Commander solution in the Large Magellanic Cloud region, plotted in Galactic coordinates. Panels show from left to right and top to bottom: a) synchrotron brightness temperature at 30 GHz with 1deg resolution (linear colour scale); b) free-free emission measure with 1deg resolution (logarithmic colour scale); c) spinning dust brightness temperature at 30 GHz with 1deg resolution (logarithmic colour scale); d) thermal dust brightness temperature at 545 GHz with 5′ resolution (logarithmic colour scale); e) synchrotron polarization amplitude, P, at 28.4 GHz with 1deg resolution (corrected for polarization leakage, linear colour scale); f) CMB temperature with 5′ resolution (linear colour scale); g) CO J = 2 → 1 emission with 5′ resolution (linear colour scale); and h) thermal dust polarization amplitude, P, at 353 GHz with 5′ resolution (corrected for polarization leakage, linear colour scale). Each map covers 15deg × 15deg, and is centred on Galactic coordinates (l,b) = (279deg,−34deg).