[evlatests] Delays and Closure
Rick Perley
rperley at nrao.edu
Tue Feb 9 18:25:10 EST 2010
Spurred by a question from Frazer and Sanjay, I've investigated the
closure issues a little more closely.
The BLCAL that I ran on the 4 Jy source was applied to the SPLITed
data -- the only deviant points remaining were those from the 'wobble'
baselines.
I thus ran SPLIT *without* the BLCAL -- and got a *very* different
picture ...
Both the RCP and LCP visibilities now show significant offsets in
the visibilities of some baselines. These are easy to separate from the
'wobble' baselines -- wobbleing baselines always oscillate about the
mean amplitude of phase. The true closure baselines are always offset
and steady -- and are only seen in amplitude. The offsets in LCP are
much larger -- up to 10%!
It was immediately found that *all* of the visible offset (closure)
baselines are identified with those antennas with large delays. This is
a one-to-one relation -- there are no baselines with large delays
without offsets. Running BLCAL on this database perfectly removes the
visible closure offsets.
The trouble is: It's my understanding that AIPS corrects for the
decorrelation from these large delays. I followed the recommended
procedure: FRING and CLCAL, which created a CL table which was then
applied for further processing.
Furthermore, comparing the amplitude closure offsets with the
measured delays shows a curious relation: All the negative offsets
arise from baselines whose delays are positive. All the positive
offsets arise from baselines where the delays are of opposite sign. Yet
these latter offsets are much smaller than the negative ones, when they
should be larger (the two contributing antennas are 'further apart' in
delay space).
This indicates that the delay correction is not being applied
correctly (or there is a pilot error by your faithful scribe).
All of this will be eliminated once we get these pesky delays out of
the system! We might then be able to measure the *true* closure offsets
...
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