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Kepler-81b , the SIMBAD biblio (32 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST08:01:10 |
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 |
---|---|---|---|---|---|---|---|---|---|
2010ApJ...725.1226S | 321 | D | X C | 8 | 22 | 70 | Five Kepler target stars that show multiple transiting exoplanet candidates. | STEFFEN J.H., BATALHA N.M., BORUCKI W.J., et al. | |
2011ApJ...728..117B | 15 | D | 1 | 321 | 310 | Characteristics of Kepler planetary candidates based on the first data set. | BORUCKI W.J., KOCH D.G., BASRI G., et al. | ||
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 | 16 | 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. | ||
2013ApJS..208...22X | 16 | D | 3 | 29 | 51 | Transit timing variation of near-resonance planetary pairs: confirmation of 12 multiple-planet systems. | XIE J.-W. | ||
2013ApJ...779..188M | 16 | D | 1 | 342 | 155 | Spectro-thermometry of M dwarfs and their candidate planets: too hot, too cool, or just right? | MANN A.W., GAIDOS E. and ANSDELL M. | ||
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...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. | ||
2014ApJ...787...80H | 16 | D | 2 | 261 | 190 | Densities and eccentricities of 139 Kepler planets from transit time variations. | HADDEN S. and LITHWICK Y. | ||
2014ApJ...790..146F | 16 | 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 | 16 | 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. | ||
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...807...45D | 16 | D | 1 | 2707 | 726 | The occurrence of potentially habitable planets orbiting M dwarfs estimated from the full Kepler dataset and an empirical measurement of the detection sensitivity. | DRESSING C.D. and CHARBONNEAU D. | ||
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. | ||
2016AJ....152..181H | 16 | D | 1 | 9279 | 22 | SETI observations of exoplanets with the Allen Telescope Array. | HARP G.R., RICHARDS J., TARTER J.C., 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. | ||
2017A&A...603A..30S | 16 | D | 6 | 2500 | 58 | Observational evidence for two distinct giant planet populations. | SANTOS N.C., ADIBEKYAN V., FIGUEIRA P., et al. | ||
2018ApJS..234....9O | 82 | X | 2 | 436 | 14 | A spectral approach to transit timing variations. | OFIR A., XIE J.-W., JIANG C.-F., et al. | ||
2018AJ....155...68W | 16 | D | 1 | 509 | 18 | Elemental abundances of Kepler Objects of Interest in APOGEE. I. Two distinct orbital period regimes inferred from host star iron abundances. | WILSON R.F., TESKE J., MAJEWSKI S.R., 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. | ||
2019RAA....19...41G | 17 | D | 1 | 1982 | 17 | Transit timing variations and linear ephemerides of confirmed Kepler transiting exoplanets. | GAJDOS P., VANKO M. and PARIMUCHA S. | ||
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 | 1 | 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..211C | 17 | D | 1 | 351 | 93 | Evolution of the radius valley around low-mass stars from Kepler and K2. | CLOUTIER R. and MENOU K. | ||
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. | ||
2021AJ....161..246J | 17 | D | 7 | 204 | 12 | Following up the Kepler field: masses of targets for transit timing and atmospheric characterization. | JONTOF-HUTTER D., WOLFGANG A., FORD E.B., et al. | ||
2022AJ....163...91J | 45 | X | 1 | 248 | ~ | Physical properties and impact parameter variations of Kepler planets from analytic light-curve modeling. | JUDKOVSKY Y., OFIR A. and AHARONSON O. | ||
2022ApJS..261...26S | 18 | D | 2 | 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. |