IViS π±ΒΆ
IViS β Interferometric Visibility-domain Inversion Software
Note
IViS is designed as a modular framework upon which new deconvolution methods can be built. In its current implementation, IViS is a generic MEM-like mosaicking framework (with w-stacking available), but it aims to incorporate arbitrary spectral models in the near future to fully exploit the spectral dimension of the data. IViS is very new, and this documentation is in its early stages β it will continue to evolve as the project develops.
Useful resources: - Github repository
Note
Parts of this code were inspired by the MPol package, which implements a Regularized Maximum Likelihood (RML) framework for radio interferometric imaging. In contrast to MPol, IViS includes native support for image-plane mosaicking with DDEs of the Primary Beam.
InstallationΒΆ
To get started, we recommend using uv to manage packages and mamba to create a clean environment with casacore:
# Install mamba (if not already available)
conda install mamba -n base -c conda-forge
# Create the IViS environment
mamba create -n ivis -y -c conda-forge \
python=3.10 casacore python-casacore gsl \
numpy scipy astropy matplotlib \
reproject radio-beam psutil tqdm joblib \
pip
conda activate ivis
# Torch CUDA wheel
python -m pip install --upgrade pip
python -m pip install --index-url https://download.pytorch.org/whl/cu124 torch
# Install uv (if not already available)
curl -LsSf https://astral.sh/uv/install.sh | sh
export PATH="$HOME/.cargo/bin:$PATH" # if needed
# Install IViS and dependencies using uv
uv pip install "ivis[gpu] @ git+https://github.com/antoinemarchal/ivis.git"
Note
To delete an environment:
mamba env remove -n ivis
DocumentationΒΆ
Contents:
Forward models:
Basics Tutorials:
API:
Note
If you use IViS, please cite our work and reference the IViS GitHub repository. When IViS matures enough, it will be published in JOSS and/or an astrophysical journal.