mg002

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    Version as of 17:25, 3 Jul 2024

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    General:

    • This experiment contains ALMA with 32x62.5MHz channels sampled at 125MHz.
    • VLBA was recorded with 2x128MHz channels
    • DBBC2 statons were recording 1x512MHz wide channel
    • Pico and Yebes inadvertendly observed in 2-pol 16x32MHz PFB mode due to a feature incompleteness in new FieldSystem

    Fringes:


    Station Frimges Comment
    Ef yes no0093.pdf Effelsberg DBBC2
    Eb yes Effelsberg RDBE
    On yes no0093.pdf  
    Aa yes no0093.pdf  
    Mh yes Mh weak fringes in LCP to Onsala at beginning. Auto-correlations indicate errors
    Pv ? Auto-correlations indicate errors
    Ys ? Auto-correlations indicate errors
    Fd yes  
    La yes  
    Pt no  
    Nl yes  
    La yes  
    Kp yes  
    Ov yes  
    Br yes Fringes only to La/Mk/Ov
    1. Mh weak fringes in LCP to Onsala at beginning. Auto-correlations indicate errors in
    2. No fringes to Pt
    3. VLBA Fringes were found using the 2x128MHz mode.
    4. Frringes between ALMA and Eb (Effelsberg RDBE 2x128MHz): Aa-Eb.pdf . SNR for Aa-Eb much lower than for Aa-Ef. Needs to be investigated

    Notes:

    1. PV scan: /mnt/disks/4/7/data/ma008_PV_093-2145.vdif marked invalid by vdifuse
    2. PV: bad statistics before 092-2100 (OK after systems was restarted at Pico)
    3. PV: Autocorrelations show repeating strong features every 65 MHz. So far no fringes (PP-LCP.ps, PP-RCP.ps)
    4. YS: Autocorrelations show repeating strong features every 65 MHz. So far no fringes (larger clock-offset?) (YY-LCP.ps, YY-RCP.ps)
    5. MH: Autoccorelations look corrupted. Suspicous of 32 MHz sub-bands displayed as full band: So far no fringes, except for LCP (weak) in Scan No064. (MM-LCP.ps     MM-RCP.ps)
    6. VLBA: subintNS has to be choosen to be 640000 when adding in VLBA (and EB) having 128 MHz wide subbands. If run with the default settings an WARNING concerning "data gaps" is received and no data is being correlated.