High-resolution, 3D radiative transfer modelling - III. The DustPedia barred galaxies

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Table C.1.

Relations between sSFR and f_young.

Galaxy ID	y = ax + b		Spearman’s coef.	Equation (4)
	a	b	ρ	a	c
NGC 1365	0.16	1.48	0.75	−0.92	−9.74
M 77	0.12	1.13	0.84	−0.80	−8.75
M 81	0.34	3.48	0.85	−0.72	−8.11
M 83	0.22	2.06	0.85	−0.96	−10.2
M 95	0.29	2.79	0.80	−1.21	−12.8
M 100	0.22	2.04	0.84	−0.83	−8.86

Notes. The relationship in Fig. C.1 is fitted with a power-law: y = ax + b; where y = log f_young, x = log[sSFR/yr⁻¹], a is the slope and b is the intercept of the best-fitting line, and ρ is the Spearman’s rank correlation coefficient. The relationship is also fitted with Eq. (4).

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