ExoNAMD
Introduction
ExoNAMD is a Python package to compute the Normalized Angular Momentum Deficit (NAMD) of exoplanetary systems. The NAMD is a measure of the dynamical excitation of a planetary system, and it can be defined as the difference between the total angular momentum of the system and the angular momentum it would have if all planets were on circular, coplanar orbits.
ExoNAMD is designed to be fast, modern, and reliable. It is built using the latest Python features and libraries, and it is tested extensively to ensure its accuracy and reliability.
Table of contents
How to install
Instructions on how to install ExoNAMD.
Install from PyPI
ExoNAMD is available on PyPI and can be installed via pip as
pip install exonamd
Install from source code
ExoNAMD is compatible (tested) with Python 3.8+
To install from source, clone the repository and move inside the directory.
Then use pip as
pip install .
Test your installation
Try importing ExoNAMD as
python -c "import exonamd; print(exonamd.__version__)"
Or running ExoNAMD itself with the help flag as
exonamd -h
If there are no errors then the installation was successful!
Documentation
ExoNAMD comes with an extensive documentation, which can be built using Sphinx.
The documentation includes a tutorial, a user guide and a reference guide.
To build the documentation, install the needed packages first via poetry:
pip install poetry
poetry install --with docs
Build the html documentation
To build the html documentation, move into the docs directory and run
make html
The documentation will be produced into the build/html directory inside docs.
Open index.html to read the documentation.
Build the pdf documentation
To build the pdf, move into the docs directory and run
make latexpdf
The documentation will be produced into the build/latex directory inside docs.
Open exonamd.pdf to read the documentation.
The developers use pdflatex; if you have another compiler for LaTex, please refer to sphinx documentation.
How to contribute
You can contribute to ExoNAMD by reporting bugs, suggesting new features, or contributing to the code itself.
If you wish to contribute to the code, please follow the steps described in the documentation under Developer Guide.
How to cite
@ARTICLE{Bocchieri2025,
author = {{Bocchieri}, Andrea and {Zak}, Jiri and {Turrini}, Diego},
title = "{ExoNAMD: Leveraging the spin-orbit angle to constrain the dynamics of multiplanetary systems}",
journal = {in preparation},
year = 2025,
}
Metadata
Release files for exonamd 0.3.1
For a detailed explanation of source distributions (sdists) and built distributions (wheels), please see the package formats documentation.
Source distribution (sdist)
| File | Size | Uploaded | |
|---|---|---|---|
| exonamd-0.3.1.tar.gz | 718.4 kB | Details |
Built distribution (wheel)
| File | Interpreter | ABI | Platform | Reset |
|---|---|---|---|---|
| exonamd-0.3.1-py3-none-any.whl | Python 3 | none | any | Details |
Total release size: 1.5 MB
Release files / exonamd-0.3.1.tar.gz
| Download URL | exonamd-0.3.1.tar.gz |
|---|---|
| Size | 718.4 kB |
| Tags | Source |
|
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| Upload date | |
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No |
| Uploaded via |
twine/6.1.0 CPython/3.10.18
|
Release files / exonamd-0.3.1-py3-none-any.whl
| Download URL | exonamd-0.3.1-py3-none-any.whl |
|---|---|
| Size | 776.2 kB |
| Tags | Python 3 |
|
SHA-256 checksum How to use checksums |
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| Upload date | |
|
Uploaded using Trusted Publishing? What is trusted publishing? |
No |
| Uploaded via |
twine/6.1.0 CPython/3.10.18
|