[trans] - Model comments
Francois BONNAREL
bonnarel.francois at wanadoo.fr
Thu Mar 19 11:17:43 CET 2020
Hi all,
My "use case" is Aladin for individual images (cubes) astrometry
managment and HiPS generation.
What would be nice with IVOA "Trans" would be to have a simple unique
way to express all kind of mappings/ transformations. this is
unfortunately not the case with WCS FITS keywords apart from the linear case
I already checked the Trans model against this use case and presented
results at two interops last year (northern fall 2018 and northern
spring 2019)
I support the idea of having Mapping independant from Frames and having
composed Mapping as a subclass of Mapping. The Mapref solution seems to
be valid for everybody. OK ? Let me illustrate this below.
* In Trans (and AST) the good idea is to have all the transformation
managed the same way and chainable.
I you have to map a simple linear WCS you will have the following sequence
Shift of pixel coordinates to CRPIX
Apply linear Matrix (CD....
coefficients) to the result of above
Deproject from projection plane or
surface to the sphere (combination trigonometric function) to obtain
"native coordinates" (relative to projection center and axes)
Rotate to obtain coordinates in the
Spatial Frame you prefer (ICRS, FK5, GALACTIC, etc...)
* Now if you assume that some distortions to linear have to be
introduced you can easily introduce a polynomial transformation
BEFORE the Matrix transformation, AFTER this transformation or even
REPLACING it, according to how the astrometric reduction has been done.
* Apart from the polynomial transformation the 4 steps above are
easily inversible and indeed it's what you do when you compute your
pixel coordinates from iCrS coordinates in order to overmlay sources
in a catalog onto an image.
But the sequence is inversed of course so I don't know how this fit
with the Complex Mapping proposed by David.
If by default anything is bidirectional and we create a
ComplexMapping with a sequence of such things. Do we assume that
"inversing" is starting from the end of sequence of simple Mappings in
the complex one ? This will work also if one of those is Bidirectional
(and parallel too).
For the use case above it would be necessary.
* Apart from that I support the idea to have the Bidirectional
as combination of two independant transformations.
I started (a long time ago) with polynomial transformations in the
case of Schmidt plates digitizations.
Two differents cases : DSS from STScI and French Mama
scans of ESO, Palomar, SERC Schmidt plates
For DSS the polynomial is only given in the direction
from pixels to World Coordinates. But actually the usual method is to
use the "Newton algorithm" to inverse the transformation. In order that
it fits well with the "implicit" inversion embedded in the
unidirectional transform
For MAMA they provided two sets of polynomial
coefficients : one for each direction. They actually started from the
same list of astrometric standards on the plate where they match the
pixel coordinates and the world coordinates. They have two distinct
minimization runs. So the transforms are really independant but they
inverse the same transformation. The Bidirectional structure is pretty
fine for that I think...
Cheers
François
Le 11/03/2020 à 18:29, CresitelloDittmar, Mark a écrit :
>
>
> On Wed, Mar 11, 2020 at 10:55 AM David Berry
> <d.berry at eaobservatory.org <mailto:d.berry at eaobservatory.org>> wrote:
>
> For me the distinction between an Operation and a Mapping is a bit
> muddled as many operations are in fact bidirectional.
>
>
> The alternate view (in the current model) is that _no_ Operation is
> bidirectional, but some Operations may be trivially inverted to
> create an inverse Operation.
> Y = X + 1 is unidirectional.. from X to Y; and can be trivially
> inverted to X = Y - 1; for the inverse Operation from Y to X.
>
> I'll workup the model in the way we've talked about here, and see how
> that plays out in the example serializations for you.
>
> I'm currently working through the Coords model examples, and will
> queue that up next.
>
> Mark
>
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