  COVER INFORMATION 

 Station:    SHANGHAI  (Code Sh ) 
 Experiment: Network Monitoring Expt
 Exp. Code:  N03L2   


Schedule Version:       1.00                                              
Processed by SCHED version: Release of 02 July 2002                       

PI:       Zsolt Paragi                                                    

Address:  JIVE                                                            
                                                                          
                                                                          
                                                                          

Phone:    +31-521-596536                                                  
EMAIL:    paragi@jive.nl                                                  
Fax:                                                                      
Phone during observation: +31-521-596536                                  

Observing mode:                                                           

Notes:    L-band NME for May03 session (256Mbps)                          
          Please send tape by express to JIVE                             
          This NME uses one THIN 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.  Frequencies are LO sum (band edge).
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)
----------------------------------------------------------------------------------------

 --- Wed  28 May 2003   Day 148 ---

 Next scan frequencies:  1632.49  1632.49  1632.49  1632.49  1648.49  1648.49
                         1648.49  1648.49
 Next BBC frequencies:    567.51   567.51   567.51   567.51   551.51   551.51
                          551.51   551.51
 Next scan bandwidths:      8.00     8.00     8.00     8.00     8.00     8.00
                            8.00     8.00

09 00 00  3C84         09 26 47  18.9 307.7  6.1      64.8     0   1  1      0  09 00 00
09 22 00  ---          09 48 51  15.2 309.7  6.5      61.7  1320   F  1  17600

09 24 00  J0607+4739   09 50 51  44.9 308.1  3.7      90.6    19   1  2  17600  09 24 00
09 29 30  =0603+476    09 56 22  44.0 308.1  3.8      89.6   330   R  1  13200

09 30 30  J0518+3306   09 57 22  32.0 292.0  4.7      71.4    18   1  2  13200  09 30 30
09 36 00  =0514+330    10 02 53  30.9 292.5  4.7      70.8   330   R  1   8800

09 36 00  DA193        10 02 53  39.9 298.1  4.1      79.7   -32   1  2   8800  09 36 00
09 41 30  ---          10 08 24  38.9 298.3  4.2      78.9   298   R  1   4400

09 45 30  3C48         10 12 25  -9.5 318.5  8.6  D   42.7   125   1  2   4400  09 45 30
09 51 00  ---          10 17 56 -10.3 319.4  8.7  D   41.8     0   R  1      0

09 55 00  3C84         10 21 56   9.9 312.9  7.0      56.9   222   1  3      0  09 55 00
10 00 30  ---          10 27 27   9.0 313.5  7.1      56.1   330   F  1   4400

10 00 30  J0310+3814   10 27 27   5.7 311.8  7.3      54.4   -13   1  3   4400  10 00 30
10 06 00  =0307+380    10 32 58   4.8 312.4  7.4  D   53.6     0   F  1   8800

10 08 00  DA193        10 34 58  33.9 299.7  4.7      75.5    22   1  3   8800  10 08 00
10 19 00  ---          10 46 00  31.8 300.4  4.8      74.1   660   F  1  17600

10 24 00  J0607+4739   10 51 01  34.8 309.2  4.7      80.2   280   1  4  17600  10 24 00
10 29 30  =0603+476    10 56 32  33.9 309.4  4.8      79.3   330   R  1  13200

10 30 30  J0518+3306   10 57 32  20.3 297.2  5.7      65.4    13   1  4  13200  10 30 30
10 36 00  =0514+330    11 03 03  19.3 297.7  5.7      64.8   330   R  1   8800

10 36 00  DA193        11 03 03  28.7 301.5  5.1      71.9   -34   1  4   8800  10 36 00
10 41 30  ---          11 08 34  27.7 301.9  5.2      71.2   296   R  1   4400

10 45 30  3C48         11 12 35 -17.2 328.7  9.6  D   32.1   162   1  4   4400  10 45 30
10 51 00  ---          11 18 05 -17.8 329.8  9.7  D   31.0     0   R  1      0
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.  Frequencies are LO sum (band edge).
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)
----------------------------------------------------------------------------------------

