The first optical validation of an XLEO: a detection in the XMM-Newton observation of the CDFS
arXiv:astro-ph/0502091 · doi:10.1086/429253
Abstract
We present the first optical validation of an X-ray Line-Emitting Object (XLEO) discovered in the XMM-Newton observation of the Chandra Deep Field South. The object is an AGN at z_x ~ 0.66. An optical spectrum of the source indeed confirms and refines (z_o = 0.665) the redshift obtained from the X-ray line. The X-ray and optical properties of the source are presented and discussed.
arXiv comment13 pages, 3 figures. Accepted for publication by ApJL
References in corpus (8)
- Stellar population synthesis at the resolution of 2003
- The Chandra Deep Field South: the 1 Million Second
- The Chandra Deep Field South: Optical Spectroscopy I
- A 3 dimensional diagnostic diagram for Seyfert 2s: probing X-ray absorption and Compton thickness
- The Spectral Energy Distributions of Low-Luminosity Active Galactic Nuclei
- ASCA observations of Seyfert 1 galaxies: I. Data Analysis, Imaging and Timing
- XMM-Newton observations expose AGN in apparently normal galaxies
- X-ray Line Emitting Objects in XMM-Newton Observations: the Tip of the Iceberg
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- 4C 39.29 - extended emission around a powerful Type 2 quasar
- An X-ray bright ERO hosting a type 2 QSO
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