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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.
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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.
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DP3: streaming processing pipeline for radio interferometric data
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This repository started as a fork of https://github.com/aroffringa/aartfaac2ms, but now also has some more tools for AARTFAAC.
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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.
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This project contains the embedded monitor and control parts for the microcontroller on the APS.
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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.
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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.
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An example repository of an CI/CD pipeline for building, testing and deploying a C++ project
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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.
Updated