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20 April 2024 |
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The ROSAT Deep Survey: VI. X-ray sources and Optical identifications of the Ultra Deep Survey | | I. Lehmann
; G. Hasinger
; M. Schmidt
; R. Giacconi
; J. Truemper
; G. Zamorani
; J.E. Gunn
; L. Pozzetti
; D.P. Schneider
; T. Stanke
; G. Szokoly
; D. Thompson
; G. Wilson
; | | Date: |
22 Mar 2001 | | Subject: | astro-ph | | Abstract: | We describe in this paper the ROSAT Ultra Deep Survey (UDS), an extension of the ROSAT Deep Survey (RDS) in the Lockman Hole. The UDS reaches a flux level of 1.2 x 10E-15 erg/cm2/s in 0.5-2.0 keV energy band, a level ~4.6 times fainter than the RDS. We present nearly complete spectroscopic identifications (90%) of the sample of 94 X-ray sources based on low-resolution Keck spectra. The majority of the sources (57) are broad emission line AGNs (type I), whereas a further 13 AGNs show only narrow emission lines or broad Balmer emission lines with a large Balmer decrement (type II AGNs) indicating significant optical absorption. The second most abundant class of objects (10) are groups and clusters of galaxies (~11%). Further we found five galactic stars and one ’’normal’’ emission line galaxy. Eight X-ray sources remain spectroscopically unidentified. The photometric redshift determination indicates in three out of the eight sources the presence of an obscured AGN in the range of 1.2 < z < 2.7. These objects could belong to the long-sought population of type 2 QSOs, which are predicted by the AGN synthesis models of the X-ray background. Finally, we discuss the optical and soft X-ray properties of the type I AGN, type II AGN, and groups and clusters of galaxies, and the implications to the X-ray backround. | | Source: | arXiv, astro-ph/0103368 | | Services: | Forum | Review | PDF | Favorites | |
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