All Tables

Table 1: The various contributions to the uncertainties on the net flux of the SCUBA maps integrated in a 120'' diameter aperture centered at $\alpha (2000) = 4^{\rm h}30^{\rm m}49^{\rm s}$ , $\delta (2000) = 64^\circ 50'55''$ .
Table 2: Net fluxes for the dust emission by the entire galaxy used for the modeling. The values take account of all the corrections mentioned in the text. ^a Madden et al. (2003), ^b Hunter et al. (1989a), ^c Hunter et al. (1989b), ^d Stickel et al. (2000) & full catalog in prep., ^e this paper, ^f Lisenfeld et al. (2002).
Table 3: Fluxes for the entire galaxy used to model the global ISRF. The values are corrected for Galactic extinction. ^a Israel (1988), ^b De Vaucouleurs et al. (1991).
Table 4: The values are those for the best fit. For comparison, we give the corresponding values for the Galaxy from Désert et al. (1990).
Table 5: Range of reliability of the physical parameters of the grains (from errors in the fitting and variations in the assumed geometry).
Table 6: Temperatures of the grains (other than VCGs). We give the minimum ( $T_{\rm min}$ ) and maximum ( $T_{\rm max}$ ) temperatures for the minimum and maximum sizes, component by component. All the grains are stochastically heated except the largest BGs where $T_{\rm min} = T_{\rm max} = T_{\rm equilibrium}$ .
Table 7: Dust masses, gas-to-dust and dust-to-metal mass ratios in NGC 1569 deduced from the parameters in Table 4. The entries corresponding to non-relevant quantities are blank for more clarity.