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Dealing with spikes
External (or internal) interference (RFI) is a common occurrence with
the longer wavelengths in use at the JCMT; that is, particularly in
spectra taken with receiver A2. Usually this is offset from the centre
of the band and is of no major concern. It seems to be worse for
position-switching and may disappear entirely in the azimuth
beamswitched mode. Sometimes, however it can be a real nuisance. An
example is given in Figure
.
Figure:
A position-switched DAS spectrum of G34.3 in the area of
239 GHz showing `ringing' caused by a strong internal interference
spike. Note that it affects only the subband in which it occurs. The
offset from zero is the result of a combination of the source
continuum emission and a difference in the airmass between the signal
and reference positions. The line features are due to CH
CCH and
CH
CN.
Such interference spikes may be very effectively removed by applying
Hanning smoothing to the spectrum:
hann
The result is shown in Figure
. A multitude of weak
line features, as expected, are now revealed. The spike itself may be
removed by using the spike-removal command:
rem-spike
Figure:
The result of applying Hanning smoothing to the spectrum shown
in Figure
. Note that the `ringing' completely
disappears, revealing previously obscured line features. The spectrum
is itself somewhat smoothed in the process.
Next: Writing Your Own Command Files
Up: A More Complete Introduction to SPECX
Previous: Spectrum Statistics
Specx Cookbook
Starlink Cookbook 8
Henry Matthews, Tim Jenness
1st March 1997
E-mail:P.W.Draper@durham.ac.uk
Copyright © 2008 Science and Technology Facilities Council