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A pythonic interface for radio astronomy interferometry data (uvfits, miriad, others)

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Do this by setting `branch = true` in the `run` section of `.coveragerc`. Without this we aren't testing all branches of an if statement, which can be particularly problematic for...

technical debt

I've been running into this error in a script lately, and without having a REPL to attach to it's basically impossible to diagnose for me. I was thinking maybe we...

good first issue
UVData

This should be useful for `.read()`, `.read_uvh5()` and its cousins, and `from_file()`.

docs

It appears that `.interp()` function will not adjust to changes made in `spline_opts` if `resuse_spline=True`. In order for `spline_opts` to work, it needs `reuse_spline=False`, which is not ideal. This should...

beams
docs

Currently, there is very limited support for select on read, which means that all data inside the MS must be read in before one can downselect the data that you...

enhancement
UVData

This can really cleanup & simplify code blocks, especially with if/else blocks for future_array_shapes and calibration type and select.

technical debt

It would be useful to be able to print the differences between objects without calling `__eq__` and we probably do not want `__eq__` to print out things by default (it's...

enhancement
UVBase

Having a look through `UVData.read_cst_beam` I get the impression it could be MUCH simplified. Some things I noticed: 1. There is a discrepancy between some of the keywords to the...

beams
technical debt

pyuvdata by necessity uses many conventions, and these are documented throughout the code API pages and tutorials. However, it'd be good to gather all these into one reference place.

docs

UVData objects support a flex pol mode where each spectral window can have a different (but only one) polarization. UVFlag should have handling when it's instantiated from a flex pol...

uvflag