Additional Info on CARMA
A.J. Beasley 7/22/2002
Sensitivity
Continuum Sensitivity (4 GHz BW, 2-pol) |
Angular Resolution & Line Sensitivity (1km/s channel, 1-pol) |
||||||||
Freq GHz |
1-min mJy |
5-hr mJy |
Config |
Beam “ |
1-min K |
5-hr K |
Beam “ |
1-min K |
5-hr K |
100 |
0.7 |
0.04 |
D |
6.3 |
0.4 |
0.02 |
2.7 |
0.7 |
0.04 |
230 |
2.2 |
0.1 |
C |
2.5 |
2.4 |
0.1 |
1.1 |
4.4 |
0.26 |
(345) |
12.0 |
0.7 |
B |
1.0 |
14.8 |
0.8 |
0.4 |
36 |
2.1 |
|
|
|
A |
0.4 |
92 |
5.3 |
0.2 |
144 |
8.4 |
Assumptions: Tsys ~80 K at 3mm, 140 K at 1 mm, 70 % efficiency, 6 10.4 m antennas + 9 6.1m antennas (i.e. no SZA).
Resolution/Configuration
CARMA will be a heterogeneous array, comprised of 3 antenna sizes: 10.4m antennas, nine 6.1m antennas and eight 3.5m antennas. CARMA will use 4 configurations (100m – 1500m) to span a range of angular scales from 0.2” to 30”. Addition of the SZA antennas (typically in a compact configuration < 100m in diameter) will enable imaging of angular scales up to 3’. The addition of more antennas will lead to higher-fidelity imaging and the ability to perform effective snapshot observations. Mosaicing observations will be standard.
Correlator Specifications
The CARMA first-light correlator will be a hardware extension of the FPGA-based COBRA correlator currently nearing completion at OVRO. The 4 GHz first-light bandwidth will be available as eight 500 MHz bands which can be tuned anywhere within the 4 GHz receiver band. Each of these 500 MHz bands can be channelized as indicated in the following table; multiple bands can be glued together to increase total velocity coverage.
Bandwidth (MHz) |
Channels |
3 mm channel spacing (km/s) |
3 mm velocity width (km/s) |
1 mm channel spacing (km/s) |
1 mm velocity
(km/s) |
|
|
|
|
|
|
512 |
16 |
96 |
1536 |
32 |
512 |
256 |
32 |
24 |
768 |
8 |
128 |
128 |
64 |
6 |
384 |
2 |
128 |
64 |
128 |
1.5 |
192 |
0.5 |
64 |
32 |
128 |
0.75 |
96 |
0.25 |
32 |
8 |
128 |
0.18 |
24 |
0.06 |
8 |
2 |
128 |
0.05 |
6 |
0.01 |
2 |
|
|
|
|
|
|