/ftp/cats/aliases/U/UGCS8



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II/314   ==OBSOLETE version of Catalogue==
23-May-2013: (by Francois Ochsenbein) See II/319
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=II/314
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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 10:19 [TAR file] -rw-r--r-- 1 cats archive 391 Jan 10 10:19 .message -rw-r--r-- 1 cats archive 49 May 23 2013 =obsolete= -r--r--r-- 1 cats archive 22023 Dec 22 2012 ReadMe -rw-r--r-- 1 cats archive 1820 Dec 22 2012 +footg5.gif -rw-r--r-- 1 cats archive 7474 Dec 22 2012 +footg5.png -rw-r--r-- 1 cats archive 15383 Dec 22 2012 +footg8.gif -rw-r--r-- 1 cats archive 45508 Dec 22 2012 +footg8.png -r--r--r-- 1 cats archive 267908 Aug 17 2012 dxs8.sam -r--r--r-- 1 cats archive 537164 Aug 17 2012 gcs8.sam -r--r--r-- 1 cats archive 448304 Jan 27 2015 las8.sam -r--r--r-- 3 cats archive 1450 Jul 19 2012 ppflags.htx -rw-r--r-- 1 cats archive 8640 Aug 22 2022 tab_2314_3_II_314_dxs8.moc.fits
Beginning of ReadMe : II/314 UKIDSS-DR8 LAS, GCS and DXS Surveys (Lawrence+ 2012) ================================================================================ UKIRT Infrared Deep Sky Survey (UKIDSS) Release 8 Lawrence A., Warren S.J., Almaini O., Edge A.C., Hambly N.C., Jameson R.F., Lucas P., Casali M., Adamson A., Dye S., Emerson J.P., Foucaud S., Hewett P., Hirst P., Hodgkin S.T., Irwin M.J., Lodieu N., McMahon R.G., Simpson C., Smail I., Mortlock D., Folger M. <Mon. Not. R. Astron. Soc. 379, 1599 (2007)> =2007MNRAS.379.1599L =2012yCat.2314....0U ================================================================================ ADC_Keywords: Surveys ; Infrared sources ; Photometry, infrared Keywords: surveys - infrared: general Description: The UKIRT Infrared Deep Sky Survey (UKIDSS) is a large-scale near-IR survey which aim is to cover 7500 square degrees of the Northern sky. The survey is carried out using the Wide Field Camera (WFCAM), with a field of view of 0.21 square degrees, mounted on the 3.8m United Kingdom Infra-red Telescope (UKIRT) in Hawaii. The project comprises five surveys (LAS, GCS, DXS, GPS and UDS). The Large Area Survey (LAS) covers an area of 4000 square degrees in high Galactic latitudes (extragalactic) in the four bands Y(1.0um) J(1.2um) H(1.6um) and K(2.2um) to a depth of K=18.4. The Galactic Clusters Survey (GCS) aims to survey ten large open star clusters and star formation associations, covering a total of 1067 square degrees in the five bands Z (0.9um), Y(1.0um) J(1.2um) H(1.6um) and K(2.2um), plus a second pass in K for proper motions, to a depth of Z=20.4, Y=20.3, J=19.5, H=18.6, K=18.6. The Deep Extragalactic Survey (DXS) aims to map 35 square degrees of sky to a 5-sigma point-source sensitivity of J=22.3 and K=20.8 in four carefully selected, multi-wavelength survey areas. The central regions of each field will also be mapped to H=21.8. The primary aim of the survey is to produce a photometric galaxy sample at a redshift of 1-2, within a volume comparable to that of the SDSS, selected in the same passband (rest frame optical). Details of the surveys can be found in the in the paper by Lawrence et al. (2007MNRAS.379.1599L), and at the UKIDSS Surveys site (http://www.ukidss.org/surveys/surveys.html). The data described here represent a subset of the UKIDSS data, limited to the public data and most representative columns. In the "Byte-by-byte Description" below the original names of the columns are given as bracketed names. Usage of the UKIDSS data: All users of UKIDSS data should include an acknowledgement in their publications as follows: "This work is based in part on data obtained as part of the UKIRT Infrared Deep Sky Survey".