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
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