2022MNRAS.512.4248E

We report the identification of radio (0.144-3 GHz) and mid-, far-infrared, and sub-mm (24-850µm) emission at the position of one of 41 UV-bright (M_UV ≲-21.25) z ≃ 6.6-6.9 Lyman-break galaxy candidates in the 1.5 deg² COSMOS field. This source, COS-87259, exhibits a sharp flux discontinuity (factor >3) between two narrow/intermediate bands at 9450 and 9700 Å and is undetected in all nine bands blueward of 9600 Å, as expected from a Lyman alpha break at z ≃ 6.8. The full multiwavelength (X-ray through radio) data of COS-87529 can be self-consistently explained by a very massive (M_* = 10^10.8 M_☉) and extremely red (rest-UV slope β = -0.59) z ≃ 6.8 galaxy with hyperluminous infrared emission (L_IR = 10^13.6 L_☉) powered by both an intense burst of highly obscured star formation (SFR ≃ 1800 M_☉ yr^–1) and an obscured (τ_9.7µm_ = 7.7±2.5) radio-loud (L_1.4 GHz_ ≃ 10^25.4 W Hz^–1) active galactic nucleus (AGN). The radio emission is compact (1.04 ± 0.12 arcsec) and exhibits an ultra-steep spectrum between 1.32 and 3 GHz (α=-1.57^+0.22_–0.21) that flattens at lower frequencies (α= -0.86^+0.22_–0.16 between 0.144 and 1.32 GHz), consistent with known z > 4 radio galaxies. We also demonstrate that COS-87259 may reside in a significant (11x) galaxy overdensity, as common for systems hosting radio-loud AGN. While we find that low-redshift solutions to the optical + near-infrared data are not preferred, a spectroscopic redshift will ultimately be required to establish the true nature of COS-87259 beyond any doubt. If confirmed to lie at z ≃ 6.8, the properties of COS-87259 would be consistent with a picture wherein AGN and highly obscured star formation activity are fairly common among very massive (M_* > 10¹⁰ M_☉) reionization-era galaxies.