  COVER INFORMATION 

 Station:    SHANGHAI  (Code Sh ) 
 Experiment: Network Monitoring Experiment
 Exp. Code:  N05K2   


Schedule Version:       1.00                                              
Processed by SCHED version:   6.02  July 2005                             

PI:       Zsolt Paragi                                                    

Address:  JIVE                                                            
          Postbus 2                                                       
          7990 AA Dwingeloo                                               
          The Netherlands                                                 

Phone:    +31-521-596536                                                  
EMAIL:    paragi@jive.nl                                                  
Fax:      31-521-597332                                                   
Phone during observation: +31-521-596500                                  

Observing mode: MKIV                                                      

Notes:    K-band NME (256 Mbps, 2-bit sampling, 8MHz filter) for session 3
          Please send the disk pack by express to JIVE                    
                                                                          
                                                                          

Schedule for SHANGHAI  (Code Sh )                                   Page   2
               Network Monitoring Experiment
  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).
  SYNC: Time correlator is expected to sync up.
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)   SYNC
----------------------------------------------------------------------------------------

 --- Wed  26 Oct 2005   Day 299 ---

 Next scan frequencies: 22219.49 22219.49 22227.49 22227.49 22235.49 22235.49
                        22243.49 22243.49
 Next BBC frequencies:    619.49   619.49   627.49   627.49   635.49   635.49
                          643.49   643.49
 Next scan bandwidths:      8.00     8.00     8.00     8.00     8.00     8.00
                            8.00     8.00

07 30 00  1253-055     17 53 54  10.2 256.8  5.0      56.9     0   1  1      0  07 30 00
07 35 00  ---          17 58 55   9.2 257.5  5.0      57.2   300   F  1      0  07 30 10

07 37 00  1253-055     18 00 55   8.7 257.7  5.1      57.2   117   1  1      0  07 37 00
07 42 00  ---          18 05 56   7.7 258.4  5.2      57.5   300   F  1      0  07 37 10

07 48 00  1611+343     18 11 57  65.0 285.0  2.0      88.9   167   1  1      0  07 48 00
07 53 00  ---          18 16 58  64.0 285.1  2.1      88.2   300   F  1      0  07 48 10

07 55 00  3C345        18 18 58  68.7 300.7  1.6     106.7    87   1  1      0  07 55 00
08 05 00  ---          18 29 00  66.9 299.4  1.8     103.8   600   F  1      0  07 55 10

08 08 00  3C345        18 32 01  66.3 299.1  1.8     103.0   176   1  1      0  08 08 00
08 10 00  ---          18 34 01  65.9 298.8  1.8     102.5   120   F  1      0  08 08 10

08 10 00  NRAO512      18 34 01  65.5 298.5  1.9     101.8    -4   1  1      0  08 10 00
08 11 30  ---          18 35 31  65.2 298.4  1.9     101.5    86   F  1      0  08 10 10

08 11 30  3C345        18 35 31  65.6 298.7  1.9     102.1    -4   1  1      0  08 11 30
08 12 30  ---          18 36 31  65.5 298.6  1.9     101.9    56   F  1      0  08 11 40

08 12 30  NRAO512      18 36 31  65.0 298.3  1.9     101.2    -4   1  1      0  08 12 30
08 14 00  ---          18 38 01  64.7 298.2  2.0     100.9    86   F  1      0  08 12 40

08 14 00  3C345        18 38 01  65.2 298.5  1.9     101.5    -4   1  1      0  08 14 00
08 15 00  ---          18 39 02  65.0 298.4  1.9     101.3    56   F  1      0  08 14 10

08 15 00  NRAO512      18 39 02  64.5 298.1  2.0     100.6    -4   1  1      0  08 15 00
08 16 30  ---          18 40 32  64.2 298.0  2.0     100.3    86   F  1      0  08 15 10

08 16 30  3C345        18 40 32  64.7 298.2  2.0     100.9    -4   1  1      0  08 16 30
08 17 30  ---          18 41 32  64.5 298.2  2.0     100.7    56   F  1      0  08 16 40

08 17 30  NRAO512      18 41 32  64.0 297.9  2.0     100.0    -4   1  1      0  08 17 30
08 19 00  ---          18 43 02  63.8 297.8  2.0      99.7    86   F  1      0  08 17 40
Schedule for SHANGHAI  (Code Sh )                                   Page   3
               Network Monitoring Experiment
  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).
  SYNC: Time correlator is expected to sync up.
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)   SYNC
----------------------------------------------------------------------------------------

 --- Wed  26 Oct 2005   Day 299 ---

08 19 00  3C345        18 43 02  64.2 298.0  2.0     100.3    -4   1  1      0  08 19 00
08 20 00  ---          18 44 02  64.0 298.0  2.0     100.1    56   F  1      0  08 19 10

08 20 00  NRAO512      18 44 02  63.6 297.7  2.1      99.5    -4   1  1      0  08 20 00
08 21 30  ---          18 45 33  63.3 297.6  2.1      99.1    86   F  1      0  08 20 10

