Top: relative spectral response (passband) for Planck’s HFI-353 GHz channel (solid line, Planck Collaboration 2013) and LABOCA (dashed line, Siringo et al. 2009). Bottom: colour corrections for the HFI-353 (solid line) and LABOCA (dashed line) as a function of the spectral index of the assumed source spectrum. The dotted line shows the conversion factor to scale the HFI-353 intensities to the nominal centre frequency of LABOCA.
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