  COVER INFORMATION 

 Station:    SHANGHAI  (Code Sh ) 
 Experiment: FTP Fringe-Test Experiment
 Exp. Code:  F09C2   


Schedule Version:       2.00                                              
Processed by SCHED version:   8.10  Bug fixs and minor enhancements       

PI:       Jun Yang                                                        

Address:  JIVE                                                            
          Postbus 2                                                       
          7990 AA Dwingeloo                                               
          The Netherlands                                                 

Phone:    +31-521-596507                                                  
EMAIL:    yang@jive.nl                                                    
Fax:                                                                      
Phone during observation: +31-521-596507                                  

Observing mode:                                                           

Notes:    FTP fringe-test only experiment.                                
          C-band (512 Mbps, 2-bit sampling, 8*16 MHz filters) for session 
          The same frequency setup as the next user experiment EM077A.    
                                                                          

Schedule for SHANGHAI  (Code Sh )                                   Page   2
               FTP Fringe-Test 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.
         For disks, the footages are really the GBytes
  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
----------------------------------------------------------------------------------------

 --- Thu  22 Oct 2009   Day 295 ---

 Next scan frequencies:  4958.49  4958.49  4974.49  4974.49  4990.49  4990.49
                         5006.49  5006.49
 Next BBC frequencies:    758.49   758.49   774.49   774.49   790.49   790.49
                          806.49   806.49
 Next scan bandwidths:     16.00    16.00    16.00    16.00    16.00    16.00
                           16.00    16.00

12 00 00  3C345        22 09 00  25.4 -57.2  5.4      69.6     0   1  1      0  12 00 00
12 10 00  ---          22 19 01  23.6 -56.5  5.6      68.3   600   F  1     39  12 00 01

12 13 00  J1800+3848   22 22 02  37.0 -62.5  4.4      77.1   153   1  1     39  12 13 00
12 20 00  =1758+388    22 29 03  35.7 -62.1  4.5      76.2   420   F  1     66  12 13 01

12 22 00  3C345        22 31 03  21.5 -55.5  5.8      66.7    92   1  1     66  12 22 00
12 30 00  ---          22 39 05  20.0 -54.9  5.9      65.7   480   F  1     97  12 22 01

12 32 00  J1800+3848   22 41 05  33.4 -61.4  4.7      74.7    94   1  1     97  12 32 00
12 40 00  =1758+388    22 49 06  31.9 -60.9  4.8      73.8   480   F  1    128  12 32 01

12 42 00  3C345        22 51 07  17.9 -53.8  6.1      64.1    93   1  1    128  12 42 00
12 50 00  ---          22 59 08  16.6 -53.1  6.3      63.0   480   F  1    159  12 42 01

12 52 00  J1800+3848   23 01 08  29.7 -60.1  5.0      72.3    94   1  1    159  12 52 00
13 00 00  =1758+388    23 09 10  28.2 -59.5  5.1      71.3   480   F  1    190  12 52 01

13 02 00  3C345        23 11 10  14.5 -52.0  6.5      61.4    93   1  1    190  13 02 00
13 10 00  ---          23 19 11  13.2 -51.2  6.6      60.3   480   F  1    221  13 02 01

13 13 00  J1800+3848   23 22 12  25.8 -58.6  5.4      69.7   155   1  1    221  13 13 00
13 20 00  =1758+388    23 29 13  24.5 -58.0  5.5      68.8   420   F  1    248  13 13 01

13 21 00  J1800+3848   23 30 13  24.4 -58.0  5.5      68.7    56   1  1    248  13 21 00
13 30 00  =1758+388    23 39 15  22.7 -57.3  5.6      67.6   540   F  1    283  13 21 01

13 31 00  J1800+3848   23 40 15  22.5 -57.2  5.7      67.4    56   1  1    283  13 31 00
13 40 00  =1758+388    23 49 16  20.9 -56.4  5.8      66.3   540   F  1    317  13 31 01

13 41 00  J1800+3848   23 50 16  20.7 -56.3  5.8      66.2    56   1  1    317  13 41 00
13 50 00  =1758+388    23 59 18  19.1 -55.6  6.0      65.0   540   F  1    352  13 41 01

13 51 00  J1800+3848   00 00 18  19.0 -55.5  6.0      64.9    56   1  1    352  13 51 00
14 00 00  =1758+388    00 09 20  17.4 -54.7  6.1      63.7   540   F  1    387  13 51 01


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


 Setup file: NME.6CM
   Matches group sh6cm in /aps3/sched8.1/catalogs/freq.dat
    Update freq. range AnTao 22Mar08

   Setup group:   11         Station: SHANGHAI          Total bit rate:  512
   Format: MKIV1:4           Bits per sample: 2         Sample rate: 32.000
   Number of channels:  8                               Speedup factor:   1.00

   Disk used to record data.

   1st LO=   4200.00   4200.00   4200.00   4200.00   4200.00   4200.00   4200.00   4200.00
   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:  11  Setup file default.  Used pcal sets:   1
   LO sum=    4958.49   4958.49   4974.49   4974.49   4990.49   4990.49   5006.49   5006.49
   BBC fr=     758.49    758.49    774.49    774.49    790.49    790.49    806.49    806.49
   Bandwd=     16.000    16.000    16.000    16.000    16.000    16.000    16.000    16.000

  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 13510 13510 13510 13510
    PCALFR2=   510   510   510   510 13510 13510 13510 13510

   Track assignments are: 
    track1=   2, 18,  3, 19, 66, 82, 67, 83
    barrel=roll_off 
 SOURCE LIST -- FTP Fringe-Test 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)

   J1642+3948        16 41 17.606227   * 16 42 58.809964     16 43 17.988388       0.26
 * 3C345             39 54 10.81495    * 39 48 36.99401      39 47 39.64611        0.40
   1641+399          /aps3/sched8.1/catalogs/sources.vlba
   J1642+39          VLBA Calib Survey - GSFC sols. - created L.Petrov 2008a_astro
                        0.567 scan hours,     37.400 baseline hours above horizon.

 * J1800+3848        17 58 44.703951   * 18 00 24.765360     18 00 44.063716       0.26
   1758+388          38 48 32.47352    * 38 48 30.69750      38 48 42.79315        0.40
   J1800+38          /aps3/sched8.1/catalogs/sources.vlba
                     VLBA Calib Survey - GSFC sols. - created L.Petrov 2008a_astro
                        1.100 scan hours,     72.076 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) 
   3C345               65.1
   J1800+3848          77.0

  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 

