Table 1.
Stations.
Name | Station | Diameter | SEFD( † ) |
---|---|---|---|
code | (m) | (Jy) | |
VLBA-Brewster | BR | 25 | 361 |
Effelsberg | EF | 100 | 19 |
VLBA-Fort Davis | FD | 25 | 327 |
Green Bank Telescope | GB | 100 | 9( † †) |
Hartebeesthoek | HH | 26 | 485 |
VLBA-Hancock | HN | 25 | 470 |
Irbene | IR | 32 | 1911( † †) |
Jodrell Bank | JB | 25 | 82 |
VLBA-Kitt Peak | KP | 25 | 489 |
VLBA-Los Alamos | LA | 25 | 648 |
Medicina | MC | 32 | 880 |
VLBA-Mauna Kea | MK | 25 | 445 |
VLBA-North Liberty | NL | 25 | 422 |
VLBA-Owens Valley | OV | 25 | 423 |
VLBA-Pie Town | PT | 25 | 397 |
Spektr – R | RA( ‡ ) | 10 | 2818 |
Robledo | RO | 70 | –( ‡ ‡) |
VLBA-Saint Croix | SC | 25 | 318 |
Torun | TR | 32 | 760 |
Westerbork | WB | 25 | 443 |
Notes. ( † )The values are calculated from the averaged system temperature, characteristic gain curve and the effective aperture size. ( ‡ )In the data, this is labeled as R1 and R2 for each of the two Earth-based sub-arrays. ( † †)These are estimated from RCP-only (see Sect. 2.2), while the others are averaged across dual polarization. ( ‡ ‡)No system temperature measurements.
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