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The reduction of integral field spectroscopy (IFS) data requires severalstages and many repetitive operations to convert raw data into, typically, alarge number of spectra. Instead there are several semiautomatic data reductiontools and here we present this data reduction process using some of the ImageReduction and Analysis Facility (IRAF) tasks devoted to reduce spectroscopicdata. After explaining the whole process, we illustrate the power of thisinstrumental technique with some results obtained for the object HH202 in theOrion Nebula (Mesa-Delgado et al., 2009).

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