v235a Setup:
| Description | The search for superluminal motion in the nearby proto-quasar candidate |
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| Antennas | At-Mp-Pa-Ho-Cd-Ti-Hh |
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| Start | 174 06:00:00 |
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| Stop | 174 18:00:00 |
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| PI | Morganti |
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| Channel 1 | DAS #1 IFP#1-LO 2268 - 2284 MHz USB RCP |
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| Channel 2 | DAS #1 IFP#1-HI 2284 - 2300 MHz USB RCP |
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| Channel 3 | DAS #1 IFP#2-LO 2268 - 2284 MHz USB LCP |
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| Channel 4 | DAS #1 IFP#2-HI 2284 - 2300 MHz USB LCP |
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| Channel 5 | DAS #2 IFP#1-LO 2300 - 2316 MHz USB RCP |
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| Channel 6 | DAS #2 IFP#1-HI 2316 - 2332 MHz USB RCP |
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| Channel 7 | DAS #2 IFP#2-LO 2300 - 2316 MHz USB LCP |
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| Channel 8 | DAS #2 IFP#2-HI 2316 - 2332 MHz USB LCP |
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| DAS 1 Skyfreq | 2284.00 MHz |
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| DAS 2 Skyfreq | 2316.00 MHz |
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| Bandwidth | 16 MHz |
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| DAS Mode | vsop.pro (telescope) |
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Ftp: ftp://ftp.atnf.csiro.au/pub/people/vlbi/v235/v235a
Comments:
Schedule has changed from original (CJP 20 June 08:00 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 DAS1.
Tibinbilla
- Connect DAS directly to VSIC
- One DAS unit is used to give 1 x 256 Mbps recording over 4 x 16 MHz channels.
- Record frequencies listed at RCP for both DAS1 and DAS2 in the table above.
Tibdinbilla uses a different setup compared to Hobart and Ceduna
Hart
Vex schedule assume you will record all 8 channels
Observing comments for each antenna:
Observing Logs
Parkes onsource flagging
Mopra onsource flagging
