Massive Black-Hole Binary Population Synthesis for Gravitational Wave Calculations ≋●≋●≋
This package, which is actively under development, is aimed at providing a comprehensive framework for MBH binary population synthesis. The framework includes modules to perform pop synth using a variety of methodologies to get a handle on both statistical and systematic uncertainties. Currently, binary populations can be synthesis based on: cosmological hydrodynamic simulations (Illustris), semi-analytic/semi-empirical models (SAMs), and observational catalogs of local galaxies and/or quasars.
The holodeck
framework is currently under substantial, active development. It will not be available on pypi
(pip
) or via conda
install until it has stabilized. Currently holodeck
requires python >= 3.8
, and tests are run on versions 3.8
, 3.9
, 3.10
.
The recommended installation for active development is to:
- OPTIONAL: create and activate a new anaconda environment to isolate your build:
conda create --name holo310 python=3.10; conda activate holo310
- Clone the holodeck repository:
git clone https://github.com/nanograv/holodeck.git
- Install the required external packages specified in the requirements file:
pip install -r requirements.txt
. OPTIONAL: install development requirements:pip install -r requirements-dev.txt
- Build the required c libraries from holodeck cython code:
cd holodeck; python setup.py build_ext -i
- Perform an development/editable local installation:
python setup.py develop
The 'editable' installation allows the code base to be modified, and have those changes take effect when using the holodeck
module without having to rebuild/reinstall it.
The best way to get started is using the demonstration/testing notebooks included in the notebooks/
directory.
The primary sources of documentation for holodeck
are this README.md
file, the notebooks included in the notebooks/
directory, and docstrings included in the source code directly. readthedocs
documentation are being written and improved, and a methods paper is in preparation.
This project is being led by the NANOGrav Astrophysics Working Group.
Details on contributions and the mandatory code of conduct can be found in the CONTRIBUTING.md file.
To-do items and changes to the API should be included in the CHANGELOG.md file.
Contributions are not only welcome but encouraged, anywhere from new modules/customizations to bug-fixes to improved documentation and usage examples. The git workflow is based around a main
branch which is intended to be (relatively) stable and operational, and an actively developed dev
branch. New development should be performed in "feature" branches (made off of the dev
branch), and then incorporated via pull-request (back into the dev
branch).
(Unit)tests should be developed in two ways: for basic functions/behaviors, standard unit-tests can be placed in the holodeck/tests/
directory. More complex functionality should be tested in notebooks (in notebooks/
) where they can also be used as demonstrations/tutorials for that behavior. The python script scripts/convert_notebook_tests.py
converts target notebooks into python scripts in the holodeck/tests/
directory, which can then be run by pytest
. The script scripts/tester.sh
will run the conversion script and then run pytest
.
Before submitting a pull request, run scripts/tester.sh -bv
to run the builtin tests.
For more comprehensive testing (e.g. against numerous python versions, and building from the sdist package), you can use the python tox
package: simply run tox
in the root directory and it will use the configuration specified in tox.ini
. The scripy scripts/run_tox.sh
is also provided to setup and execute tox tests and required environments.
Formatting:
New code should generally abide by PEP8 formatting, with numpy style docstrings <https://numpydoc.readthedocs.io/en/latest/format.html>
_. Exceptions are:
- lines may be broken at either 100 or 120 columns
Notebooks:
Please strip all notebook outputs before commiting notebook changes. The [nbstripout](https://github.com/kynan/nbstripout)
package is an excellent option to automatically strip all notebook output only in git commits (i.e. it doesn't change your notebooks in-place). You can also use nbconvert
to strip output in place: jupyter nbconvert --clear-output --inplace <NOTEBOOK-NAME>.ipynb
.
Copyright (c) 2022, NANOGrav
The holodeck
package uses an MIT license.
A NANOGrav paper on holodeck
is currently in preparation.