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KOI-4777 , the SIMBAD biblio (16 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST16:41:06 |
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...770...43M | 16 | D | 2 | 202 | 41 | Testing the metal of late-type Kepler planet hosts with iron-clad methods. | MANN A.W., GAIDOS E., KRAUS A., et al. | ||
2014AJ....147..119C | 16 | D | 1 | 8010 | 91 | Contamination in the Kepler field. Identification of 685 KOIs as false positives via ephemeris matching based on Q1-Q12 data. | COUGHLIN J.L., THOMPSON S.E., BRYSON S.T., et al. | ||
2014ApJ...788..114R | 16 | D | 1 | 184 | 17 | M-dwarf rapid rotators and the detection of relatively young multiple M-star systems. | RAPPAPORT S., SWIFT J., LEVINE A., 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. | ||
2016ApJ...822...86M | 16 | D | 1 | 6130 | 337 | False positive probabilities for all Kepler objects of interest: 1284 newly validated planets and 428 likely false positives. | MORTON T.D., BRYSON S.T., COUGHLIN J.L., et al. | ||
2016MNRAS.457.2877G | 16 | D | 1 | 4245 | 141 | They are small worlds after all: revised properties of Kepler M dwarf stars and their planets. | GAIDOS E., MANN A.W., KRAUS A.L., et al. | ||
2017MNRAS.465.2634A | 16 | D | 2 | 5400 | 21 | Transit shapes and self-organizing maps as a tool for ranking planetary candidates: application to Kepler and K2. | ARMSTRONG D.J., POLLACCO D. and SANTERNE A. | ||
2018AJ....155..161Z | 16 | D | 1 | 1274 | 24 | Robo-AO Kepler survey. IV. The effect of nearby stars on 3857 planetary candidate systems. | ZIEGLER C., LAW N.M., BARANEC C., 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. | ||
2019AJ....158...58C | 17 | D | 2 | 107 | ~ | Autoregressive planet search: application to the Kepler mission. | CACERES G.A., FEIGELSON E.D., BABU G.J., et al. | ||
2020ApJ...890...23L | 17 | D | 1 | 4935 | 35 | Current population statistics do not favor photoevaporation over core-powered mass loss as the dominant cause of the exoplanet radius gap. | LOYD R.O.P., SHKOLNIK E.L., SCHNEIDER A.C., et al. | ||
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. | ||
2020AJ....160..253L | 17 | D | 1 | 3432 | 12 | An increase in small-planet occurrence with metallicity for late-type dwarf stars in the Kepler field and its implications for planet formation. | LU C.X., SCHLAUFMAN K.C. and CHENG S. | ||
2022AJ....163....3C | 2643 | A | D | X C | 59 | 14 | 3 | A hot Mars-sized exoplanet transiting an M dwarf. | CANAS C.I., MAHADEVAN S., COCHRAN W.D., et al. |
2023ApJ...954L..50E | 19 | D | 1 | 205 | ~ | Living with a Red Dwarf: The Rotation-Age Relationships of M Dwarfs. | ENGLE S.G. and GUINAN E.F. |