Observing and Reducing IFUs: INTEGRAL and PMAS—Properties of the Ionized Gas in HH 202

Figure 1

Section of a Hα HST image of Orion [4] with a sampling of 1 arcsec (top left, white box indicates the FoV of a typical 2D PMAS observation). A result of this PMAS observation with spaxels of 1 × 1 arcsec is shown on the top right. Bottom left shows a section of the data cube observed where we can see a monochromatic image at the upper slice. Bottom right shows an integrated spectrum of a group of spaxels and a flux map integrated over an emission line (figure extracted from the Ph.D. thesis of M. Núñez-Díaz).