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2023 Session I (c231)

Modified 09:49, 3 May 2023 by jwagner | Page History

    Version as of 16:10, 21 Nov 2024

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    		 Sources DOYS UT Freq Stations Status PI Comment
                       
                       
                       
                       

    General comments

    • ALMA scheduled, will have 3 MHz frequency offset
    • LMT runs off Oscilloquartz xtal without H-maser/Rb
    • LMT is linear polarized, has a feed rotator active during calibration scans that ought to return to 'origin' for VLBI scans avoiding any per-scan instrumental polarization angle offsets
    • MOPRA is linear polarized
    • TAMNA is not observing due to broken maser
    • Draft schedules: https://cloud.mpifr-bonn.mpg.de/index.php/s/J6SYRbxWJ8zMRF2

    Recording media

    See the media distribution plan