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WFI Reduction Tips | ![]() |
This page gives some help in the reduction of WFI images following the experience gained by the EIS Team with the Pilot Public Survey.
A starting point for instructions on general reduction of CCD
images and spectra is given in
Iraf is:
ccdproc
user guide (press SHIFT-Click to load).
The IRAF MSCRED
reduction package, developed at NOAO, is currently used by in our pipeline
for the removal of the instrument fingerprint. It exist already
compiled for different platform and can be simply downloaded and
installed following the instructions present at the MSCRED page at
NOAO (see the readme file).
The header of the images provided by the WFI is still lacking
(June 1999) some information needed by the MSCRED package to
quietly reduce the data. In order to fix the needed keywords we
have written a simple IRAF script that have
to be used on the images before the reduction with MSCRED.
A general shell script is also provided
that allows the additon to the PRIMARY header of the image the
keyword FILTER.
The value of this keyword is extracted from the standard ESO
keyword:HIERARCH ESO INS FILT NAME.
The keyword FILTER is the main driver of the reduction with MSCRED.
To properly deal with the different reading ports of each CCD
and/or different filters MSCRED need a set-up file.
WARNING: these scripts are provided as they are, without warranty. They have been developed by Mario Nonino as part of EIS team effort to develop the EIS Pilot Public Survey WFI image reduction pipeline and they will eventually be improved and/or corrected in the furure without notice.