/ftp/cats/aliases/K/./KOI_3_



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J/ApJS/210/19     Kepler planetary candidates. IV. 22 months     (Burke+, 2014)
The following files can be converted to FITS (extension .fit or fit.gz)
	table1.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/ApJS/210/19
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drwxr-xr-x 14 cats archive 230 Jan 14 2015 [Up] drwxr-xr-x 3 cats archive 308 Jan 13 2023 [TAR file] -rw-r--r-- 1 cats archive 467 Dec 19 2022 .message -r--r--r-- 1 cats archive 7308 Aug 22 2016 ReadMe -rw-r--r-- 1 cats archive 1037 Apr 27 2015 +footg5.gif -rw-r--r-- 1 cats archive 2724 Apr 27 2015 +footg8.gif -r--r--r-- 1 cats archive 541100 Apr 1 2014 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/ApJS/210/19 Kepler planetary candidates. IV. 22 months (Burke+, 2014) ================================================================================ Planetary candidates observed by Kepler IV: planet sample from Q1-Q8 (22 months). Burke C.J., Bryson S.T., Mullally F., Rowe J.F., Christiansen J.L., Thompson S.E., Coughlin J.L., Haas M.R., Batalha N.M., Caldwell D.A., Jenkins J.M., Still M., Barclay T., Borucki W.J., Chaplin W.J., Ciardi D.R., Clarke B.D., Cochran W.D., Demory B.-O., Esquerdo G.A., Gautier III T.N., Gilliland R.L., Girouard F.R., Havel M., Henze C.E., Howell S.B., Huber D., Latham D.W., Li J., Morehead R.C., Morton T.D., Pepper J., Quintana E., Ragozzine D., Seader S.E., Shah Y., Shporer A., Tenenbaum P., Twicken J.D., Wolfgang A. <Astrophys. J. Suppl. Ser., 210, 19 (2014)> =2014ApJS..210...19B ================================================================================ ADC_Keywords: Planets ; Stars, double and multiple ; Stars, diameters ; Stars, masses ; Effective temperatures ; Surveys Mission_Name: Kepler Keywords: catalogs; eclipses; planetary systems; space vehicles Abstract: We provide updates to the Kepler planet candidate sample based upon nearly two years of high-precision photometry (i.e., Q1-Q8). From an initial list of nearly 13400 threshold crossing events, 480 new host stars are identified from their flux time series as consistent with hosting transiting planets. Potential transit signals are subjected to further analysis using the pixel-level data, which allows background eclipsing binaries to be identified through small image position shifts during transit. We also re-evaluate Kepler Objects of Interest (KOIs) 1-1609, which were identified early in the mission, using substantially more data to test for background false positives and to find additional multiple systems. Combining the new and previous KOI samples, we provide updated parameters for 2738 Kepler planet candidates distributed across 2017 host stars. From the combined Kepler planet candidates, 472 are new from the Q1-Q8 data examined in this study. The new Kepler planet candidates represent  40% of the sample with R_P_ 1R_oplus_ and represent  40% of the low equilibrium temperature (T_eq_<30 K) sample. We review the known biases in the current sample of Kepler planet candidates relevant to evaluating planet population statistics with the current Kepler planet candidate sample. Description: In 2011 November, the Q1-Q8 (22 months of data) Kepler pipeline run generated one or more TCEs (threshold crossing events) for  13400 Kepler targets out of  191000 targets searched.