The systematic search for z ≳ 5 active galactic nuclei in the Chandra Deep Field South

We investigate early black hole (BH) growth through the methodical search for z ≳ 5 active galactic nuclei (AGN) in the Chandra Deep Field South. We base our search on the Chandra 4-Ms data with flux limits of 9.1x10^-18 (soft, 0.5-2 keV) and 5.5x10^-17 erg s^-1 cm^-2 (hard, 2-8 keV). At z ~ 5, this corresponds to luminosities as low as ~10⁴² (~10⁴³) ergs^-1 in the soft (hard) band and should allow us to detect Compton-thin AGN with MBH > 10⁷M{bull's eye} and Eddington ratios >0.1. Our field (0.03 deg²) contains over 600z ~ 5 Lyman Break Galaxies. Based on lower redshift relations, wewould expect ~ 20 of them to hostAGN. After combining the Chandra data with Great Observatories Origins Deep Survey (GOODS)/Advanced Camera for Surveys (ACS), CANDELS/Wide Field Camera 3 and Spitzer/Infrared Array Camera data, the sample consists of 58 high-redshift candidates. We run a photometric redshift code, stack the GOODS/ACS data, apply colour criteria and the Lyman Break Technique and use the X-ray Hardness Ratio. We combine our tests and using additional data find that all sources are most likely at low redshift. We also find five X-ray sources without a counterpart in the optical or infrared which might be spurious detections. We conclude that our field does not contain any convincing z ≳5 AGN. Explanations for this result include a low BH occupation fraction, a low AGN fraction, short, super-Eddington growth modes, BH growth through BH- BH mergers or in optically faint galaxies. By searching for z ≳5 AGN, we are setting the foundation for constraining early BH growth and seed formation scenarios.