Cband calibration.
23sep 2000 (last mod 16feb01..focus gain)
Description:
On/off position switching on continuum sources was done at cband using
the correlator. The setup was:
One minute integration's on and then off source followed by a 10
second cal on/off in the off source position.
Try to track sources rise to set.
Record 4 25 Mhz bands centered at RF frequencies: 5000, 4900, 5100,
and 5200 Mhz.
Use the total power information, cal values, and source flux to compute
tsys, gain, sefd.
Fit the data to a function of (az,za).
Compare the measured gain with the expected gain. Include losses
from pitch, roll, and focus.
Daily Info:
The dates for the observations and the sources observed are:
25aug00 : J0318+164 (CTA21)
26aug00 : J0318+164 (CTA21)
27aug00 : B0116+082
29aug00 : B1609+266
01sep00 : B0453+227
03sep00 : J2445+099
The high uncorrelated cal was used during the runs (this is 2 separate
diodes).
Cal values by freq and polarization
Freq [Mhz]
|
cal polA [K]
|
cal polB [K]
|
5000
|
26.9
|
25.6
|
4900
|
26.8
|
26.4
|
5100
|
27.4
|
25.6
|
5200
|
27.0
|
24.5
|
The plots have all the data over plotted with different symbols for each
source. Dotted lines are polA and dashed lines are polB. All four frequencies
are over plotted (so there are 8 symbols arranged vertically at each za).
The figures are:
-
SEFD vs za.
-
Tsys vs za. The separate lines are different polarization and frequencies.
-
Gain (average) vs za. The average is (gainA+gainB)*.5. This was used since
the cband receiver uses linear polarization and one of the source was polarized.
-
Cal scale factor vs za. This is (cal In Kelvins)/(Cal deflection in correlator
units). This should be a flat line for each run since the attenuators were
not changed (within a source). Variations are probably do to gain changes
in the if/lo.
-
Fractional polarization defined as (gaina-gainb)/(gaina+gainb). All
4 frequencies are over plotted. The literature for B0453+227 (open box
source) quotes a fractional polarization of 8.1% at cband. This is very
close to what we measure.
The average gain, Tsys, Gain/Tsys, and fractional polarization (at 5 Ghz)
are plotted in a 2-d plot vs az,za. Up is feed in the north and to the
left is the feed in the west (when the source is rising). The length of
the arrow is an absolute measure of the value. The angle the arrow makes
with the vertical is a relative measure of the strength. The table
at the lower left averages the value over all the dish, za 0-5,5-10,10-15,
and 15-20 degrees. The figures are:
-
Average gain [K/Jy]. 1 tick= 1 K/Jy. Horizontal is maximum and 180 deg
(down) is 1/2 of maximum.
-
Tsys [Kelvins]. 1 tick=10K. Up is minimum temperature and 180 deg
(down) is 2*TsysMin.
-
Gain/Tsys [Tsys/Jy]. 1 tick= .03 Tsys/Jy. up is maximum, down is
1/2 maximum.
-
Fractional polarization. 1 tick=.02 (2%). Up is 0 fracPol, down is 10%.
Fitting the data to f(az,za):
The data is fit to:
f(az,za)=c0 + c1*(za-10)+c2*(za-10)^2+c3*(za-10)^3+
c4*cos( az)+c5*sin( az)+c6*cos(2az)+c7*sin(2az)+
c8*cos(3az)+c9*sin(3az)
Sefd-fit,
Tsys-fit, gainAvg-fit These plots have all 4 frequencies
and polA,B over plotted. The (za-10) terms are for za 0 through 20 degrees
(unlike some of the other fits that used (za-14) for za > 14).
-
SEFD - fit. Units are Jy/Tsys.
-
Tsys - fit. Units are deg K.
-
AvgGain - Fit in K/Jy.
gainBySample,gainOverplotFit,PRFloss,
and prfAzTerms. These plots take a closer look at the gain fit
and how the azimuth terms of the fit compare to the azimuth terms of the
gain loss computed from pitch,roll, and focus. The figures are:
-
AvgGain versus sample for all 4 frequencies.
