KOI-3557 , the SIMBAD biblio

KOI-3557 , the SIMBAD biblio (20 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.23CEST09:28:20


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Title First 3 Authors
2011AJ....141...83P viz 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 viz 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 viz 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 viz 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 viz 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 viz 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 viz 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 viz 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 viz 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 viz 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 viz 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 viz 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 viz 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 viz 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 viz 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 viz 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 viz 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 viz 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.

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