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| Kepler-971b , the SIMBAD biblio (20 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST22:55:22 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
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 |
15 | D | 2 | 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. | ||
|
2014ApJS..210...19B |
15 | 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...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. | ||
|
2015ApJS..217...31M |
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. | |||||
|
2016AJ....152..158T |
16 | D | 1 | 4388 | 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. | ||
|
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...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. | ||
|
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. | ||
|
2019RAA....19...41G |
16 | D | 1 | 1982 | 17 | Transit timing variations and linear ephemerides of confirmed Kepler transiting exoplanets. | GAJDOS P., VANKO M. and PARIMUCHA S. | ||
|
2019ApJ...875...29M |
16 | 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 |
16 | D | 1 | 4069 | 2 | Visual analysis and demographics of Kepler transit timing variations. | KANE M., RAGOZZINE D., FLOWERS X., et al. | ||
|
2020AJ....159..239G |
16 | D | 1 | 1408 | ~ | Updated parameters and a new transmission spectrum of HD 97658b. | GUO X., CROSSFIELD I.J.M., DRAGOMIR D., et al. | ||
|
2021MNRAS.505.1293S |
17 | D | 1 | 573 | 7 | Systematic search for long-term transit duration changes in Kepler transiting planets. | SHAHAF S., MAZEH T., ZUCKER S., et al. | ||
|
2022MNRAS.510.3449B |
17 | D | 1 | 508 | 7 | Exoplanets in the Galactic context: planet occurrence rates in the thin disc, thick disc, and stellar halo of Kepler stars. | BASHI D. and ZUCKER S. | ||
|
2022ApJS..261...26S |
17 | D | 1 | 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. |