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20070103 report
HARP array-centred pointing during UT 20061222 - 20070103
Since the last report on HARP pointing,
the method of acquiring pointing has been changed from being receptor-centred
to being array-centred.
155 data have been logged during these 12 days over Christmas
and are displayed below with only average collimation offsets removed:
Click for better view
There is no separation of data (by k-mirror position ?)
as seen last time.
The scatters (rms) in (dS,dZ) (after removal of two obvious outliers)
are (4.3", 3.3") and there is some systematic effect in the
dS-vs-Z plot (centre-left) that needs addressing.
Part of these (large-ish) scatters might be the use of global
collimation terms; nightly variations in collimation are quite
possible. The remainder of the scatter - above and beyond the
nominal (2",2") we might expect from a 'good' model - is undoubtedly
due to the lack of accounting for the k-mirror and HARP-centre
misalignments, but it is somewhat reassuring that the coefficients
we seek in Per's expressions
-dAz = x0*sin(2K) + y0*(1+cos(2K)) - x0'*cos(E-2K) - y0'*sin(E-2K)
-dEl = x0*(1-cos(2K)) + y0*sin(2K) + x0'*sin(E-2K) - y0'*cos(E-2K)
must be fairly small - as may also be concluded from
some of the HARP commissioning tests.
20070111
K-mirror positions for these data ( 155 in all) were extracted
from the JCMT_LOG.log files and the coefficients in
Per's formulae
-dAz = + xo*sin(2K) -dEl = + xo*(1-cos(2K))
+ yo*(1+cos(2K)) + yo*sin(2K)
- x'*cos(E-2K) + x'*sin(E-2K)
- y'*sin(E-2K) - y'*cos(E-2K)
were varied to best reproduce the observed pointing residuals.
The optimal values of (xo yo x' y') are
(apparently) (0 0 0 1) +- (1 1 1 1) arcseconds.
The residuals do bottom out at the above position, but the
minima are shallow; see below how the residuals in
azimuth(left) and elevation(right) vary with the value of the
4 coefficients:
Click for better views
Either
- these formulae do not describe the error functions of the k-mirror
- there are other more dominant terms still to be incorporated, or
- the residuals are dominated by noise rather than any systematics such as these.
(Note that there is no information regarding the state of vibration/oscillation
of the SMU during these measurements).
Two other terms have been suggested :
dAz = -x2*sin(K) - y2*cos(K)
dEl = x2*cos(K) - y2*sin(K)
and the optimum combination of (xo yo x' y' x2 y2) is
(-6 +3 -11 +9 -13 -6)
with residuals in (az,el) of (3.0", 3.8"); better than 'raw' -
and only slightly worse than the residuals from the
RxA pointing run of 13 January -
but not 'nominal'.
And it's maybe not the cup on the 18th that we've found, but
a shallow bunker on the edge of the green.
It still seems necessary to return to basics - starting with a redetermination of the
RxA pointing model.
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