https://github.com/RadioAstronomySoftwareGroup/pyuvdata
Revision ea050a88ff8215e0ea3438f6eb2a02c687af797e authored by Bryna Hazelton on 14 October 2021, 22:49:54 UTC, committed by Bryna Hazelton on 14 October 2021, 23:15:15 UTC
Don't use np.real_if_close because it's flaky (seen to fail in Conda builds but not in our standard CI). Instead warn if the imaginary part is larger than expected (presumably because of floating point accuracy issues) and then force to real.
1 parent f8a44d2
Tip revision: ea050a88ff8215e0ea3438f6eb2a02c687af797e authored by Bryna Hazelton on 14 October 2021, 22:49:54 UTC
Fix conversion of non-crosspol power beams to real
Fix conversion of non-crosspol power beams to real
Tip revision: ea050a8
File | Mode | Size |
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.circleci | ||
.github | ||
ci | ||
docs | ||
pyuvdata | ||
scripts | ||
.codecov.yml | -rw-r--r-- | 124 bytes |
.coveragerc | -rw-r--r-- | 158 bytes |
.gitignore | -rw-r--r-- | 1.0 KB |
.pre-commit-config.yaml | -rw-r--r-- | 1.0 KB |
.readthedocs.yml | -rw-r--r-- | 559 bytes |
CHANGELOG.md | -rw-r--r-- | 35.0 KB |
CODE_OF_CONDUCT.md | -rw-r--r-- | 3.5 KB |
LICENSE | -rw-r--r-- | 1.3 KB |
MANIFEST.in | -rw-r--r-- | 296 bytes |
README.md | -rw-r--r-- | 12.4 KB |
environment.yaml | -rw-r--r-- | 443 bytes |
paper.bib | -rw-r--r-- | 3.9 KB |
paper.md | -rw-r--r-- | 1.9 KB |
pyproject.toml | -rw-r--r-- | 206 bytes |
setup.cfg | -rw-r--r-- | 903 bytes |
setup.py | -rw-r--r-- | 5.0 KB |
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