[daip] weights, dividing by models
Olaf Wucknitz
wucknitz at astro.uni-bonn.de
Fri Feb 29 12:52:52 EST 2008
Hi Eric,
I made some tests with UVSUB (OPCODE=DIV) to see what happens to the
weights. When using the gridded-FFT method, I find that indeed the weights
are scaled with amplitude**2.
However, if I use SMODEL or DFT computation of a CC model, the weights are
instead scaled with the amplitude.
Do CALIB, FRING, BLCAL and others use the same routines to divide by a
model? I find it a bit difficult to follow these parts of the source code
with all the branches for different model types etc.
Cheers,
Olaf
> I suspect that the comments somewhere are not correct. The weights are
> scaled by the square of the amplitudes at present - I suspect that the
> amplitude was used in the earliest of days. Note that this weighting
> seems to cause model fits (e.g. CALIB) to fail when the model
> improves! This is why such tasks have a DOWEIGHT parameter to take
> weights to some power (e.g. 1/2) so that weights do not differ by so
> much between short and long spacings.
>
> Eric Greisen
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