flaremodel is a Python package designed for one-zone modeling of astrophysical synchrotron sources.
The code aims to provide modular interface for the modeling of synchrotron sources with efficient low level utility functions written in C - the cfuncs module.
These functions constitute the core of the flaremodel. The Python interface is built on top of these functions for convenience and guidance to formulate new models.
Multithreading support is implemented with OpenMP at a lower level in the cfuncs module where it is found useful.
At the same time, these low level functions bypass the infamous Global Interpreter Lock (GIL) of Python.
In simple words, users can implement efficient high level multithreading on python side when low level C functions are used and avoid the costly overheads of multiprocessing.
Our documentation covers the installation, module references and examples.
The documentation mostly covers the usage of the code. The detailed methodology/physics are covered in our paper.
The examples introduced in the paper are provided as jupyter notebooks in notebooks/ directory of the tarball and can also serve as a test of the compiled code.
Please cite the paper when the code is used in academical studies. Note that the paper refers to our first stable release.