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Kepler-210b , the SIMBAD biblio (19 results) | C.D.S. - SIMBAD4 rel 1.7 - 2021.01.27CET18:48:59 |
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 |
---|---|---|---|---|---|---|---|---|---|
2020AJ....159..211C ![]() |
19 | D | 1 | 351 | ~ | Evolution of the radius valley around low-mass stars from Kepler and K2. | CLOUTIER R. and MENOU K. | ||
2020AJ....159..239G ![]() |
19 | D | 1 | 1408 | ~ | Updated parameters and a new transmission spectrum of HD 97658b. | GUO X., CROSSFIELD I.J.M., DRAGOMIR D., et al. | ||
2018AJ....155...68W ![]() |
17 | D | 1 | 509 | 10 | Elemental abundances of Kepler Objects of Interest in APOGEE. I. Two distinct orbital period regimes inferred from host star iron abundances. | WILSON R.F., TESKE J., MAJEWSKI S.R., et al. | ||
2018AJ....155..206A ![]() |
17 | D | 3 | 183 | ~ | Systematic search for rings around Kepler planet candidates: constraints on ring size and occurrence rate. | AIZAWA M., MASUDA K., KAWAHARA H., et al. | ||
2018ApJ...866...99B ![]() |
17 | D | 1 | 7129 | 101 | Revised radii of Kepler stars and planet's using Gaia Data Release 2. | BERGER T.A., HUBER D., GAIDOS E., et al. | ||
2018MNRAS.477..808L | 366 | D | X C | 8 | 17 | 1 | Atmospheric mass-loss of extrasolar planets orbiting magnetically active host stars. | LALITHA S., SCHMITT J.H.M.M. and DASH S. | |
2017AJ....154..160S | 17 | D | 1 | 149 | 5 | Average albedos of close-in super-earths and super-Neptunes from statistical analysis of long-cadence Kepler secondary eclipse data. | SHEETS H.A. and DEMING D. | ||
2016A&A...594A..41I | 42 | X | 1 | 3 | 2 | Glimpses of stellar surfaces. I. Spot evolution and differential rotation of the planet host star Kepler-210. | IOANNIDIS P. and SCHMITT J.H.M.M. | ||
2016AJ....152..158T ![]() |
17 | D | 1 | 4386 | 18 | 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. | ||
2015ApJ...807...45D ![]() |
16 | D | 1 | 2708 | 411 | 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. | ||
2015ApJS..217...16R ![]() |
16 | D | 1 | 8625 | 84 | Planetary candidates observed by Kepler. V. Planet sample from Q1-Q12 (36 months). | ROWE J.F., COUGHLIN J.L., ANTOCI V., et al. | ||
2014A&A...564A..33I ![]() |
326 | X C | 7 | 5 | 5 | Kepler-210: An active star with at least two planets. | IOANNIDIS P., SCHMITT J.H.M.M., AVDELLIDOU C., et al. | ||
2014A&A...566A.103L ![]() |
16 | D | 1 | 359 | 67 | High-resolution imaging of Kepler planet host candidates. A comprehensive comparison of different techniques. | LILLO-BOX J., BARRADO D. and BOUY H. | ||
2014ApJ...784...45R ![]() |
16 | D | 1 | 1691 | 227 | 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 ![]() |
16 | D | 1 | 918 | 322 | 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. | ||
2014ApJ...794..133S | 179 | D | X | 5 | 41 | 21 | Statistical eclipses of close-in Kepler sub-saturns. | SHEETS H.A. and DEMING D. | |
2014ApJS..210...19B ![]() |
16 | D | 1 | 5860 | 162 | Planetary candidates observed by Kepler IV: planet sample from Q1-Q8 (22 months). | BURKE C.J., BRYSON S.T., MULLALLY F., et al. | ||
2013ApJS..204...24B ![]() |
16 | D | 1 | 3274 | 779 | 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. | ||
2012ApJ...756..185F ![]() |
16 | 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. |
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