Version as of 10:23, 23 Nov 2024

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    C241A Correlation Report

    General information

    • Session info: http://www3.mpifr-bonn.mpg.de/div/vlbi/globalmm/
    • Station feedback: Gl late due to storm (https://docs.google.com/spreadsheets...gid=1941489491), bad weather at Pv in the beginning and at Ef, Ys lost scans 0376, 0377, Mh was offline 2024-04-19 1228 to 1400 UTC,  c241a was observed from 109-22:00 to 110-06:50 UT, 110-10:00 to 110-10:37 UT. Nn did not observe due to storm in the beginning, then due to a cabling error, we were on the "regular" 3mm band R&S SMA 100A synthesizer that was referenced to the maser (it should have sufficient quality for VLBI, however). We switched to the VLBI specific R&S SMA 100B just before starting c241b, and the following observations of c241b and c241c were done with it, Aa good, no KT

    Status

    what date
    started e-transfer for PV(2/2), Ys, On, Mh, sent email to KVN/Mp (awaiting start), Ef done 22.04.2024
    Fringes between Pv, On, Ys, Ef, Mh, sync error for Mh and probably Ys (missing frames) but only in the first few scans? 24.04.2024
    KVN data transfer started (complete), At & Mp still missing, but contacted via email to check 26.04.2024
    GLT, AA on the way, JCMT not yet 12.06.2024
    AA arrived, to be scanned in, JCMT is halfway through the data transfer, JCMT done 05.07.2024
    GLT arrived, filelist done, looking for fringe done 21.08.2024
    Correlation commenced, test run through, comments below 22.08.2024

    Fringes

    Station Fringes Plots Comments
    Ef y    
    Nn y    
    Pv y    
    Ys y    
    Mh y    
    On y    
    Gl      
    KVN (3) y    
    VLBA(8) y (FD & MK have fringes in B part)    

    Notes

     

    From test run: KVN_PC has a significant delay, due to the double peak problem, KVN has a big delay rate offset w.r.t. to LA. fixed.

    Post-Correlation checks

    Residuals

    FITS completeness (pclist)