Linking dust emission to fundamental properties in galaxies: the low-metallicity picture

Free Access

Issue		A&A Volume 582, October 2015


Article Number		A121
Number of page(s)		42
Section		Extragalactic astronomy
DOI		https://doi.org/10.1051/0004-6361/201526067
Published online		22 October 2015

Online material

Fig. 12

DGS SEDs: the observed SEDs include the Herschel data (purple crosses) as well as any available ancillary data (in orange). The different symbols refer to the different instruments: Xs for 2MASS bands, stars for Spitzer IRAC and MIPS, diamonds for WISE, and triangles for IRAS. The IRS spectrum is shown in orange. The total modelled SED in black is the sum of the stellar (green) and dust (red) contributions, and eventually of the modified black-body contribution (yellow). The modelled points in the different bands are the filled blue circles.

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	Fig. 12 continued.
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	Fig. 12 continued.
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	Fig. 13 KINGFISH SEDs: the colours and symbols are the same as in Fig. 12.
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	Fig. 13 continued.
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	Fig. 13 continued.
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Table 4

DGS and KINGFISH stellar mass and star-formation parameters.

Table 5

Updated Herschel flux densities for the DGS sample.

Table 6

Spitzer IRAC flux densities for the DGS sample.

Table 7

WISE flux densities for the DGS sample.

Table 8

2MASS and IRAS flux densities from the literature for the DGS sample.

Table 9

DGS and KINGFISH dust parameters.

© ESO, 2015

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