Open bennahugo opened 4 years ago
It is at least an order of magnitude faster to average this compared to oldsplit
ok just checked the resulting images to ensure the uv coordinates are correct. Everything seems to be in place the maximum error is about e-4 down from the peak
@bennahugo the UVW coordinates are lerped, I guess if that ever becomes a problem then spline fitting may be appropriate.
I don't think it is a problem @sjperkins everything seems to be well within smearing tolerances
Great stuff!
@sjperkins if you give me permission to push I can push my small fixes up
@sjperkins @sphemakh @o-smirnov I'm reasonably happy this works as advertised. I've Performed basic visibility inspection after averaging with XOVA to test the averager in production use - as a drop in replacement in my polarization calibration pipeline. From #7, after adding a switch to average "CORRECTED_DATA" I can confirm that the flags are correctly handled - the percentages are spot on. I also run through a basic pol cal to make sure that the data can be calibrated succesfully. Indeed there are no problems here:
Spectrum is spot on: Phase is spot on:
Prepolcal:
PKSB1934-638:
3C286 (coloured per correlation - crosshands at about 10% linearly polarized):
Original dataset:
Average dataset:
Postpolcal (Ignore RFI affected bands - cannot be leakage calibrated):
PKSB1934-638
3C286: