[evlatests] C-Band Imaging comparisons: VLA vs. WIDAR
Bryan Butler
bbutler at nrao.edu
Tue Jul 7 16:20:42 EDT 2009
so is the conclusion from this that aside from the closure corrections
needed, the WIDAR data is good?
-bryan
Rick Perley wrote, On 7/7/09 13:59:
> I've now been able process the C-band parallel data sets taken last
> July 4/5.
>
> 1) As noted before, all WIDAR images are rotated by 180 degrees
> about the phase center.
>
> 2) The calibrator was 2007+404, an excellent unresolved source. The
> VLA data, after closure corrections (recall that both VLA and EVLA
> antennas are included here) provided a decent map with 28000:1 DR.
> (There's a weak background source, 2 mJy, located 30 arcsec to the NW).
> The WIDAR data are expected to provide a slightly better Dynamic
> Range: 10 antennas with 512 MHz total BW, vs. 15 antennas with 200 MHz
> total BW, so the sensitivity should be slightly better. To obtain this,
> I had to apply closure corrections to the WIDAR data as well -- the
> corrections are distressingly large: typically 0.2% for subbands 1 and
> 2, and up to 2% for subbands 3 and 4. (These latter two sub-bands were
> placed outside the old polarizers' range, and four of the antennas in
> the WIDAR subarray have old polarizers. The large corrections needed
> for subbands 3 and 4 should not be viewed with especially concern, as
> they are likely due to the polarizers.). The 'final' DR was 40,000:1.
> The same weak secondary is easily seen -- reflected about the origin.
>
> 3) Cygnus A: The VLA image, after standard self-calibration,
> provided a nice image with perhaps 1000:1 DR -- about what is expected
> for this very powerful and heavily resolved object with the old
> correlator.
> The WIDAR image provides about the same formal DR, but is notably poorer
> in its true fidelity. I attribute this primarily to the poor (u,v)
> coverage -- we have a lack of intermediate spacings which are needed to
> better link the long and short spacings.
>
> I'll now move to the very messy 20cm data.
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