Thermal emission distribution in G330.2+1.0. The component retrieved by pGMCA that we identify as thermal emission is shown on the left. In the middle, we show the component retrieved by pGMCA that we identify as synchrotron emission. On the right, we show an XMM-Newton three-color image of G330.2+1.0, with 0.4–1.2 keV emission in red, 1.2–2.0 keV emission in green, and 2.0–7.0 keV emission in blue. The contours of our thermal emission component are overlaid in white; they appear in the green clump region that was studied in Williams et al. (2018) and shown to harbor thermal emission. The scales are logarithmic.