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2017 Mar (c171)

Modified 13:58, 8 Aug 2017 by alef | Page History
    Table of contents
    1. 1. Correlation Status March 2017

    Version as of 04:50, 25 Nov 2024

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    Correlation Status March 2017

     

    Project

    Code

    Block

    Code

    Sources

    DOYS

    UT

    Frq

    Stations

    Status

    PI

    Comment
    MN001 C171A 3C84 89-90 8:30-1:30 86 Eb,Yb,On,Mh,KVN,GB,VLBA Correlated, quality check Nagai  
    MA009   M87 89-90 22-13 86 Eb,Yb,On,Mh,Pv,KVN,GB,VLBA Correlated, quality check Asada  
    MB005 C171B NGC1052 90 9:30-24 86 Eb,Yb,On,Mh,Pv,GB,VLBA,Nt(7mm) Correlated quality check Baczko  
    MM07B C171C Fermi sources 90-92 19-18:20 86 Eb,Yb,On,Mh,Pv,KVN,GB,VLBA Correlated quality check Marscher  
    MG002 - OJ287 92-93 17:20-07 86 Eb,Yb,On,Mh,Pv,Aa,VLBA Pass1 correlation done Gomez ALMA mode
    MB007 - Sgr* 93 03-15:20 86 Eb,Yb,Pv,GB,Aa,VLBA Pass1 correlation done Brinkerink ALMA mode
    MA008 - 3C273 93-94 19-11 86 Eb,Yb,Pv,On,Mh,Aa,VLBA Correlating Akiyama ALMA mode

     

    General comments:

    Whole session:

    • Ys has (as usual) observed  LCP only
    • Pt has fringes only in parts of the experiment and only to a few stations

    ALMA-mode:

    • MH no fringes. Strange AC indicating error in setup of firmware. MH has a rare DBBC setup.
    • Pv: used 32 MHz PFB by mistake. Not included in first run with 58 MHz sub-bands.
    • Ys fringes in MB007. Seems to have used 32 MHz PFB in other 2 observations.
    • ALMA: first time with GMVA and good fringes