Fig. 7.

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Left: Resolved SFMS. Each circle point represents a pixel from Fig. 4 with a cutoff at radii greater than 55 kpc, color-coded as a function of distance to the galactic center. The black squares represent the uncertainty-weighted mean data points in the 0.25 dex M★ bins, the error bars show the scatter within the mass bin, and the thick solid gray line is the uncertainty-weighted (ODR) linear fit to the data. The shaded area traces the 1σ scatter around the linear fits. We included linear relations of resolved SFMS from the literature in dashed colored lines (Abdurro’uf et al. 2022 in red, Lin et al. 2019 in blue, Cano-Díaz et al. 2019 in yellow, and Ellison et al. 2021 in green). Center: Resolved Kennicutt-Schmidt relation. The gray line represents the ODR linear fit of the data points above the 4σ detection threshold. The dashed black line indicates the fit to the PHANGS sample across all morphological masks from Querejeta et al. (2021). Right: Resolved MGMS. The legend is similar to the middle panel.
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