Issue |
A&A
Volume 563, March 2014
|
|
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Article Number | A31 | |
Number of page(s) | 22 | |
Section | Extragalactic astronomy | |
DOI | https://doi.org/10.1051/0004-6361/201322803 | |
Published online | 28 February 2014 |
Online material
Appendix A: Data tables
Gas masses for the DGS, KINGFISH and G11 samples.
Dust masses for the KINGFISH and G11 samples.
Appendix B: G/D with morphological type, stellar mass and star formation rate
In this appendix, we present how the sample distributes in morphological types, stellar masses and star formation rates (Fig. B.2). The morphological types were taken from NED. The stellar masses were obtained from the formula of Eskew et al. (2012) using the 3.6 and 4.5 μm IRAC flux densities. Whenever IRAC data was not available, we compute synthetic IRAC photometry from the SEDs. The SFR were converted from TIR luminosities using the Kennicutt (1998) formula. We also present the G/D as a function of these three parameters (Fig. B.3) and as a function of the specific star formation rate (SSFR, Fig. B.1). SSFR is defined as the star formation rate divided by the stellar mass: SFR/M∗.
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Fig. B.1
G/D as a function of SSFR for the 2 values of XCO: XCO,MW (top) and XCO,Z (bottom). The colours code for the metallicity of the galaxies and the symbols differentiate between the three samples: DGS (crosses), KINGFISH (downward triangles) and G11 (stars). |
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Fig. B.2
Morphological type distributions (top), stellar mass distributions (centre), and star formation rate distributions (bottom) of the DGS (purple), KINGFISH (orange) and G11 (green) samples. In each panel, the total distribution is indicated in grey. |
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Fig. B.3
G/D as a function of morphological type (top row), stellar mass (centre row) and star formation rate (bottom row) for the 2 values of XCO: XCO,MW (left column) and XCO,Z (right column). The colours code for the metallicity of the galaxies and the symbols differentiate between the three samples: DGS (crosses), KINGFISH (downward triangles) and G11 (stars). |
Open with DEXTER |
© ESO, 2014
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