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lbaops:lbaapr2009:vt11rholog

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://www.evlbi.atnf.csiro.au/lba-live/lba-0-f0-p0.html
and
http://www.evlbi.atnf.csiro.au/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/vt11rholog.txt · Last modified: 2015/12/18 16:38 (external edit)