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An X-Ray-selected Active Galactic Nucleus at z = 4.6 Discovered by the CYDER Survey*

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© 2004. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Ezequiel Treister et al 2004 ApJ 603 36 DOI 10.1086/381432

0004-637X/603/1/36

Abstract

We present the discovery of a high-redshift, X-ray-selected active galactic nucleus (AGN) by the Calan-Yale Deep Extragalactic Research (CYDER) survey: CXOCY J033716.7-050153, located at z = 4.61, the second high-redshift AGN discovered by this survey. Here we present its optical, near-IR, and X-ray properties and compare it with other optical and X-ray-selected high-redshift AGNs. The optical luminosity of this object is significantly lower than most optically selected high-redshift quasars. It also has a lower rest-frame UV to X-ray emission ratio than most known quasars at this redshift. This mild deviation can be explained either by dust obscuring the UV radiation of a normal radio-quiet AGN emitting at 10% of its Eddington luminosity or because this is intrinsically a low-luminosity radio-loud AGN with a supermassive black hole of ~108 M emitting at 1% of its Eddington luminosity. Deep radio observations can discriminate between these two hypotheses.

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Footnotes

  • Partly based on observations collected at the European Southern Observatory, Chile, under program 72.A-0509.

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10.1086/381432