Fig. 3
Long wavelength emission of dust in the DHGL medium. Grey symbols and curves indicate the observed emission spectrum (see Sect. 4.1) for NH = 1020 H cm-2. The spectrum is a FIRAS (COBE satellite) measurment. Squares and diamonds are the photometric measurments from DIRBE (COBE) and WMAP, respectively. Black lines are the model output and black squares the modeled DIRBE points taking into account instrumental transmission and color corrections.
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