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2023 Session I (c231)

Modified 12:38, 26 Apr 2023 by jwagner | Page History

    Version as of 10:34, 3 Jul 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
    • Draft schedules v3: https://cloud.mpifr-bonn.mpg.de/index.php/s/J6SYRbxWJ8zMRF2

    Recording media

     

    Station obs time [hr] Required [TB] Media Capacity Status (Nov 2022)
    PT 97 + 11.5 99 MPI%8007 80  
    NL 97 + 11.5 99 MPI%8008 80  
    OV 97 + 11.5 99 MPI%8015 80  
    MK 67 + 11.5 72 MPI%8019 80  
    BR 90 + 11.5 92 MPI%8021 80  
    FD 97 + 11.5 99 MPI%8028 80  
    LA 97 + 11.5 99 MPI%8029 80  
    KP 97 + 11.5 99 MPI%8026 80  
    HN 11.5 11 MPIH%016 48  
    SC 11.5 11 MPIH%017 48  
    GB 54 49      
    NOEMA 83.5 73 MPI%8022 MPI%8023 2 x 80  
    ALMA 55        
    EF 83.5 76 e-transfer    
    YS 83.5 76 e-transfer    
    MH 83.5 76 e-transfer    
    ON 83.5 76 e-transfer    
    KVN 53 / station 48 / station e-transfer    
    LMT 65 < 59*      
    ATCA 39.5        
    MOPRA 39.5 36      
    GLT 87 79      
    Haystack 3.5 3      

    Notes:

    Assuming 50% duty cyle for all stations

    * LMT: based on 65 hours as indicated by the schedule, but LMT can only observe at night time. Requirements will be less


    Preliminary pool:

    128: 10

    112: 10

    80: 6

    64: 8

    48: 1

    32: 1