A nearby galaxy perspective on dust evolution - Scaling relations and constraints on the dust build-up in galaxies with the DustPedia and DGS samples

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Table 3.

Robustness assessment.

Run	Median	68% interval	95% interval	Number of sources
Least-squares	0.86	0.128–1.50	2.83×10⁻⁶–7.0	783
Non-hierarchical Bayesian	0.92	0.0223–1.22	0.000164–3.7	798
No Planck and IRAS data	1.19	1.00–1.60	0.69–2.44	783
Galliano et al. (2011) AC mixture	0.91	0.69–0.97	0.51–1.15	798
Galliano et al. (2011) AC mixture	0.60	0.48–0.68	0.37–0.80	798
MBB with β = 1.79	0.85	0.61–1.08	0.35–1.39	798
MBB with β free	1.00	0.43–2.75	0.183–5.3	798
Draine & Li (2007) ISRF distribution	0.71	0.49–1.31	0.186–4.6	798
CIGALE	0.70	0.50–1.06	0.227–3.6	756

Notes. Statistics of the comparison between the reference run and the various tests of Figs. 4–6. The median, 68% and 95% intervals refer to the distribution of the quantity in the first column. See Sect. 3.3 for more details.

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