Table 3: Dust components derived from SED fitting of NGC 4013, NGC 5907 and NGC 4565 in the FIR/submm/mm regime. We decompose the spectrum into 2 components; warm dust of temperature $T^{\rm W}$ and cold dust of temperature $T^{\rm C}$ . The ratio of cold dust mass to warm dust mass is given as $\frac{M^{\rm C}}{M^{\rm W}}$ . An index of 1.5 has been assumed for the wavelength dependency of the emissivity ( $Q\propto \lambda ^{-1.5}$ ).
Galaxy $T^{\rm W}$ $T^{\rm C}$ $\frac{M^{\rm C}}{M^{\rm W}}$

(K) (K)

NGC 4013 39 23 49

NGC 4565 43 20 99

NGC 5907 28 13 5.7

**Table 3:** Dust components derived from SED fitting of NGC 4013, NGC 5907 and NGC 4565 in the FIR/submm/mm regime. We decompose the spectrum into 2 components; warm dust of temperature $T^{\rm W}$ and cold dust of temperature $T^{\rm C}$ . The ratio of cold dust mass to warm dust mass is given as $\frac{M^{\rm C}}{M^{\rm W}}$ . An index of 1.5 has been assumed for the wavelength dependency of the emissivity ( $Q\propto \lambda ^{-1.5}$ ).
Galaxy	$T^{\rm W}$	$T^{\rm C}$	$\frac{M^{\rm C}}{M^{\rm W}}$
	(K)	(K)
NGC 4013	39	23	49
NGC 4565	43	20	99
NGC 5907	28	13	5.7

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