Open AccessA small‐area faint KX redshift survey for QSOs in the ESO Imaging Survey Chandra Deep Field South
Author(s) -
Croom Scott M.,
Warren S.J.,
Glazebrook K.
Publication year - 2001
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1046/j.1365-8711.2001.04846.x
Subject(s) - qsos , physics , astrophysics , chandra deep field south , redshift , extinction (optical mineralogy) , astronomy , photometry (optics) , stars , galaxy , optics
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 (48 arcmin 2 ) we have identified compact objects with colours redder than the stellar sequence that are brighter than . We have obtained spectra of 33 candidates, using the LDSS++ spectrograph on the Anglo‐Australian Telescope (AAT). Amongst the 11 bluer candidates, with , three are confirmed as QSOs. Identification of the 22 redder candidates with 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 sources brighter than 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 at is . Because identification of the red subsample is substantially incomplete, the 2 σ upper limit on the density of reddened QSOs is large, <1150 deg −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 .