Notes. (1) Galaxy Name. (2) Distance to object (references on distances are given in James et al. 2002; Draine et al. 2007; Galliano et al. 2008; and Galametz et al. 2009). (3) Metallicity of the galaxy. (4) 450 μm flux. (5) 850 μm flux (^a 870 μm fluxes estimated through LABOCA observations). (6) Hi mass of the galaxy. (7) H₂ mass of the galaxy. (8) Total dust mass estimated from our SED modelling performed with measures below 300 μm. (9) Total dust mass estimated from our SED modelling performed with submm data (^b A cold dust component of 10 K with an emissivity β = 1 is added to the model to account for the submm excess).

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