C | Gregorian C(3.95 to 5.85 GHz) |
K | Gregorian K(18.0 to 26.5 GHz) |
B | Gregorian Ka B(26.0 to 40.0 GHz) |
U | Gregorian Ku U(12.4 to 15.4 GHz) |
L | Gregorian L(1.15 to 1.73 GHz) |
Q | Gregorian Q(40.0 to 50.0 GHz) |
S | Gregorian S(1.73 to 2.6 GHz) |
X | Gregorian X(8.2 to 10.0 GHz) |
3 | Prime Focus 1-1 3(0.29 to 0.395 GHz) |
4 | Prime Focus 1-2 4(0.385 to 0.520 GHz) |
6 | Prime Focus 1-3 6(0.51 to 0.69 GHz) |
8 | Prime Focus 1-4 8(0.68 to 0.92 GHz) |
A | Prime Focus 2 A(0.91 to 1.23 GHz) |
B | Berkley Caltech Pulsar Machine |
R | Caltech-Green Bank-Swinbourne Recorder 2 |
C | Coherent Green Bank-Berkley Pulsar Processor |
D | GBT Digital Continuum Receiver |
S | GBT Spectrometer |
2 | S2 recorder |
P | Spectral Processor |
G | Spectrometer Pulsar Spigot Mode |
O | User supplied or new backend |
V | VLBA recorder and DAR |
A | Astronomy |
M | Maintenance |
T | Tests |
D | Shutdown |
K | Calibration |
C | Commissioning |
N | Notscheduled |
S | Setup |