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Kepler-396b , the SIMBAD biblio (34 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.18CEST03:18:29 |
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 |
---|---|---|---|---|---|---|---|---|---|
2013ApJ...778..110M | 585 | S X C | 13 | 23 | 0 | Eight planets in four multi-planet systems via transit timing variations in 1350 days. | MING Y., LIU H.-G., HUI Z., et al. | ||
2014ApJS..210...19B | 16 | 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 | 16 | 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 | 16 | 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. | ||
2015ApJ...798...66D | 40 | X | 1 | 296 | 60 | The photoeccentric effect and proto-hot jupiters. III. A paucity of proto-hot jupiters on super-eccentric orbits. | DAWSON R.I., MURRAY-CLAY R.A. and JOHNSON J.A. | ||
2015ApJ...799..180S | 16 | D | 1 | 431 | 118 | A statistical reconstruction of the planet population around Kepler solar-type stars. | SILBURT A., GAIDOS E. and WU Y. | ||
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. | ||
2015ApJS..217...31M | 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 | 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. | ||
2016AJ....152..158T | 16 | D | 1 | 4387 | 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 | 97 | D | X | 3 | 231 | 145 | Kepler planet masses and eccentricities from TTV analysis. | HADDEN S. and LITHWICK Y. | |
2017AJ....154...66F | 219 | D | X | 6 | 90 | 6 | The densities of planets in multiple stellar systems. | FURLAN E. and HOWELL S.B. | |
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. | ||
2017A&A...603A..30S | 16 | D | 4 | 2500 | 58 | Observational evidence for two distinct giant planet populations. | SANTOS N.C., ADIBEKYAN V., FIGUEIRA P., 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. | ||
2018A&A...615A..79V | 83 | 9 | Kepler Object of Interest Network. I. First results combining ground- and space-based observations of Kepler systems with transit timing variations. | VON ESSEN C., OFIR A., DREIZLER S., 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...874L..31T | 17 | D | 1 | 403 | 62 | Connecting giant planet atmosphere and interior modeling: constraints on atmospheric metal enrichment. | THORNGREN D. and FORTNEY J.J. | ||
2019ApJ...875...29M | 17 | 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 | 17 | D | 1 | 4069 | 2 | Visual analysis and demographics of Kepler transit timing variations. | KANE M., RAGOZZINE D., FLOWERS X., et al. | ||
2019AJ....157..174O | 17 | 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. | ||
2019AJ....157..235C | 17 | D | 2 | 415 | 7 | Observations of the Kepler field with TESS: predictions for planet yield and observable features. | CHRIST C.N., MONTET B.T. and FABRYCKY D.C. | ||
2020AJ....159...41T | 17 | D | 1 | 564 | ~ | Estimating planetary mass with deep learning. | TASKER E.J., LANEUVILLE M. and GUTTENBERG N. | ||
2020AJ....160..108B | 17 | 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. | ||
2021MNRAS.503.4092B | 322 | D | X C | 7 | 124 | ~ | Revisiting the Kepler field with TESS: Improved ephemerides using TESS 2 min data. | BATTLEY M.P., KUNIMOTO M., ARMSTRONG D.J., et al. | |
2022AJ....163...91J | 18 | D | 1 | 248 | ~ | Physical properties and impact parameter variations of Kepler planets from analytic light-curve modeling. | JUDKOVSKY Y., OFIR A. and AHARONSON O. | ||
2022AJ....163..128W | 18 | D | 1 | 1570 | 6 | The influence of 10 unique chemical elements in shaping the distribution of Kepler planets. | WILSON R.F., CANAS C.I., MAJEWSKI S.R., et al. | ||
2022AJ....164...42J | 1093 | D | X C | 24 | 79 | 3 | TESS Observations of Kepler Systems with Transit Timing Variations. | JONTOF-HUTTER D., DALBA P.A. and LIVINGSTON J.H. | |
2022ApJS..261...26S | 18 | D | 7 | 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. | ||
2024AJ....167...20Z | 20 | D | 1 | 230 | ~ | The Breakthrough Listen Search for Intelligent Life: Detection and Characterization of Anomalous Transits in Kepler Lightcurves. | ZUCKERMAN A., DAVENPORT J.R.A., CROFT S., et al. |