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Fig. 5


Comparison of the dust masses obtained in this paper and those derived by Tabatabaei et al. (2014) with two MBBs. Each point corresponds to one pixel on the sky. Only independent data points have been considered to compare both masses (see text for details). The mean value and standard deviation of the ratio between the dust mass derived from Tabatabaei et al. (2014) and from this study is 1.7 (dashed line) and 0.7, respectively. The relative uncertainties for the dust masses derived in this paper are ~25%.

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