/ftp/cats/II/301



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II/301              The DEEP2-DR1 Photometric Catalog               (Coil+ 2004)
The following files can be converted to FITS (extension .fit or fit.gz)
	catalog.dat.gz
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=II/301
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drwxr-xr-x 351 cats archive 8192 Mar 25 10:13 [Up] drwxr-xr-x 3 cats archive 4096 Jan 13 2023 [TAR file] -rw-r--r-- 1 cats archive 465 Dec 19 2022 .message -r--r--r-- 1 cats archive 4653 Nov 13 2012 ReadMe -rw-r--r-- 1 cats archive 1040 Dec 12 2012 +footg5.gif -rw-r--r-- 1 cats archive 3178 Dec 12 2012 +footg8.gif -r--r--r-- 1 cats archive 24589049 Nov 13 2012 catalog.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html] drwxr-xr-x 2 cats archive 4096 Mar 23 2016 fits
Beginning of ReadMe : II/301 The DEEP2-DR1 Photometric Catalog (Coil+ 2004) ================================================================================ Evolution and Color Dependence of the Galaxy Angular Correlation Function: 350,000 Galaxies in 5 Square Degrees Coil Alison L., Newman Jeffrey A., Kaiser Nick, Davis Marc, Ma Chung-Pei, Kocevski Dale D., Koo David C. <Astrophys. J. 617, 765 (2004)> =2004ApJ...617..765C ================================================================================ ADC_Keywords: Galaxies, photometry; Photometry, VRI ; Surveys Keywords: galaxies: statistics ; galaxies: evolution ; cosmology: large-scale structure of universe Description: The Deep Extragalactic Evolutionary Probe (DEEP) is a multi-year program which uses the twin 10m Keck Telescopes and the Hubble Space Telescope (HST) to conduct a truly large-scale survey of distant, faint, field galaxies. The broad scientific goals include: the formation and evolution of galaxies, the origin of large-scale structure, the nature of the dark matter, and the geometry of the Universe. This project is led by the Lick Observatory at University of California (UC) Santa Cruz, in collaboration with UC Berkeley, University of Hawaii (UH) Manoa, Johns Hopkins University, University of Chicago and California Institute of Technology. The photometric data were taken with the CFH12K camera on the 3.6-meter Canada-France-Hawai'i Telescope. Each DEEP2 field is covered by multiple CFHT/CFH12K pointings with each pointing numbered within its respective