Python tools for calculating ionospheric behavior on large scales
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Updated
Dec 15, 2017 - C
Python tools for calculating ionospheric behavior on large scales
Compute linear polarization of the radiation emitted from the molecular cloud in magnetic field using LVG approximation.
Convolution kernel set generator used to create custom sets of kernels needed for W-Projection based convolutional gridding/degridding (https://arxiv.org/abs/0807.4161)
a high-performance C/C++ FITSWebQL SE (Supercomputer Edition)
The Broadband Radio Astronomy Tools (BRATS) is a software package for Linux and Mac which provides a variety of tools for the spectral analysis of both new broad-bandwidth radio data, along with legacy support for narrowband telescopes.
Utility library for working with search- and fold-mode PSRFITS pulsar data files.
Patches to the YMW16 Galactic free electron model and a Python wrapper.
C code (pgplot) for the analysis and visualisation of absorption spectra from radio telescopes
a high-performance FORTRAN & C (replaced Julia (replaced Fortran 2018)) FITSWEBQL SE (Supercomputer Edition)
DiFX(Distributed FX) correlator
a Rust implementation of the C/C++ FITSWebQL
Multi-channel filterbank spectrometer for detecting the 21-cm cosmological signal and Cosmic Dawn signature. Runs on Raspberry Pi with cavity filter array for simultaneous spectral analysis of the global 21-cm hydrogen line signal from high-redshift epochs.
SAGECal is a fast, memory efficient and GPU accelerated radio interferometric calibration program. It supports all source models including points, Gaussians and Shapelets. Distributed calibration using MPI and consensus optimization is enabled. Both spectral and spatial priors can be used as constraints. Tools to build/restore sky models are inc…
giza - a scientific plotting library for C/Fortran
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