Non-standard grain properties, dark gas reservoir, and extended submillimeter excess, probed by Herschel in the Large Magellanic Cloud

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Table A.1

Submillimeter properties of our dust compositions.

	“Standard model”	“AC model”

β	2	1.7
κ_abs(160 μm)	1.4m² kg^-1	1.6m² kg^-1

Notes. The two parameters β and κ_abs(160 μm) are the parameters to approximate our dust opacities (Fig. A.1) with Eq. (A.1).

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