[evlatests] Compression tables
Rick Perley
rperley at nrao.edu
Mon Jul 30 19:18:40 EDT 2012
A noontime test of the PDif compression on Taurus A ran today. I
tried all frequency bands. Compression was seen up to and including
K-band. The primary beam, combined with the spectral slope of the
source and the higher system noise combine to make the power increment
too small to be useful at Ka and Q bands.
The increment to system temperature caused by the source is
approximately:
60K at L, S, and C bands.
40K at X band
25K at Ku-band
10K at K band.
In this, and succeeding messages, I'll give the 'compression factor'
for each of these bands, for each IF and antenna. This is defined as:
(PDif on Tau A)/(PDif on cold sky). Values are in percent.
In this message, I give the L-band values. The data were taken with
128 MHz BW, at 1465 and 1820 MHz.
Antenna A B C D
-------------------------------------------------------
1 88 90 93 91
2 93 92 89 83
3 99 97 92 91
4 94 92 88 90
5 97 98 96 94
6 98 93 94 97
7 97 98 97 96
8 93 95 97 92
9 97 95 99 100
10 in the barn
11 99 97 98 100
12 97 97 97 97
13 98 85 100 89
14 99 96 96 95
15 99 96 97 100
16 96 92 95 93
17 100 100 97 100
18 93 89 84 81
19 very noisy data
20 93 94 93 93
21 87 88 93 86
22 95 95 91 90
23 89 94 88 92
24 91 91 98 98
25 67 67 82 82
26 93 93 94 94
27 99 100 99 100
28 99 noisy 96 noisy
------------------------------------------------------------
Comment: Except for a few antennas (notably ea25), the compression
is rather small, and very uniform amongst the antennas. The compression
is definitely much less than for Cygnus A at this frequency -- the ratio
of the fluxes is about 1.6:1 (1513 Jy for Cyg A, 930 for Taurus A). The
notable difference in compression may be a manifestation of the
nonlinearity in the response.
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