SETUP FILE INFORMATION:
   NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings.
 SOURCE LIST -- ToO of J1628-4152
     Catalog positions marked with *. 
     Precession of date coordinates is based on stop time of first scan.
     Names used in schedule marked with *. 
     Short names used in VLA and SNAP files marked with +. 
     Observation date used in B1950/J2000 coordinate conversion (PRECDATE):  1979.900
     No adjustments are made for rates (DRA, DDEC).

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

 * J1628-4152        16 25 18.560956   * 16 28 47.283000     16 29 02.556945 
                    -41 46 03.55065    *-41 52 39.05000     -41 53 07.20177 
                     From catalog imbedded in main SCHED input file.

 * J1610-3958        16 06 58.660724   * 16 10 21.879090     16 10 36.862083 
                    -39 51 10.33021    *-39 58 58.32740     -39 59 32.07736 
                     From catalog imbedded in main SCHED input file.

 * J1604-4441        16 00 59.740734   * 16 04 31.026384     16 04 46.597997 
   1600-445         -44 33 21.12640    *-44 41 31.85626     -44 42 05.70785 
   J1604-44          /home/arana/cwalker/sched/catalogs/sources.vlba
                     ICRF - Ext.1 Source - 1998 IERS Annual Report



  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) 
   J1628-4152          63.7
   J1610-3958          67.2
   J1604-4441          68.1

  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