SFRs derived from IR luminosity (8–1000 μm; with the calibration of Kennicutt 1998) vs. those derived from [C ii] (blue), [O i] (red; with the calibration of De Looze et al. 2014), and Hα (green, higher values include dust correction as derived by Christensen et al. 2008) lines. Circles denote PACS spaxels, and squares denote the entire host. The IR estimates are from Michałowski et al. (2014b). The Hα estimate for the WR region is from Christensen et al. (2008), and for the entire host from Sollerman et al. (2005). Dotted lines show the locations at which the SFR_line is higher than the SFR_IR by the indicated factors. The SFRs derived from line ([C ii], [O i], Hα) indicators are higher than those from continuum (UV, IR, radio) indicators.