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lbaops:lbadec2009:vt10i [2009/12/09 15:03]
cehotan
lbaops:lbadec2009:vt10i [2015/12/18 16:38] (current)
Line 7: Line 7:
 ^PI                 | Stansby | ^PI                 | Stansby |
  
-Setup lba6cm-2p-1IF:+Setup:
  
 ^Station Modes                 | Cd Ho | ^Station Modes                 | Cd Ho |
Line 13: Line 13:
 ^Channel 2          | '' ​ IFP#2 4784 - 4848 MHz USB LCP''​ | ^Channel 2          | '' ​ IFP#2 4784 - 4848 MHz USB LCP''​ |
 ^DAS 1 Skyfreq ​     | 4816 MHz | ^DAS 1 Skyfreq ​     | 4816 MHz |
-^Bandwidth ​         | 64 MHz         ​+^Bandwidth ​         | 64 MHz | 
-^DAS Mode           ​| ​64MHz_n.pro |+^DAS Mode           ​| ​64MHZ_N.pro |
  
 Ftp: [[ftp://​ftp.atnf.csiro.au/​pub/​people/​vlbi/​vt10/​vt10i]] Ftp: [[ftp://​ftp.atnf.csiro.au/​pub/​people/​vlbi/​vt10/​vt10i]]
Line 24: Line 24:
  
 Please note that this is NOT a fringe test, we need to keep the raw data and ship it back to Curtin. Please note that this is NOT a fringe test, we need to keep the raw data and ship it back to Curtin.
 +
 +Chris tells me that we cannot flip the 64 MHz band in the DAS. I think this means that the Hobart and Ceduna bands might be flipped with respect to each other, but we should be able to fix this during correlation. For reference, fauto shows that the Ceduna band is recorded with higher frequencies in smaller channel numbers.
  
 ===== Observing comments for each antenna: ===== ===== Observing comments for each antenna: =====
lbaops/lbadec2009/vt10i.txt · Last modified: 2015/12/18 16:38 (external edit)