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DP3: streaming processing pipeline for radio interferometric data

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.

LOFAR2 Beamformed Pulsar Folding Pipeline (PulP2-DSPSR-folding) in CWL implementation

Lots Of Things Used Somewhere

Kas based Yocto image build to generate the OS images and support configuration / functionality around running PyPCC translators on LOFAR2 station raspberry pi CM4 modules.

LOFAR Initial Calibration Pipeline, previously known as prefactor

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.

Trout is responsible for deploying Hawkbit to the Central Monitor. Hawkbit is used for updating the Raspberry Pi's of Lofar in the field.

The ci/cd contains configuration scripting, which have to be run when a clean install of the db is done

HDL project code

Deploys LOFAR sofware on LOFAR stations from all our repositories that need software on a station.

Central Monitoring and Operational Control of LOFAR Stations

SDP to Uniboard translator

Rapthor: the LOFAR DDE Pipeline

A cookiecutter template to create a new C++ project with CI/CD pipeline for building, testing and deploying a C++ project.

New rendition of the Transients Pipeline. Original version: https://github.com/transientskp/tkp/tree/master

A fork of https://git.astron.nl/lofar2.0/cobalt, with only the Beamformer kernel code and tests. Refactored to make the code 'stand-alone' as much as possible, while still being somewhat compatible with the original code. Since the original repository is over 500 Mb, all large files have been pruned from the history.