTRONG D.J., MERU F., BAYLISS D., et al.
2020AJ....159...41T viz 16       D               1 564 ~ Estimating planetary mass with deep learning. TASKER E.J., LANEUVILLE M. and GUTTENBERG N.
2020A&A...634A..43O 16       D               1 141 104 Revisited mass-radius relations for exoplanets below 120 M⊕. OTEGI J.F., BOUCHY F. and HELLED R.
2020AJ....159..239G viz 16       D               1 1408 ~ Updated parameters and a new transmission spectrum of HD 97658b. GUO X., CROSSFIELD I.J.M., DRAGOMIR D., et al.
2020MNRAS.496.1149L 41           X         1 12 ~ Flyby encounters between two planetary systems II: exploring the interactions of diverse planetary system architectures. LI D., MUSTILL A.J. and DAVIES M.B.
2020AJ....160..108B viz 16       D               1 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.
2021MNRAS.503.2825H 17       D               1 79 ~ Implications of an improved water equation of state for water-rich planets. HUANG C., RICE D.R., GRANDE Z.M., et al.
2021A&A...649L...5B 17       D               2 41 19 Dry or water world? How the water contents of inner sub-Neptunes constrain giant planet formation and the location of the water ice line. BITSCH B., RAYMOND S.N., BUCHHAVE L.A., et al.
2021MNRAS.505.1293S viz 17       D               1 573 7 Systematic search for long-term transit duration changes in Kepler transiting planets. SHAHAF S., MAZEH T., ZUCKER S., et al.
2021ApJ...921...24S viz 17       D               1 328 1 The occurrence-weighted median planets discovered by transit surveys orbiting solar-type stars and their implications for planet formation and evolution. SCHLAUFMAN K.C. and HALPERN N.D.
2021A&A...656A.157B 17       D               1 48 9 Constraining stellar rotation and planetary atmospheric evolution of a dozen systems hosting sub-Neptunes and super-Earths. BONFANTI A., FOSSATI L., KUBYSHKINA D., et al.
2022ApJ...924....9H 43           X         1 17 10 Sculpting the sub-Saturn occurrence rate via atmospheric mass loss. HALLATT T. and LEE E.J.
2022MNRAS.511.1043W viz 43           X         1 32 22 A pair of sub-Neptunes transiting the bright K-dwarf TOI-1064 characterized with CHEOPS. WILSON T.G., GOFFO E., ALIBERT Y., et al.
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.
2022RAA....22g2003J 85               F     1 114 7 CHES: A Space-borne Astrometric Mission for the Detection of Habitable Planets of the Nearby Solar-type Stars. JI J.-H., LI H.-T., ZHANG J.-B., et al.
2023MNRAS.519.6028R 17       D               1 86 7 Exoplanet atmosphere evolution: emulation with neural networks. ROGERS J.G., JANO MUNOZ C., OWEN J.E., et al.
2023AJ....165..125A viz 17       D               1 578 ~ Planetary Orbit Eccentricity Trends (POET). I. The Eccentricity-Metallicity Trend for Small Planets Revealed by the LAMOST-Gaia-Kepler Sample. AN D.-S., XIE J.-W., DAI Y.-Z., et al.
2024AJ....167...20Z viz 18       D               1 230 ~ The Breakthrough Listen Search for Intelligent Life: Detection and Characterization of Anomalous Transits in Kepler Lightcurves. ZUCKERMAN A., DAVENPORT J.R.A., CROFT S., et al.
2024ApJS..270....8W viz 18       D               2 250 ~ The Kepler Giant Planet Search. I. A Decade of Kepler Planet-host Radial Velocities from W. M. Keck Observatory. WEISS L.M., ISAACSON H., HOWARD A.W., et al.
2024AJ....167..194D viz 45           X         1 11 ~ The TESS-Keck Survey. XVIII. A Sub-Neptune and Spurious Long-period Signal in the TOI-1751 System. DESAI A., TURTELBOOM E.V., HARADA C.K., et al.
2024A&A...685A.143M viz 18       D               1 535 ~ Planets similar in size are often dissimilar in interior. MAMONOVA E., SHAN Y., HATALOVA P., et al.
2025ApJ...987...85R 19       D               1 241 ~ Characterizing Exoplanets for Assessing Their Potential Habitability. RODRIGUEZ-MOZOS J.M. and MOYA A.

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