  COVER INFORMATION 

 Station:    SHANGHAI  (Code Sh ) 
 Experiment: Network Monitoring Expt
 Exp. Code:  C00L4   


Schedule Version:      99.90                                              
Processed by SCHED version: Release of 28 April 2000                      

PI:       Denise Gabuzda                                                  

Address:  JIVE                                                            
                                                                          
                                                                          
                                                                          

Phone:    +06-51-27-10-85(home)                                           
EMAIL:    gabuzda@jive.nl                                                 
Fax:                                                                      
Phone during observation: +31-521-596536 (work)                           

Observing mode:                                                           

Notes:    Network Monitoring Experiment sep00                             
          Please send tape by express to JIVE                             
          -----------------------------------                             
          This NME uses one THICK tape/station                            

Schedule for SHANGHAI  (Code Sh )                                   Page   2
               Network Monitoring Expt
  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)
----------------------------------------------------------------------------------------

 --- Wed  15 Nov 2000   Day 320 ---

 Next scan frequencies:  1650.49  1650.49  1658.49  1658.49
 Next BBC frequencies:    549.51   549.51   541.51   541.51
 Next scan bandwidths:      8.00     8.00     8.00     8.00

17 00 00  0059+581     04 45 09  43.9 323.1  3.7     101.3     0   1  1      0  17 00 00
17 13 00  ---          04 58 11  42.2 322.7  3.9      98.3   780   F  1   8775

17 19 47  2007+777     05 04 59  22.2 350.8  9.0      41.0   338   1  2   8775  17 19 47
17 32 47  ---          05 18 01  21.8 351.3  9.2      38.0   780   R  1      0

17 33 47  2007+777     05 19 01  21.8 351.4  9.2      37.8    58   1  3      0  17 33 47
17 46 47  ---          05 32 03  21.4 352.0  9.4      34.8   780   F  1   8775

17 47 47  2007+777     05 33 04  21.3 352.0  9.5      34.6    58   1  4   8775  17 47 47
18 00 47  ---          05 46 06  20.9 352.6  9.7      31.6   780   R  1      0

18 08 30  0059+581     05 53 50  35.0 322.4  4.9      86.2   401   1  5      0  18 08 30
18 21 30  ---          06 06 52  33.3 322.6  5.1      83.5   780   F  1   8775

18 22 30  0059+581     06 07 52  33.1 322.6  5.1      83.3    58   1  6   8775  18 22 30
18 35 30  ---          06 20 54  31.4 322.9  5.3      80.7   780   R  1      0

18 43 49  2007+777     06 29 15  19.9 354.8 10.4      21.8   433   1  7      0  18 43 49
18 56 49  ---          06 42 17  19.7 355.5 10.6      18.8   780   F  1   8775

18 57 49  2007+777     06 43 17  19.7 355.5 10.6      18.6    58   1  8   8775  18 57 49
19 10 49  ---          06 56 19  19.5 356.2 10.8      15.7   780   R  1      0

19 19 26  0059+581     07 04 58  25.8 324.4  6.0      72.1   452   1  9      0  19 19 26
19 32 26  ---          07 18 00  24.2 325.0  6.3      69.5   780   F  1   8775

19 33 26  0059+581     07 19 00  24.1 325.1  6.3      69.3    58   1 10   8775  19 33 26
19 46 26  ---          07 32 02  22.5 325.8  6.5      66.8   780   R  1      0

19 55 13  2007+777     07 40 50  19.0 358.6 11.6       5.6   459   1 11      0  19 55 13
20 08 13  ---          07 53 53  19.0 359.4 11.8       2.6   780   F  1   8775

20 09 13  2007+777     07 54 53  19.0 359.4 11.8       2.4    58   1 12   8775  20 09 13
20 22 13  ---          08 07 55  19.0 360.1-12.0      -0.6   780   R  1      0

20 30 16  0059+581     08 16 00  17.4 328.6  7.2      58.4   418   1 13      0  20 30 16
20 43 16  ---          08 29 02  16.0 329.5  7.4      55.9   780   F  1   8775
Schedule for SHANGHAI  (Code Sh )                                   Page   3
               Network Monitoring Expt
  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)
----------------------------------------------------------------------------------------

 --- Wed  15 Nov 2000   Day 320 ---

20 44 16  0059+581     08 30 02  15.9 329.6  7.5      55.7    58   1 14   8775  20 44 16
20 57 16  ---          08 43 04  14.5 330.7  7.7      53.2   780   R  1      0


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


 Setup file: NME.18CM
   Matches group sh18cm in /aps3/sched/catalogs/freq.dat
    Huang Xinyong 170300, dual pol but narrow(?)

   Setup group:   10         Station: SHANGHAI          Total bit rate:  128
   Format: MKIV1:4           Bits per sample: 2         Sample rate: 16.000
   Number of channels:  4    Passes/head pos:   1       Speedup factor:   2.00

   Tape speeds: Low density - 135.000 ips,  High density -  80.00 ips
   Time per pass for   8820 ft, Low density tapes is: 00:13:04

   1st LO=  2200.00  2200.00  2200.00  2200.00
   Net SB=        U        U        U        U
   Pol.  =     RCP      LCP      RCP      LCP 
   BBC   =        1        2        3        4
   BBC SB=        L        L        L        L
   IF    =       C        A        C        A 

  The following frequency sets based on this setup were used.

   Frequency Set:  10  Setup file default.  Used pcal sets:   1
   LO sum=   1650.49  1650.49  1658.49  1658.49
   BBC fr=    549.51   549.51   541.51   541.51
   Bandwd=     8.000    8.000    8.000    8.000

  The following pulse cal sets were used with this setup:

   Pulse cal detection set:   1  PCAL = 1MHZ
    PCALXB1=   S1    S3    S1    S3    S1    S2    S3    S4 
    PCALXB2=   S2    S4    S2    S4    M1    M2    M3    M4 
    PCALFR1=   510   510  6510  6510     0     0     0     0
    PCALFR2=   510   510  6510  6510     0     0     0     0

   Track assignments are: 
    track1=   2, 18,  3, 19
    barrel=roll_off 
 SOURCE LIST -- Network Monitoring Expt
     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) 

   J0102+5824        00 59 43.470978   * 01 02 45.762386     01 02 49.925972 
 * 0059+581          58 08 04.84745    * 58 24 11.13660      58 24 34.12184 
   J0102+58          /aps3/sched/catalogs/sources.vlba
                     USNO - Ref Frame 1998-6, Eubanks June 1998

   J2005+7752        20 07 20.430203   * 20 05 30.998531     20 05 27.595259 
 * 2007+777          77 43 58.12307    * 77 52 43.24760      77 53 10.12485 
   J2005+77          /aps3/sched/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) 
   0059+581           132.6
   2007+777           104.2

  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 

