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lbaops:lbanov2006:v190e
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Table of Contents
v190e Setup:\\
| Description | 3 cm disk-based pulsar astrometry |
|---|---|
| Antennas | At-Mp-Pa-Ho-Cd-Ti |
| Start | 320 09:00:00 |
| Stop | 320 21:00:00 |
| PI | Adam Deller |
| Channel 1 | DAS #1 IFP#1-LO 8409 - 8425 MHz USB RCP |
| Channel 2 | DAS #1 IFP#1-HI 8425 - 8441 MHz USB RCP |
| Channel 3 | DAS #1 IFP#2-LO 8409 - 8425 MHz USB LCP |
| Channel 4 | DAS #1 IFP#2-HI 8425 - 8441 MHz USB LCP |
| Channel 5 | DAS #2 IFP#1-LO 8441 - 8457 MHz USB RCP |
| Channel 6 | DAS #2 IFP#1-HI 8457 - 8473 MHz USB RCP |
| Channel 7 | DAS #2 IFP#2-LO 8441 - 8457 MHz USB LCP |
| Channel 8 | DAS #2 IFP#2-HI 8457 - 8473 MHz USB LCP |
| DAS 1 Skyfreq | 8425.00 |
| DAS 2 Skyfreq | 8457.00 |
| Bandwidth | 16 MHz |
| Recorder | Disk |
| DAS Mode | vsop.pro (telescope) |
Comments:\\
'This is a disk based experiment. Do NOT delete the data after recording!!!!
Disk allocations for each telescope are listed under the telescope specific notes, linked to below.
ATCA, Mopra, Parkes will use the “Huygens cable”. Hobart, Tidbinbilla, and Ceduna will use the standard flat cable, no jumper.\
\
Observing comments for each antenna:\\
lbaops/lbanov2006/v190e.1163109194.txt.gz · Last modified: 2015/12/18 16:38 (external edit)
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