This shows you the differences between two versions of the page.
Both sides previous revision Previous revision Next revision | Previous revision | ||
lbaops:lbajun2007:v210a [2007/06/13 12:22] chris.phillips |
lbaops:lbajun2007:v210a [2007/06/13 12:32] stingay |
||
---|---|---|---|
Line 1: | Line 1: | ||
- | ===== v210a Setup:\\\ ===== | + | ===== v210a Setup:\ ===== |
- | ^Description | + | ^Description |
- | ^Antennas | + | ^Antennas |
- | ^Start | + | ^Start |
- | ^Stop | 171 16: | + | ^Stop | 171 16: |
- | ^PI | Tingay |\\\ | + | ^PI | Tingay |\ |
- | ^Channel 1 | '' | + | ^Channel 1 | '' |
- | ^Channel 2 | '' | + | ^Channel 2 | '' |
- | ^Channel 3 | '' | + | ^Channel 3 | '' |
- | ^Channel 4 | '' | + | ^Channel 4 | '' |
- | ^Channel 5 | '' | + | ^Channel 5 | '' |
- | ^Channel 6 | '' | + | ^Channel 6 | '' |
- | ^Channel 7 | '' | + | ^Channel 7 | '' |
- | ^Channel 8 | '' | + | ^Channel 8 | '' |
- | ^DAS 1 Skyfreq | + | ^DAS 1 Skyfreq |
- | ^DAS 2 Skyfreq | + | ^DAS 2 Skyfreq |
- | ^Bandwidth | + | ^Bandwidth |
- | ^DAS Mode | vsop.pro ([[http:// | + | ^DAS Mode | vsop.pro ([[http:// |
- | \\\ | + | |
- | Ftp: [[ftp:// | + | |
- | ----\\\ | + | |
- | \\\ | + | |
- | ===== 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 Hobart, Ceduna, and Tidbinbilla, | + | |
\ | \ | ||
- | Details of disks to be used, disko setup, and telescope-specific comments appear under the links below.\\\ | + | Ftp: [[ftp:// |
- | \\\ | + | ----\ |
- | ===== Observing comments for each antenna:\\\ ===== | + | \ |
+ | ===== 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 Hobart, Ceduna, and Tidbinbilla, | ||
+ | \ | ||
+ | Details of disks to be used, disko setup, and telescope-specific comments appear under the links below.\ | ||
+ | \ | ||
+ | ===== Observing comments for each antenna:\ ===== | ||
- | | [[.: | + | | [[.: |
- | ----\\\ | + | ----\ |
- | ===== Observing Logs\\\ ===== | + | ===== Observing Logs\ ===== |
- | [[http:// | + | [[http:// |
- | [[http:// | + | [[http:// |