  COVER INFORMATION 

 Station:    SHANGHAI  (Code Sh ) 
 Experiment: NME-FTP test at S/X band
 Exp. Code:  N09SX1  


Schedule Version:       1.00                                              
Processed by SCHED version:   8.00  2008 December Release                 

PI:       Jun Yang                                                        

Address:  JIVE                                                            
          Postbus 2                                                       
          7990AA Dwingeloo                                                
          The Netherlands                                                 

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

Observing mode: Astrometrical mode at S/X band                            

Notes:    Only RCP, 256 Mbps, 2-bit sampling, 8 Subands/BBCs.             
          Check that autoftp settings to JIVE are OK.                     
          The next user experiment EH023B would use both sidebands.       
                                                                          

Schedule for SHANGHAI  (Code Sh )                                   Page   2
               NME-FTP test at S/X band
  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
----------------------------------------------------------------------------------------

 --- Wed  17 Jun 2009   Day 168 ---

 Next scan frequencies:  2248.99  2264.99  2280.99  2296.99  8360.99  8376.99
                         8392.99  8408.99
 Next BBC frequencies:    648.99   664.99   680.99   696.99   739.01   723.01
                          707.01   691.01
 Next scan bandwidths:      8.00     8.00     8.00     8.00     8.00     8.00
                            8.00     8.00

12 00 00  1156+295     13 48 17  66.6 272.3  1.8      78.5     0   1  1      0  12 00 00
12 15 00  ---          14 03 20  63.4 273.9  2.1      78.1   900   F  1     29  12 00 01

12 17 30  4C39.25      14 05 50  33.9 298.7  4.6      75.1    99   1  1     29  12 17 30
12 30 00  ---          14 18 22  31.5 299.5  4.8      73.6   750   F  1     53  12 17 31

12 32 30  1156+295     14 20 53  59.6 275.6  2.3      77.5   101   1  1     53  12 32 30
12 40 00  ---          14 28 24  58.0 276.3  2.5      77.2   450   F  1     68  12 32 31

12 42 30  4C39.25      14 30 54  29.2 300.3  5.1      72.0   100   1  1     68  12 42 30
12 50 00  ---          14 38 25  27.8 300.8  5.2      71.1   450   F  1     82  12 42 31

12 52 30  1156+295     14 40 56  55.4 277.4  2.7      76.6   102   1  1     82  12 52 30
13 00 00  ---          14 48 27  53.8 278.1  2.8      76.2   450   F  1     97  12 52 31

13 02 30  4C39.25      14 50 58  25.5 301.8  5.4      69.5   101   1  1     97  13 02 30
13 10 00  ---          14 58 29  24.2 302.3  5.5      68.6   450   F  1    111  13 02 31

13 12 30  1156+295     15 00 59  51.1 279.2  3.0      75.5   103   1  1    111  13 12 30
13 20 00  ---          15 08 30  49.5 279.8  3.1      75.1   450   F  1    126  13 12 31

13 22 30  4C39.25      15 11 01  21.9 303.3  5.7      67.0   102   1  1    126  13 22 30
13 30 00  ---          15 18 32  20.6 304.0  5.8      66.1   450   F  1    140  13 22 31

13 32 30  1156+295     15 21 02  46.9 280.9  3.4      74.4   104   1  1    140  13 32 30
13 40 00  ---          15 28 34  45.3 281.6  3.5      73.9   450   F  1    155  13 32 31

13 42 30  4C39.25      15 31 04  18.4 305.0  6.1      64.4   103   1  1    155  13 42 30
13 50 00  ---          15 38 35  17.1 305.7  6.2      63.5   450   F  1    169  13 42 31

13 52 30  1156+295     15 41 06  42.7 282.6  3.7      73.2   105   1  1    169  13 52 30
14 00 00  ---          15 48 37  41.1 283.3  3.8      72.7   450   F  1    184  13 52 31

14 02 30  4C39.25      15 51 07  14.9 306.9  6.4      61.8   104   1  1    184  14 02 30
14 10 00  ---          15 58 39  13.6 307.6  6.5      60.8   450   F  1    198  14 02 31
Schedule for SHANGHAI  (Code Sh )                                   Page   3
               NME-FTP test at S/X band
  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
----------------------------------------------------------------------------------------

 --- Wed  17 Jun 2009   Day 168 ---

14 12 30  1156+295     16 01 09  38.5 284.4  4.0      71.8   107   1  1    198  14 12 30
14 20 00  ---          16 08 40  36.9 285.0  4.1      71.3   450   F  1    213  14 12 31

14 22 30  4C39.25      16 11 11  11.5 308.8  6.7      59.1   106   1  1    213  14 22 30
14 30 00  ---          16 18 42  10.3 309.6  6.9      58.1   450   F  1    227  14 22 31

14 32 30  1156+295     16 21 12  34.4 286.1  4.4      70.4   108   1  1    227  14 32 30
14 40 00  ---          16 28 44  32.8 286.8  4.5      69.9   450   F  1    242  14 32 31

14 42 00  OQ208        16 30 44  58.9 274.3  2.4      76.1    74   1  1    242  14 42 00
14 50 00  ---          16 38 45  57.2 275.1  2.5      75.8   480   F  1    257  14 42 01

