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

<table>Wavelength calibration using Cu-Ne-Ar calibration lamp spectra ((a) using <i>identify</i>), and application of this wavelength calibration solution to the rest of the spectra ((b) using <i>reidentify</i>).</table>

Advances in Astronomy

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Figure 5

Figure 5: Observing and Reducing IFUs: INTEGRAL and PMAS—Properties of the Ionized Gas in HH 202 