/ftp/cats/aliases/K/./KX_1_



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J/MNRAS/328/150     KX redshift survey                       (Croom+, 2001)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
	table?.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/MNRAS/328/150
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drwxr-xr-x 9 cats archive 186 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 4096 Jan 13 2023 [TAR file] -rw-r--r-- 1 cats archive 468 Dec 19 2022 .message -r--r--r-- 1 cats archive 5680 Apr 5 2006 ReadMe -rw-r--r-- 1 cats archive 614 Sep 19 2007 +footg5.gif -rw-r--r-- 1 cats archive 2287 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 1322 Mar 11 2002 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 3358 Mar 11 2002 table2.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 138 Mar 11 2002 table3.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 1607 Mar 11 2002 table4.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : J/MNRAS/328/150 KX redshift survey (Croom+, 2001) ================================================================================ A small-area faint KX redshift survey for QSOs in the ESO Imaging Survey Chandra Deep Field South. Croom S.M., Warren S.J., Glazebrook K. <Mon. Not. R. Astron. Soc. 328, 150 (2001)> =2001MNRAS.328..150C ================================================================================ ADC_Keywords: X-ray sources ; Redshifts ; QSOs ; Galaxies, IR ; Galaxies, photometry Keywords: surveys - galaxies: active - quasars: general - infrared: galaxies Abstract: In this paper we present preliminary spectroscopic results from a small-area faint K-excess (KX) survey, and compare KX selection against UVX selection. The aim of the KX method is to produce complete samples of QSOs that are flux-limited in the K band, in order to minimize any selection bias in samples of QSOs from the effects of reddening and extinction. Using the photometric catalogue of the ESO Imaging Survey Chandra Deep Field South (48arcmin^2^) we have identified compact objects with J-K colours redder than the stellar sequence that are brighter than K=19.5. We have obtained spectra of 33 candidates, using the LDSS++ spectrograph on the Anglo-Australian Telescope (AAT). Amongst the 11 bluer candidates, with V-J<3, three are confirmed as QSOs. Identification of the 22 redder candidates with V-J>=3 is substantially incomplete, but so far no reddened QSOs have been found. Near-infrared spectroscopy will be more effective in identifying some of these targets. Only two UVX (U-B<-0.2) sources brighter than K=19.5 are found that are not also KX selected. These are both identified as galactic stars. Thus KX selection appears to select all UVX QSOs. The surface density of QSOs in the blue subsample (V-J<3) at K<=19.5 is 325^+136^_-177_deg^-2^. Because identification of the red subsample (V-J>=3) is substantially incomplete, the 2sigma upper limit on the density of reddened QSOs is large, <1150deg^-2^. As anticipated, at these faint magnitudes the KX sample includes several compact galaxies. Of the 14 with measured redshifts, there are roughly equal numbers of early- and late-type objects. Nearly all the early-type galaxies are found in a single structure at z=0.66.