14 52 00  1156+295     16 40 46  30.4 287.9  4.7      69.0    73   1  1    257  14 52 00
15 00 00  ---          16 48 47  28.7 288.6  4.8      68.4   480   F  1    273  14 52 01

15 02 00  OQ208        16 50 47  54.6 276.3  2.7      75.4    75   1  1    273  15 02 00
15 10 00  ---          16 58 48  52.9 277.1  2.9      75.0   480   F  1    288  15 02 01

15 12 00  1156+295     17 00 49  26.3 289.7  5.0      67.4    74   1  1    288  15 12 00
15 20 00  ---          17 08 50  24.7 290.5  5.1      66.8   480   F  1    304  15 12 01

15 22 00  OQ208        17 10 50  50.4 278.2  3.1      74.5    75   1  1    304  15 22 00
15 30 00  ---          17 18 52  48.7 278.9  3.2      74.1   480   F  1    319  15 22 01

15 32 30  1156+295     17 21 22  22.2 291.7  5.4      65.7   104   1  1    319  15 32 30
15 40 00  ---          17 28 53  20.7 292.4  5.5      65.1   450   F  1    334  15 32 31

15 42 00  OQ208        17 30 54  46.2 280.0  3.4      73.5    76   1  1    334  15 42 00
15 50 00  ---          17 38 55  44.5 280.7  3.5      73.0   480   F  1    349  15 42 01

15 52 00  1156+295     17 40 55  18.3 293.6  5.7      64.0    74   1  1    349  15 52 00
16 00 00  ---          17 48 57  16.7 294.4  5.8      63.3   480   F  1    365  15 52 01

16 02 00  OQ208        17 50 57  41.9 281.8  3.7      72.3    76   1  1    365  16 02 00
16 10 00  ---          17 58 58  40.3 282.5  3.9      71.9   480   F  1    380  16 02 01

16 12 00  1156+295     18 00 59  14.4 295.7  6.0      62.1    75   1  1    380  16 12 00
16 20 00  ---          18 09 00  12.9 296.5  6.1      61.4   480   F  1    396  16 12 01

16 22 00  OQ208        18 11 00  37.7 283.6  4.1      71.1    77   1  1    396  16 22 00
16 30 00  ---          18 19 02  36.1 284.4  4.2      70.6   480   F  1    411  16 22 01


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


 Setup file: n09sx1.set
 --- WARNING ---  This group does not match an entry in the frequency catalog.
                  This might be ok because the catalog is not complete.
                  But be very careful to be sure that the setup is correct.

   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=   1600.00   1600.00   1600.00   1600.00   9100.00   9100.00   9100.00   9100.00
   Net SB=         U         U         U         U         U         U         U         U
   Pol.  =      RCP       RCP       RCP       RCP       RCP       RCP       RCP       RCP 
   BBC   =         9        10        11        12         1         2         3         4
   BBC SB=         U         U         U         U         L         L         L         L
   IF    =        B         B         B         B         A         A         A         A 

  The following frequency sets based on this setup were used.

   Frequency Set:   8  Setup file default.  Used pcal sets:   1
   LO sum=    2248.99   2264.99   2280.99   2296.99   8360.99   8376.99   8392.99   8408.99
   BBC fr=     648.99    664.99    680.99    696.99    739.01    723.01    707.01    691.01
   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=    10    10    10    10  6010  6010  6010  6010
    PCALFR2=    10    10    10    10  6010  6010  6010  6010

   Track assignments are: 
    track1=   2, 10, 18, 26,  3, 11, 19, 27
    barrel=roll_off 
 SOURCE LIST -- NME-FTP test at S/X band
     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)

   J0927+3902        09 23 55.319214   * 09 27 03.013935     09 27 38.681100       0.26
   0923+392          39 15 23.56647    * 39 02 20.85187      39 00 00.18650        0.40
 * 4C39.25           /aps3/sched8.0/catalogs/sources.vlba
   J0927+39          VLBA Calib Survey - GSFC sols. - created L.Petrov 2008a_astro
                        0.958 scan hours,     33.315 baseline hours above horizon.

   J1159+2914        11 56 57.786210   * 11 59 31.833911     12 00 02.046357       0.23
 * 1156+295          29 31 25.73875    * 29 14 43.82685      29 11 38.01056        0.40
   J1159+29          /aps3/sched8.0/catalogs/sources.vlba
                     VLBA Calib Survey - GSFC sols. - created L.Petrov 2008a_astro
                        1.783 scan hours,     64.092 baseline hours above horizon.

   J1407+2827        14 04 45.615156   * 14 07 00.394414     14 07 27.647639       0.23
   1404+286          28 41 29.23519    * 28 27 14.69022      28 24 33.82586        0.40
   J1407+28          /aps3/sched8.0/catalogs/sources.vlba
 * OQ208             VLBA Calib Survey - GSFC sols. - created L.Petrov 2008a_astro
                        0.800 scan hours,     28.766 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) 
   4C39.25             49.3
   1156+295            81.9
   OQ208              106.4

  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 

