A Python package for simulating and modeling astronomical sources from radio interferometric observations
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Updated
May 18, 2023 - Python
A Python package for simulating and modeling astronomical sources from radio interferometric observations
A 3D FDM program of thermal calculation with Fabry–Pérot interferometry simulator powered by OpenCL. This is used in the link below.
A Jupyter notebook with a simple class to compute CO sizes and fluxes using the semi-analytical method developed by Zagaria et al. (2023b).
AIRCARS is an automated Stokes I calibration and imaging pipeline for spectroscopic snapshot imaging with solar observations made using the Murchison Widefield Array (MWA).
A project in which we study the feasibility of correlation calibration (Sievers 2016) in the Murchison Widefield Array in attempt to bridge the gap between Redudant Calibration and Sky Model Based Calibration
CUPRSI: A GPU-based algorithm for retrieving reflection responses by seismic interferometry from passive source seismic recordings
Simulating the Calibration of Arrays with Redundancy: a project to understand the impact of position errors on redundant calibration.
A pure rust implementation of the pyuvdata interferometric data interface.
Tool for repeating earthquakes searching and analysis
TUT FYS-1010 Physics Laboratory 1, 2017
A simple investigation on applying kalman filters to InSAR data
日本発の衛星データプラットフォーム Tellus のオウンドメディア「宙畑」の記事、https://sorabatake.jp/18669 で利用しているコードです。
Repository for programs used to generate figures for some published projects.
Script for the calculation of visibility and closure phase for different hour angles
Control interface of the GH13 experimental platform to study single nanoemitters aka CARODOTManip
Simple, fast package for simulating radio interferometric visibilities using the radio interferometry measurement equation (RIME)
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