Fig. 6.
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Spatially resolved conversion (W[CII]) factor as a function of the [CII] surface brightness (Σ[CII]) within ≈30 pc size pixels (colored points) in the ISM of SERRA galaxies. The color-code reflects the metallicity within each pixel. The best-fit relation (dispersion) from Eq. (10), for different metallicities, is plotted with dotted lines (shaded areas), using the same color-code. The inset shows the PDF of the log error between the W[CII] obtained pixel by pixel using the best-fit relation and the actual one from the simulation.
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