-
AvgGain versus sample for 5000 Ghz with the fit over plotted. The polarized
source B0453+227 is not fitting very well even though we're using the average
gain.
-
GainLoss computed from pitch,roll, and focus. The gain is down by
55% at high za.
-
Fit to avgGain 5000 Mhz. The upper coefficients are the fit to the measured
data. The bottom coefficients are the gain computed from the pitch, roll,
and focus errors, and then scaled to a maximum gain of 3.2 Jy (this was
the measured maximum). The plots show the azimuth terms for each fit (solid
measured data, dots - pitch,roll,focus). The 3 az terms line up in phase
pretty well. The 1az and 2az terms are out of phase. They are probably
caused by residuals from the za fit looking like azimuth term. We have
undersampled in the (az,za) plane especially at low zenith angle where
we only have samples close to 90 and 270 degrees.
az components
of SEFD,Tsys,Gain, and avgGain . These plots show the azimuth components
(1az,2az,3az) for the sefd, tsys, gain, and average gain. All 4 frequencies
are over plotted. PolA is solid and polB is the dotted line. The coefficients
for 5000 Mhz are also printed on the plot. PolA on the top and polB on
the lower portion.
Warnings on using the fits:
There are only 5 sources used in the fits. Of these 3 are in the south
and 2 are in the north. There are no rise to set tracks for any of the
northern sources and there are no sources above 27 deg dec or below 8 deg
dec. For sources with decs close to those used in the fit, the sigmas of
the fits should be ok. For high or low dec sources, care should be taken.
Coefficients from the fits:
Below are listed the coefficients from the various fits. The first column
in each row specifies the data that was fit.
For gainAvg there is just one fit while gain,tsys,sefd have a separate
fit for polA and polB.
> Aug/sep00 sbn
> last computed: Sat Sep 23 14:59:40 2000
> fit Ids
> 1 GainAvg
> 2 Gain
> 3 tsys
> 4 sefd
fId
|
frq
|
c0
|
za-10
|
(za-10)^2
|
(za-10)^3
|
cosAz
|
sinAz
|
cos2Az
|
sin2az
|
cos3az
|
sin3az
|
sigma
|
pol
|
calVal
|
1
|
5000.
|
1.7538e+00
|
-1.0252e-01
|
2.2021e-03
|
1.0623e-04
|
4.5354e-02
|
1.2862e-01
|
-2.3625e-01
|
-7.3604e-02
|
-1.2753e-01
|
-1.0821e-01
|
1.6848e-01
|
a
|
0.00
|
1
|
4900.
|
1.8711e+00
|
-1.0681e-01
|
2.1033e-03
|
7.7822e-05
|
6.3580e-02
|
1.3139e-01
|
-2.4989e-01
|
-7.6052e-02
|
-1.2665e-01
|
-1.1205e-01
|
1.7032e-01
|
a
|
0.00
|
1
|
5100.
|
1.6987e+00
|
-9.8949e-02
|
2.4332e-03
|
6.6633e-05
|
1.4377e-02
|
1.2597e-01
|
-2.3501e-01
|
-7.5637e-02
|
-1.1814e-01
|
-1.0295e-01
|
1.6653e-01
|
a
|
0.00
|
1
|
5200.
|
1.5757e+00
|
-9.9210e-02
|
2.4778e-03
|
7.8476e-05
|
2.7343e-02
|
1.1970e-01
|
-2.3414e-01
|
-6.5800e-02
|
-1.1183e-01
|
-1.0053e-01
|
1.5696e-01
|
a
|
0.00
|
2
|
5000.
|
1.7595e+00
|
-1.0173e-01
|
1.6072e-03
|
1.4080e-04
|
3.8623e-02
|
1.7846e-01
|
-2.5155e-01
|
-1.2617e-01
|
-8.9766e-02
|
-9.6326e-02
|
1.5601e-01
|
a
|
26.9
|
2
|
5000.
