Michele Doro
Michele Doro
Is there a special reason why the range for bounds ends at 1e-18 msun and does not go to lower values?
I have to still have a look at the code, but I just ask, is there a way already coded to plot the constraints in number density per cubic parsec?...
`gammapy.astro.darkmatter` makes use of the `AtProduction_gamma.dat` file which contains the spectral points of an annihilation events for different channel. Now the file is read after downloading it along with a...
Hi @GernotMaier. For some time now I am collaborating with Paolo Giommi on the development of a portal for access to astronomical data. The story is long and the aim...
There are two yaml files with the same name. One in input/sources for the specific source, and one in data/year/paper/ for a specific paper about possibly another source. The name...