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| KOI-2159.02 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST00:39:23 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2014ApJ...784...45R |
15 | D | 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...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. | ||
|
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. | ||
|
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. | ||
|
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. | ||
|
2018AJ....156...83Z |
16 | D | 1 | 337 | 14 | Robo-AO Kepler Survey. V. The effect of physically associated stellar companions on planetary systems. | ZIEGLER C., LAW N.M., BARANEC C., 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. | ||
|
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. |