Exploring Gravitationally Lensed z ≳ 6 X-Ray Active Galactic Nuclei Behind the RELICS Clusters

• Published in: The Astrophysical journal Vol. 927; no. 1; pp. 34 - 46
• Main Authors: Bogdán, Ákos, Kovács, Orsolya E., Jones, Christine, Forman, William R., Kraft, Ralph P., Strait, Victoria, Coe, Dan, Bradač, Maruša
• Format: Journal Article
• Language: English
• Published: Philadelphia The American Astronomical Society 01.03.2022; IOP Publishing
• Subjects: Active galactic nuclei; Astrophysics; Black holes; Deposition; Emission analysis; Emissions control; Galactic clusters; Galaxies; Galaxy clusters; Gravitational lenses; Gravitational lensing; High-redshift galaxies; Ionization; Luminosity; Polls & surveys; Quasars; Red shift; Space telescopes; Star & galaxy formation; Star formation; Star formation rate; Stars & galaxies; Statistical methods; Stellar mass; Supermassive black holes; Telescopes; X ray sources; X ray telescopes; X-ray active galactic nuclei; X-ray astronomy; X-ray emissions; X-rays
• ISSN: 0004-637X; 1538-4357
• DOI: 10.3847/1538-4357/ac4ae5

Although observations of high-redshift quasars demonstrate that many supermassive black holes (BHs) reached large masses within one billion years after the Big Bang, the origin of the first BHs is still a mystery. A promising way to constrain the origin of the first BHs is to explore the average properties of z ≳ 6 BHs. However, typical BHs remain hidden from X-ray surveys, which is due to their relatively faint nature and the limited sensitivity of X-ray telescopes. Gravitational lensing provides an attractive way to study this unique galaxy population as it magnifies the faint light from these high-redshift galaxies. Here, we study the X-ray emission originating from 155 gravitationally lensed z ≳ 6 galaxies that were detected in the Reionization Lensing Cluster Survey. We utilize Chandra X-ray observations to search for active galactic nuclei (AGNs) in the individual galaxies and in the stacked galaxy samples. We did not identify an individual X-ray source that was undoubtedly associated with a high-redshift galaxy. We stack the signal from all galaxies and do not find a statistically significant detection. We split our sample based on stellar mass, star formation rate, and lensing magnification and stack these subsamples. We obtain a 2.2 σ detection for massive galaxies with an X-ray luminosity of (3.7 ± 1.6) × 10 42 erg s −1 , which corresponds to a (3.0 ± 1.3) × 10 5 M ⊙ BH accreting at its Eddington rate. Other stacks remain undetected and we place upper limits on the AGN emission. These limits imply that the bulk of BHs at z ≳ 6 either accrete at a few percent of their Eddington rate and/or are 1–2 orders of magnitude less massive than expected based on the stellar mass of their host galaxy.