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KOI-1075 , the SIMBAD biblio (20 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.05.07CEST03:35:50 |
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 |
---|---|---|---|---|---|---|---|---|---|
2011AJ....141...83P | 15 | D | 1 | 1891 | 430 | Kepler eclipsing binary stars. I. Catalog and principal characterization of 1879 eclipsing binaries in the first data release. | PRSA A., BATALHA N., SLAWSON R.W., et al. | ||
2011ApJ...736...19B | 15 | D | 1 | 1507 | 867 | Characteristics of planetary candidates observed by Kepler. II. Analysis of the first four months of data. | BORUCKI W.J., KOCH D.G., BASRI G., et al. | ||
2011AJ....142..160S | 15 | D | 1 | 2325 | 365 | Kepler eclipsing binary stars. II. 2165 eclipsing binaries in the second data release. | SLAWSON R.W., PRSA A., WELSH W.F., et al. | ||
2012ApJS..199...24T | 15 | D | 1 | 5394 | 66 | Detection of potential transit signals in the first three quarters of Kepler mission data. | TENENBAUM P., CHRISTIANSEN J.L., JENKINS J.M., et al. | ||
2013MNRAS.436.1883W | 16 | D | 1 | 961 | 136 | Rotation periods, variability properties and ages for Kepler exoplanet candidate host stars. | WALKOWICZ L.M. and BASRI G.S. | ||
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. | ||
2014MNRAS.437.3473A | 16 | D | 1 | 2614 | 45 | A catalogue of temperatures for Kepler eclipsing binary stars. | ARMSTRONG D.J., GOMEZ MAQUEO CHEW Y., FAEDI F., et al. | ||
2014AJ....147..119C | 16 | D | 2 | 8010 | 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. | ||
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. | ||
2016AJ....151...68K | 16 | D | 1 | 2914 | 316 | Kepler eclipsing binary stars. VII. The catalog of eclipsing binaries found in the entire Kepler data set. | KIRK B., CONROY K., PRSA A., et al. | ||
2016ApJ...822...86M | 16 | D | 1 | 6130 | 337 | False positive probabilities for all Kepler objects of interest: 1284 newly validated planets and 428 likely false positives. | MORTON T.D., BRYSON S.T., COUGHLIN J.L., et al. | ||
2016ApJS..224...37G | 16 | D | 1 | 239 | 24 | White-light flares on close binaries observed with Kepler. | GAO Q., XIN Y., LIU J.-F., et al. | ||
2016A&A...594A..39F | 16 | D | 1 | 51408 | 86 | Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra. | FRASCA A., MOLENDA-ZAKOWICZ J., DE CAT P., et al. | ||
2017MNRAS.465.2634A | 16 | D | 1 | 5400 | 21 | Transit shapes and self-organizing maps as a tool for ranking planetary candidates: application to Kepler and K2. | ARMSTRONG D.J., POLLACCO D. and SANTERNE A. | ||
2017AJ....154..250L | 16 | D | 1 | 2280 | 72 | Tidal synchronization and differential rotation of Kepler eclipsing binaries. | LURIE J.C., VYHMEISTER K., HAWLEY S.L., et al. | ||
2018ApJS..235....5Q | 16 | D | 2 | 2048 | 72 | Physical properties and evolutionary states of EA-type eclipsing binaries observed by LAMOST. | QIAN S.-B., ZHANG J., HE J.-J., et al. | ||
2018AJ....155..161Z | 16 | D | 2 | 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...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. | ||
2019AJ....157..235C | 42 | X | 1 | 415 | 7 | Observations of the Kepler field with TESS: predictions for planet yield and observable features. | CHRIST C.N., MONTET B.T. and FABRYCKY D.C. | ||
2019ApJS..244...43Z | 17 | D | 1 | 1328 | 22 | Unbiased distribution of binary parameters from LAMOST and Kepler observations. | ZHANG J., QIAN S.-B., WU Y., et al. |