XMM-Newton Science Analysis System: Users' Guide


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Next: 5.6.3 The new class of cool pixels Up: 5.6 Running the RGS processor rgsproc Previous: 5.6.1 Events, sources and selection criteria


5.6.2 Pixel-by-pixel offset subtraction

One of the standard procedures applied during rgsproc is a so-called offset correction which is designed to deal with an additive noise property of CCDs. Usually, an identical value is used for every pixel in a CCD node. Since SAS v6, an alternative has been offered that takes advantage of offset values that have been determined for each of the individual $171\times128$ pixels in a node from routine instrumental monitoring data. These offset data, which form part of the ODF, are accumulated every 3 revolutions thus also providing each pixel with its offset history. While experience of this alternative approach is being built up, it is not offered as the automatic choice but users are encouraged to try it and let us know if they are able to endorse the advantages described in early trials (see Technical report XMM-SOC-CAL-TN-0046 [12]).

The alternative offset method is selected with the withdiagoffset switch as in the following example :

 rgsproc withsrc=yes srclabel=Mkn421 \
                      srcstyle=radec srcra=166.113808 srcdec=+38.208833 \
                      withdiagoffset=yes


next up previous contents
Next: 5.6.3 The new class of cool pixels Up: 5.6 Running the RGS processor rgsproc Previous: 5.6.1 Events, sources and selection criteria
European Space Agency - XMM-Newton Science Operations Centre