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.

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.

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

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

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.

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

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).

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

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