  COVER INFORMATION 

 Station:    HART_S2   (Code Hh ) 
 Experiment: VSOP observation of  J1733-13  at 5  GHz
 Exp. Code:  w030e3  


Schedule Version:       1.00                                              
Processed by SCHED version: Release of 28 April 2000                      

PI:       S. Tingay                                                       

Address:  Australia Telescope National Facility                           
          Paul Wild Observatory                                           
          Narrabri, NSW 2390, Australia                                   
                                                                          

Phone:    +61 2 679 23245                                                 
EMAIL:    stingay@atnf.csiro.au                                           
Fax:      +61 2 679 04090                                                 
Phone during observation:                                                 

Observing mode: VSOP, 5  GHz continuum, 128-2-2                           

Notes:    Fringe finder :  1548+056                                       
                                                                          
                                                                          
                                                                          

Schedule for HART_S2   (Code Hh )                                   Page   2
               VSOP observation of  J1733-13  at 5  GHz
  UP:  D => Below limits;  H => Below horizon mask.  blank => Up.
  Early: Seconds between end of slew and start.   Dwell: On source seconds. 
  Tapes: Drive, Index, Start footage / Direction, Head Group, End footage.
  TPStart:  Tape motion start time.
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)
----------------------------------------------------------------------------------------

 --- Mon   5 Jun 2000   Day 157 ---

 Next scan frequencies:  4930.00  4946.00
 Next BBC frequencies:    144.00   160.00
 Next scan bandwidths:     16.00    16.00

17 00 00  J1733-13     11 48 27   9.1 100.2 -5.7    -114.6     0   1  1     52  17 00 00
17 15 00  ---          12 03 29  12.4  98.7 -5.5    -114.1   900   F  1    367

17 18 00  1548+056     12 06 30  27.3  68.3 -3.7    -122.9   176   1  1    422  17 18 00
17 28 00  ---          12 16 32  29.4  66.7 -3.6    -123.9   600   F  1    632

17 30 00  J1733-13     12 18 32  15.8  97.1 -5.2    -113.6   116   1  1    674  17 30 00
18 00 00  ---          12 48 37  22.5  94.1 -4.7    -112.9  1800   F  1   1304

18 00 00  J1733-13     12 48 37  22.5  94.1 -4.7    -112.9    -2   1  1   1304  18 00 00
19 00 00  ---          13 48 47  36.0  87.6 -3.7    -112.7  3598   F  1   2564

19 00 00  J1733-13     13 48 47  36.0  87.6 -3.7    -112.7    -2   1  1   2564  19 00 00
19 50 00  ---          14 38 55  47.2  81.1 -2.9    -114.1  2998   F  1   3614

19 50 00  J1733-13     14 38 55  47.2  81.1 -2.9    -114.1    -2   1  1   3614  19 50 00
20 00 00  ---          14 48 57  49.4  79.6 -2.7    -114.7   598   F  1   3824


SETUP FILE INFORMATION:
   NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings.


 Setup file: /home/sched/short-term/progs/current/setups/vsop4930_s2.set
   Matches group hh6cm_c in /home/sched/short-term/progs/current/catalogs/freq.dat

   Setup group:    4         Station: HART_S2           Total bit rate:  128
   Format: S2                Bits per sample: 2         Sample rate: 32.000
   Number of channels:  2    Passes/head pos:   1       Speedup factor:   1.00

   Tape speeds: Low density -   6.300 ips,  High density -   4.20 ips
   Time per pass for   7600 ft, High density tapes is: 06:01:54

   1st LO=  4786.00  4786.00
   Net SB=        U        U
   Pol.  =     LCP      LCP 
   BBC   =        1        3
   BBC SB=        U        U
   IF    =       1N       1N

  The following frequency sets based on this setup were used.

   Frequency Set:   4  Setup file default.  No pcal detection.
   LO sum=   4930.00  4946.00
   BBC fr=    144.00   160.00
   Bandwd=    16.000   16.000

   Track assignments are: 
    track1=   0,  0
    barrel=roll_off 
 SOURCE LIST -- VSOP observation of  J1733-13  at 5  GHz
     Catalog positions marked with *. 
     Position of date is for stop time of first scan.
     Names used in schedule marked with *. 
     Short names used in VLA and SNAP files marked with +. 

   Source                         Source position (RA/Dec) 
                        (B1950)           (J2000)           (Date) 

   J1550+0527        15 48 06.931008   * 15 50 35.269241     15 50 36.861680 
 * 1548+056          05 36 11.23062    * 05 27 10.44815      05 27 11.67547 
   J1550+05          /home/sched/short-term/progs/current/catalogs/sources.vlba
                     USNO - Ref Frame 1998-6, Eubanks June 1998

   J1733-1304        17 30 13.535185   * 17 33 02.705782     17 33 04.455520 
   1730-130         -13 02 45.83980    *-13 04 49.54828     -13 04 46.66468 
 * J1733-13          /home/sched/short-term/progs/current/catalogs/sources.vlba
   NRAO530           USNO - Ref Frame 1998-6, Eubanks June 1998



  The solar corona can cause unstable phases for sources too close to the Sun.
  SCHED provides warnings at individual scans for distances less than 10 degrees.
  The distance from the Sun to each source in this schedule is:
    Source         Sun distance (deg) 
   1548+056           147.7
   J1733-13           167.0

  Barry Clark estimates from predictions by Ketan Desai of IPM scattering sizes 
  that the Sun will cause amplitude reductions on the  longest VLBA baselines 
  at a solar distance of 60deg F^(-0.6) where F is in GHz. 
  For common VLBI bands, this is: 
       327 MHz        117. deg 
       610 MHz         81. deg 
       1.6 GHz         45. deg 
       2.3 GHz         36. deg 
       5.0 GHz         23. deg 
       8.4 GHz         17. deg 
      15.0 GHz         12. deg 
      22.0 GHz          9. deg 
      43.0 GHz          6. deg 

