CRPropa is a public astrophysical simulation framework for propagating extraterrestrial ultra-high energy particles. https://crpropa.github.io/CRPropa3/
Currently the photon density is set to 0 in tabular photon fields for all redshift $z < 0$.
With this change the density $n(\epsilon, z=0)$ will be used instead. This is of course only an approximation for small future redshifts. Therefore a KISS warning will be given if $z<-1$ is reached.
I also updated the example notebook for the Sim4D in the folder "doc/pages/example_notebooks/Sim4D". This will for the moment not be shown on the documentation website. I would wait for the upcomming revision of the documentation to build it.
This PR fixes #414.
Currently the photon density is set to 0 in tabular photon fields for all redshift $z < 0$. With this change the density $n(\epsilon, z=0)$ will be used instead. This is of course only an approximation for small future redshifts. Therefore a KISS warning will be given if $z<-1$ is reached.
I also updated the example notebook for the Sim4D in the folder "doc/pages/example_notebooks/Sim4D". This will for the moment not be shown on the documentation website. I would wait for the upcomming revision of the documentation to build it.