Performance of the GBT at 2.3 GHz (13 cm)
Measurements done April 19, 2004.
June 22, 2004;
Y. Kovalev, F. Ghigo
Introduction
GBT
gain curve measurements in the
13 cm band (S-band)
were done April 19, 2004.
The gain versus elevation was measured by observing several
strong calibration sources over a wide range of elevations
using the peak procedure.
The subreflector focus was adjusted about once per hour.
The observations were done at a frequency of 2240 MHz
with a bandwidth of 80 MHz. The frequency
was chosen to match the
VLBA S-band.
A hybrid was used to produce LCP and RCP output
from linearly polarized feed horns.
Weather conditions were good (partly cloudy).
The active surface (zero offset: ON, FEM model: OFF)
and dynamical corrections were in use for this run.
Summary
| Channel
| Maximum Gain
| Tsys (high elevation)
| Tcal
|
| LCP
| 1.91 K/Jy
| 19.5 K
| 2.10 K
|
| RCP
| 1.75 K/Jy
| 19.5 K
| 2.15 K
|
- The atmospheric opacity is tau = 0.009
- Correcting for opacity makes very little difference in
the curve of gain versus elevation.
- The difference in gain between the two polarization is about 9%,
which is about the uncertainty in the noise calibration
temperatures (Tcals), hence probably not significant.
Observing Procedure
Observing of the calibration sources was done using the "peak"
procedure and fitting gaussians with
"GFM"
(see description of this procedure
here).
System Temperature Measurements
The Tsys values as calculated by
"GFM"
from each "peak" procedure, are plotted in Figure 1.
Some of the system temperature measurements were corrupted
by RFI. They are not used in our calculations.
Figure 2: system temperature vs elevation
A simple model for the atmosphere was fitted by least-squares
to the data:
Tsys = T0 + Tatm (1 - exp(-Tau*A)),
in which airmass A = 1/sin(Elev), T0 is extrapolated
noise temperature for airmass = 0 (sum of the receiver temperature,
antenna and groud contribution, etc.), tau is the atmospheric
opacity.
The fitted parameters are as follows (assuming Tatm = 260 K):
| Parameter | Fit to LCP data | Fit to RCP data |
| T0 | 16.12 K | 16.44 K |
| Tau | 0.0091 | 0.0086 |
Tipping scan
More study of Tsys versus elevation was done by a tipping scan, driving
the antenna from 8 to 60 degrees elevation at 50 degrees azimuth,
and recording the system temperature five times per second.
Figure 3 shows these scans and the model fits
using a similar model as above.
The opacities, which is depend more on the low elevation data, agree
well with those derived from the "peak" data.
Figure 3: Tipping Scans.
Gain Curve Measurements
The Tant values for observed sources were calculated by
"GFM"
from each "peak" procedure.
The following sources forming standard scale were observed:
3C48
(0134+329),
3C147
(0538+498),
3C286
(1328+307),
3C295
(1409+524).
Most of the time was spend observing the last two sources.
We have used
Baars et al. (1977) parameters for the spectra of the
sources 3C48, 3C286, 3C295. Significant change in flux of 3C147
encouradged us to use
Ott et al. (1994) spectra parameters for it.
The size correction factor taken from
Ott et al. (1994) was applied.
Actual values (size correction factor applied)
of calibrators flux density in use are as follows:
| Calibrator | Flux density, Jy |
| 3C48 | 10.81 |
| 3C123 | 32.31 |
| 3C147 | 15.13 |
| 3C286 | 11.65 |
| 3C295 | 14.64 |
Gain = Tant/Sstandard is plotted on Figure 4.
Figure 4: noncorrected gain curve
A second order polynomial was least-square-fitted to the data.
The maximum value of the gain was taken as the DPFU.
Resulted gain curve as a function of the zenith distance (ZD=90-Elev, deg.)
has the following form:
Gain[LCP,RCP] = DPFU[LCP,RCP] * (A0 + A1 * ZD + A2 * ZD^2).
The fitted parameters for not corrected gain are as follows:
A0, A1, A2 = 0.97935, +1.1154e-3, -1.7833e-05
| Parameter | Fit to LCP data | Fit to RCP data |
| DPFU | 1.91 K/Jy | 1.75 K/Jy |
| Mean gain for elev. 20-87 deg. | 1.89 K/Jy | 1.73 K/Jy |
Figure 5: corrected for atmospheric absorption gain curve
A second order polynomial was least-square-fitted to the data.
The maximum value of the corrected gain was taken as the DPFU_corr.
Resulted gain curve as a function of the zenith distance (ZD=90-Elev, deg.)
has the following form:
Gain_corr[LCP,RCP] = DPFU_corr[LCP,RCP] * (A0_corr + A1_corr * ZD + A2_corr * ZD^2).
The fitted parameters for corrected gain are as follows:
(A0, A1, A2)_corr = 0.97423, +1.2704e-3, -1.7900e-5
| Parameter | Fit to LCP data | Fit to RCP data |
| DPFU_corr | 1.93 K/Jy | 1.75 K/Jy |
| Mean gain_corr for elev. 20-87 deg. | 1.91 K/Jy | 1.74 K/Jy |
The luck of low elevation data in this run calls for additional
gain curve measurements, when appropriate period of GBT
time will be available.
Efficiency Estimation
We have estimated the GBT efficiency, assuming that projected
geometrical GBT area is equal to 7853.98 m^2.
Error in the efficiency estimation is about 10% and
comes from the uncertanty of Tcal value.
Efficiency is plotted on Figure 4.
Figure 4: efficiency