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The AARTFAAC code, taken from the svn repository (https://svn.astron.nl/Triple-A/) and ported to git.

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

This project contains the embedded monitor and control parts for the microcontroller on the APS.

This project will contain all the necessary code to monitor and control the devices on an APS in an easily configurable fashion and then transmit it through the OPC ua protocol.

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

Data Access Library (DAL) provides access to the HDF5 radio astronomy data produced by the LOFAR telescope, operated by ASTRON (Netherlands Institute for Radio Astronomy).

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.

DP3: streaming processing pipeline for radio interferometric data

DP3: streaming processing pipeline for radio interferometric data

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.

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.

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.

Fork of https://github.com/tango-controls-hdbpp/libhdbpp-timescale