Kepler-107c , the SIMBAD biblio

Kepler-107c , the SIMBAD biblio (75 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST17:00:11

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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
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.
2013ApJ...767..127H viz 15       D               1 189 246 Fundamental properties of Kepler planet-candidate host stars using asteroseismology. HUBER D., CHAPLIN W.J., CHRISTENSEN-DALSGAARD J., et al.
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.
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...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...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.
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...808..126V 94       D     X         3 105 201 Eccentricity from transit photometry: small planets in Kepler multi-planet systems have low eccentricities. VAN EYLEN V. and ALBRECHT S.
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.
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.
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.
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.
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 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.
2019NatAs...3..416B 982     A D     X C       24 8 56 A giant impact as the likely origin of different twins in the Kepler-107 exoplanet system. BONOMO A.S., ZENG L., DAMASSO M., et al.
2019AJ....158..108A 16       D               1 11 ~ Signatures of obliquity in thermal phase curves of hot Jupiters. ADAMS A.D., MILLHOLLAND S. and LAUGHLIN G.P.
2019ApJ...883...79D 43           X         1 19 52 Homogeneous analysis of hot Earths: masses, sizes, and compositions. DAI F., MASUDA K., WINN J.N., et al.
2020MNRAS.491.5287O viz 16       D               1 127 43 Testing exoplanet evaporation with multitransiting systems. OWEN J.E. and CAMPOS ESTRADA B.
2020A&A...634A..43O 58       D     X         2 141 104 Revisited mass-radius relations for exoplanets below 120 M⊕. OTEGI J.F., BOUCHY F. and HELLED R.
2020A&A...637A..13M viz 43           X         1 10 25 High-resolution spectroscopy of flares and CMEs on AD Leonis. MUHEKI P., GUENTHER E.W., MUTABAZI T., et al.
2020MNRAS.496.1166D 165           X         4 5 ~ Atmosphere loss in planet-planet collisions. DENMAN T.R., LEINHARDT Z.M., CARTER P.J., 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.
2020A&A...641A..92T viz 125           X         3 8 17 Characterization of the K2-38 planetary system. Unraveling one of the densest planets known to date. TOLEDO-PADRON B., LOVIS C., SUAREZ MASCARENO A., et al.
2020MNRAS.499..932P 58       D     X         2 40 35 Chemical fingerprints of formation in rocky super-Earths' data. PLOTNYKOV M. and VALENCIA D.
2020PASP..132j2001H 123           X         3 47 26 Solar system physics for Exoplanet research. HORNER J., KANE S.R., MARSHALL J.P., et al.
2021MNRAS.504.4634G 460     A D S   X C F     9 38 23 Caught in the act: core-powered mass-loss predictions for observing atmospheric escape. GUPTA A. and SCHLICHTING H.E.
2021A&A...652A.110L 17       D               1 82 7 Why do more massive stars host larger planets? LOZOVSKY M., HELLED R., PASCUCCI I., 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.
2021Sci...374..330A 43           X         1 47 73 A compositional link between rocky exoplanets and their host stars. ADIBEKYAN V., DORN C., SOUSA S.G., et al.
2022AJ....163...13B 17       D               2 165 3 Period ratio sculpting near second-order mean-motion resonances. BAILEY N., GILBERT G. and FABRYCKY D.
2022A&A...657A..68A viz 44           X         1 9 10 The HD 137496 system: A dense, hot super-Mercury and a cold Jupiter. AZEVEDO SILVA T., DEMANGEON O.D.S., BARROS S.C.C., et al.
2022MNRAS.510.2041C viz 43           X         1 315 3 The GALAH Survey: improving our understanding of confirmed and candidate planetary systems with large stellar surveys. CLARK J.T., WRIGHT D.J., WITTENMYER R.A., et al.
2022MNRAS.510.3449B viz 17       D               1 508 7 Exoplanets in the Galactic context: planet occurrence rates in the thin disc, thick disc, and stellar halo of Kepler stars. BASHI D. and ZUCKER S.
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.
2022MNRAS.513.1680D 85           X         2 5 ~ Atmosphere loss in oblique Super-Earth collisions. DENMAN T.R., LEINHARDT Z.M. and CARTER P.J.
2022A&A...662A..19J 85               F     1 12 9 Nucleation and growth of iron pebbles explains the formation of iron-rich planets akin to Mercury. JOHANSEN A. and DORN C.
2022A&A...665A.154B viz 85           X         2 32 6 HD 23472: a multi-planetary system with three super-Earths and two potential super-Mercuries,. BARROS S.C.C., DEMANGEON O.D.S., ALIBERT Y., et al.
2022MNRAS.517.3132R 315       D     X   F     7 11 3 Forming iron-rich planets with giant impacts. REINHARDT C., MEIER T., STADEL J.G., et al.
2022ApJ...940..144S 85           X         2 5 ~ Rocky Histories: The Effect of High Excitations on the Formation of Rocky Planets. SCORA J., VALENCIA D., MORBIDELLI A., et al.
