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Kepler-132b , the SIMBAD biblio (23 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST02:50:57 |
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 |
---|---|---|---|---|---|---|---|---|---|
2012Natur.486..375B | 15 | D | 1 | 378 | 520 | An abundance of small exoplanets around stars with a wide range of metallicities. | BUCHHAVE L.A., LATHAM D.W., JOHANSEN A., 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. | ||
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...783....4W | 16 | D | 1 | 487 | 103 | Influence of stellar multiplicity on planet formation. I. Evidence of suppressed planet formation due to stellar companions within 20 AU and validation of four planets from the Kepler multiple planet candidates. | WANG J., XIE J.-W., BARCLAY T., et al. | ||
2014ApJ...784...44L | 198 | X | 5 | 47 | 179 | Validation of Kepler's multiple planet candidates. II. Refined statistical framework and descriptions of systems of special interest. | LISSAUER J.J., MARCY G.W., BRYSON S.T., 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...790..146F | 55 | D | X | 2 | 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. | |
2015AJ....149...55E | 16 | D | 6 | 48 | 34 | High-resolution multi-band imaging for validation and characterization of small Kepler planets. | EVERETT M.E., BARCLAY T., CIARDI D.R., 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 | 16 | D | 1 | 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 | 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. | ||
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. | ||
2017AJ....154..109F | 16 | D | 1 | 900 | 847 | The California-Kepler Survey. III. A gap in the radius distribution of small planets. | FULTON B.J., PETIGURA E.A., HOWARD A.W., 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. | ||
2018ApJ...864L..38D | 16 | D | 1 | 109 | 49 | Larger mutual inclinations for the shortest-period planets. | DAI F., MASUDA K. and WINN J.N. | ||
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 | 17 | 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 | 17 | 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. | ||
2019A&A...624A..46L | 125 | X | 3 | 9 | 4 | Co-orbital exoplanets from close-period candidates: the TOI-178 case. | LELEU A., LILLO-BOX J., SESTOVIC M., et al. | ||
2019MNRAS.485.3999M | 17 | 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 | 17 | D | 1 | 4069 | 2 | Visual analysis and demographics of Kepler transit timing variations. | KANE M., RAGOZZINE D., FLOWERS X., et al. |