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lbaops:lbamar2007:v209a
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v209a Setup:
| Description | 13 cm imaging of NGC 4945 |
|---|---|
| Antennas | At-Mp-Pa-Ho-Cd-Ti |
| Start | 80 09:00:00 |
| Stop | 80 20:59:00 |
| PI | Emil Lenc |
| Channel 1 | DAS #1 IFP#1-LO 2269 - 2285 MHz USB RCP |
| Channel 2 | DAS #1 IFP#1-HI 2285 - 2301 MHz USB RCP |
| Channel 3 | DAS #1 IFP#2-LO 2269 - 2285 MHz USB LCP |
| Channel 4 | DAS #1 IFP#2-HI 2285 - 2301 MHz USB LCP |
| Channel 5 | DAS #2 IFP#1-LO 2301 - 2317 MHz USB RCP |
| Channel 6 | DAS #2 IFP#1-HI 2317 - 2333 MHz USB RCP |
| Channel 7 | DAS #2 IFP#2-LO 2301 - 2317 MHz USB LCP |
| Channel 8 | DAS #2 IFP#2-HI 2317 - 2333 MHz USB LCP |
| DAS 1 Skyfreq | 2285.00 |
| DAS 2 Skyfreq | 2317.00 |
| Bandwidth | 16 MHz |
| Recorder | Disk |
| DAS Mode | vsop.pro (telescope) |
Ftp: ftp://ftp.atnf.csiro.au/pub/people/vlbi/v209/v209a
Comments:
This is a disk based experiment. Do NOT delete the data after recording!!!!
Connect DAS directly to VSIC
At the ATCA, Mopra, and Parkes, both DAS units are used to give 2 x 256 Mbps = 512 Mbps recording over 8 x 16 MHz channels, using the Huygens cable.
At Hobart, Ceduna, and Tidbinbilla, one DAS unit is used to give 1 x 256 Mbps recording over 4 x 16 MHz channels.
Details of disks to be used, disko setup, and telescope-specific comments appear under the links below.
Read these instructions in conjunction with the disk usage plans that were sent out to each telescope for far more information.
Observing comments for each antenna:
Observing Logs
lbaops/lbamar2007/v209a.txt · Last modified: 2015/12/18 16:38 by 127.0.0.1
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