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Fig. 8

image

Spectral energy distribution of the BCG of Phoenix in the FIR from the PACS (100 and 160 μm) and SPIRE (250, 350, 500 μm) instruments onboard the Herschel Space Observatory. The red dotted line and the blue dashed line show the best fit to the SED for the AGN and starburst template, respectively.

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