TJAN24

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    Combined revision comparison

    Comparing version 12:39, 12 Feb 2020 by jwagner with version 12:44, 12 Feb 2020 by jwagner.

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    • Fringe test between PV and NOEMA at 3mm
    • Done with the EHT setup 4x2GHz dual-pol
    • PV with 2-of-4 x R2DBE and 1 x DBBC3; on sky demonstration of DBBC3 GMVA fringes
    • PV had poor IF bandpass equalization, and e.g., scan No0028 SNR~450 over 2x512MHz improves to SNR~630 with 32x64MHz zooms NOEMA had low optical power in parts of Rx LSB

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    Version from 12:39, 12 Feb 2020

    This revision modified by jwagner (Ban)

    ...

    • Fringe test between PV and NOEMA at 3mm
    • Done with the EHT setup 4x2GHz dual-pol
    • PV with 2-of-4 x R2DBE and 1 x DBBC3; on sky demonstration of DBBC3 GMVA fringes
    • PV poor IF bandpass equalization, e.g., scan No0028 SNR~450 over 2x512MHz improves to SNR~630 with 32x64MHz zooms
    • NOEMA had low optical power in parts of Rx LSB

    ...

    Version as of 12:44, 12 Feb 2020

    This revision modified by jwagner (Ban)

    ...

    • Fringe test between PV and NOEMA at 3mm
    • Done with the EHT setup 4x2GHz dual-pol
    • PV with 2-of-4 x R2DBE and 1 x DBBC3; on sky demonstration of DBBC3 GMVA fringes
    • PV had poor IF bandpass equalization, and NOEMA had low optical power in parts of Rx LSB

    ...