The nature and likely redshift of GLEAM J0917โ0012
The nature and likely redshift of GLEAM J0917โ0012
Abstract We previously reported a putative detection of a radio galaxy at $z=10.15$ , selected from the GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey. The redshift of this source, GLEAM J0917โ0012, was based on three weakly detected molecular emission lines observed with the Atacama Large Millimetre Array (ALMA). โฆ