A dusty compact object bridging galaxies and quasars at cosmic dawn
S. Fujimoto, G. B. Brammer, D. Watson, G. E. Magdis, V. Kokorev, T. R., Greve, S. Toft, F. Walter, R. Valiante, M. Ginolfi, R. Schneider, F., Valentino, L. Colina, M. Vestergaard, R. Marques-Chaves, J. P. U. Fynbo, M., Krips, C. L. Steinhardt, I. Cortzen, F. Rizzo

TL;DR
This paper reports the discovery of GNz7q, a dust-enshrouded, ultraviolet compact object at redshift 7.19, likely representing a transitional phase in early black hole and galaxy evolution, bridging dusty starbursts and luminous quasars.
Contribution
It provides the first observational evidence of a transitioning quasar at cosmic dawn, supporting simulation predictions of black hole growth stages in the early Universe.
Findings
GNz7q is a dust-enshrouded starburst with high star formation rate.
The object shows an ultraviolet compact source with faint X-ray emission.
Properties suggest it is a precursor to luminous quasars at later times.
Abstract
Understanding how super-massive black holes form and grow in the early Universe has become a major challenge since the discovery of luminous quasars only 700 million years after the Big Bang. Simulations indicate an evolutionary sequence of dust-reddened quasars emerging from heavily dust-obscured starbursts that then transition to unobscured luminous quasars by expelling gas and dust. Although the last phase has been identified out to a redshift of 7.6, a transitioning quasar has not been found at similar redshifts owing to their faintness at optical and near-infrared wavelengths. Here we report observations of an ultraviolet compact object, GNz7q, associated with a dust-enshrouded starburst at a redshift of z=7.1899+/-0.0005. The host galaxy is more luminous in dust emission than any other known object at this epoch, forming 1,600 solar masses of stars per year within a central radius…
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