Kepler-79c , the SIMBAD biblio

Kepler-79c , the SIMBAD biblio (32 results) C.D.S. - SIMBAD4 rel 1.7 - 2019.11.20CET09:17:06


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Title First 3 Authors
2019AJ....157..174O viz 19       D               1 176 ~ Discovery of a third transiting planet in the Kepler-47 circumbinary system. OROSZ J.A., WELSH W.F., HAGHIGHIPOUR N., et al.
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.
2017AJ....154....5H viz 61       D     X         2 231 38 Kepler planet masses and eccentricities from TTV analysis. HADDEN S. and LITHWICK Y.
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.
2017MNRAS.466.1868C 17       D               1 176 16 An overabundance of low-density Neptune-like planets. CUBILLOS P., ERKAEV N.V., JUVAN I., 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...820...39J 17       D               1 107 48 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 17       D               1 99 95 Probabilistic mass-radius relationship for sub-Neptune-sized planets. WOLFGANG A., ROGERS L.A. and FORD E.B.
2015ApJ...799..180S viz 17       D               1 431 69 A statistical reconstruction of the planet population around Kepler solar-type stars. SILBURT A., GAIDOS E. and WU Y.
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.
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.
2015ApJS..217...31M viz 17       D               1 2033 146 Planetary candidates observed by Kepler. VI. Planet sample from Q1–Q16 (47 months). MULLALLY F., COUGHLIN J.L., THOMPSON S.E., et al.
2015MNRAS.453.4089S 17       D               1 103 3 Tides alone cannot explain Kepler planets close to 2:1 MMR. SILBURT A. and REIN H.
2014A&A...566A.103L viz 16       D               2 359 67 High-resolution imaging of Kepler planet host candidates. A comprehensive comparison of different techniques. LILLO-BOX J., BARRADO D. and BOUY H.
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...785...15J viz 429       D     X C       10 33 59 Kepler-79's low density planets. JONTOF-HUTTER D., LISSAUER J.J., ROWE J.F., et al.
2014ApJ...787...80H viz 16       D               3 261 93 Densities and eccentricities of 139 Kepler planets from transit time variations. HADDEN S. and LITHWICK Y.
2014ApJ...787..173H 16       D               2 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 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.
2014ApJ...792....1L 20       D               1 45 207 Understanding the mass-radius relation for sub-neptunes: radius as a proxy for composition. LOPEZ E.D. and FORTNEY J.J.
2014ApJ...796...48Z viz 16       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.
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..213...17P 16       D               1 19 8 Analytical solution for waves in planets with atmospheric superrotation. I. Acoustic and inertia-gravity waves. PERALTA J., IMAMURA T., READ P.L., et al.
2013ApJS..204...24B viz 16       D               1 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.
2013ApJS..208...22X viz 17       D               3 29 44 Transit timing variation of near-resonance planetary pairs: confirmation of 12 multiple-planet systems. XIE J.-W.
2012ApJ...753..170W 379       D S   X C       8 9 26 Predicting the configuration of a planetary system: KOI-152 observed by Kepler. WANG S., JI J. and ZHOU J.-L.
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.
2011ApJ...728..117B viz 16       D               1 321 239 Characteristics of Kepler planetary candidates based on the first data set. BORUCKI W.J., KOCH D.G., BASRI G., et al.
2010ApJ...725.1226S 158           X C       3 22 60 Five Kepler target stars that show multiple transiting exoplanet candidates. STEFFEN J.H., BATALHA N.M., BORUCKI W.J., et al.

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2019.11.20-09:17:06

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