Very high redshift X-ray-selected active galactic nuclei in the Chandra Deep Field-North

  • A. J. Barger
  • , L. L. Cowie
  • , P. Capak
  • , D. M. Alexander
  • , F. E. Bauer
  • , W. N. Brandt
  • , G. P. Garmire
  • , A. E. Hornschemeier

Research output: Contribution to journalArticlepeer-review

82 Scopus citations

Abstract

Deep Chandra X-ray exposures provide an efficient route for locating optically faint active galactic nuclei (AGNs) at high redshifts. We use deep multicolor optical data to search for z > 5 AGNs in the 2 Ms X-ray exposure of the Chandra Deep Field-North. Of the 423 X-ray sources bright enough (z′ < 25.2) for a color-color analysis, at most one lies at z = 5-6, and none at z > 6. The one z > 5 object is spectroscopically confirmed at z = 5.19. Only 31 of the 77 sources with z′ > 25.2 are undetected in the B or V bands at the 2 σ level and could lie at z > 5. There are too few moderate-luminosity AGNs at z = 5-6.5 to ionize the intergalactic medium.

Original languageEnglish (US)
Pages (from-to)L61-L64
JournalAstrophysical Journal
Volume584
Issue number2 II
DOIs
StatePublished - Feb 20 2003

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

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