Cosimo Nigro

Hello @registerrier, yes `agnpy` is using the same format! For the old EBL models I just copied the FITS files in `gammapy-data`. And for the Saldana Lopez 2021, @IlariaViale created...

Hello @aleberti I am looking into this, It is difficult to include Table 4 of the Franceschini 2018 paper as an opacity model readable by Gammapy. The redshift values at...

Hello everyone, as @dhomeier, some of these quantities, like the dimensionless accretion rate (m dot) and the Eddington luminosity are computed when a Shakura Sunyaev accretion disk (`SSDisk`) is initialised....

Hello @dimaniad6, @IlariaViale, do you think you will have some time in the next days to work on this?

Thanks for the updates @dimaniad6, @IlariaViale, I did not mean to rush you. By the way, when you reply to GitHub notifications via mail your reply is also posted on...

I am not talking of individual bins but when the entire exposure is 0. This is clearly and indication of a possible problem with the dataset.

Hello @pguenth, thanks for reporting this! I think this is the only point where I use the logging https://github.com/cosimoNigro/agnpy/blob/7afc1f89ae0a7d6e6770b5f2e50e538064efd962/agnpy/fit/__init__.py#L1 i.e. to notify the user if `sherpa` and `Gammapy` are not...

Copying @jsitarek's last comment from issue #50 > I did some simple calculations using this disk absorption, the details are in the attached notebook > [check_tau_disk.ipynb.gz](https://github.com/cosimoNigro/agnpy/files/5735523/check_tau_disk.ipynb.gz) > > some conclusions:...

No updates here after PR #76, still there is this order-of-magnitude mismatch in the energy threshold where the absorption becomes relevant.

Hello @jsitarek, in an attempt to revive this long-standing issue I created [this notebook](https://github.com/cosimoNigro/agnpy/blob/master/experiments/basic/disk_absorption_dermer_finke_comparison.ipynb) re-implementing from scratch the formula for the absorption from Finke 2016 and comparing it against another...