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The EveryBeam library is a library that provides the antenna response pattern for several instruments, such as LOFAR (and LOBES), SKA (OSKAR), MWA, JVLA, etc.

DP3: streaming processing pipeline for radio interferometric data

DP3: streaming processing pipeline for radio interferometric data

An example repository of an CI/CD pipeline for building, testing and deploying a C++ project

A cookiecutter template ready to create a new Python project that will support C/C++ Binary Extensions in Wheels using scikit-build-core, pybind11 and cibuildwheel

Common functions used in DP3, EveryBeam, WSClean. Like AOCommon but AOCommon is header-only and schaapcommon is not.

This repository started as a fork of https://github.com/aroffringa/aartfaac2ms, but now also has some more tools for AARTFAAC.

Raspberry pi pico code to control LOFAR high-band antenna tiles

Image Domain Gridding (IDG) is a fast method for convolutional resampling (gridding/degridding) of radio astronomical data (visibilities). Direction-dependent effects (DDEs) or A-tems can be applied in the gridding process.

This project is a fork of the original GPU De-dedispersion library (https://github.com/ajameson/dedisp/), intended to be used/modified for the FDD project.

The EveryBeam library is a library that provides the antenna response pattern for several instruments, such as LOFAR (and LOBES), SKA (OSKAR), MWA, JVLA, etc.

The EveryBeam library is a library that provides the antenna response pattern for several instruments, such as LOFAR (and LOBES), SKA (OSKAR), MWA, JVLA, etc.