/ftp/cats/ii/316



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II/316              UKIDSS-DR6 Galactic Plane Survey      (Lucas+ 2012)
The following files can be converted to FITS (extension .fit or fit.gz)
	gps6.sam
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=II/316
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drwxr-xr-x 351 cats archive 8192 Mar 25 10:13 [Up] drwxr-xr-x 3 cats archive 4096 Jan 10 10:46 [TAR file] -rw-r--r-- 1 cats archive 450 Jan 10 10:45 .message -r--r--r-- 1 cats archive 12033 Aug 31 2012 ReadMe -rw-r--r-- 1 cats archive 1307 Jan 10 10:44 +footg5.gif -rw-r--r-- 1 cats archive 3398 Jan 10 10:46 +footg5.png -rw-r--r-- 1 cats archive 8723 Jan 10 10:44 +footg8.gif -rw-r--r-- 1 cats archive 20631 Jan 10 10:46 +footg8.png -rw-r--r-- 1 cats archive 530000 Aug 31 2012 gps6.sam -r--r--r-- 3 cats archive 1450 Jul 19 2012 ppflags.htx
Beginning of ReadMe : II/316 UKIDSS-DR6 Galactic Plane Survey (Lucas+ 2012) ================================================================================ UKIRT Infrared Deep Sky Survey (UKIDSS) Galactic Plane Survey (GPS) Release 6 UKIDSS Consortium <Mon. Not. R. Astron. Soc. 391, 136 (2008)> =2008MNRAS.391..136L =2012yCat.2316....0U ================================================================================ ADC_Keywords: Surveys ; Infrared sources ; Photometry, infrared ; Galactic plane Keywords: survey ; methods: data analysis ; stars: formation ; stars: circumstellar matter; Galaxy: stellar content Description: The UKIDSS Galactic Plane Survey (GPS) is one of the five near infrared Public Legacy Surveys that are being undertaken by the UKIDSS consortium, using the Wide Field Camera on the United Kingdom Infrared Telescope. It is surveying 1868 deg^2^ of the northern and equatorial Galactic plane at Galactic latitudes -5deg<b<5deg in the J, H and K filters and a  300 deg^2^ area of the Taurus-Auriga-Perseus molecular cloud complex in these three filters and the 2.12mum (1-0)S(1)H_2_ filter. It will provide data on   3x10^9^ sources. The survey use the Wide Field Camera (WFCAM, see Casali et al. 2007A&A...467..777C) on the United Kingdom Infrared Telescope (UKIRT). The typical 90% completeness limits in uncrowded fields are K=18.0, H=18.75, J=19.5, with uncertainties of about 0.2mag.