/ftp/cats/ii/211



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II/211              K-band survey in high galactic latitude (Glazebrook+ 1994)
The following files can be converted to FITS (extension .fit .fiz or .fiZ)
	ircam.dat catalog.dat spectro.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=II/211
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drwxr-xr-x 351 cats archive 8192 Mar 25 10:13 [Up] drwxr-xr-x 3 cats archive 320 Jan 12 2023 [TAR file] -rw-r--r-- 1 cats archive 485 Dec 19 2022 .message -r--r--r-- 1 cats archive 7190 Dec 11 2015 ReadMe -rw-r--r-- 1 cats archive 1045 Dec 11 2015 +footg5.gif -rw-r--r-- 1 cats archive 3421 Dec 11 2015 +footg8.gif -r--r--r-- 1 cats archive 61498 Nov 8 1996 catalog.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 18876 Nov 8 1996 ircam.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 11779 Nov 8 1996 spectro.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : II/211 K-band survey in high galactic latitude (Glazebrook+ 1994) ================================================================================ An imaging K-band survey- I. The catalogue, star and galaxy counts. Glazebrook K., Peacock J.A., Collins C.A., Miller L. <Mon. Not. R. Astron. Soc. 266, 65 (1994)> =1994MNRAS.266...65G II. The redshift survey and galaxy evolution in the infrared. Glazebrook K., Peacock J.A., Miller L., Collins C.A. <Mon. Not. R. Astron. Soc. 275, 169 (1995)> =1995MNRAS.275..169G ================================================================================ ADC_Keywords: Photometry, CCD ; Photometry, infrared ; Surveys ; Redshifts Keywords: surveys - stars: low-mass, brown dwarfs - galaxies: evolution - infrared: general Description: The survey is a high galactic latitude, large area (552 square arcmin) blank-field sample to a 5sigma limit of K=17.3mag. Star-galaxy discrimination is performed. The infrared observations were made over the period 1987-1988, using the infrared camera IRCAM at the 3.8m UKIRTelescope at Mauna Kea, Hawai. The pixel size is 1.2arcsec. The redshift survey (spectro.dat) concerns 124 galaxies of the survey, and was carried out on the Anglo-Australian telescope and the William Herschel telescope at La Palma over the period 1990-1992, with a multi-fibre spectrograph for the brighter objects (R<19), long and multi-slit spectrographs for fainter objects.