Extended Data Fig. 2: SEDs of the cold dust emission of FRB 20201124A.
From: A nebular origin for the persistent radio emission of fast radio bursts
Estimated values are based on the NOEMA upper limits at 236 GHz and 250 GHz (cyan squares). a, SED computed in one beam towards the FRB position as seen in the VLA 15-GHz map. The best-fitting curves with fixed [Tdust (K), β] = [20, 1.5], [20, 2.0], [30, 1.5], [30, 2.0] are plotted as solid violet, dashed violet, solid blue and dashed blue lines, respectively. b, SED of the cold dust emission of FRB 20201124A based on the NOEMA upper limits at 236 GHz and 250 GHz (cyan squares) computed for the region >3σ in the 6-GHz map. The best-fitting curves with fixed [Tdust (K), β] = [20, 1.5], [20, 2.0], [30, 1.5], [30, 2.0] are plotted as solid violet, dashed violet, solid blue and dashed blue lines, respectively.
