| Station | Diameter (m) | Zenith Tsys (K) | Gain (K/Jy) | Eta (%) | SEFD (Jy) |
|---|---|---|---|---|---|
| Effelsberg | 80.0 (eff.) |
130.0 | 0.140 | 7.7 | 929 |
| Plateau de Bure | 34.8 | 90.0 | 0.220 | 65 | 409 |
| Pico Veleta | 30.0 | 90.0 | 0.140 | 55 | 643 |
| VLBA | 25.0 | 100.0 | 0.034 | 19 | 2941 |
| Onsala | 20.0 | 300.0 | 0.049 | 43 | 6122 |
| Metsähovi | 14.0 | 300.0 | 0.017 | 30 | 17647 |
| - | Plateau de Bure | Pico Veleta | Onsala | Metsähovi | VLBA |
|---|---|---|---|---|---|
| Effelsberg | 69 |
86 |
265 |
450 |
184 |
| Plateau de Bure | - | 57 |
176 |
300 |
122 |
| Pico Veleta | - | - | 221 |
374 |
153 |
| Onsala | - | - | - | 1156 | 472 |
| Metsähovi | - | - | - | - | 801 |
| VLBA | - | - | - | - | 327 |
| Highest Baseline Sensitivity: | 57 mJy |
| |
|
| Array Sensitivity: | 21 mJy in 20 secs or 0.65 mJy in 12 hr adopting |
| (all European telescopes | a duty cycle (time on source/total time) of 0.5. |
| + 8 VLBA antennas) | These numbers have to be increased by a |
| |
factor of exp(tau*A) , i.e. for tau=0.1 |
| |
and airmass A= 1/sin (elv) = 2, the factor is 1.22 |
| Depending on weather conditions, the phase stability and atmospheric |
| coherence time can vary between ~10 seconds and ~200 seconds. |
| Assuming the following observing parameters: |
|
|
MKV/VLBA 512-8-2, single polarisation |
|
|
128.0 MHz (512 Mbit/s) |
|
|
20.0 sec (typical coherence time) |
|
|
7.*sigma |
|
|
2 Bit |
Useful formulae: |
|
B. Simulated uv-coverage for the Global 3mm-VLBI Array
1. uv-plot of a source with a declination of 70 degree 2. uv-plot of a source with a declination of 40 degree 3. uv-plot of a source with a declination of 0 degree |
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