Dust spectral energy distributions of nearby galaxies: an insight from the Herschel Reference Survey

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Volume 565 (May 2014)

A&A, 565 (2014) A128

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Table 3

Statistics from the relations of the mock catalogs (Fig. 1).

Parameter	Bands	Linear fit: A + Bx		Spearman coef.	Stat of X_est/X_true

		A	B	ρ	median	σ

U_min	all	0.03	1.07	0.94	1.07	0.20
	no 8 μm	0.03	1.07	0.94	1.06	0.20
	no 22−24 μm	0.08	0.81	0.91	0.86	0.19
	no 60−70 μm	0.07	1.18	0.92	1.18	0.30
	no SPIRE	0.21	1.15	0.87	1.24	0.34

γ	all	0.00	1.25	0.94	1.18	1.36
	no 8 μm	0.00	1.17	0.94	1.19	1.43
	no 22−24 μm	0.02	1.25	0.74	3.77	6.43
	no 60−70 μm	0.00	1.14	0.94	1.23	1.36
	no SPIRE	0.00	1.10	0.93	1.17	1.33

q_PAH	all	0.74	0.71	0.92	0.89	0.11
	no 8 μm	1.00	0.61	0.88	0.85	0.20
	no 22−24 μm	0.88	0.55	0.79	0.77	0.15
	no 60−70 μm	1.01	0.63	0.89	0.89	0.17
	no SPIRE	0.84	0.69	0.92	0.89	0.14

log L_IR	all	0.00	1.00	1.00	1.00	0.00
	no 8 μm	0.01	1.00	1.00	1.00	0.00
	no 22−24 μm	−0.03	1.00	1.00	1.00	0.00
	no 60−70 μm	−0.09	1.01	1.00	1.00	0.00
	no SPIRE	−0.02	1.00	1.00	1.00	0.00

log M_dust	all	−0.03	1.00	0.99	0.99	0.01
	no 8 μm	−0.04	1.00	0.99	0.99	0.01
	no 22−24 μm	−0.05	1.01	1.01	1.00	0.01
	no 60−70 μm	0.06	0.98	0.98	0.99	0.01
	no SPIRE	−0.14	1.01	1.01	0.99	0.02

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