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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:
- Follow the procedure described in section
to produce a
first estimate of the map.
- Use KAPPA:ZAPLIN (with parameter ZAPTYPE set to ``bad'') to
create a copy of the image in which the area containing the offending source has
been replaced with ``bad'' values.
- Use SIMCRDD to generate simulated CRDD files using the
output from KAPPA:ZAPLIN as the trial sky input, and the original
CRDD files to define the position and PSF for each sample. The
simulated samples corresponding to the source area will hold ``bad'' values.
- Use SETQUAL to assign a quality name (let's assume you use the
quality name ``SOURCE'') to the samples in the original CRDD files
which fall in the source region. To do this the input NDFs should be
the original CRDD files, and the mask NDFs should be the ones
generated by SIMCRDD. The SETQUAL function should be ``HS''.
This ensures that the quality ``SOURCE'' is held by all the samples
which are bad in the CRDD files generated by SIMCRDD (i.e.
all samples falling within the source region).
- Run DESTCRDD on the original input CRDD files,
specifying ``.NOT.SOURCE'' for parameter QEXP. This causes all
the samples with quality ``SOURCE'' to be excluded from the estimation
of the detector backgrounds. Note, it does not mean that these samples
will be excluded from the output CRDD files!
- Run BACKCRDD on the output CRDD files from
DESTCRDD, specifying ``.NOT.SOURCE'' for parameter QEXP. This
causes all the samples with quality ``SOURCE'' to be excluded from the
estimation of the CRDD file backgrounds.
- Run MAPCRDD again on the output CRDD files from
BACKCRDD.
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: 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