|
This is a 2-channel system for VLBI
observations.
| Frequency
[GHz] |
Channel |
Polarisation |
Tcal [K] |
Tsys [K] |
Sensitivity [K/Jy] |
SEFD [Jy] |
Aperture Eff. [%] |
TMB/S [K/Jy] |
Main Beam Eff. [%] |
FWHM [arcsec] |
Last update |
| 21.73 |
A |
LCP |
5.1 |
78 |
0.90 |
96 |
28 |
1.8 |
47 |
36.5 |
Jul 2007 |
| 21.73 |
B |
RCP |
4.9 |
84 |
0.90 |
105 |
28 |
1.8 |
47 |
36.4 |
Jul 2007 |
| 22.23 |
A |
LCP |
5.0 |
91 |
0.9 |
110 |
30 |
1.8 |
47 |
36.5 |
Jul 2008 |
| 22.23 |
B |
RCP |
5.0 |
88 |
0.9 |
105 |
30 |
1.8 |
47 |
36.5 |
Jul 2008 |
| 23.05 |
A |
LCP |
3.4 |
83 |
0.9 |
97 |
30 |
1.8 |
48 |
36 |
Jul 2008 |
| 23.05 |
B |
RCP |
3.7 |
70 |
0.9 |
91 |
30 |
1.8 |
47 |
36 |
Jul 2008 |
|
normalized Gain curve
(G = A0 + A1·Elv + A2·Elv2)
|
Observed in |
|
A0 = 0.95282 A1 = 3.6092E-3
A2 = -6.8913E-5 |
Mar 2003 |
|
A0 = 0.91119
A1 = 4.7557E-3
A2 = -6.2902E-5 |
Feb 2007 |
Comments:
- Note that the system temperature at this frequency depends
strongly on weather conditions!
- The new gain curve (Feb 2007) was corrected for opacity. Because of the
previous point it is always recommended to correct data at 1.3cm for
opacity.
- Typical zenith tau values range from 0.05 to 0.2. An option might be
also the use of data from the
water-vapour radiometer.
|