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Fig. 1.

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rSFMS (bottom left) and rMGMS (bottom right) measured at 150 pc resolution for all galaxies in our sample. For reference and to guide the eye, the various solid colored lines represent the binned trends (bins of 0.15 dex) obtained for each environment, accounting for nondetections as detailed in Pessa et al. (2021). The black solid line shows the same measurement for all environments simultaneously. The dashed lines show the binned trends obtained when nondetections are neglected from the analysis. The panels on the top row show the detection fraction of ΣSFR (left) and Σmol (right), defined as the fraction of pixels with a measurement above our detection threshold in each bin of Σ. The horizontal dotted line marks the detection fraction level of 60%.

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