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Instrument Collimations
Instrument Collimations
This document is a guide for the Pointing Guru in the use of observed
pointing offsets.
- Collimations are instrument-specific offsets from the model.
- The collimations are kept in Rx/FE-specific files :
- /jac_sw/itsroot/src/wrappers/rxa/initialise/instrument_rxa.ent
- /jac_sw/itsroot/src/wrappers/rxb/initialise/instrument_rxb.ent
- /jac_sw/itsroot/src/wrappers/rxw/initialise/instrument_rxwb.ent
- /jac_sw/itsroot/src/wrappers/rxw/initialise/instrument_rxwd.ent
- /jac_sw/itsroot/src/harpb/XML/instrument_harpb.ent
and are called X (azimuth collimation) and Y (elevation
collimation).
- For whichever instrument/receiver/FrontEnd is recognized as our
primary instrument, the collimations should be (0,0).
- Updates of the pointing model
should be done (for convenience) using data from the 'primary' FE,
while the collimations for the other receivers may be updated
using smaller datasets.
The instructions below treat,
in order of increasing confusion, the various datasets
that may be available for use in updating the collimations:
Large pointing datasets obtained with the primary FE should
be analyzed using
TPOINT
with appropriate input of the current JCMT pointing model.
TPOINT outputs the values for the (7) parameters of the new model
which may then be transferred to the appropriate file
(/jac_sw/itsroot/src/tcs/thi/THI.tide)
for future use.
Small datasets or single pointings with other receivers may be used
only to update their collimations.
If (uaz,uel) are the means of the observed offsets
as recorded in the last two columns of the
TPOINT .pnt file
then a TPOINT analysis of the data using the following command sequence
will produce values of CA and IE that are related to the
default values, CAdefault, IEdefault,
as stored in the collimation files above,
and to uaz and uel as follows:
- CA = CAdefault + uaz
- IE = IEdefault - uel
(See this example data analysis.)
These new values of CA,IE may be entered as the defaults for future
improved performance, i.e. for residuals (uaz,uel)
that should be more preciesly (0,0).
If small datasets or single pointings with the primary-FE
show non-zero offsets and if these are interpreted to reflect
changes to the overall collimation of the telescope, then they
may be used to update the pointing model terms CA and IE
(which will then affect future pointings with any receiver).
However, there is a sign convention that must be obeyed,
as was revealed in a previous document.
Simply put, if you point with JCMT/primary-FE and observe pointing offsets
in azimuth and elevation of (uaz,uel) -- and you wish
to rectify the pointing model so that future pointings
(with any receiver) will appear at
offsets of (0,0) -- then you should run the data through TPOINT,
FIX all 7 parameters, USE IE CA, note the changes to these two collimation
values, and change
* CA to old_CA + d(CA)
* IE to old_IE - d(IE)
Large pointing datasets taken with other receivers
pose the greatest challenge. They ought certainly to allow
the model to be updated, but the impact on the collimations
is where it gets messy. Things are simpler if such data are taken
under circumstances
where there is no expectation of a change in relative collimations.
Consider first the acquisition of a large pointing dataset
obtained with receiver Rx in circumstances
where no change to the model is expected.
Analysis by TPOINT should suggest
no changes to the values for CA, IE, meaning, in reality,
no changes to the differences in collimations between Rx and the
primary-FE,
meaning in effect no changes to the collimations for Rx,
since those for the primary-FE are maintained at (0,0). If non-zero
offsets are
seen you are faced with determining, separately (how ?)
whether the problem lies with the model or the receiver (collimations).
Suppose instead that there is a need to redetermine the model
using Rx under circumstances that ought to preserve the relative collimations.
Suppose that
- the old receiver collimations were (XRx,YRx)
- when processed with TPOINT
the new data show non-zero changes in (CA,IE)
of (uazdata,ueldata),
as well as to the other model parameters.
What to do with the collimations ? and the others parameters ?
-
Changes to the other parameters reflect structural
misalignments which should be common to all receivers
and may be incorporated into the TPOINT pointing model
irrespective of the RX used.
-
The collimations for the primary-FE may be left as (0,0).
-
Those for Rx must remain as
(XRx,YRx) . . .
- . . so the new values of CA,IE
suggested by the TPOINT analysis may then be used as if
they had been determined by use of primary-FE data; i.e.
change CA to (CA + uazdata), IE to (IE - ueldata).
If data are taken with Rx when both the model and the relative collimations
may have changed then any resulting model
may work (i.e. generate no further observational offsets)
only for Rx itself. The relative collimations will need
establishing separately and the system reverted eventually
to one based on the primary-FE.
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