2 Processing

The following steps were followed:

1.

Check the AAR derived with the OLP version 5.2 to see if there are points belonging to the spectral line which are flagged as glitched.

2.

Derive a new SPD and AAR in which glitch detection is disabled by setting the parameter alpha in CAL06 to a very high value.

3.

Compare those lines in which some points are identified as glitched in the standard AAR, to the corresponding ones in the non-deglitched AAR.

4.

Flatfield/Rebin both AARs and fit a Gaussian to the lines of interest to calculate the line fluxes.