User Tools

Site Tools



This shows you the differences between two versions of the page.

Link to this comparison view

Both sides previous revision Previous revision
Next revision
Previous revision
lbaops:lbaapr2009:vt12iholog [2009/03/27 09:14]
lbaops:lbaapr2009:vt12iholog [2015/12/18 16:38] (current)
Line 1: Line 1:
-This was the set up we used on day 085, March 25th: \\ 
-Agilent LO 10.5 \\ 
-smy 808 MHz \\ 
-DAS profile: ho16x2_n \\ 
-VSIB to DAS S2 rec out: Direct cable \\ 
-te093ho.snp and te093ho.prc were the drudg generated the test schedule files. \\ 
-Fringes to Mopra and data streamed OK to JIVE \\ 
-eVLBI fringes during Chris'​s correlation,​ url as follows: \\ 
-http://​​lba-live/​lba-0-f0-p0.html \\ 
-and \\ 
-http://​​lba-live/​lba-0-f0-p1.html \\ 
-The DAS profile has some LSB channels and as a result you need to allow for this when working out where the 5 MHz coherence tone should be. \\ 
-In this case the 2 coherence tones are 4951 and 4961. The sky frequency is 4956. \\ 
-regards, Brett. 27/3/09 
lbaops/lbaapr2009/vt12iholog.txt · Last modified: 2015/12/18 16:38 (external edit)