Cookies

We use cookies to ensure that we give you the best experience on our website. By continuing to browse this repository, you give consent for essential cookies to be used. You can read more about our Privacy and Cookie Policy.


Durham Research Online
You are in:

The 4 Ms Chandra Deep Field-South number counts apportioned by source class : pervasive active galactic nuclei and the ascent of normal galaxies.

Lehmer, B.D. and Xue, Y.Q. and Brandt, W.N. and Alexander, D.M. and Bauer, F.E. and Brusa, M. and Comastri, A. and Gilli, R. and Hornschemeier, A.E. and Luo, B. and Paolillo, M. and Ptak, A. and Shemmer, O. and Schneider, D.P. and Tozzi, P. and Vignali, C. (2012) 'The 4 Ms Chandra Deep Field-South number counts apportioned by source class : pervasive active galactic nuclei and the ascent of normal galaxies.', Astrophysical journal., 752 (1). p. 46.

Abstract

We present 0.5-2 keV, 2-8 keV, 4-8 keV, and 0.5-8 keV (hereafter soft, hard, ultra-hard, and full bands, respectively) cumulative and differential number-count (log N-log S) measurements for the recently completed ≈4 Ms Chandra Deep Field-South (CDF-S) survey, the deepest X-ray survey to date. We implement a new Bayesian approach, which allows reliable calculation of number counts down to flux limits that are factors of ≈1.9-4.3 times fainter than the previously deepest number-count investigations. In the soft band (SB), the most sensitive bandpass in our analysis, the ≈4 Ms CDF-S reaches a maximum source density of ≈27,800 deg-2. By virtue of the exquisite X-ray and multiwavelength data available in the CDF-S, we are able to measure the number counts from a variety of source populations (active galactic nuclei (AGNs), normal galaxies, and Galactic stars) and subpopulations (as a function of redshift, AGN absorption, luminosity, and galaxy morphology) and test models that describe their evolution. We find that AGNs still dominate the X-ray number counts down to the faintest flux levels for all bands and reach a limiting SB source density of ≈14,900 deg-2, the highest reliable AGN source density measured at any wavelength. We find that the normal-galaxy counts rise rapidly near the flux limits and, at the limiting SB flux, reach source densities of ≈12,700 deg-2 and make up 46% ± 5% of the total number counts. The rapid rise of the galaxy counts toward faint fluxes, as well as significant normal-galaxy contributions to the overall number counts, indicates that normal galaxies will overtake AGNs just below the ≈4 Ms SB flux limit and will provide a numerically significant new X-ray source population in future surveys that reach below the ≈4 Ms sensitivity limit. We show that a future ≈10 Ms CDF-S would allow for a significant increase in X-ray-detected sources, with many of the new sources being cosmologically distant (z >~ 0.6) normal galaxies.

Item Type:Article
Keywords:Cosmology, Observations, Galaxies, Active, Starburst, X-rays.
Full text:(VoR) Version of Record
Download PDF
(2461Kb)
Status:Peer-reviewed
Publisher Web site:http://dx.doi.org/10.1088/0004-637X/752/1/46
Publisher statement:© 2012. The American Astronomical Society. All rights reserved. Printed in the U.S.A.
Date accepted:No date available
Date deposited:23 December 2013
Date of first online publication:2012
Date first made open access:No date available

Save or Share this output

Export:
Export
Look up in GoogleScholar