Source name      : J1800+78  
  Observation type : Continuum  
  Frequencies      :  1634.00   1650.00 
  Correlator       : Socorro    
  UTC range        : 319:10:00 to 319:18:00  
  Start date       : Thu,2001-Nov-15  
  Length (hrs)     :  8.00   
  No. of GRTs      : 11  
  Note             :     
 
 Scheduled duration of data recording at each Ground Radio Telescope. 
 (Note: there is one line per GRT per tape (or tape set). 
 There may be gaps during which no data is recorded) 
 
        SC : 2001:319:10:00:00 to 2001:319:18:00:00    (VLBA)   
        HN : 2001:319:10:00:00 to 2001:319:18:00:00    (VLBA)   
        NL : 2001:319:10:00:00 to 2001:319:18:00:00    (VLBA)   
        FD : 2001:319:10:00:00 to 2001:319:18:00:00    (VLBA)   
        LA : 2001:319:10:00:00 to 2001:319:18:00:00    (VLBA)   
        PT : 2001:319:10:00:00 to 2001:319:18:00:00    (VLBA)   
        KP : 2001:319:10:00:00 to 2001:319:18:00:00    (VLBA)   
        OV : 2001:319:10:00:00 to 2001:319:18:00:00    (VLBA)   
        BR : 2001:319:10:00:00 to 2001:319:18:00:00    (VLBA)   
        MK : 2001:319:10:00:00 to 2001:319:18:00:00    (VLBA)   
        UD : 2001:319:10:00:00 to 2001:319:14:30:00    (VSOP)   
 
 Scheduled duration of data recording at each Tracking Station 
 
        UZ : 2001:319:12:28:44 to 2001:319:13:58:24    (VLBA)  
 

Nominal, as-scheduled, (u,v) coverage for this observation


 Apogee and perigee passes 

             2001:319:11:56:00      PERIGEE
             2001:319:15:05:00       APOGEE
 


Merger details :
Data share details :
KSP details :
Correlator release date :
This page last modified : 18-apr-2006

Explanation of telescope and tracking station codes Look for observation and calibration files on the VLBA web site
here (http://www.vlba.nrao.edu/astro/VOBS/astronomy/nov01/w503a).
Also check for the correlator release letter to the PI,
which may be archived in the sniffer directory with a name like
this (http://www.vlba.nrao.edu/astro/VOBS/astronomy/nov01/w503a/sniffer/W503A.20011115.sniff.gz.

Explanation of VSOP observation codes

Please let us know if any of the information on this page is wrong!