Spatially resolved stellar populations and emission line properties in nearby galaxies with J-PLUS - I. Method and first results for the M101 group

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Fig. A.4.

Left: Maps of the effective V-band dust optical depth ( $\tilde{τ}$ $\tilde{\tau}$ ). The central and right panels show RGB composites with the i, r, and g bands before and after correction for dust, respectively.

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