|
This system can be used for sensitive continuum,
spectroscopy, and pulsar observations. Additionally, it will
be employed in search-programs for space-debris. Be
aware, that this band may be influenced by RFI.
The central horn has two circular polarizations, each of the outer
six horns two linear polarizations.
| 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 |
| 1.400 |
A |
LCP |
4.5 |
25 |
1.5 |
17 |
54 |
2.0 |
75 |
~550 |
2007 |
|
normalized Gain curve
(G = A0 + A1·Elv + A2·Elv2)
|
Observed in |
|
A0 = 1.0 A1 = 0.0
A2 = 0.0 |
|
Comments:
- Extensive tests are planned for summer 2008.
|