Raspberry pi pico code to control LOFAR high-band antenna tiles
Common functions used in DP3, EveryBeam, WSClean. Like AOCommon but AOCommon is header-only and schaapcommon is not.
This project contains the embedded monitor and control parts for the microcontroller on the APS.
DP3: streaming processing pipeline for radio interferometric data
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.
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 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.
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.