pyuvdata
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RadioAstronomySoftwareGroup
A pythonic interface for radio astronomy interferometry data (uvfits, miriad, others)
Once #1391 is merged, there is one outstanding gains table type left to build support for, which is the polarization leakage terms (in CASA parlance, "D Jones"). I wasn't able...
We need to write up a proper description of CalH5, similar to the UVH5 memo.
## Description All the metadata which is really about the telescope (rather than the dataset) has been pulled out into a Telescope object which is then attached to each object...
## Description This is a refactor of some code that has existed in pyuvsim for some time with some new functionality to make it easier to work with analytic beams....
Some OVRO-LWA pipelines write model visibilities to an ms column called "MODEL_DATA". pyuvdata currently only supports a column called "MODEL." It would be helpful to have more flexibility in column...
It would be useful if a single UVFlag object could support multiple flag_arrays, since we often now run multiple distinct flaggers on the same data and keeping the provenance of...
Currently if one tries to select data that doesn't exist, it errors. This also happens (at least in some methods, but maybe not mir or miriad? @kartographer?) if only some...
- remove support the old array shapes - remove support for old phasing including the phase_type, phase_center_ra/dec, frame, epoch attributes - Always require spw_id_array (so can remove the flex_spw boolean)...
Hi there, When reading raw MWA fits files with 1kHz Frequency resolution, and without `remove_coarse_band=False` I get this error. ``` ValueError: mwax passband shapes are only available for 40 kHz...
We've got a project that is hitting a bottleneck due to the lack of select on read for MWA correlator fits files. We should discuss the feasibility of implementing it...
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A pythonic interface for radio astronomy interferometry data (uvfits, miriad, others)