 --- Wed  28 May 2003   Day 148 ---

10 55 00  3C84         11 22 06   1.0 319.8  8.0  D   47.5   218   1  5      0  10 55 00
11 00 30  ---          11 27 37   0.2 320.5  8.1  D   46.6     0   F  1   4400

11 00 30  J0310+3814   11 27 37  -3.3 319.4  8.3  D   45.2    -4   1  5   4400  11 00 30
11 06 00  =0307+380    11 33 08  -4.1 320.2  8.4  D   44.3     0   F  1   8800

11 08 00  DA193        11 35 08  22.9 303.8  5.7      67.8    58   1  5   8800  11 08 00
11 19 00  ---          11 46 10  21.0 304.7  5.8      66.4   660   F  1  17600

11 20 00  J0607+4739   11 47 10  25.7 311.9  5.7      71.1    42   1  6  17600  11 20 00
11 25 30  =0603+476    11 52 41  24.8 312.2  5.8      70.3   330   R  1  13200

11 26 30  J0518+3306   11 53 41   9.9 302.8  6.6      59.2     8   1  6  13200  11 26 30
11 32 00  =0514+330    11 59 12   8.9 303.5  6.7      58.5   330   R  1   8800

11 35 30  DA193        12 02 43  18.1 306.1  6.1      64.2   177   1  6   8800  11 35 30
11 46 30  ---          12 13 45  16.2 307.1  6.3      62.7   660   R  1      0

11 47 30  3C84         12 14 45  -5.8 327.0  8.9  D   38.5    18   1  7      0  11 47 30
11 53 00  ---          12 20 16  -6.4 327.9  9.0  D   37.5     0   F  1   4400

11 53 00  J0310+3814   12 20 16 -10.0 327.3  9.2  D   36.1    -3   1  7   4400  11 53 00
11 58 30  =0307+380    12 25 47 -10.7 328.2  9.2  D   35.1     0   F  1   8800

12 00 30  DA193        12 27 47  13.8 308.4  6.5      60.8    79   1  7   8800  12 00 30
12 11 30  ---          12 38 49  12.0 309.5  6.7      59.3   660   F  1  17600

12 12 30  J0607+4739   12 39 49  17.5 315.6  6.5      62.8    40   1  8  17600  12 12 30
12 18 00  =0603+476    12 45 20  16.7 316.1  6.6      61.9   330   R  1  13200

12 19 00  J0518+3306   12 46 20   0.8 309.0  7.5  D   52.6    19   1  8  13200  12 19 00
12 24 30  =0514+330    12 51 51  -0.2 309.8  7.6  D   51.8     0   R  1   8800

12 28 00  DA193        12 55 21   9.3 311.2  7.0      57.0   194   1  8   8800  12 28 00
12 39 00  ---          13 06 23   7.5 312.4  7.2      55.4   660   R  1      0

12 40 00  3C84         13 07 23 -11.2 335.3  9.8  D   28.5    12   1  9      0  12 40 00
12 45 30  ---          13 12 54 -11.7 336.3  9.9  D   27.4     0   F  1   4400

12 45 30  J0310+3814   13 12 54 -15.4 336.3 10.0  D   26.0    -2   1  9   4400  12 45 30
12 51 00  =0307+380    13 18 25 -15.8 337.4 10.1  D   24.8     0   F  1   8800

12 53 00  DA193        13 20 25   5.3 314.0  7.4      53.3    71   1  9   8800  12 53 00
13 04 00  ---          13 31 27   3.7 315.3  7.6  D   51.6     0   F  1  17600
Schedule for SHANGHAI  (Code Sh )                                   Page   4
               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.  Frequencies are LO sum (band edge).
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)
----------------------------------------------------------------------------------------

 --- Wed  28 May 2003   Day 148 ---

13 10 00  J0607+4739   13 37 28   9.3 320.9  7.5      53.3   344   1 10  17600  13 10 00
13 15 30  =0603+476    13 42 59   8.5 321.5  7.6      52.4   330   R  1  13200

13 15 30  J0518+3306   13 42 59  -8.1 316.9  8.4  D   44.3   -14   1 10  13200  13 15 30
13 21 00  =0514+330    13 48 30  -8.9 317.8  8.5  D   43.4     0   R  1   8800

13 21 00  DA193        13 48 30   1.1 317.4  7.9  D   49.0    -3   1 10   8800  13 21 00
13 32 00  ---          13 59 32  -0.4 318.8  8.1  D   47.2     0   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-1HEAD.18CM
   Matches group sh18cm in /aps3/sched/catalogs/freq.dat
    Huang Xinyong 170300, dual pol but narrow(?)

