Cosimo Nigro
Cosimo Nigro
Systematic errors on FluxPoints would be a nice feature to add. This is similar to [what is already available in sherpa](https://sherpa.readthedocs.io/en/latest/data/index.html#errors). This feature will definitely improve the fitting of MWL...
Hello, is there a way, by using the NED query, to directly obtain the spectral energy distribution (SED) of a source? I am referring to the table provided in the...
**Is your feature request related to a problem? Please describe.** The fit fails without raising a specific warning in case the exposure in the spectral datasets is 0. However I...
@IlariaViale, @dimaniad6, let us use this branch to work on the implementation of the photomeson interactions. We are following the analytical parametrisation of Kelner Aharonian 2008 (https://arxiv.org/abs/0803.0688).
This is a draft PR that adds physical particle distributions, i.e. solutions of the electrons kinetic equations, along the usual analytical functions.
I was asked to add a feature to return the different SED components after a fit. This would allow for example, to compute the synchrotron and SSC luminosities, separately, after...
Despite having been introduced in #132, proton synchrotron cannot be used in a fit. This issue is a reminder to add the proton synchrotron scenario to the list of fittable...
Now that we have both the release paper and the zenodo we should add clear citation instructions. We might use this [citation file format](https://citation-file-format.github.io/). It seems a good option, but...
We added the absorption on synchrotron photons to the code and the tests, but not to the docs. A paragraph should be added in the Absorption section.
As suggested by @jsitarek in issue #50, I am opening a different issue for each of the absorption crosschecks. This one regards the absorption on the photon field of the...