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The correlator has 8 independent units, which can be placed
anywhere in the 100-680 MHz band. 7 different modes of configuration
are available, characterized in the following by couples of total
bandwidth/number of channels. In the 3 DSB modes (320MHz/128,
160MHz/256, 80MHz/512 - see Table) the two central channels may be
perturbed by the Gibbs phenomenon if the observed source has a strong
continuum. When using these modes, it is recommended to avoid
centering the most important part of the lines in the middle of the
band of the correlator unit. In the remaining SSB modes (160MHz/128,
80MHz/256, 40MHz/512, 20MHz/512) the two central channels are not
affected by the Gibbs phenomenon and, therefore, these modes may be
preferable for some spectroscopic studies.
Should the NGRx become available, the spectral configuration will be
adjusted with consultation of the principal investigators.
Spacing |
Channels |
Bandwidth |
Mode |
(MHz) |
|
(MHz) |
|
0.039 |
|
20 |
SSB |
0.078 |
|
40 |
SSB |
0.156 |
|
80 |
DSB |
0.312 |
|
80 |
SSB |
0.625 |
|
160 |
DSB |
1.250 |
|
160 |
SSB |
2.500 |
|
320 |
DSB |
Note that 5% of the passband is lost at each end of a
subband. The 8 units can be independently connected either with the
3mm or 1.3mm IFs.
Next: Sun Avoidance
Up: Call for Observing Proposals
Previous: Coordinates and Velocities
Clemens Thum
2006-07-07