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The bright radio source, GLEAM J091734
$-$001243 (hereafter GLEAM J0917
$-$0012), was previously selected as a candidate ultra-high redshift (
$z \gt 5$) radio galaxy due to its compact radio size and faint magnitude (
$K(\mathrm{AB})=22.7$). Its redshift was not conclusively determined from follow-up millimetre and near-infrared spectroscopy. Here we present new HST WFC3 G141 grism observations which reveal several emission lines including [NeIII]
$\lambda$3867, [NeV]
$\lambda$3426 and an extended (
$\approx 4.8\,$kpc), [OII]
$\lambda$3727 line which confirm a redshift of 
$3.004\pm0.001$. The extended component of the [OII]
$\lambda$3727 line is co-spatial with one of two components seen at 2.276 GHz in high resolution (
$60\times 20\,$mas) Long Baseline Array data, reminiscent of the alignments seen in local compact radio galaxies. The BEAGLE stellar mass (
$\approx 2\times 10^{11}\,\textit{M}_\odot$) and radio luminosity (
$L_{\mathrm{500MHz}}\approx 10^{28}\,$W Hz
$^{-1}$) put GLEAM J0917
$-$0012 within the distribution of the brightest high-redshift radio galaxies at similar redshifts. However, it is more compact than all of them. Modelling of the radio jet demonstrates that this is a young, 
$\approx 50\,$kyr old, but powerful, 
$\approx 10^{39}\,$W, compact steep spectrum radio source. The weak constraint on the active galactic nucleus bolometric luminosity from the [NeV]
$\lambda$3426 line combined with the modelled jet power tentatively implies a large black hole mass, 
$\ge 10^9\,\textit{M}_\odot$, and a low, advection-dominated accretion rate, i.e. an Eddington ratio 
$\le 0.03$. The [NeV]
$\lambda$3426/[NeIII]
$\lambda$3867 vs [OII]
$\lambda$3727/[NeIII]
$\lambda$3867 line ratios are most easily explained by radiative shock models with precursor photoionisation. Hence, we infer that the line emission is directly caused by the shocks from the jet and that this radio source is one of the youngest and most powerful known at cosmic noon. We speculate that the star-formation in GLEAM J0917
$-$0012 could be on its way to becoming quenched by the jet.
We present the second data release for the GaLactic and Extragalactic All-sky Murchison Widefield Array eXtended (GLEAM-X) survey. This data release is an area of 12 892-deg
$^2$ around the South Galactic Pole region covering 20 h40 m
$\leq$RA
$\leq$6 h40 m, -90
$^\circ$
$\leq$Dec
$\leq$+30
$^\circ$. Observations were taken in 2020 using the Phase-II configuration of the Murchison Widefield Array (MWA) and covering a frequency range of 72–231 MHz with twenty frequency bands. We produce a wideband source finding mosaic over 170–231 MHz with a median root-mean-squared noise of 
$1.5^{+1.5}_{-0.5}$ mJy beam
$^{-1}$. We present a catalogue of 624 866 components, including 562 302 components which are spectrally fit. This catalogue is 98% complete at 50 mJy, and a reliability of 98.7% at a 5 
$\sigma$ level, consistent with expectations for this survey. The catalogue is made available via Vizier, and the PASA datastore and accompanying mosaics for this data release are made available via AAO Data Central and SkyView.
