Table 1 gives the surveyed geographic locations
of the 10 antennas comprising the VLBA, plus the 2-character codes
used to identify the antennas (Napier 1995). The antennas are ordered
East through West. All locations are based on the WGS84 ellipsoid
used by the GPS system1,
with Earth radius
km and flattening
.
See Napier (1995) for further site information.
| North | West | |||
| Latitude | Longitude | Elevation | Code | |
| Location | [
|
[
|
[m] | |
| Saint Croix, VI | 17:45:23.68 | 64:35:01.07 | 16 | SC |
| Hancock, NH | 42:56:00.99 | 71:59:11.69 | 296 | HN |
| North Liberty, IA | 41:46:17.13 | 91:34:26.88 | 222 | NL |
| Fort Davis, TX | 30:38:06.11 | 103:56:41.34 | 1606 | FD |
| Los Alamos, NM | 35:46:30.45 | 106:14:44.15 | 1962 | LA |
| Pie Town, NM | 34:18:03.61 | 108:07:09.06 | 2365 | PT |
| Kitt Peak, AZ | 31:57:22.70 | 111:36:44.72 | 1902 | KP |
| Owens Valley, CA | 37:13:53.95 | 118:16:37.37 | 1196 | OV |
| Brewster, WA | 48:07:52.42 | 119:40:59.80 | 250 | BR |
| Mauna Kea, HI | 19:48:04.97 | 155:27:19.81 | 3763 | MK |
Several other radio telescopes often participate in VLBI observing in conjunction with the VLBA. These include the Very Large Array (VLA), either with up to 27 antennas added in phase (Y27) or with a single antenna (Y1); the Green Bank Telescope (GBT); Arecibo; Effelsberg; the European VLBI Network (EVN); plus (occasionally) various geodetic antennas or the NASA Deep Space Network. For details on how to propose for these extra telescopes, see Section 21.1.
A total of up to 100 hours per four-month trimester has
been reserved for a High Sensitivity Array (HSA) composed of the
VLBA, Y27, GBT, Arecibo, and Effelsberg; the HSA is described at
http://www.nrao.edu/HSA/ . In this context, users should be aware
that Arecibo only operates at frequencies up to 10 GHz, and can view
sources only within about
of its zenith; see
http://www.naic.edu for further information about Arecibo's
properties. The VLA and GBT are NRAO facilities, while Arecibo is
operated by the National Astronomy and Ionosphere Center, and
Effelsberg is operated by Germany's Max Planck Institut für
Radioastronomie (MPIfR). Table 2 lists the locations of
the HSA telescopes.