Description:
This program
should be used to reduce SCAN/MAP data taken using the technique described by
Emerson (1995, ASP Conf Ser 75, 309). The deconvolution is performed using Fast Fourier
techniques.
Usage:
remdbm [-h] [-v] [-out=] [-noams] [-filter] files
Parameters:
h
Help
message
v
Version number. Also indicates whether ADAM communication is enabled.
out=file
Filename of output image.
Default is ‘final.sdf’
noams
Turn off ADAM messaging if available. Default is false. Ignored if ADAM messaging is not available.
filter
Turns on high frequency filtering. When used, data at frequencies greater than that
to which the telescope is sensitive are set to zero.
files
List of input files to be
processed. Shell wildcards are allowed. See notes for restrictions.
Examples:
remdbm
_reb.sdf
Process all files matching the pattern and write the result to final.sdf. remdbm -out=m82
o66_lon_reb o67_lon_reb o68_lon_reb o69_lon_reb
Process the four input images. The output
filename is set to m82.sdf. remdbm -filter -noams *_reb.sdf
Process the supplied files with high
frequency filtering. Do not use the messaging system. Notes:
The following restrictions apply:
-
Each image should contain a single chop configuration.
-
Each image must have identical dimensions and pixel size (they do not need to be square)
-
The images must be rebinned in the same coordinate system as the chop throw.
Related
Applications
Copyright © 1997-2000,2003 Particle Physics and Astronomy Research Council