Kepler-25b , the SIMBAD biblio

Kepler-25b , the SIMBAD biblio (66 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST10:18:05


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Title First 3 Authors
2012MNRAS.421.2342S viz 95       D       C       1 23 131 Transit timing observations from Kepler - III. Confirmation of four multiple planet systems by a Fourier-domain study of anticorrelated transit timing variations. STEFFEN J.H., FABRYCKY D.C., FORD E.B., et al.
2012ApJ...750..113F viz 1 32 70 Transit timing observations from Kepler. II. Confirmation of two multiplanet systems via a non-parametric correlation analysis. FORD E.B., FABRYCKY D.C., STEFFEN J.H., et al.
2012ApJ...750..114F viz 1 50 176 Transit timing observations from Kepler. IV. Confirmation of four multiple-planet systems by simple physical models. FABRYCKY D.C., FORD E.B., STEFFEN J.H., et al.
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 170       D     X C       4 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.
2013ApJ...763...12B 49           X         1 6 126 Emerging trends in a period-radius distribution of close-in planets. BEAUGE C. and NESVORNY D.
2013ApJS..204...24B viz 16       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 16       D               1 189 246 Fundamental properties of Kepler planet-candidate host stars using asteroseismology. HUBER D., CHAPLIN W.J., CHRISTENSEN-DALSGAARD J., et al.
2013A&A...552A.119S viz 16       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...772...74W 79             C       1 59 175 Density and eccentricity of Kepler planets. WU Y. and LITHWICK Y.
2013ApJ...773...98B 39           X         1 49 29 Exoplanet characterization by proxy: a transiting 2.15 RPlanet near the habitable zone of the late K dwarf Kepler-61. BALLARD S., CHARBONNEAU D., FRESSIN F., et al.
2013ApJ...774...52L 79           X         2 18 43 Are the Kepler near-resonance planet pairs due to tidal dissipation? LEE M.H., FABRYCKY D. and LIN D.N.C.
2013A&A...560A.112M 16       D               1 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 16       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 293       D     X C       7 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 19       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 16       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 16       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 16       D               2 261 190 Densities and eccentricities of 139 Kepler planets from transit time variations. HADDEN S. and LITHWICK Y.
2014ApJ...787..173H 212       D     X         6 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...12B 39           X         1 32 37 Kepler-93b: a terrestrial world measured to within 120 km, and a test case for a new Spitzer observing mode. BALLARD S., CHAPLIN W.J., CHARBONNEAU D., et al.
2014ApJ...790..146F viz 16       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.
2014PASJ...66...94B 80           X         2 13 47 Determination of three-dimensional spin-orbit angle with joint analysis of asteroseismology, transit lightcurve, and the Rossiter-McLaughlin effect : Cases of HAT-P-7 and Kepler-25. BENOMAR O., BENOMAR K., SHIBAHASHI H., et al.
2014A&A...572A...2B 40           X         1 14 30 Characterization of the planetary system Kepler-101 with HARPS-N. A hot super-Neptune with an Earth-sized low-mass companion. BONOMO A.S., SOZZETTI A., LOVIS C., et al.
2014A&A...572A..51F 16       D               1 111 15 Revisiting the correlation between stellar activity and planetary surface gravity. FIGUEIRA P., OSHAGH M., ADIBEKYAN V.Z., 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...804...59D 214       D     X         6 83 29 Low false positive rate of Kepler candidates estimated from a combination of Spitzer and follow-up observations. DESERT J.-M., CHARBONNEAU D., TORRES G., et al.
2015ApJ...808..126V 16       D               3 105 201 Eccentricity from transit photometry: small planets in Kepler multi-planet systems have low eccentricities. VAN EYLEN V. and ALBRECHT S.
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...820...39J 17       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...825...19W viz 18       D               1 99 221 Probabilistic mass-radius relationship for sub-Neptune-sized planets. WOLFGANG A., ROGERS L.A. and FORD E.B.
2016AJ....152..158T viz 16       D               1 4387 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.
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 97       D     X         3 231 145 Kepler planet masses and eccentricities from TTV analysis. HADDEN S. and LITHWICK Y.
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.
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..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.
2018MNRAS.479.4786V 18       D               1 117 318 An asteroseismic view of the radius valley: stripped cores, not born rocky. VAN EYLEN V., AGENTOFT C., LUNDKVIST M.S., 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.
2018MNRAS.480.1767M 16       D               2 3 ~ A periodic configuration of the Kepler-25 planetary system. MIGASZEWSKI C. and GOZDZIEWSKI K.
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.
2019RAA....19...41G viz 17       D               2 1982 17 Transit timing variations and linear ephemerides of confirmed Kepler transiting exoplanets. GAJDOS P., VANKO M. and PARIMUCHA S.
2019ApJ...875...29M viz 17       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 17       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 17       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.
2019AJ....157..235C viz 17       D               2 415 7 Observations of the Kepler field with TESS: predictions for planet yield and observable features. CHRIST C.N., MONTET B.T. and FABRYCKY D.C.
2019A&A...630A.135U viz 17       D               1 501 16 Beyond the exoplanet mass-radius relation. ULMER-MOLL S., SANTOS N.C., FIGUEIRA P., et al.
2019MNRAS.490.1509K 17       D               1 54 ~ Asteroseismic investigation of 20 planet and planet-candidate host stars. KAYHAN C., YILDIZ M. and CELIK ORHAN Z.
2020AJ....159...41T viz 17       D               1 564 ~ Estimating planetary mass with deep learning. TASKER E.J., LANEUVILLE M. and GUTTENBERG N.
2020A&A...634A..43O 43           X         1 141 104 Revisited mass-radius relations for exoplanets below 120 M. OTEGI J.F., BOUCHY F. and HELLED R.
2020ApJ...894..115P 44           X         1 20 27 Orbital parameter determination for wide stellar binary systems in the age of Gaia. PEARCE L.A., KRAUS A.L., DUPUY T.J., et al.
2020AJ....160..108B viz 17       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.503.4092B 17       D               4 124 ~ Revisiting the Kepler field with TESS: Improved ephemerides using TESS 2 min data. BATTLEY M.P., KUNIMOTO M., ARMSTRONG D.J., et al.
2021AJ....161..246J viz 17       D               9 204 12 Following up the Kepler field: masses of targets for transit timing and atmospheric characterization. JONTOF-HUTTER D., WOLFGANG A., FORD E.B., 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.
2022A&A...659L...7S viz 46           X         1 6 6 Transit timing variations of AU Microscopii b and c. SZABO G.M., GARAI Z., BRANDEKER A., et al.
2022AJ....164...42J 18       D               4 79 3 TESS Observations of Kepler Systems with Transit Timing Variations. JONTOF-HUTTER D., DALBA P.A. and LIVINGSTON J.H.
2022ApJS..261...26S viz 18       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.
2023A&A...669A..63B 327           X         7 44 5 DREAM I. Orbital architecture orrery. BOURRIER V., ATTIA O., MALLONN M., et al.
2023A&A...676A.130G 93               F     1 70 ~ DREAM III. A helium survey in exoplanets on the edge of the hot Neptune desert with GIANO-B at TNG. GUILLUY G., BOURRIER V., JAZIRI Y., et al.
2024ApJS..270....8W 20       D               1 246 ~ 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.

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