Q and U as assumed to be normalized. The normalization is given by the spectrum.
Also, V is an input but it's not used inside the function. While I doubt anyone will use it, we must at least set it to 0 by default.
Note: It would be nice the check that Q and U are indeed normalized, but in practice it would be hard to do since they can be function. So we would have to evaluate them at every single point!
https://github.com/threeML/astromodels/blob/dev/astromodels/core/polarization.py#L128-L135
Q and U as assumed to be normalized. The normalization is given by the spectrum.
Also, V is an input but it's not used inside the function. While I doubt anyone will use it, we must at least set it to 0 by default.
Note: It would be nice the check that Q and U are indeed normalized, but in practice it would be hard to do since they can be function. So we would have to evaluate them at every single point!
https://github.com/threeML/astromodels/blob/dev/astromodels/core/polarization.py#L128-L135