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lbaops:lbaoct2010:v316d
Table of Contents
v316d
| Description | Methanol Maser Proper Motion Measurement of the LMC |
|---|---|
| Antennas | At-Cd-Ho-Mp-Pa-Hh |
| Start | 299 12:30:00 |
| Stop | 299 23:00:00 |
| PI | A.J. Beasley |
Setup v316d.5cm: nif=2
| Station Modes | At Cd Ho Mp Pa |
|---|---|
| Channel 1 | IFP#1-LO 6642 - 6658 MHz USB RCP |
| Channel 2 | IFP#1-HI 6658 - 6674 MHz USB RCP |
| Channel 3 | IFP#2-LO 6642 - 6658 MHz USB LCP |
| Channel 4 | IFP#2-HI 6658 - 6674 MHz USB LCP |
| DAS 1 Skyfreq | 6658 MHz |
| Bandwidth | 16 MHz |
| DAS Mode | vsop.pro (telescope) |
Ftp: ftp://ftp.atnf.csiro.au/pub/people/vlbi/v316/v316d
The frequency setup is the same as for the maser observation sections of the v255 experiments.
Break down of the schedule
1230 - 1245 : Fringe finder 0208-512 1245 - 1901 : Target sources (also one fringe finder at 1755 UT for 15 min) 1901 - 1913 : Fringe finder 0208-512 (Hart joins experiment) 1913 - 2249 : Target sources 2249 - 2300 : Fringe finder 0637-752
Once Hart joins the experiment there are 30 second gaps in the schedule every 15-20 minutes to keep the Mark IV/V system happy. This will have no effect on the LBA telescopes.
Comments:
Observing comments for each antenna:
Observing Logs
Parkes onsource flagging
ATCA onsource flagging
Mopra onsource flagging
Mopra Tsys
(plot)
Parkes Tsys
Weather
lbaops/lbaoct2010/v316d.txt ۤ Last modified: 2015/12/18 16:38 (external edit)
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