|
1.7482e+00
|
-1.0332e-01
|
2.7971e-03
|
7.1665e-05
|
5.2085e-02
|
7.8781e-02
|
-2.2096e-01
|
-2.1039e-02
|
-1.6529e-01
|
-1.2010e-01
|
1.8550e-01
|
b
|
25.6
|
2
|
4900.
|
1.8710e+00
|
-1.0566e-01
|
1.5471e-03
|
1.1014e-04
|
6.2089e-02
|
1.7709e-01
|
-2.7138e-01
|
-1.2596e-01
|
-8.5959e-02
|
-1.0270e-01
|
1.5535e-01
|
a
|
26.8
|
2
|
4900.
|
1.8711e+00
|
-1.0796e-01
|
2.6596e-03
|
4.5504e-05
|
6.5072e-02
|
8.5684e-02
|
-2.2841e-01
|
-2.6142e-02
|
-1.6735e-01
|
-1.2139e-01
|
1.9027e-01
|
b
|
26.4
|
2
|
5100.
|
1.7204e+00
|
-9.7922e-02
|
1.8217e-03
|
9.6961e-05
|
1.5222e-02
|
1.7909e-01
|
-2.5218e-01
|
-1.2492e-01
|
-8.1434e-02
|
-9.2455e-02
|
1.5428e-01
|
a
|
27.4
|
2
|
5100.
|
1.6770e+00
|
-9.9977e-02
|
3.0448e-03
|
3.6305e-05
|
1.3532e-02
|
7.2843e-02
|
-2.1784e-01
|
-2.6354e-02
|
-1.5484e-01
|
-1.1344e-01
|
1.8320e-01
|
b
|
25.6
|
2
|
5200.
|
1.5751e+00
|
-9.8451e-02
|
1.9623e-03
|
1.2240e-04
|
3.1590e-02
|
1.5949e-01
|
-2.4937e-01
|
-1.0773e-01
|
-7.7952e-02
|
-9.1447e-02
|
1.4373e-01
|
a
|
27.0
|
2
|
5200.
|
1.5763e+00
|
-9.9969e-02
|
2.9932e-03
|
3.4555e-05
|
2.3096e-02
|
7.9912e-02
|
-2.1891e-01
|
-2.3868e-02
|
-1.4570e-01
|
-1.0962e-01
|
1.7479e-01
|
b
|
24.5
|
3
|
5000.
|
2.9646e+01
|
-5.2949e-03
|
2.6610e-02
|
4.7184e-03
|
2.4074e-01
|
-1.0340e-01
|
-1.4674e-01
|
8.0792e-02
|
5.8742e-02
|
-7.4206e-02
|
3.6441e-01
|
a
|
26.9
|
3
|
5000.
|
3.3267e+01
|
5.2876e-03
|
2.5501e-02
|
4.2942e-03
|
3.2478e-01
|
-1.1396e-01
|
2.2163e-01
|
2.4978e-01
|
-2.4552e-02
|
-1.3815e-01
|
3.5408e-01
|
b
|
25.6
|
3
|
4900.
|
2.9410e+01
|
-1.0514e-02
|
2.8579e-02
|
5.0288e-03
|
3.3184e-01
|
-5.6961e-02
|
-1.5974e-01
|
3.1137e-02
|
5.1334e-02
|
-4.0229e-02
|
3.6840e-01
|
a
|
26.8
|
3
|
4900.
|
3.2641e+01
|
4.5705e-03
|
2.6681e-02
|
4.5254e-03
|
3.4549e-01
|
-7.9204e-02
|
2.3530e-01
|
1.7151e-01
|
-1.9551e-04
|
-6.4149e-02
|
3.2038e-01
|
b
|
26.4
|
3
|
5100.
