The discovery of a highly accreting, radio-loud quasar at z=6.82

TL;DR

This paper reports the discovery of a highly accreting, radio-loud quasar at redshift 6.82, providing insights into early massive galaxy and black hole formation during the epoch of reionization.

Contribution

It presents the first detailed characterization of a z=6.82 radio-loud quasar, including its black hole mass, accretion rate, and radio properties, expanding knowledge of high-redshift radio-loud AGN.

Findings

Quasar at z=6.82 with super-Eddington accretion

Largest ionized region measured at this redshift

Evidence of a second steep-spectrum radio source nearby

Abstract

Radio sources at the highest redshifts can provide unique information on the first massive galaxies and black holes, the densest primordial environments, and the epoch of reionization. The number of astronomical objects identified at z>6 has increased dramatically over the last few years, but previously only three radio-loud (R2500>10) sources had been reported at z>6, with the most distant being a quasar at z=6.18. Here we present the discovery and characterization of P172+18, a radio-loud quasar at z=6.823. This source has an MgII-based black hole mass of ~3x10^8 Msun and is one of the fastest accreting quasars, consistent with super-Eddington accretion. The ionized region around the quasar is among the largest measured at these redshifts, implying an active phase longer than the average lifetime of the z>6 quasar population. From archival data, there is evidence that its 1.4 GHz emission has decreased by a factor of two over the last two decades. The quasar's radio spectrum between 1.4 and 3.0 GHz is steep (alpha=-1.31) and has a radio-loudness parameter R2500~90. A second steep radio source (alpha=-0.83) of comparable brightness to the quasar is only 23.1" away (~120 kpc at z=6.82; projection probability <2%), but shows no optical or near-infrared counterpart. Further follow-up is required to establish whether these two sources are physically associated.