Radio and Sub-millimeter Astronomy ================================== **Just started** -------------- - `casacore - Suite of C++ libraries for radio astronomy data processing `__ - The **casacore** package contains the core libraries of the old **AIPS++/CASA** package. This split was made to get a better separation of core libraries and applications. **CASA** is now built on top of **Casacore**. - **python-casacore**: Python bindings for casacore, a library used in radio astronomy. Document can be `found here `__ - `pyuvdata - A pythonic interface for radio astronomy interferometry data (uvfits, miriad, others) `__ - **pyuvdata** defines a pythonic interface to interferometric data sets. Currently pyuvdata supports reading and writing of miriad, uvfits, and uvh5 files and reading of **CASA** measurement sets and FHD (Fast Holographic Deconvolution) visibility save files. - Online document is `here `__ - `pyuvsim - A comprehensive simulation package for radio interferometers in python `__ - A number of analysis tools are available to simulate the output of a radio interferometer (CASA, OSKAR, FHD, PRISim, et al), however each makes numerical approximations to enable speed ups. - `wise - Wavelet Image Segmentation and Evaluation tool `__ - **wise** is developed to address the issue of detecting significant features in radio interferometric images and obtaining reliable velocity field from cross-correlation of these regions in multi-epoch observations. - Detection of structural information is performed using the segmented wavelet decomposition (SWD) method. - `GaussPy - A Python tool for implementing Autonomous Gaussian Decomposition `__ - Based on the work of `Autonomous Gaussian Decomposition `__ - `gausspyplus - Fully automated Gaussian decomposition package for emission line spectra `__ - **GaussPy+** is based on **GaussPy**: A python tool for implementing the Autonomous Gaussian Decomposition algorithm. - `Scintillometry - A Package for Radio Baseband Data Reduction `__ - **Scintillometry** is a package for reduction and analysis of radio baseband data, optimized for pulsar scintillometry science. `Online document is here `__ - `SoFiA - The HI Source Finding Application `__ - **SoFiA**, the Source Finding Application, is a new HI source finding pipeline intended to find and parametrise galaxies in HI data cubes. - The version 2 which is reimplemented in **C** can be `found here `__ - `galario - Gpu Accelerated Library for Analysing Radio Interferometer Observations `__ - **galario** is a library that exploits the computing power of modern graphic cards (GPUs) to accelerate the comparison of model predictions to radio interferometer observations.