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| Kepler-128c , the SIMBAD biblio (42 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST10:22:38 |
| 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 |
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. | ||
|
2011PASP..123..412W |
15 | D | 1 | 2897 | 398 | The Exoplanet Orbit Database. | WRIGHT J.T., KAKHOURI O., MARCY G.W., et al. | ||
|
2013ApJS..204...24B |
15 | D | 2 | 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 |
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...770...69P |
15 | D | 1 | 245 | 238 | A plateau in the planet population below twice the size of Earth. | PETIGURA E.A., MARCY G.W. and HOWARD A.W. | ||
|
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. | ||
|
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...80H |
15 | D | 2 | 261 | 190 | Densities and eccentricities of 139 Kepler planets from transit time variations. | HADDEN S. and LITHWICK Y. | ||
|
2014ApJ...790..146F |
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. | ||
| 2015AJ....149...55E | 16 | D | 3 | 48 | 34 | High-resolution multi-band imaging for validation and characterization of small Kepler planets. | EVERETT M.E., BARCLAY T., CIARDI D.R., et al. | ||
|
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. | ||
| 2015ApJ...808..126V | 16 | D | 1 | 105 | 201 | Eccentricity from transit photometry: small planets in Kepler multi-planet systems have low eccentricities. | VAN EYLEN V. and ALBRECHT S. | ||
|
2015ApJ...809....8B |
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. | ||
| 2016ApJ...820...39J | 39 | X | 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...828...44H | 135 | D | X | 4 | 20 | 51 | Numerical and analytical modeling of transit timing variations. | HADDEN S. and LITHWICK Y. | |
|
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. | ||
|
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...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. | ||
|
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. | ||
|
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. | ||
|
2019AJ....157..174O |
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. | ||
| 2019MNRAS.490.1509K | 16 | D | 1 | 54 | ~ | Asteroseismic investigation of 20 planet and planet-candidate host stars. | KAYHAN C., YILDIZ M. and CELIK ORHAN Z. | ||
|
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. | ||
|
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. | ||
| 2021ApJ...921..142C | 17 | D | 1 | 15 | 4 | On the importance of wave-planet interactions for the migration of two super-Earths embedded in a protoplanetary disk. | CUI Z., PAPALOIZOU J.C.B. and SZUSZKIEWICZ E. | ||
|
2022AJ....163...91J |
17 | D | 1 | 504 | ~ | Physical properties and impact parameter variations of Kepler planets from analytic light-curve modeling. | JUDKOVSKY Y., OFIR A. and AHARONSON O. | ||
|
2023A&A...669A.117L |
235 | D | X C | 5 | 57 | ~ | Removing biases on the density of sub-Neptunes characterised via transit timing variations Update on the mass-radius relationship of 34 Kepler planets. | LELEU A., DELISLE J.-B., UDRY S., et al. | |
|
2023AJ....165..125A |
17 | D | 1 | 578 | ~ | Planetary Orbit Eccentricity Trends (POET). I. The Eccentricity-Metallicity Trend for Small Planets Revealed by the LAMOST-Gaia-Kepler Sample. | AN D.-S., XIE J.-W., DAI Y.-Z., et al. | ||
|
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. | ||
| 2023MNRAS.521.2535G | 87 | F | 1 | 5 | ~ | Mantle mineralogy limits to rocky planet water inventories. | GUIMOND C.M., SHORTTLE O. and RUDGE J.F. | ||
| 2023MNRAS.522.1914C | 87 | F | 1 | 13 | 2 | Exciting the transit timing variation phases of resonant sub-Neptunes. | CHOKSI N. and CHIANG E. | ||
|
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. | ||
| 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.143M |
18 | D | 1 | 535 | ~ | Planets similar in size are often dissimilar in interior. | MAMONOVA E., SHAN Y., HATALOVA P., et al. | ||
|
2025AJ....169...90O |
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. |