Disentangling emission from star-forming regions in the Magellanic Clouds: Linking [O iii]λ88 µm and 24 µm

Open Access

Table B.3

Parameters for the different treatments of the map, 1σ uncertainties, and R² parameter as an indication of the goodness-of-fit of the regression model.

MIPS data	Slope	Intercept	R²
Original	0.872±0.015	−1.534±0.077	0.763
Tiled diffuse emission	0.869±0.013	−1.484±0.071	0.797
Zoomed diffuse emission	0.864±0.014	−1.532±0.071	0.793
Point sources subtracted	0.879±0.012	−1.446±0.065	0.824

“Original” is for noncorrected data, “tiled” and “zoomed diffuse emission” are the two calculation of the diffuse emission from the software used to extract the point sources, and “point source subtracted” is for the original MIPS 24µm maps with point sources subtracted.

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