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| Kepler-406c , the SIMBAD biblio (41 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST05:04:15 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2014ApJS..210...19B |
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. | ||
|
2014ApJS..210...20M |
95 | D | C | 3 | 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 | 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...783....4W |
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 |
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...787..173H | 93 | D | C | 3 | 58 | 38 | Mass-radius relations and core-envelope decompositions of super-earths and sub-neptunes. | HOWE A.R., BURROWS A. and VERNE W. | |
| 2015ApJ...801...41R | 44 | X | 1 | 52 | 558 | Most 1.6 Earth-radius planets are not rocky. | ROGERS L.A. | ||
|
2015ApJS..217...16R |
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. | ||
| 2015A&A...577A..83D | 44 | X | 1 | 16 | 186 | Can we constrain the interior structure of rocky exoplanets from mass and radius measurements? | DORN C., KHAN A., HENG K., et al. | ||
|
2016ApJ...825...19W |
17 | D | 1 | 99 | 221 | Probabilistic mass-radius relationship for sub-Neptune-sized planets. | WOLFGANG A., ROGERS L.A. and FORD E.B. | ||
| 2016ApJ...828...80K | 80 | C | 1 | 26 | 74 | Atmosphere-interior exchange on hot, rocky exoplanets. | KITE E.S., FEGLEY B.Jr, SCHAEFER L., et al. | ||
|
2016AJ....152..158T |
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 |
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 |
16 | D | 1 | 231 | 145 | Kepler planet masses and eccentricities from TTV analysis. | HADDEN S. and LITHWICK Y. | ||
|
2017AJ....154..108J |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
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. | ||
|
2019MNRAS.485.3999M |
16 | D | 1 | 474 | ~ | Planetary magnetism as a parameter in exoplanet habitability. | McINTYRE S.R.N., LINEWEAVER C.H. and IRELAND M.J. | ||
|
2019AJ....157..171K |
16 | D | 1 | 4069 | 2 | Visual analysis and demographics of Kepler transit timing variations. | KANE M., RAGOZZINE D., FLOWERS X., et al. | ||
|
2020AJ....159...41T |
16 | D | 1 | 564 | ~ | Estimating planetary mass with deep learning. | TASKER E.J., LANEUVILLE M. and GUTTENBERG N. | ||
| 2020A&A...634A..43O | 41 | X | 1 | 141 | 104 | Revisited mass-radius relations for exoplanets below 120 M⊕. | OTEGI J.F., BOUCHY F. and HELLED R. | ||
| 2020PASP..132h4402Q | 16 | D | 1 | 63 | ~ | Forecasting rates of volcanic activity on terrestrial exoplanets and implications for cryovolcanic activity on extrasolar ocean worlds. | QUICK L.C., ROBERGE A., MLINAR A.B., et al. | ||
|
2020AJ....160..108B |
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. | ||
|
2021A&A...645A...7K |
17 | D | 1 | 1569 | 17 | Determining the true mass of radial-velocity exoplanets with Gaia. Nine planet candidates in the brown dwarf or stellar regime and 27 confirmed planets. | KIEFER F., HEBRARD G., LECAVELIER DES ETANGS A., et al. | ||
| 2021AJ....161..284M | 85 | C | 1 | 23 | 37 | ARES. V. No evidence for molecular absorption in the HST WFC3 spectrum of GJ 1132 b. | MUGNAI L.V., MODIRROUSTA-GALIAN D., EDWARDS B., et al. | ||
|
2021ApJ...921...24S |
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. | ||
|
2022MNRAS.510.3449B |
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 |
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. | ||
|
2022A&A...662A..15M |
17 | D | 1 | 733 | 3 | Tidally driven tectonic activity as a parameter in exoplanet habitability. | McINTYRE S.R.N. | ||
|
2023ApJ...946...61L |
17 | D | 1 | 257 | ~ | A Spectroscopic Analysis of a Sample of K2 Planet-host Stars: Stellar Parameters, Metallicities and Planetary Radii. | LOAIZA-TACURI V., CUNHA K., SMITH V.V., et al. | ||
|
2023A&A...674A..39G |
17 | D | 1 | 130 | 18 | Gaia Data Release 3 A golden sample of astrophysical parameters. | GAIA COLLABORATION, CREEVEY O.L., SARRO L.M., et al. | ||
|
2024ApJS..270....8W |
18 | D | 2 | 250 | ~ | 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. | ||
|
2024A&A...685A.143M |
18 | D | 1 | 535 | ~ | Planets similar in size are often dissimilar in interior. | MAMONOVA E., SHAN Y., HATALOVA P., et al. | ||
| 2025MNRAS.539..405W | 47 | X | 1 | 46 | ~ | A link between rocky planet composition and stellar age. | WEEKS A., VAN EYLEN V., HUBER D., et al. |