3D Gas Datacube

[danielegaggero]

Hi,

it would ve very useful to include the possibility to compute the pi0 emission from a gas model provided as a 3D datacube (for instance as FITS file), or a generic smooth function f(x,y,z) provided by the user. The model would not necessarily be defined in the whole Galaxy, it could be a zoomed-in map of the GC region, or a relevant star-forming region for instance.

Would it be possible to modify the pi0 integrator to include this possibility?

thanks!
Daniele