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A ultra-high precision package for simulating radio interferometers in python on compute clusters.

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updates: - [github.com/pycqa/isort: 5.10.1 → 5.11.1](https://github.com/pycqa/isort/compare/5.10.1...5.11.1)

continuous integration

## Description This PR adds the following performance-enhancing features in the context of setting up a simulation from config: 1. Ability to do partial reading of beams (if they are...

enhancement

I am attempting to run a pyuvsim simulation using `run_uvdata_uvsim` function. I am using `simsetup.SkyModelData` to format a diffuse Healpix map that I can pass to the simulation function, but...

bug

## Description Strip out handling in tests for pyuvdata versions older than 2.2.8 (which we now require) ## Motivation and Context ## Types of changes - [x] Other ## Checklist:...

technical debt

This issue is mostly a reminder that we should do a bit of a group review of the simsetup part of pyuvsim. A few notes: 1. There seem to be...

technical debt

In our telecon the other day, we looked at the calculation of uvw's (which eventually go into the visibility calculation) for telescopes on the moon. When initializing from a parameter...

bug

I find the implementation of `AnalyticBeam` extremely restrictive and difficult to use for a number of reasons. I'll try to outline my ideas here, and open up discussion for ideas...

enhancement
needs research

@StellanBechtold has been working to replicate the visibilities for a single source simulation using only the alt/az calculation in the SkyModel object and an analytic beam. He's found that when...

wontfix

The code that takes the UVBeam data array into the jones matrix (in antenna.py) assumes a beam that has E-field components aligned with the azimuth and zenith angle axes. This...

enhancement

## Description Relax the requirement that there are always 2 feeds leading to 4 polarizations. Now allow for a single feed. Still require that there are Nfeed^2 polarizations. Needs changelog...

enhancement