pyuvdata
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RadioAstronomySoftwareGroup
A pythonic interface for radio astronomy interferometry data (uvfits, miriad, others)
Wide-band calibrations were introduced with UVCal future array shapes, but the `uvcalibrate` function does not support them yet.
see #1102 and #1105 for reference
Generally need to add more checking as is done with the other objects. In particular, make sure the right thing happens in the case of overlapping and differently sorted data....
see #1102 and #1105 for reference
Potential things: - antenna positions (already on Telescope) - antenna system temperatures - primary beam pointing errors - weather (might be just per site or maybe per antenna) - associated...
Once #979 is merged, the phasing memo will need to be updated to reflect the changes in how UVData objects are phased.
It would be helpful to have an integration between UVData and UVFlag to easily apply time-, frequency-, and/or baseline-dependent flags to a UVData object. One option would be writing a...
Antenna table describes the hypothetical, fully-working MWA array for FHD sav->uvfits conversions. However, the actual data may have non-reporting antennas, and thus the recorded uvfits is smaller (i.e. cross-correlations for...
The current approach is to put the entire extra_keywords dict into the main MS table as a dict called "pyuvdata_extra". Will this work if there are arrays or more complicated...
There is a minor issue w/ the MIRIAD file reader, where so-called "extra" variables (i.e., those other than the explicitly listed/known variables found in `default_miriad_variables` and `other_miriad_variables`) in the MIRIAD...
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A pythonic interface for radio astronomy interferometry data (uvfits, miriad, others)