Fig. 4
Observed FIR/(sub)mm SEDs showing pre-burst Herschel/ AKARI data (blue) and FIFI-LS burst values (red) together with the corresponding (sub)mm fluxes from Brogan et al. (2019). The upper 24 μm MIPS limit is indicated as well. The solid lines represent the reddened graybody fits (cf. Sect. 4.1). The second epoch FIFI-LS data and the corresponding fit appear bf in green.
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