`SNR Hadronic Synthesis` is a Python pipeline to synthesise **hadronic gamma-ray emission** from 3D (M)HD simulations of supernova remnants (SNRs).
The code is **generic** and not hard-coded to any particular object: it takes PLUTO-like simulation outputs and builds gamma-ray maps and SEDs in a fully reproducible way.
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## Getting started
## Project and context
To make it easy for you to get started with GitLab, here's a list of recommended next steps.
This software has been developed by **Anna Marretta** within theresearch activities of the **PNRR–CATMAD** project (CUP: C53C22000350006), carried out at the **University of Palermo (UNIPA)** and the **INAF – Palermo Astronomical Observatory (OAPA)**.
Already a pro? Just edit this README.md and make it your own. Want to make it easy? [Use the template at the bottom](#editing-this-readme)!
The CATMAD project is led by **Prof. Marco Miceli** and involves a research group including
**Sabina Ustamujic, Antonio Tutone, Fabio Reale, Salvatore Orlando,
Costanza Argiroffi, Paolo Pagano, Marco Barbera, and Oleh Petruk.**
## Add your files
Although developed in the CATMAD framework, this repository represents an **independent and original software effort** by the author. It provides a **modular and general pipeline** for synthesizing hadronic gamma-ray emission from 3D (M)HD simulations of supernova remnants.
-[ ] [Create](https://docs.gitlab.com/ee/user/project/repository/web_editor.html#create-a-file) or [upload](https://docs.gitlab.com/ee/user/project/repository/web_editor.html#upload-a-file) files
-[ ] [Add files using the command line](https://docs.gitlab.com/topics/git/add_files/#add-files-to-a-git-repository) or push an existing Git repository with the following command:
The pipeline assumes a SNR expanding in an intercloud medium with uniform density \(n_0\), interacting with different interstellar clouds.
-[ ] [Set up project integrations](https://www.ict.inaf.it/gitlab/anna.marretta/snr-hadronic-synthesis/-/settings/integrations)
You provide 3D PLUTO-like outputs (`rho`, `tr*`, etc.) in `.flt` format, and the physical parameters of the simulation (explosion energy, ambient density, distance to the source, …).
The code then:
## Collaborate with your team
1. Builds a geometrical/physical **mask** around the shock.
2. Computes the **distance** from the explosion centre for each cell (`r_pc.flt`).
3. Computes a **Sedov-like acceleration time** (`t_s_mask.flt`) and a **Bell-like amplified magnetic field** (`B_sat.flt`).
4. Derives the maximum proton energy **E_max** using one of two models:
**Reference:** Celli et al. (2019), *MNRAS, 490, 4317*.
5. Builds **density 3D distributions** for shocked material (`rho_masked`) and for gamma-emitting material after cooling (`rho_cooling`).
6. Computes a **global scaling factor** for the proton spectra so that the total proton energy \(W_p\) matches a target value.
7. Builds a voxel-wise **amplitude map**\( A(\mathbf{x}) \propto d/d_{\max} \).
8. Computes the **gamma-ray map** and the **total SED** using Naima’s hadronic `PionDecay` model.
9. Provides utilities to **plot the gamma-ray map** (rotation + integration) and the **SED**.
-[ ] [Invite team members and collaborators](https://docs.gitlab.com/ee/user/project/members/)
-[ ] [Create a new merge request](https://docs.gitlab.com/ee/user/project/merge_requests/creating_merge_requests.html)
-[ ] [Automatically close issues from merge requests](https://docs.gitlab.com/ee/user/project/issues/managing_issues.html#closing-issues-automatically)
Use the built-in continuous integration in GitLab.
All functionality is exposed through a **Typer-based CLI** via `main.py`.
-[ ] [Get started with GitLab CI/CD](https://docs.gitlab.com/ee/ci/quick_start/)
-[ ] [Analyze your code for known vulnerabilities with Static Application Security Testing (SAST)](https://docs.gitlab.com/ee/user/application_security/sast/)
-[ ] [Deploy to Kubernetes, Amazon EC2, or Amazon ECS using Auto Deploy](https://docs.gitlab.com/ee/topics/autodevops/requirements.html)
-[ ] [Use pull-based deployments for improved Kubernetes management](https://docs.gitlab.com/ee/user/clusters/agent/)
-[ ] [Set up protected environments](https://docs.gitlab.com/ee/ci/environments/protected_environments.html)
There are two main usage modes:
***
### 1. Interactive wizard (recommended)
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