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lbaops:lbajun2007:v211b
Table of Contents
v211b Setup:
| Description | VLBI observations of Infrared-Faint Radio Sources |
|---|---|
| Antennas | Pa-At-Mp-Ho-Cd |
| Start | 172 15:00:00 |
| Stop | 173 03:01:00 |
| PI | Enno Middelberg |
| Channel 1 | DAS #1 IFP#1-LO 1352 - 1368 MHz USB RCP |
| Channel 2 | DAS #1 IFP#1-HI 1368 - 1384 MHz USB RCP |
| Channel 3 | DAS #1 IFP#2-LO 1352 - 1368 MHz USB LCP |
| Channel 4 | DAS #1 IFP#2-HI 1368 - 1384 MHz USB LCP |
| Channel 5 | DAS #2 IFP#1-LO 1384 - 1400 MHz USB RCP |
| Channel 6 | DAS #2 IFP#1-HI 1400 - 1416 MHz USB RCP |
| Channel 7 | DAS #2 IFP#2-LO 1384 - 1400 MHz USB LCP |
| Channel 8 | DAS #2 IFP#2-HI 1400 - 1416 MHz USB LCP |
| DAS 1 Skyfreq | 1368.00 MHz |
| DAS 2 Skyfreq | 1400.00 MHz |
| Bandwidth | 16 MHz |
| DAS Mode | vsop.pro (telescope) |
Ftp: ftp://ftp.atnf.csiro.au/pub/people/vlbi/v211/v211b
Comments:
Frequencies have changed from original (CJP 21 June 13:00 UT)
Please note disks recorded in observatory links below
Parkes, Mopra, ATCA
- Connect DAS to VSIC using “Huygens” Cable
- Both DAS units are used to give 2 x 256 Mbps = 512 Mbps recording over 8 x 16 MHz channels
Hobart, Ceduna
- Connect DAS directly to VSIC
- One DAS unit is used to give 1 x 256 Mbps recording over 4 x 16 MHz channels.
- Recorded data will match the frequencies/polarisations listed in the table for DAS2.
Observing comments for each antenna:
Observing Logs
lbaops/lbajun2007/v211b.txt · Last modified: 2015/12/18 16:38 by 127.0.0.1
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