08 21 30  3C345        18 45 33  63.8 297.8  2.0      99.8    -4   1  1      0  08 21 30
08 22 30  ---          18 46 33  63.6 297.8  2.1      99.5    56   F  1      0  08 21 40

08 24 30  NRAO512      18 48 33  62.7 297.4  2.1      98.5   115   1  1      0  08 24 30
08 26 00  ---          18 50 03  62.4 297.3  2.2      98.2    90   F  1      0  08 24 40

08 26 00  3C345        18 50 03  62.9 297.5  2.1      98.8    -4   1  1      0  08 26 00
08 27 00  ---          18 51 04  62.7 297.5  2.1      98.5    56   F  1      0  08 26 10

08 27 00  NRAO512      18 51 04  62.2 297.3  2.2      98.0    -4   1  1      0  08 27 00
08 28 30  ---          18 52 34  62.0 297.2  2.2      97.6    86   F  1      0  08 27 10

08 28 30  3C345        18 52 34  62.4 297.4  2.2      98.2    -4   1  1      0  08 28 30
08 29 30  ---          18 53 34  62.2 297.3  2.2      98.0    56   F  1      0  08 28 40

08 29 30  NRAO512      18 53 34  61.8 297.1  2.2      97.4    -4   1  1      0  08 29 30
08 31 00  ---          18 55 04  61.5 297.0  2.2      97.1    86   F  1      0  08 29 40

08 31 00  3C345        18 55 04  61.9 297.2  2.2      97.7    -4   1  1      0  08 31 00
08 32 00  ---          18 56 04  61.8 297.2  2.2      97.5    56   F  1      0  08 31 10

08 32 00  NRAO512      18 56 04  61.3 297.0  2.3      96.9    -4   1  1      0  08 32 00
08 33 30  ---          18 57 35  61.0 296.9  2.3      96.6    86   F  1      0  08 32 10

08 33 30  3C345        18 57 35  61.5 297.1  2.2      97.2    -4   1  1      0  08 33 30
08 34 30  ---          18 58 35  61.3 297.1  2.3      97.0    56   F  1      0  08 33 40

08 34 30  NRAO512      18 58 35  60.8 296.9  2.3      96.4    -4   1  1      0  08 34 30
08 36 00  ---          19 00 05  60.5 296.8  2.3      96.1    86   F  1      0  08 34 40

08 36 00  3C345        19 00 05  61.0 297.0  2.3      96.7    -4   1  1      0  08 36 00
08 37 00  ---          19 01 05  60.8 296.9  2.3      96.5    56   F  1      0  08 36 10

08 37 00  NRAO512      19 01 05  60.3 296.8  2.3      95.9    -4   1  1      0  08 37 00
08 38 30  ---          19 02 36  60.0 296.7  2.4      95.6    86   F  1      0  08 37 10

08 38 30  3C345        19 02 36  60.5 296.9  2.3      96.2    -4   1  1      0  08 38 30
08 39 30  ---          19 03 36  60.3 296.8  2.3      96.0    56   F  1      0  08 38 40
Schedule for SHANGHAI  (Code Sh )                                   Page   4
               Network Monitoring Experiment
  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).
  SYNC: Time correlator is expected to sync up.
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)   SYNC
----------------------------------------------------------------------------------------

 --- Wed  26 Oct 2005   Day 299 ---

08 41 30  NRAO512      19 05 36  59.5 296.6  2.4      95.1   115   1  1      0  08 41 30
08 43 00  ---          19 07 06  59.2 296.6  2.4      94.8    90   F  1      0  08 41 40

08 43 00  3C345        19 07 06  59.6 296.7  2.4      95.3    -4   1  1      0  08 43 00
08 44 00  ---          19 08 06  59.5 296.7  2.4      95.1    56   F  1      0  08 43 10

08 44 00  NRAO512      19 08 06  59.0 296.5  2.5      94.6    -4   1  1      0  08 44 00
08 45 30  ---          19 09 37  58.7 296.5  2.5      94.3    86   F  1      0  08 44 10

08 45 30  3C345        19 09 37  59.2 296.6  2.4      94.8    -4   1  1      0  08 45 30
08 46 30  ---          19 10 37  59.0 296.6  2.5      94.6    56   F  1      0  08 45 40

08 46 30  NRAO512      19 10 37  58.5 296.5  2.5      94.1    -4   1  1      0  08 46 30
08 48 00  ---          19 12 07  58.2 296.4  2.5      93.9    86   F  1      0  08 46 40

08 48 00  3C345        19 12 07  58.7 296.5  2.5      94.4    -4   1  1      0  08 48 00
08 49 00  ---          19 13 07  58.5 296.5  2.5      94.2    56   F  1      0  08 48 10

08 49 00  NRAO512      19 13 07  58.0 296.4  2.5      93.7    -4   1  1      0  08 49 00
08 50 30  ---          19 14 37  57.7 296.4  2.6      93.4    86   F  1      0  08 49 10

08 50 30  3C345        19 14 37  58.2 296.5  2.5      93.9    -4   1  1      0  08 50 30
08 51 30  ---          19 15 38  58.0 296.4  2.5      93.7    56   F  1      0  08 50 40

