I. HeywoodY. ContrerasD. J. B. SmithA. CoorayL. DunneL. GómezIbar, EduardoEduardoIbarR. J. IvisonM. J. JarvisM. J. MichałowskiD. A. RiechersP. van der Werf2025-12-072025-12-072016-10-2710.1093/mnras/stw27742-s2.0-85021362140https://cris-uv-2.scimago.es/handle/123456789/7551WOS:000393785500004Observations using the 7-mm receiver system on the Australia Telescope Compact Array have revealed large reservoirs of molecular gas in two high-redshift radio galaxies: HATLAS J090426.9+015448 (<it>z</it> = 2.37) and HATLAS J140930.4+003803 (<it>z</it> = 2.04). Optically, the targets are very faint, and spectroscopy classifies them as narrow-line radio galaxies. In addition to harbouring an active galactic nucleus the targets share many characteristics of sub-mm galaxies. Far-infrared data from <it>Herschel</it>-Astrophysical Terahertz Large Area Survey suggest high levels of dust (>109 M<inf>⊙</inf>) and a correspondingly large amount of obscured star formation (∼1000 M<inf>⊙</inf> yr−1). The molecular gas is traced via the <it>J</it> = 1 → 0 transition of 12CO, its luminosity implying total H<inf>2</inf> masses of (1.7 ± 0.3) × 1011 and (9.5 ± 2.4) × 1010 (α<inf>CO</inf>/0.8) M<inf>⊙</inf> in HATLAS J090426.9+015448 and HATLAS J140930.4+003803, respectively. Both galaxies exhibit molecular line emission over a broad (∼1000 km s−1) velocity range and feature double-peaked profiles. We interpret this as evidence of either a large rotating disc or an on-going merger. Gas depletion time-scales are ∼100 Myr. The 1.4-GHz radio luminosities of our targets place them close to the break in the luminosity function. As such they represent ‘typical’ <it>z</it> > 2 radio sources, responsible for the bulk of the energy emitted at radio wavelengths from accretion-powered sources at high redshift, and yet they rank amongst the most massive systems in terms of molecular gas and dust content. We also detect 115-GHz rest-frame continuum emission, indicating a very steep high-radio-frequency spectrum, possibly classifying the targets as compact steep spectrum objects.enacceso abiertoAstronomy And AstrophysicsSpace And Planetary Sciencearticle