Very High Redshift X-Ray-selected Active Galactic Nuclei in the Chandra Deep Field-North

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.

[1]  W. Brandt,et al.  The Redshift Evolution of the 2-8 keV X-Ray Luminosity Function , 2003, astro-ph/0301231.

[2]  S. Odewahn,et al.  A Simple Prediction of the Surface Density of Galaxies at z ≃ 6 , 2002, astro-ph/0208080.

[3]  W. N. Brandt,et al.  X-Ray, Optical, and Infrared Imaging and Spectral Properties of the 1 Ms Chandra Deep Field North Sources , 2002 .

[4]  M. A. Strauss,et al.  Exploratory Chandra Observations of the Three Highest Redshift Quasars Known , 2002, astro-ph/0202235.

[5]  S. Mathur,et al.  Chandra Detection of Highest Redshift (z ~ 6) Quasars in X-Rays , 2002, astro-ph/0202202.

[6]  L. Cowie,et al.  Approaching Reionization: The Evolution of the Lyα Forest from z = 4 to z = 6 , 2002, astro-ph/0202165.

[7]  Paul S. Smith,et al.  Discovery of a z = 4.93, X-Ray-selected Quasar by the Chandra Multiwavelength Project (ChaMP) , 2002, astro-ph/0201379.

[8]  W. Brandt,et al.  The 2-8 keV X-Ray Number Counts Determined from Chandra Blank Field Observations , 2002, astro-ph/0201186.

[9]  V. Narayanan,et al.  Evidence for Reionization at z ∼ 6: Detection of a Gunn-Peterson Trough in a z = 6.28 Quasar , 2001, astro-ph/0108097.

[10]  V. Narayanan,et al.  A Survey of z > 5.8 Quasars in the Sloan Digital Sky Survey. I. Discovery of Three New Quasars and the Spatial Density of Luminous Quasars at z ∼ 6 , 2001, astro-ph/0108063.

[11]  W. Brandt,et al.  The Chandra Deep Field North Survey. VI. The Nature of the Optically Faint X-Ray Source Population , 2001, astro-ph/0107450.

[12]  E. al.,et al.  Composite Quasar Spectra from the Sloan Digital Sky Survey , 2001, astro-ph/0105231.

[13]  A. Szalay,et al.  High-Redshift Quasars Found in Sloan Digital Sky Survey Commissioning Data. IV. Luminosity Function from the Fall Equatorial Stripe Sample , 2001 .

[14]  Scott M. Croom,et al.  The 2dF QSO Redshift Survey — I. The optical luminosity function of quasi-stellar objects , 2000 .

[15]  H. Spinrad,et al.  Discovery of a Color-selected Quasar at z = 5.50 , 2000, The Astrophysical journal.

[16]  Z. Haiman,et al.  X-Ray Emission from the First Quasars , 1999, astro-ph/9904340.

[17]  R. Nichol,et al.  High-Redshift Quasars Found in Sloan Digital Sky Survey Commissioning Data , 1999, astro-ph/0103228.

[18]  Martin J. Rees,et al.  Radiative Transfer in a Clumpy Universe. III. The Nature of Cosmological Ionizing Sources , 1998, astro-ph/9809058.

[19]  M. Rees,et al.  High-redshift galaxies, their active nuclei and central black holes , 1997, astro-ph/9712259.

[20]  Z. Haiman,et al.  Observational Signatures of the First Quasars , 1997, astro-ph/9710208.

[21]  P. Hewett,et al.  The Soft X-Ray Properties of a Large Optical QSO Sample: ROSAT Observations of the Large Bright Quasar Survey , 1995 .

[22]  Y. Pei The Luminosity Function of Quasars , 1995 .