KOI-1003 , the SIMBAD biblio

KOI-1003 , the SIMBAD biblio (30 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST13:07:02

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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
2002AJ....123.3460M viz 65 68 Planets in stellar clusters extensive search. I. Discovery of 47 low-amplitude variables in the metal-rich cluster NGC 6791 with millimagnitude image subtraction photometry. MOCHEJSKA B.J., STANEK K.Z., SASSELOV D.D., et al.
2003AJ....125.3175M 52 15 Long-term variability survey of the old open cluster NGC 6791. MOCHEJSKA B.J., STANEK K.Z. and KALUZNY J.
2005AJ....129.2856M viz 107 41 Planets in stellar clusters extensive search. III. A search for transiting planets in the metal-rich open cluster NGC 6791. MOCHEJSKA B.J., STANEK K.Z., SASSELOV D.D., et al.
2007A&A...471..515D viz 75           X         2 127 34 Variable stars in the open cluster NGC 6791 and its surrounding field. DE MARCHI F., PORETTI E., MONTALTO M., et al.
2011ApJ...736...19B viz 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.
2011ApJ...738..170M viz 15       D               1 997 230 On the low false positive probabilities of Kepler planet candidates. MORTON T.D. and JOHNSON J.A.
2011ApJS..197....2F viz 15       D               1 980 66 Transit timing observations from Kepler. I. Statistical analysis of the first four months. FORD E.B., ROWE J.F., FABRYCKY D.C., et al.
2011ApJS..197...12D 15       D               1 124 184 Lack of inflated radii for Kepler giant planet candidates receiving modest stellar irradiation. DEMORY B.-O. and SEAGER S.
2012ApJS..199...24T viz 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.
2012ApJ...752...72D viz 15       D               1 229 7 A correlation between the eclipse depths of Kepler gas giant candidates and the metallicities of their parent stars. DODSON-ROBINSON S.E.
2012ApJ...756..185F viz 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.
2012ApJ...756..186S viz 15       D               1 811 35 Transit timing observations from Kepler. VI. Potentially interesting candidate systems from fourier-based statistical tests. STEFFEN J.H., FORD E.B., ROWE J.F., et al.
2013A&A...553A..17S 78         O X         2 43 36 Multiple planets or exomoons in Kepler hot Jupiter systems with transit timing variations? SZABO R., SZABO GY.M., DALYA G., et al.
2013ApJS..208...16M viz 16       D               1 1518 139 Transit timing observations from Kepler. VIII. Catalog of transit timing measurements of the first twelve quarters. MAZEH T., NACHMANI G., HOLCZER T., et al.
2014ApJS..210...19B viz 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.
2014AJ....147..119C viz 16       D               1 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 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.
2015MNRAS.447.2714B viz 16       D               1 209 133 Flare stars across the H-R diagram. BALONA L.A.
2015ApJ...809....8B viz 16       D               1 112329 282 Terrestrial planet occurrence rates for the Kepler GK dwarf sample. BURKE C.J., CHRISTIANSEN J.L., MULLALLY F., 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               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.
2016ApJ...832..207R 2893 T K A D S   X C       70 2 6
KOI-1003: a new spotted, eclipsing RS CVn binary in the Kepler field. 		ROETTENBACHER R.M., KANE S.R., MONNIER J.D., 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.
2018AJ....155..177D viz 16       D               1 124 2 Stellar obliquity and magnetic activity of planet-hosting stars and eclipsing binaries based on transit chord correlation. DAI F., WINN J.N., BERTA-THOMPSON Z., et al.
2018MNRAS.473.5532R 43           X         1 26 59 BRITE-Constellation high-precision time-dependent photometry of the early O-type supergiant ζ puppis unveils the photospheric drivers of its small- and large-scale wind structures. RAMIARAMANANTSOA T., MOFFAT A.F.J., HARMON R., et al.
2019ApJS..241...29Y viz 17       D               1 3421 70 The flare catalog and the flare activity in the Kepler mission. YANG H. and LIU J.
2021ApJS..254...13G 466     A S   X C       9 10 56 Allesfitter: flexible star and exoplanet inference from photometry and radial velocity. GUNTHER M.N. and DAYLAN T.
2021RAA....21...89L 44           X         1 6 ~ A study of the global magnetic activity of the star Kepler-17 using light curve inversion with bipartite regularization. LUO T., LIANG Y.-Y., IP W.-H., et al.
2021AJ....162...98B viz 17       D               1 2175 ~ Seeking echoes of circumstellar disks in Kepler light curves. BROMLEY B.C., LEONARD A., QUINTANILLA A., et al.
2023AJ....165..247P 47           X         1 6 ~ KIC 7284688: A Solar-type Eclipsing Binary with Rapidly Varying O'Connell Effect. PAN Y. and ZHANG X.

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