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lbaops:lbajun2008:v209c
Table of Contents
v209c Setup:
| Description | 13 cm imaging of NGC 253 |
|---|---|
| Antennas | At-Mp-Pa-Ho-Cd-Ti |
| Start | 157 16:00:00 |
| Stop | 158 02:00:00 |
| PI | Emil Lenc |
| Channel 1 | DAS #1 IFP#1-LO 2226 - 2242 MHz USB RCP |
| Channel 2 | DAS #1 IFP#1-HI 2242 - 2258 MHz USB RCP |
| Channel 3 | DAS #1 IFP#2-LO 2226 - 2242 MHz USB LCP |
| Channel 4 | DAS #1 IFP#2-HI 2242 - 2258 MHz USB LCP |
| Channel 5 | DAS #2 IFP#1-LO 2258 - 2274 MHz USB RCP |
| Channel 6 | DAS #2 IFP#1-HI 2274 - 2290 MHz USB RCP |
| Channel 7 | DAS #2 IFP#2-LO 2258 - 2274 MHz USB LCP |
| Channel 8 | DAS #2 IFP#2-HI 2274 - 2290 MHz USB LCP |
| DAS 1 Skyfreq | 2242.00 MHz |
| DAS 2 Skyfreq | 2274.00 MHz |
| Bandwidth | 16 MHz |
| DAS Mode | vsop.pro (telescope) |
Ftp: ftp://ftp.atnf.csiro.au/pub/people/vlbi/v209/v209c
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 Tidbinbilla, Hobart and Ceduna, one DAS unit is used to give 1 x 256 Mbps recording over 4 x 16 MHz channels. These channels will match the frequencies listed at RCP for both DAS1 and DAS2 in the table above.
Details of disks to be used, disko setup, and telescope-specific comments appear under the links below.
Observing comments for each antenna:
Observing Logs
lbaops/lbajun2008/v209c.txt · Last modified: 2015/12/18 16:38 by 127.0.0.1
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