Kepler-79b , the SIMBAD biblio

Kepler-79b , the SIMBAD biblio (58 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST11:36:44

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2010ApJ...725.1226S 91       D       C       5 22 70 Five Kepler target stars that show multiple transiting exoplanet candidates. STEFFEN J.H., BATALHA N.M., BORUCKI W.J., et al.
2011ApJ...728..117B viz 15       D               1 321 310 Characteristics of Kepler planetary candidates based on the first data set. BORUCKI W.J., KOCH D.G., BASRI G., et al.
2012ApJ...753..170W 321       D S   X C       7 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 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.
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.
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...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...785...15J viz 442       D     X C       11 33 105 Kepler-79's low density planets. JONTOF-HUTTER D., LISSAUER J.J., ROWE J.F., 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 15       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.
2014A&A...566A.103L viz 15       D               2 359 102 High-resolution imaging of Kepler planet host candidates. A comprehensive comparison of different techniques. LILLO-BOX J., BARRADO D. and BOUY H.
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.
2014ApJ...792....1L 20       D               1 45 511 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 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.
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.
2015ApJS..217...31M viz 16       D               1 2033 213 Planetary candidates observed by Kepler. VI. Planet sample from Q1–Q16 (47 months). MULLALLY F., COUGHLIN J.L., THOMPSON S.E., et al.
2015ApJ...809....8B viz 16       D               1 112329 282 Terrestrial planet occurrence rates for the Kepler GK dwarf sample. BURKE C.J., CHRISTIANSEN J.L., MULLALLY F., 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...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...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.
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.
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 56       D     X         2 231 145 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.
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.
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.
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               1 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.
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...886...72M 18       D               1 17 38 Tidally induced radius inflation of sub-Neptunes. MILLHOLLAND S.
2020AJ....159...41T viz 16       D               1 564 ~ Estimating planetary mass with deep learning. TASKER E.J., LANEUVILLE M. and GUTTENBERG N.
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.
2020PASP..132e4401Z 16       D               1 81 38 Utilizing small telescopes operated by citizen scientists for transiting Exoplanet follow-up. ZELLEM R.T., PEARSON K.A., BLASER E., et al.
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.
2020AJ....160..201C viz 140       D     X         4 31 22 A featureless infrared transmission spectrum for the super-puff planet Kepler-79d. CHACHAN Y., JONTOF-HUTTER D., KNUTSON H.A., et al.
2021ApJ...908..114Y 167     A D     X         5 16 9 A simplified photodynamical model for planetary mass determination in low-eccentricity multitransiting systems. YOFFE G., OFIR A. and AHARONSON O.
2021MNRAS.503.4092B 17       D               1 124 ~ 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               7 204 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.
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.
2021AJ....162...55Y viz 17       D               1 70 13 How close are compact multiplanet systems to the stability limit? YEE S.W., TAMAYO D., HADDEN 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.
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.
2022ApJS..261...26S viz 17       D               3 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...676L...8V 17       D               1 10 ~ Rocky sub-Neptunes formed by pebble accretion: Rain of rock from polluted envelopes. VAZAN A. and ORMEL C.W.
2024AJ....167..103J viz 197       D     X         5 190 ~ Kepler Multitransiting System Physical Properties and Impact Parameter Variations. JUDKOVSKY Y., OFIR A. and AHARONSON O.
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.
2024A&A...687L...1L viz 18       D               1 140 ~ Resonant sub-Neptunes are puffier. LELEU A., DELISLE J.-B., BURN R., et al.
2025AJ....169...90O viz 112       D     X         3 194 ~ Planetary Mass Determinations from a Simplified Photodynamical Model-Application to the Complete Kepler Dataset. OFIR A., YOFFE G. and AHARONSON O.
2025ApJ...981..142X 19       D               1 94 ~ Amplifying Resonant Repulsion with Inflated Young Planets, Overlooked Inner Planets, and Nonzero Initial Δ. XU Y. and DAI F.

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