KOI-245.02 , the SIMBAD biblio

KOI-245.02 , the SIMBAD biblio (28 results) C.D.S. - SIMBAD4 rel 1.7 - 2019.11.18CET16:17:07


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Title First 3 Authors
2019MNRAS.485.3999M 19       D               1 474 ~ Planetary magnetism as a parameter in exoplanet habitability. McINTYRE S.R.N., LINEWEAVER C.H. and IRELAND M.J.
2018AJ....155...48W viz 18       D               1 911 22 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 18       D               1 57 32 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.
2018MNRAS.479.4786V 18       D               1 117 42 An asteroseismic view of the radius valley: stripped cores, not born rocky. VAN EYLEN V., AGENTOFT C., LUNDKVIST M.S., et al.
2017AJ....154..108J viz 17       D               1 3237 46 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 17       D               1 900 146 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.
2016AJ....152..158T viz 17       D               1 4386 18 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.
2016ApJ...825...19W viz 17       D               1 99 95 Probabilistic mass-radius relationship for sub-Neptune-sized planets. WOLFGANG A., ROGERS L.A. and FORD E.B.
2015ApJ...801...41R 130           X         3 52 280 Most 1.6 Earth-radius planets are not rocky. ROGERS L.A.
2015ApJ...808..126V 17       D               2 105 85 Eccentricity from transit photometry: small planets in Kepler multi-planet systems have low eccentricities. VAN EYLEN V. and ALBRECHT S.
2015ApJ...809....8B viz 17       D               1 112329 139 Terrestrial planet occurrence rates for the Kepler GK dwarf sample. BURKE C.J., CHRISTIANSEN J.L., MULLALLY F., et al.
2015ApJ...815....5S viz 42           X         1 31 18 Detailed abundances of stars with small planets discovered by Kepler. I. The first sample. SCHULER S.C., VAZ Z.A., KATIME SANTRICH O.J., et al.
2015ApJS..217...16R viz 17       D               1 8625 84 Planetary candidates observed by Kepler. V. Planet sample from Q1-Q12 (36 months). ROWE J.F., COUGHLIN J.L., ANTOCI V., et al.
2014A&A...562A..80K 41           X         1 18 8 Impact of photo-evaporative mass loss on masses and radii of water-rich sub/super-Earths. KUROSAKI K., IKOMA M. and HORI Y.
2014A&A...566A.103L viz 16       D               1 359 67 High-resolution imaging of Kepler planet host candidates. A comprehensive comparison of different techniques. LILLO-BOX J., BARRADO D. and BOUY H.
2014A&A...570A..36M 46           X         1 5 26 From planetesimals to planets: volatile molecules. MARBOEUF U., THIABAUD A., ALIBERT Y., et al.
2014ApJ...783....4W viz 16       D               1 487 55 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...783L...6W 20       D               1 66 288 The mass-radius relation for 65 exoplanets smaller than 4 earth radii. WEISS L.M. and MARCY G.W.
2014ApJ...784...45R viz 16       D               1 1691 227 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...790..146F viz 16       D               1 918 322 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.
2014ApJS..210...19B viz 16       D               1 5860 162 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 183       D     X C       4 94 251 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.
2013ApJ...767..127H viz 16       D               1 189 177 Fundamental properties of Kepler planet-candidate host stars using asteroseismology. HUBER D., CHAPLIN W.J., CHRISTENSEN-DALSGAARD J., et al.
2013ApJ...771..107E viz 16       D               1 756 47 Spectroscopy of faint Kepler mission exoplanet candidate host stars. EVERETT M.E., HOWELL S.B., SILVA D.R., et al.
2013ApJS..204...24B viz 16       D               2 3274 701 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.
2013Natur.494..452B 274           X   F     5 4 120 A sub-Mercury-sized exoplanet. BARCLAY T., ROWE J.F., LISSAUER J., et al.
2012ApJ...756..185F viz 16       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.
2012Natur.486..375B viz 16       D               1 378 334 An abundance of small exoplanets around stars with a wide range of metallicities. BUCHHAVE L.A., LATHAM D.W., JOHANSEN A., et al.

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2019.11.18-16:17:07

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