[evlatests] EVLA and VLA Tsys measurements
Rick Perley
rperley at nrao.edu
Wed May 30 18:43:02 EDT 2007
In reviewing last night's L-band data, some notable problems in Tsys
values were seen.
In general, the measured values for (backend) Tsys for EVLA antennas
are noisier (less accurate) than those from the VLA. In addition, some
antennas from both arrays are showingTsys fluctuations (or errors in the
measurement of Tsys) of ~0.5K on ~minute timescales.
I would expect to see an rms level in measured value of Tsys of roughly:
sigma_T ~ 2*(Tsys/Tcal)*Tsys/sqrt(B.T)
where B is the bandwidth, and T the effective integration time. The
factor '2' comes from the 50% switching noise diode.
The ratio Tsys/Tcal is normally set to about 20 for both EVLA and
VLA. The characteristic averaging time is 10 seconds. The BW was
12.5 MHz. From these, we should see:
sigma_T ~ 0.0035*Tsys -- about 0.1 K for a normal Tsys.
Accurate measures of changes in Tsys are important, as they are
needed to convert the correlation coefficients to visibility flux
densites.
1) EVLA Antennas: (all at L-band):
In general, the apparent noise in the measurements is at least twice
that expected. This is easily seen for antennas 13, 14, 16, 21, 24, and
26. But the Tsys fluctuations are much better on 23 and 17.
Two antennas --
2) VLA antennas:
In general, the noise is at or better than the calculated level.
But there are notable exceptions:
3C, 5A, and 4 (all IFs) are quite poor.
All antennas show some degree of Tsys fluctuations on ~minute
timescales. These are usually less than 0.1K, so are comparable with
the noise in the measurements. But some antennas are spectacularly worse:
1(all IFs) shows ~1K variations.
28 C and D (in LCP) shows 1 to 2 K variations.
By looking at the detailed calibration solutions, we could determine
if these Tsys variations are real (in which case the corrected
visibilities will not show any fluctuations) are not. The current
dataset is not well suited for this, as the calibrator scans are only 50
seconds long, so i haven't tried this.
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