[fitswcs] RADESYS = 'GAPPT'
Steve Allen
sla at ucolick.org
Wed Mar 16 14:50:05 EDT 2011
On Wed 2011-03-16T11:38:00 -0700, Rob Seaman hath writ:
> Which is all to say that another possibility is to ignore the
> telescope pointing and run the astrometry.net code from a
> postprocessing command.
That is the next step, but instruments with small FOV will benefit
from a good initial WCS.
Still, there is value in recording the telescope pointing.
An archive full of images with telescope-based coordinates and
post-processed astrometric coordinates should be a useful engineering
tool for diagnosing the pointing system.
> For other instrumentation such as multi-object spectrographs, the
> notion of telescope pointing is quite a bit different. What does it
> mean for a bench spectrograph to be "on-target"?
In the case of slitmask-based spectrographs each is either
astrometrically on-target or not providing object data.
--
Steve Allen <sla at ucolick.org> WGS-84 (GPS)
UCO/Lick Observatory--ISB Natural Sciences II, Room 165 Lat +36.99855
1156 High Street Voice: +1 831 459 3046 Lng -122.06015
Santa Cruz, CA 95064 http://www.ucolick.org/~sla/ Hgt +250 m
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