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KOI-3557 , the SIMBAD biblio (20 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST08:24:28 |
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. | ||
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. | ||
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. | ||
2015AJ....149...18K | 95 | D | C | 2 | 97 | 61 | Detection of stars within : ∼0.8 in of Kepler objects of interest. | KOLBL R., MARCY G.W., ISAACSON H., 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. | ||
2015ApJ...814..130M | 16 | D | 1 | 2846 | 162 | An increase in the mass of planetary systems around lower-mass stars. | MULDERS G.D., PASCUCCI I. and APAI D. | ||
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. | ||
2016A&A...594A..39F | 16 | D | 2 | 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. | ||
2017AJ....153...71F | 16 | D | 1 | 3575 | 164 | The Kepler follow-up observation program. I. A catalog of companions to Kepler stars from high-resolution imaging. | FURLAN E., CIARDI D.R., EVERETT M.E., 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. | ||
2016PASP..128g4502M | 16 | D | 1 | 305 | 14 | Identifying false alarms in the Kepler planet candidate catalog. | MULLALLY F., COUGHLIN J.L., THOMPSON S.E., et al. | ||
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. | ||
2018MNRAS.478.1272H | 16 | D | 1 | 100 | 1 | The fidelity of Kepler eclipsing binary parameters inferred by the neural network. | HOLANDA N. and DA SILVA J.R.P. | ||
2019ApJ...879...69T | 17 | D | 1 | 222609 | 141 | The Payne: self-consistent ab initio fitting of stellar spectra. | TING Y.-S., CONROY C., RIX H.-W., et al. | ||
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. | ||
2020AJ....160..120J | 17 | D | 1 | 365761 | 238 | APOGEE data and spectral analysis from SDSS Data Release 16: seven years of observations including first results from APOGEE-South. | JONSSON H., HOLTZMAN J.A., ALLENDE PRIETO C., et al. | ||
2022AJ....163..128W | 18 | D | 1 | 1570 | 6 | The influence of 10 unique chemical elements in shaping the distribution of Kepler planets. | WILSON R.F., CANAS C.I., MAJEWSKI S.R., et al. |