Welcome to easyfermi's documentation! ===================================== The graphical interface `easyfermi `_ provides a user-friendly way to analyze *Fermi*-LAT data, making use of `fermipy `_, `gammapy `_, `astropy `_, and `emcee `_. **easyfermi** allows for several different analysis on Fermi-LAT data, such as: * Modeling of the region of interest (RoI) using the `Binned likelihood analsyis `_. * Generating TS and residual maps for the RoI. * Extracting a spectral energy distribution (SED) for a target. * Correcting an SED for EBL absorption. * Generating a light curve for a target (adaptive or constant time bins). * Localizing a source or fitting its spatial extension. * Fitting several SED models with a MCMC approach. Check out the :doc:`usage` section for further information, including the GUI :ref:`installation`. Acknowledging *easyfermi* --------------------- To acknowledge *easyfermi* in a publication please cite `de Menezes, R. 2022 `_. Since easyfermi relies on fermipy, gammapy, astropy, and emcee, please also cite `Wood et al. 2017 `_, `Donath et al. 2023 `_, `Astropy Collaboration et al. 2018 `_, and `Foreman-Mackey et al. 2013 `_. The EBL models adopted in *easyfermi* are from: - `Franceschini et al. 2008 `_. - `Finke et al. 2010 `_. - `Dominguez et al. 2011 `_. - `Franceschini & Rodighiero 2017 `_. - `Saldana-Lopez et al. 2021 `_. If you make use of one of these models in your publication, please cite the corresponding paper. Contents -------- .. toctree:: usage Basic_analysis lightcurve SED localization extension custom_analysis