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A MUSE map of the central Orion Nebula (M 42)

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Figure

Fig. 1. Inverse grayscale representation of the white-light image of the final mosaic
Table 1. FITS extensions in the provided files a .
Fig. 2. Centroiding residuals versus wavelength for four bright stars in the field. Each panel shows horizontal and vertical distances to the mean center of the star in lighter dashed and dotted curves, and the radius as a solid dark curve
Fig. 4. Velocities measured within the “blue” slit of Baldwin et al.
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