  COVER INFORMATION 

 Station:    SHANG_S2  (Code Sh ) 
 Experiment: VSOP observation of  J2101+03  at 5 GHz
 Exp. Code:  vs08v   


Schedule Version:       2.00                                              
Processed by SCHED version: Release of 28 April 2000                      

PI:       The VSOP Survey Program, Hirabayashi Lab.                       

Address:  Institute of Space and Astronautical Science,                   
          3-1-1 Yoshinodai, Sagamihara, Kanagawa 229-8510                 
          JAPAN                                                           
                                                                          

Phone:    81-427-59-8340                                                  
EMAIL:    vsog@vsop.isas.ac.jp                                            
Fax:      81-427-59-8340                                                  
Phone during observation:                                                 

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

Notes:    Fringe finder : J1733-13                                        
                                                                          
                                                                          
                                                                          

Schedule for SHANG_S2  (Code Sh )                                   Page   2
               VSOP observation of  J2101+03  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)
----------------------------------------------------------------------------------------

 --- Tue  14 Nov 2000   Day 319 ---

 Next scan frequencies:  4800.00  4816.00
 Next BBC frequencies:    600.00   616.00
 Next scan bandwidths:     16.00    16.00

03 29 50  J1733-13     15 08 49  33.9 136.3 -2.4     -37.4     0   1  1     52  03 29 50
03 35 00  ---          15 14 00  34.6 137.5 -2.3     -36.4   310   F  1    161

04 15 00  J2101+03     15 54 07  13.1  93.6 -5.1     -58.9  2310   1  1    216  04 15 00
04 25 00  ---          16 04 08  15.3  95.0 -5.0     -58.7   600   F  1    426

04 25 00  J2101+03     16 04 08  15.3  95.0 -5.0     -58.7    -2   1  1    426  04 25 00
04 50 00  ---          16 29 12  20.6  98.4 -4.5     -58.1  1498   F  1    951

04 50 00  J2101+03     16 29 12  20.6  98.4 -4.5     -58.1    -2   1  1    951  04 50 00
05 00 00  ---          16 39 14  22.7  99.8 -4.4     -57.7   598   F  1   1161

05 00 00  J2101+03     16 39 14  22.7  99.8 -4.4     -57.7    -2   1  1   1161  05 00 00
06 00 00  ---          17 39 24  35.2 109.5 -3.4     -54.0  3598   F  1   2421

06 00 00  J2101+03     17 39 24  35.2 109.5 -3.4     -54.0    -2   1  1   2421  06 00 00
07 00 00  ---          18 39 34  46.8 122.1 -2.4     -46.6  3598   F  1   3681

07 00 00  J2101+03     18 39 34  46.8 122.1 -2.4     -46.6    -2   1  1   3681  07 00 00
07 30 00  ---          19 09 39  52.0 130.5 -1.9     -40.7  1798   F  1   4311

07 31 50  J1733-13     19 11 29  39.9 211.9  1.6      27.7   -55   1  1   4349  07 31 50
07 37 00  ---          19 16 40  39.3 213.4  1.7      28.9   255   F  1   4458

07 47 00  J1733-13     19 26 42  38.1 216.1  1.9      31.2   593   1  1   4512  07 47 00
07 52 00  ---          19 31 42  37.4 217.4  2.0      32.3   300   F  1   4617

08 30 00  J2101+03     20 09 49  60.0 153.4 -0.9     -22.6  2150   1  1   4672  08 30 00
09 00 00  ---          20 39 54  62.1 168.3 -0.4     -10.0  1800   F  1   5302

09 00 00  J2101+03     20 39 54  62.1 168.3 -0.4     -10.0    -2   1  1   5302  09 00 00
09 20 00  ---          20 59 57  62.6 179.1  0.0      -0.8  1198   F  1   5722

09 20 00  J2101+03     20 59 57  62.6 179.1  0.0      -0.8    -2   1  1   5722  09 20 00
09 40 00  ---          21 20 00  62.3 189.9  0.3       8.5  1198   F  1   6142

09 40 00  J2101+03     21 20 00  62.3 189.9  0.3       8.5    -2   1  1   6142  09 40 00
10 00 00  ---          21 40 03  61.1 200.2  0.6      17.2  1198   F  1   6562
Schedule for SHANG_S2  (Code Sh )                                   Page   3
               VSOP observation of  J2101+03  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)
----------------------------------------------------------------------------------------

 --- Tue  14 Nov 2000   Day 319 ---

10 00 00  J2101+03     21 40 03  61.1 200.2  0.6      17.2    -2   1  1   6562  10 00 00
10 15 00  ---          21 55 06  59.8 207.3  0.9      23.2   898   F  1   6877

10 15 00  J2101+03     21 55 06  59.8 207.3  0.9      23.2    -2   1  1   6877  10 15 00
10 45 00  ---          22 25 11  56.3 219.8  1.4      33.3  1798   F  1   7507


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/vsop4800_s2.set
   Matches group sh6cm in /home/sched/short-term/progs/current/catalogs/freq.dat
    from Huang Xinyong 170300, change in LO

   Setup group:    5         Station: SHANG_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=  4200.00  4200.00
   Net SB=        U        U
   Pol.  =     LCP      LCP 
   BBC   =        1        3
   BBC SB=        U        U
   IF    =       A        A 

  The following frequency sets based on this setup were used.

   Frequency Set:   5  Setup file default.  Used pcal sets:   1
   LO sum=   4800.00  4816.00
   BBC fr=    600.00   616.00
   Bandwd=    16.000   16.000

  The following pulse cal sets were used with this setup:

   Pulse cal detection set:   1  PCAL = 1MHZ
    PCALXB1=   S1    S1    S1    S2    S1    OFF   OFF   OFF
    PCALXB2=   S2    S2    M1    M2    S2    OFF   OFF   OFF
    PCALFR1=  1000 13000     0     0  2000     0     0     0
    PCALFR2=  1000 13000     0     0  2000     0     0     0

   Track assignments are: 
    track1=   0,  0
    barrel=roll_off 
 SOURCE LIST -- VSOP observation of  J2101+03  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) 

   J1733-1304        17 30 13.535185   * 17 33 02.705782     17 33 03.231785 
   1730-130         -13 02 45.83980    *-13 04 49.54828     -13 04 45.01770 
 * J1733-13          /home/sched/short-term/progs/current/catalogs/sources.vlba
   NRAO530           USNO - Ref Frame 1998-6, Eubanks June 1998

   J2101+0341        20 59 08.011544   * 21 01 38.834164     21 01 40.160170 
   2059+034          03 29 41.48334    * 03 41 31.32060      03 41 47.02326 
 * J2101+03          /home/sched/short-term/progs/current/catalogs/sources.vlba
                     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) 
   J1733-13            32.6
   J2101+03            87.0

  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 