|
3.1710e+01
|
-1.0501e-02
|
2.5680e-02
|
4.6052e-03
|
3.1931e-01
|
-6.1445e-02
|
-2.3277e-01
|
3.1076e-02
|
7.1353e-02
|
-5.6437e-02
|
3.5082e-01
|
a
|
27.4
|
3
|
5100.
|
3.5399e+01
|
-2.0882e-03
|
2.6172e-02
|
4.1104e-03
|
2.1904e-01
|
-9.8081e-02
|
1.8428e-01
|
2.1979e-01
|
4.8789e-02
|
-8.4922e-02
|
3.0030e-01
|
b
|
25.6
|
3
|
5200.
|
3.2746e+01
|
-1.8575e-02
|
2.7299e-02
|
4.6411e-03
|
1.9768e-01
|
-8.9377e-02
|
-2.7594e-01
|
2.1869e-02
|
1.2002e-01
|
-2.3809e-02
|
3.3813e-01
|
a
|
27.0
|
3
|
5200.
|
3.8200e+01
|
-5.1859e-03
|
2.9278e-02
|
4.4261e-03
|
1.1369e-01
|
-1.1408e-01
|
2.5612e-01
|
2.2965e-01
|
1.1856e-01
|
-4.6731e-02
|
3.4049e-01
|
b
|
24.5
|
4
|
5000.
|
1.7241e+01
|
7.0702e-01
|
3.4483e-02
|
5.5505e-03
|
-3.3028e-01
|
-2.7133e+00
|
1.7465e+00
|
1.6785e+00
|
1.2727e+00
|
8.4311e-01
|
2.0695e+00
|
a
|
0.00
|
4
|
5000.
|
1.9495e+01
|
7.8065e-01
|
2.3975e-02
|
5.5690e-03
|
-4.6761e-01
|
-1.7991e+00
|
1.7915e+00
|
7.2553e-01
|
2.1500e+00
|
8.4309e-01
|
2.2767e+00
|
b
|
0.00
|
4
|
4900.
|
1.5991e+01
|
6.1422e-01
|
3.4339e-02
|
6.2111e-03
|
-3.1686e-01
|
-2.2721e+00
|
1.6682e+00
|
1.3720e+00
|
1.0068e+00
|
8.3401e-01
|
1.6178e+00
|
a
|
0.00
|
4
|
4900.
|
1.7812e+01
|
6.9026e-01
|
2.7024e-02
|
5.9715e-03
|
-4.5340e-01
|
-1.6187e+00
|
1.6013e+00
|
6.6129e-01
|
1.8809e+00
|
7.4953e-01
|
1.9713e+00
|
b
|
0.00
|
4
|
5100.
|
1.8834e+01
|
7.2955e-01
|
3.1566e-02
|
6.7915e-03
|
-1.7929e-02
|
-2.8269e+00
|
2.0495e+00
|
1.6149e+00
|
1.1538e+00
|
1.0240e+00
|
2.0251e+00
|
a
|
0.00
|
4
|
5100.
|
2.1639e+01
|
8.4592e-01
|
2.1025e-02
|
6.7685e-03
|
-1.0466e-01
|
-1.9057e+00
|
2.1549e+00
|
7.5133e-01
|
2.2469e+00
|
9.8772e-01
|
2.4585e+00
|
b
|
0.00
|
4
|
5200.
|
2.1252e+01
|
8.8631e-01
|
3.6725e-02
|
7.3856e-03
|
-2.6240e-01
|
-3.2168e+00
|
2.3352e+00
|
1.8293e+00
|
1.4162e+00
|
1.2037e+00
|
2.3313e+00
|
a
|
0.00
|
4
|
5200.
|
2.4848e+01
|
9.9814e-01
|
2.9116e-02
|
8.7642e-03
|
-2.7345e-01
|
-2.4805e+00
|
2.5540e+00
|
9.6929e-01
|
2.6657e+00
|
1.1516e+00
|
2.9753e+00
|
b
|
0.00
|
processing: x101/cb/calsep00/doit.pro
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