pyuvdata
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A pythonic interface for radio astronomy interferometry data (uvfits, miriad, others)
Based on ability to select, but may require more work.
This replaces issue #114 which has been partially addressed.
It would convenient to be able to average the visibilities and weights as a function of frequency (i.e. go from 80kHz resolution to 160kHz resolution). There currently isn't an option...
Setting `read_data=False` will substantially speed up the script if the attribute is metadata.
It would be nice to have a list of the methods on our primary user classes at the top of the doc pages with links to the detailed docstrings for...
We now have a read_cst method that works if the beams are exported properly from CST. The consensus is that rather than trying to read all sorts of CST beams,...
cst_beam fails to read the following header from a standard CST output file `Theta [deg.] Phi [deg.] Abs(Dir.)[dBi ] Abs(Theta)[dBi ] Phase(Theta)[deg.] Abs(Phi )[dBi ] Phase(Phi )[deg.] Ax.Ratio[dB ] ------------------------------------------------------------------------------------------------------------------------------------------------------`...
uvbeam, as implemented, uses interp1d with default args. There are a number of instances where more customized frequency interpolation may be desirable. Two primary modes that may be desirable include:...