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Improved Destriping and Background Removal

Sometimes, a very bright extended source can ``fool'' DESTCRDD or BACKCRDD into thinking that the background level in a given detector data stream is higher than it actually is. If this artificially high background is subtracted from the data, the resulting images can display lower background levels on the in-scan sides of the source than on the cross-scan sides. The applications DESTCRDD and BACKCRDD contain filtering algorithms which can be tuned to reduce these sorts of effects, but if necessary, the ``Quality'' system used by IRAS90 can also be used. This requires the user to identify ``source regions'' which are to be excluded from the estimation of the destriping constants and background levels. There are several ways in which this can be done; for instance the KAPPA applications ZAPLIN can be used to manually identify and remove source regions from an initial map:

The ICL procedure ``MASTER'' described in appendix [*] contains an alternative approach to improved destriping in which the source regions are identified automatically. In addition, MASTER uses the extra trick of running the data through DESTCRDD and BACKCRDD twice.



next up previous contents
Next: Using IRAS90 - Details
Up: Recipes for Common Operations
Previous: Producing Colour Corrected Surface Brightness Images

IRAS90 --- IRAS Survey and PO Data Analysis Package --- Reference Guide
Starlink User Note 163
David S. Berry, W Gong, D C Parsons
19 February 1995
E-mail:ussc@star.rl.ac.uk

Copyright © 2008 Science and Technology Facilities Council