08 51 30  NRAO512      19 15 38  57.5 296.3  2.6      93.2    -4   1  1      0  08 51 30
08 53 00  ---          19 17 08  57.3 296.3  2.6      93.0    86   F  1      0  08 51 40

08 53 00  3C345        19 17 08  57.7 296.4  2.6      93.5    -4   1  1      0  08 53 00
08 54 00  ---          19 18 08  57.5 296.4  2.6      93.3    56   F  1      0  08 53 10

08 54 00  NRAO512      19 18 08  57.1 296.3  2.6      92.8    -4   1  1      0  08 54 00
08 55 30  ---          19 19 38  56.8 296.3  2.6      92.5    86   F  1      0  08 54 10

08 55 30  3C345        19 19 38  57.2 296.4  2.6      93.0    -4   1  1      0  08 55 30
08 56 30  ---          19 20 38  57.1 296.3  2.6      92.8    56   F  1      0  08 55 40

08 56 30  NRAO512      19 20 38  56.6 296.2  2.7      92.4    -4   1  1      0  08 56 30
08 58 00  ---          19 22 09  56.3 296.2  2.7      92.1    86   F  1      0  08 56 40

08 58 00  3C345        19 22 09  56.8 296.3  2.6      92.6    -4   1  1      0  08 58 00
09 00 00  ---          19 24 09  56.4 296.3  2.7      92.2   116   F  1      0  08 58 10

09 16 00  CEPA         19 40 12  46.0 390.6 -3.3    -111.4   769   1  1      0  09 16 00
09 26 00  ---          19 50 13  47.1 390.0 -3.1    -114.1   600   F  1      0  09 16 10


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


 Setup file: 256MBPS.1CM
   Matches group sh1cm in /aps3/sched/catalogs/freq.dat
    From Porcas, from Huang Xinyong 231198

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

   Disk used to record data.

   1st LO=  21600.00  21600.00  21600.00  21600.00  21600.00  21600.00  21600.00  21600.00
   Net SB=         U         U         U         U         U         U         U         U
   Pol.  =      RCP       LCP       RCP       LCP       RCP       LCP       RCP       LCP 
   BBC   =         1         2         3         4         5         6         7         8
   BBC SB=         U         U         U         U         U         U         U         U
   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=   22219.49  22219.49  22227.49  22227.49  22235.49  22235.49  22243.49  22243.49
   BBC fr=     619.49    619.49    627.49    627.49    635.49    635.49    643.49    643.49
   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=   510   510   510   510  6510  6510  6510  6510
    PCALFR2=   510   510   510   510  6510  6510  6510  6510

   Track assignments are: 
    track1=   2, 10, 18, 26,  3, 11, 19, 27
    barrel=roll_off 
 SOURCE LIST -- Network Monitoring Experiment
     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).
     Scan hours are for recording scans only. 
     Baseline hours are only counted for scans above horizon at both ends.

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

 * CEPA              22 54 19.025469   * 22 56 17.967000     22 56 32.218784       0.00
                     61 45 46.53012    * 62 01 48.75000      62 03 53.33329        0.00
                     From catalog imbedded in main SCHED input file.
                        0.167 scan hours,      4.667 baseline hours above horizon.

   J1256-0547        12 53 35.831289   * 12 56 11.166557     12 56 27.684167       0.20
 * 1253-055         -05 31 07.99581    *-05 47 21.52467     -05 49 07.49011        0.31
   3C279             /aps3/sched/catalogs/sources.vlba
   J1256-05          VLBA Calib Srcs - GSFC sols. - catalog 2004f_astro
                        0.167 scan hours,      4.667 baseline hours above horizon.

   J1613+3412        16 11 47.914253   * 16 13 41.064244     16 13 52.804011       0.24
 * 1611+343          34 20 19.83395    * 34 12 47.90897      34 11 59.11783        0.40
   J1613+34          /aps3/sched/catalogs/sources.vlba
                     VLBA Calib Srcs - GSFC sols. - catalog 2004f_astro
                        0.083 scan hours,      2.333 baseline hours above horizon.

   J1640+3946        16 38 48.169686   * 16 40 29.632770     16 40 40.016768       0.26
   1638+398          39 52 30.08665    * 39 46 46.02846      39 46 10.68422        0.40
   J1640+39          /aps3/sched/catalogs/sources.vlba
 * NRAO512           VLBA Calib Srcs - GSFC sols. - catalog 2004f_astro
                        0.450 scan hours,     11.293 baseline hours above horizon.

   J1642+3948        16 41 17.606231   * 16 42 58.809968     16 43 09.168952       0.26
   1641+399          39 54 10.81493    * 39 48 36.99399      39 48 02.90308        0.40
 * 3C345             /aps3/sched/catalogs/sources.vlba
   J1642+39          VLBA Calib Srcs - GSFC sols. - catalog 2004f_astro
                        0.517 scan hours,     12.989 baseline hours above horizon.



  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) 
   CEPA               120.4
   1253-055            17.8
   1611+343            56.1
   NRAO512             63.8
   3C345               64.2

  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 

