About the draft itself Re: WD-SIA-2.0
Petr Skoda
skoda at sunstel.asu.cas.cz
Tue May 6 18:27:20 PDT 2014
On Tue, 6 May 2014, Arnold Rots wrote:
> But the usage of wavelength in radio astronomy is never precise
> and is equivalent to the role band designations (L, C, U, K, ...) play.
exactly - the precise wavelength/energy range can be stated (with
sufficient precision) only for spectra. But for IMAGE (SIA !)
it is always very difficult to state what energy/wavelength range is
exactly covered - this goes to filters description and more subtle
metadata. So the only relevant information you can get from image original
metadata from data acquisition system is something like BANDNAME - the
transformation to energy is done artificially during publishing phase when
some VO publisher tries to understand those BANDNAME ids and translate
them using some tables - a nice source of errors the scientist might be
tracking a long time ....
But as it is (as was said some time ago) job for the client not SIA
server, I am very wondering what the final solution will be and whether
the scientists will accept the IVOA view of consistent data model ;-)
BTW - polarisation states are not strictly enumerated and never one image
is only in given stokes value- there are cross-talks, partial
pollarization etc ..... again depends on type and quality of
filters and its definition .... so its similar to BANDNAME as well.
>
> I am old enough to remember that some optical astronomers
> supported the modernization of replacing wavelength by
> wavenumber - physically more meaningful (like frequency).
a lot of theoretical and model (even measured) spectra are still presented
in wave numbers - for larger range it is more natural than logorithms etc
....
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