Description:
Each bolometer is analysed
independently, the mean and standard deviation are calculated, any points greater than NSIGMA
sigma from the mean are treated as spikes and removed. Note that for mapping this despiking
algorithm is only useful for very weak sources; bright sources will be removed (since a bolometer
jiggles on and off bright sources). Photometry observations do not suffer from this problem as
the bolometers are always on source.
Usage:
scuclip in out nsigma
Parameters:
IN =
NDF (Read)
This is the name of the input demodulated data file
MSG_FILTER = CHAR
(Read)
Message output level. Allowed values are QUIET, NORM and VERB. Default
is NORM. If MSG_FILTER is set to VERBOSE the number of spikes removed from each
bolometer is reported.
NSIGMA = DOUBLE (Read)
Number of sigma beyond which data are
thought to be spikes. If this number is positive an iterative clip will be performed (ie the
standard deviation is recalculated after clipping and points lying outside the new range are
removed). If it is negative then iterative clipping is switched off.
OUT = NDF (Write)
Output
data file.
Examples:
scuclip infile outfile 5
Clip any data points that are further than 5
sigma from the mean. The clipping is done on a per bolometer basis and is iterative.
scuclip infile outfile -5
Clip any data points that are further than 5 sigma from the mean.
The clipping is done on a per bolometer basis and only one pass of clipping is performed.
Notes:
Related Applications
Implementation Status:
The despiking routine sets QUALITY bit 5 to bad. It does not
affect the data. The effects of despiking can be removed by using the
Kappa task
setbb to unset
quality bit 5.
Copyright © 1997-2000,2003 Particle Physics and Astronomy Research Council