2023AJ....165...47E 44           X         1 35 1 TOI-1075 b: A Dense, Massive, Ultra-short-period Hot Super-Earth Straddling the Radius Gap. ESSACK Z., SHPORER A., BURT J.A., 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.
2023ApJ...944...42U 17       D               1 56 6 The Nominal Ranges of Rocky Planet Masses, Radii, Surface Gravities, and Bulk Densities. UNTERBORN C.T., DESCH S.J., HALDEMANN J., et al.
2023AJ....165...97R 44           X         1 12 3 A Reanalysis of the Composition of K2-106b: An Ultra-short-period Super-Mercury Candidate. RODRIGUEZ MARTINEZ R., GAUDI B.S., SCHULZE J.G., et al.
2023A&A...673A..17M 44           X         1 8 1 Forming super-Mercuries: Role of stellar abundances. MAH J. and BITSCH B.
2023A&A...674A.137L 104       D     X         3 122 ~ Quantitative correlation of refractory elemental abundances between rocky exoplanets and their host stars. LIU Z. and NI D.
2023A&A...675A..52C viz 44           X         1 25 ~ An unusually low-density super-Earth transiting the bright early-type M-dwarf GJ 1018 (TOI-244). CASTRO-GONZALEZ A., DEMANGEON O.D.S., LILLO-BOX J., et al.
2023ApJ...955L...3G 44           X         1 18 ~ Company for the Ultra-high Density, Ultra-short Period Sub-Earth GJ 367 b: Discovery of Two Additional Low-mass Planets at 11.5 and 34 Days. GOFFO E., GANDOLFI D., EGGER J.A., et al.
2023A&A...677A..33B viz 17       D               1 120 ~ Cold Jupiters and improved masses in 38 Kepler and K2 small planet systems from 3661 HARPS-N radial velocities No excess of cold Jupiters in small planet systems. BONOMO A.S., DUMUSQUE X., MASSA A., et al.
2024AJ....167..103J viz 18       D               1 190 ~ Kepler Multitransiting System Physical Properties and Impact Parameter Variations. JUDKOVSKY Y., OFIR A. and AHARONSON O.
2024MNRAS.529..141G 45           X         1 52 ~ A new mass and radius determination of the ultra-short period planet K2-106b and the fluffy planet K2-106c. GUENTHER E.W., GOFFO E., SEBASTIAN D., et al.
2024MNRAS.529.2577D 403           X C F     7 6 ~ Formation of super-Mercuries via giant impacts. DOU J., CARTER P.J. and LEINHARDT Z.M.
2024ApJ...966..185C 18       D               1 140 ~ Where Are the Water Worlds? Identifying Exo-water-worlds Using Models of Planet Formation and Atmospheric Evolution. CHAKRABARTY A. and MULDERS G.D.
2024A&A...685A...5P viz 90           X         2 18 ~ Discovery of two warm mini-Neptunes with contrasting densities orbiting the young K3V star TOI-815. PSARIDI A., OSBORN H., BOUCHY F., 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.
2024ApJS..272...35Z 45           X         1 8 ~ Comparison of Machine-learning and Bayesian Inferences for the Interior of Rocky Exoplanets with Large Compositional Diversity. ZHAO Y., LIU Z., NI D., et al.
2024AJ....168..281B 90           X         2 40 ~ Revisiting the Relationship Between Rocky Exoplanet and Stellar Compositions: Reduced Evidence for a Super-Mercury Population. BRINKMAN C.L., POLANSKI A.S., HUBER D., et al.
2024A&A...692A..67A 18       D               2 68 ~ Linking the primordial composition of planet building disks to the present-day composition of rocky exoplanets. ADIBEKYAN V., DEAL M., DORN C., et al.
2025ApJ...978L..41L 19       D               1 13 ~ Most High-density Exoplanets Are Unlikely to Be Remnant Giant Planet's Cores. LIN Z., CAMBIONI S. and SEAGER S.
2025ApJ...980L..40L 93           X         2 14 ~ Carving the Edges of the Rocky Planet Population. LEE E.J. and OWEN J.E.
2025A&A...694A..15B viz 93             C       1 9 ~ KOBE-1: The first planetary system from the KOBE survey Two planets likely residing in the sub-Neptune mass regime around a late K-dwarf. BALSALOBRE-RUZA O., LILLO-BOX J., SILVA A.M., et al.
2025AJ....169..216T viz 47           X         1 10 ~ Utilizing Machine Learning to Predict Host Stars and the Key Elemental Abundances of Small Planets. TORRES-QUIJANO A.R., HINKEL N.R., WHEELER III C.H., et al.
2025A&A...696A.174C 159       D     X   F     3 17 ~ Can metal-rich worlds form by giant impacts? CAMBIONI S., WEISS B.P., ASPHAUG E., et al.
2025MNRAS.539..405W 19       D               3 46 ~ A link between rocky planet composition and stellar age. WEEKS A., VAN EYLEN V., HUBER D., et al.
2025ApJ...993..235R 373           X C       7 60 ~ Terrestrial Exoplanet Internal Structure Constraints Enabled by Comprehensive Host Star Characterization Reveal That Terrestrial Planets in Mean Motion Resonances Are Water Rich. ROSS A., REGGIANI H., SCHLAUFMAN K.C., et al.
2025A&A...704A.108C 65       D     X         2 111 ~ Refractory element abundances in rocky planets and their host stars: Revisiting the compositional link. CHEN X. and NI D.
2026ApJ...997..253P 170       D     X         4 41 ~ Evidence of 1:1 Slope between Rocky Super-Earths and Their Host Stars. PLOTNYKOV M., VALENCIA D., ROSS A., et al.
2026ApJ...998...46T 150           X         3 4 ~ Origins of Mercury's Big Heart of Iron: Exploring Pathways to Form High Core Mass Fraction Planets via N-body Simulations. TAJER H., WANG J., CHILDS A.C., et al.

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