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Fig. 11

Fig. 11 Refer to the following caption and surrounding text.

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(a) Resolved SFMS kernel-density estimate (KDE): dust-corrected Hα-based ΣSFR versus Σ for Voronoi bins. Solid and dashed lines show the best-fit resolved SFMS and ±1σ envelope from Cano-Díaz et al. (2016). (b) Integrated SFMS for the whole galaxy, main body, and northern clump compared to the local SFMS (Cano-Díaz et al. 2016). Filled circles: Hα-based SFRs (Appendix B); open circles: FUV-based SFRs (Appendix C.1). Triangles show the pPXF-inferred mean SFR in the youngest SFH bin (30 Myr template, which integrates over the past ~40 Myr).

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