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| Kepler-345c , the SIMBAD biblio (20 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST05:41:33 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2012ApJ...756..185F |
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 |
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. | ||
|
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...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...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. | ||
|
2014ApJ...791...35L |
15 | D | 1 | 800 | 137 | Robotic laser adaptive optics imaging of 715 Kepler exoplanet candidates using Robo-AO. | LAW N.M., MORTON T., BARANEC C., et al. | ||
| 2014ApJ...794L...5K | 15 | D | 1 | 51 | 18 | On the frequency of potential Venus analogs from Kepler data. | KANE S.R., KOPPARAPU R.K. and DOMAGAL-GOLDMAN S.D. | ||
|
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. | ||
|
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. | ||
|
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. | ||
|
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. | ||
|
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. | ||
|
2020AJ....159..211C |
16 | D | 1 | 351 | 93 | Evolution of the radius valley around low-mass stars from Kepler and K2. | CLOUTIER R. and MENOU K. | ||
| 2022ApJ...930L...6U | 17 | D | 1 | 19 | 4 | Mantle Degassing Lifetimes through Galactic Time and the Maximum Age Stagnant-lid Rocky Exoplanets Can Support Temperate Climates. | UNTERBORN C.T., FOLEY B.J., DESCH S.J., et al. | ||
|
2023A&A...669A.117L |
17 | D | 2 | 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. | ||
|
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 |
19 | D | 1 | 194 | ~ | Planetary Mass Determinations from a Simplified Photodynamical Model-Application to the Complete Kepler Dataset. | OFIR A., YOFFE G. and AHARONSON O. |