|
other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
| KOI-4419 , the SIMBAD biblio (16 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST09:03:08 |
| 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...779..165J | 207 | D | X C | 5 | 37 | 20 | A survey for very short-period planets in the Kepler data. | JACKSON B., STARK C.C., ADAMS E.R., et al. | |
|
2014AJ....147..119C |
15 | D | 1 | 8013 | 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...787...47S |
15 | D | 1 | 222 | 160 | A study of the shortest-period planets found with Kepler. | SANCHIS-OJEDA R., RAPPAPORT S., WINN J.N., 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. | ||
|
2017ApJ...835...75J |
56 | D | X | 2 | 211 | 3 | Rotation periods of wide binaries in the Kepler field. | JANES K.A. | |
| 2018ApJ...853...59C | 16 | D | 1 | 116 | ~ | Flare activity of wide binary stars with Kepler. | CLARKE R.W., DAVENPORT J.R.A., COVEY K.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. | ||
|
2020ApJ...890...23L |
16 | D | 1 | 4936 | 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 |
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. | ||
|
2020AJ....160..253L |
16 | 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. | ||
| 2021MNRAS.504.5327A | 17 | D | 1 | 7000 | 19 | Exoplanet validation with machine learning: 50 new validated Kepler planets. | ARMSTRONG D.J., GAMPER J. and DAMOULAS T. | ||
|
2022AJ....163..179P |
17 | D | 1 | 2962 | 39 | The California-Kepler Survey. X. The Radius Gap as a Function of Stellar Mass, Metallicity, and Age. | PETIGURA E.A., ROGERS J.G., ISAACSON H., et al. | ||
|
2024AJ....168...92L |
18 | D | 1 | 209 | ~ | Variations in the Radius Distribution of Single- and Compact Multiple-transiting Planets. | LIBERLES B.T., DITTMANN J.A., ELARDO S.M., et al. | ||
|
2024AJ....168..109S |
18 | D | 2 | 702 | ~ | Resonant and Ultra-short-period Planet Systems Are at Opposite Ends of the Exoplanet Age Distribution. | SCHMIDT S.P., SCHLAUFMAN K.C. and HAMER J.H. | ||
|
2024A&A...689A.250C |
18 | D | 1 | 3075 | ~ | Mapping the exo-Neptunian landscape A ridge between the desert and savanna. | CASTRO-GONZALEZ A., BOURRIER V., LILLO-BOX J., et al. |