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Table 5:

Parameters of our SED models using or not submm constraints and Dust-to-Gas mass ratios of our galaxies.
  Haro 11 Mrk 1089 NGC 1705
  no submm submm no submm submm no submm submm
$M_{\rm dust}$($M_\odot $) 6.2 $\times$ 106 1.7 $\times$ 107 ($\pm$40$\%$) 3 $\times$ 107 5.12 $\times$ 107 ($\pm$20$\%$) a 2.9 $\times$ 104 1.3 $\times$ 106 ($\pm$50$\%$)
$f_{\rm PAH}$ 0.22 0.1 0.18 0.18 0.11 4.4 $\times$ 10-2
$\alpha $ 1.88 1.73 2.21 2.18 2.5 1.84
$U_{\rm min}$ 12.2 1.44 1.5 0.82 3.68 9 $\times$ 10-3
$U_{\rm max}$ 1.3 $\times$ 105 5.77 $\times$ 104 3.84 $\times$ 105 3.5 $\times$ 105 1.47 $\times$ 104 8.67 $\times$ 102
             
$M_{\rm HI}$($M_\odot $) $\sim $108 2.7 $\times$ 1010 4.1 $\times$ 107 b
$M_{\rm dust}$/ $M_{\rm HI}$ 6 $\times$ 10-2 0.17 10-3 1.9 $\times$ 10-3 7 $\times$ 10-4 3.2 $\times$ 10-2
a Bold numbers are the dust mass and the dust-to-gas mass ratio values of our prefered SED for the galaxy Mrk 1089.
b HI mass associated with the aperture chosen for the dust mass determination, namely 80% of the the total HI mass.

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