2021MNRAS.508L..58B

We report ALMA Band 9 continuum observations of the normal, dusty star-forming galaxy A1689-zD1 at z = 7.13, resulting in a ∼4.6 σ detection at 702 GHz. For the first time, these observations probe the far-infrared spectrum shortward of the emission peak of a galaxy in the Epoch of Reionization (EoR). Together with ancillary data from earlier works, we derive the dust temperature, T_d, and mass, M_d, of A1689-zD1 using both traditional modified blackbody spectral energy density fitting, and a new method that relies only on the [C II] 158 µm line and underlying continuum data. The two methods give T_d = (42⁺¹³_–7, 40⁺¹³_–7) K, and M_d = (1.7^+1.3_–0.7, 2.0^+1.8_–1.0) ×10⁷ M_☉. Band 9 observations improve the accuracy of the dust temperature (mass) estimate by ∼50 per cent (6 times). The derived temperatures confirm the reported increasing T_d-redshift trend between z = 0 and 8; the dust mass is consistent with a supernova origin. Although A1689-zD1 is a normal UV-selected galaxy, our results, implying that ∼85 per cent of its star-formation rate is obscured, underline the non-negligible effects of dust in EoR galaxies.