   Setup group:    8         Station: SHANGHAI          Total bit rate:  256
   Format: MKIV1:2           Bits per sample: 2         Sample rate: 16.000
   Number of channels:  8    Passes/head pos:   1       Speedup factor:   1.00

   Tape speeds: Low density - 270.000 ips,  High density - 160.00 ips
   Time per pass for  17600 ft, High density tapes is: 00:22:00

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

  The following frequency sets based on this setup were used.

   Frequency Set:   8  Setup file default.  Used pcal sets:   1
   LO sum=    1632.49   1632.49   1632.49   1632.49   1648.49   1648.49   1648.49   1648.49
   BBC fr=     567.51    567.51    567.51    567.51    551.51    551.51    551.51    551.51
   Bandwd=      8.000     8.000     8.000     8.000     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    S5    S7    S1    S3    S5    S7 
    PCALXB2=   S2    S4    S6    S8    S2    S4    S6    S8 
    PCALFR1=   490   510   490   510  6490  6510  6490  6510
    PCALFR2=   490   510   490   510  6490  6510  6490  6510

   Track assignments are: 
    track1=   2, 10, 18, 26,  3, 11, 19, 27
    barrel=roll_off 
 SOURCE LIST -- Network Monitoring Expt
     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) 

   J0137+3309        01 34 49.826365   * 01 37 41.299431     01 37 50.593291 
   0134+329          32 54 20.25881    * 33 09 35.13299      33 10 23.14838 
 * 3C48              /aps3/sched/catalogs/sources.vlba
   J0137+33          ICRF - Ext.1 Source - 1998 IERS Annual Report

 * J0310+3814        03 07 37.554113   * 03 10 49.879971     03 11 00.049548 
   0307+380          38 03 34.47090    * 38 14 53.83788      38 15 31.98890 
                     /aps3/sched/catalogs/sources.vlba
                     VLBA Calib. Survey - ICRF Frame - reduced by GSFC group - Aug 2001

   J0319+4130        03 16 29.567273   * 03 19 48.160103     03 19 58.608439 
   0316+413          41 19 51.91592    * 41 30 42.10305      41 31 18.85042 
 * 3C84              /aps3/sched/catalogs/sources.vlba
   J0319+41          ICRF - Ext.1 Source - 1998 IERS Annual Report

 * J0518+3306        05 14 48.670936   * 05 18 05.142458     05 18 15.710203 
   0514+330          33 03 04.11904    * 33 06 13.36462      33 06 28.43799 
                     /aps3/sched/catalogs/sources.vlba
                     VLBA Calib. Survey - ICRF Frame - reduced by GSFC group - Aug 2001

   J0555+3948        05 52 01.407166   * 05 55 30.805609     05 55 42.136171 
   0552+398          39 48 21.94585    * 39 48 49.16500      39 48 56.85131 
 * DA193             /aps3/sched/catalogs/sources.vlba
   J0555+39          ICRF - Ext.1 Source - 1998 IERS Annual Report

 * J0607+4739        06 03 36.208470   * 06 07 23.254984     06 07 35.501693 
   0603+476          47 40 10.99357    * 47 39 46.94223      47 39 53.13801 
                     /aps3/sched/catalogs/sources.vlba
                     VLBA Calib. Survey - ICRF Frame - reduced by GSFC group - Aug 2001



  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) 
   3C48                37.5
   J0310+3814          22.4
   3C84                23.7
   J0518+3306          17.5
   DA193               27.5
   J0607+4739          34.0

  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 

