Very High Redshift X-ray Selected Agn in the Chandra Deep Field-north

نویسندگان

  • A. J. Barger
  • F. E. Bauer
  • W. N. Brandt
  • G. P. Garmire
  • A. E. Hornschemeier
چکیده

Deep Chandra X-ray exposures provide an efficient route for locating optically faint active galactic nuclei (AGN) at high redshifts. We use deep multicolor optical data to search for z > 5 AGN 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 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 2σ level and could lie at z > 5. There are too few moderate luminosity AGN at z = 5− 6.5 to ionize the intergalactic medium. Subject headings: cosmology: observations — galaxies: active — galaxies: evolution — galaxies: formation — galaxies: distances and redshifts

برای دانلود رایگان متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

The Compton-thick AGN in the CDFN

We present X-ray spectral analysis of the brightest sources (f2−10 keV > 10 −15 erg cm s ) in the Chandra Deep Field North. Our sample consists of 222 sources; for the vast majority (171) either a spectroscopic or a photometric redshift is available. Our goal is to discover the Compton-thick AGN in a direct way i.e. through their X-ray spectra. Compton-thick AGN give away their presence in X-ra...

متن کامل

24 μ m properties of X - ray selected AGN

We examine the 24 μm to X-ray color of 157 X-ray–selected AGN as a function of X-ray obscuration and optical classification in the Chandra Deep Field South. The sample consists of the Chandra hard–band detections with 2–8 keV flux > 10 erg s cm. A deep 24 μm mosaic obtained with Spitzer provides mid–infrared fluxes for the sample. Since obscured AGN locally have higher 24 μm/2–8 keV ratios than...

متن کامل

The Chandra Deep Field - North Survey . Xvi

We present X-ray spectral analyses of the three z > 4 Active Galactic Nuclei (AGNs) thus far spectroscopically identified in the Chandra Deep Field-North Survey, at redshifts of 5.186, 4.424, and 4.137. These analyses are made possible by the extremely deep exposure (≈ 2 Ms) and the low Chandra background. The rest-frame ≈ 2.5–40 keV spectra are the first for optically faint (two of the three s...

متن کامل

Unveiling Obscured Accretion in the Chandra Deep Field South

We make use of deep HST, VLT, Spitzer and Chandra data on the Chandra Deep Field South to constrain the number of Compton thick AGN in this field. We show that sources with high 24μm to optical flux ratios and red colors form a distinct source population, and that their infrared luminosity is dominated by AGN emission. Analysis of the X-ray properties of these extreme sources shows that most of...

متن کامل

The X-ray Background and the Deep X-ray Surveys

The deep X-ray surveys performed by the two major X-ray observatories on flight, Chandra and XMM, are being resolving the bulk of the cosmic X-ray background (XRB) in the 2–10 keV energy band, where the sky flux is dominated by extragalactic emission. Although the actual fraction depends on the absolute sky flux, which is measured with an uncertainty of ∼ 40%, most of the XRB is already resolve...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2003