20000702 report
Repeat of Transit tracking
SUMMARY
Three further tests were carried out of the 's-correction' - the
lookup table that corrects the elevation pointing across transit.
The results are still frustratingly inconclusive, and a redetermination
of the underlying error function is suggested.
The 'transit' problem was noticed first in
April . A correction was
installed on 16 May, but recent checks in
May and
June
have been inconclusive for various reasons.
The new tracking tests were done during poor weather over the past
weekend, using the SCUBA
map16 method
:
| UT Date |
20000702 |
20000702 |
20000703 |
| source |
3c279 |
Uranus |
Uranus |
| HST start |
18:13 |
02:00 |
01:51 |
| HST end |
19:21 |
04:16 |
04:10 |
elevation at transit |
64o |
55o |
55o |
typical seeing |
1.0" |
0.2" |
0.2" |
Pointing residuals |
|
|
|
The elevation pointing residuals from the run on 3c279 suggested
that the s-correction term was perhaps deficient
in accounting for the elevation errors
properly, with the observed residuals showing a possible 2" residual
s-function.
However, the odd behaviour of the azimuth residuals at azimuth
195 suggest other possible problems, perhaps with the stability of the
atmosphere in the early evening.
Thus, a
second experiment was performed that night, on Uranus. The Uranus
residuals are notable for their good azimuth performance (rms errors
of 0.6" in more than 2 hours of tracking) and
the strong elevation systematic, of amplitude 4", but lying asymmetrically
around transit. The poor SCUBA
noise performance at this time is noted : it might have invalidated
data of a fainter source, but the brightness of Uranus must surely
be enough to overwhelm the extra bolometer noise.
Nonetheless, the experiment was repeated on Uranus the following evening -
when the noise on the SCUBA LW array had abated -
with essentially the same results. Both the Uranus results, though,
are quite different in character from the 3c279 results, and
an explanation has not yet presented itself.
Had we only these two self-consistent Uranus runs, my inclination
would be to repeat the experiment
without the s-correction activated in order to re-establish the
underlying error function. But how do we explain the difference
between the 3c279 data and those on Uranus ?
Iain Coulson
03 Jul 2000
|