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--- lbaops:lbadec2009:vt10i [2005/04/07 08:23]
Unknown
+++ lbaops:lbadec2009:vt10i [2009/12/09 15:20]
cehotan
@@ Line 10: / Line 10: @@
 ^Station Modes                 | Cd Ho |
-^Channel 1          | ''  IFP#1 4808 - 4824 MHz USB RCP'' |
+^Channel 1          | ''  IFP#1 4784 - 4848 MHz USB RCP'' |
-^Channel 2          | ''  IFP#2 4808 - 4824 MHz USB LCP'' |
+^Channel 2          | ''  IFP#2 4784 - 4848 MHz USB LCP'' |
-^DAS 1 Skyfreq      | 4824  MHz |
+^DAS 1 Skyfreq      | 4816 MHz |
-^Bandwidth          | 16 MHz         |
+^Bandwidth          | 64 MHz |
-^DAS Mode           | vsop.pro ([[http://www.atnf.csiro.au/vlbi/dasmodes/16-2IF-1p-c.html|telescope]]) |
+^DAS Mode           | 64MHZ_N.pro |
 Ftp: [[ftp://ftp.atnf.csiro.au/pub/people/vlbi/vt10/vt10i]]
@@ Line 21: / Line 21: @@
 ===== Comments: =====
-Cd Ho: Note the use of the dual sideband vsop profile. Only the lower sideband should be selected for transfer.
+This is a 64 MHz bandwidth experiment. Please make sure that the BG3 cable is used to connect the DAS to the VSIC. The setup has been made similar to other 4.8 GHz experiments during this run to minimise the need for configuration changes. Please contact Aidan or Bruce at Ceduna if there are any questions about the setup.
+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: =====

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