  COVER INFORMATION 

 Station:    SHANGHAI  (Code Sh ) 
 Experiment: Observations of the core of the giant radio galaxy J145049+100649
 Exp. Code:  EH032A  


Schedule Version:       4.00
Processed by SCHED version:  11.40  Release 11.4.  March 14, 2015

PI:       G.H. Heald

Address:  ASTRON
          Oude Hoogeveensedijk 4
          Dwingeloo
          The Netherlands

Phone:    +31 521 595 774
EMAIL:    heald@astron.nl
Fax:      +31 521 595 101
Phone during observation: +31 521 595 774

Observing mode: Phase-referencing of a source at 18cm (512 Mb/s)

Notes:    Place additional information here (note2-4 available)
 
 
 

Schedule for SHANGHAI  (Code Sh )                                   Page   2
               Observations of the core of the giant radio galaxy J145049+100649
  UP:  D => Below limits;  H => Below horizon mask;  W => still slewing at end;  blank => Up.
  Early: Seconds between end of slew and start.   Dwell: On source seconds. 
  Disk: GBytes recorded to this point.
  TPStart:  Recording start time.  Frequencies are LO sum (band edge).
  SYNC: Time correlator is expected to sync up.
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Disk   TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell   GBytes    SYNC
----------------------------------------------------------------------------------------

 --- Sat  17 Oct 2015   Day 290 ---

 Next scan frequencies:  1634.49  1634.49  1634.49  1634.49  1650.49  1650.49  1650.49  1650.49
                         1666.49  1666.49  1666.49  1666.49  1682.49  1682.49  1682.49  1682.49
 Next BBC frequencies:    665.51   665.51   665.51   665.51   649.51   649.51   649.51   649.51
                          633.51   633.51   633.51   633.51   617.51   617.51   617.51   617.51
 Next scan bandwidths:      8.00     8.00     8.00     8.00     8.00     8.00     8.00     8.00
                            8.00     8.00     8.00     8.00     8.00     8.00     8.00     8.00

08 12 53  J1450+0910   17 59 46  41.1 253.7  3.1      56.3     0        0   08 12 53
08 14 43  =1448+093    18 01 46  40.7 254.1  3.2      56.5   110        7   08 12 54

08 14 43  UGC09555     18 01 36  41.3 255.0  3.2      57.2    -5        7   No stop 
08 23 43  ---          18 10 38  39.4 256.6  3.3      57.8   535       42   08 14 44

08 24 18  J1450+0910   18 11 13  38.7 255.7  3.3      57.2    30       42   08 24 18
08 26 18  =1448+093    18 13 13  38.3 256.1  3.4      57.3   120       49   08 24 19

08 26 18  UGC09555     18 13 13  38.9 257.0  3.4      57.9    -5       49   No stop 
08 35 18  ---          18 22 15  37.0 258.5  3.5      58.5   535       84   08 26 19

08 38 19  OQ208        18 25 15  34.8 284.9  4.3      70.2   150       84   08 38 19
08 43 09  ---          18 30 16  33.8 285.3  4.4      69.8   290      103   08 38 20

08 46 08  J1450+0910   18 33 06  34.1 259.3  3.7      58.4   149      103   08 46 08
08 47 58  =1448+093    18 35 07  33.7 259.6  3.7      58.5   110      110   08 46 09

08 47 58  UGC09555     18 34 57  34.3 260.5  3.7      59.1    -5      110   No stop 
08 56 58  ---          18 43 58  32.4 261.9  3.9      59.4   535      144   08 47 59

08 57 33  J1450+0910   18 44 33  31.7 261.1  3.9      58.9    30      144   08 57 33
08 59 33  =1448+093    18 46 33  31.3 261.4  3.9      59.0   120      152   08 57 34

08 59 33  UGC09555     18 46 33  31.8 262.3  3.9      59.5    -5      152   No stop 
09 08 33  ---          18 55 35  29.9 263.6  4.1      59.8   535      187   08 59 34

09 09 08  J1450+0910   18 56 10  29.3 262.8  4.1      59.4    30      187   09 09 08
09 11 08  =1448+093    18 58 10  28.8 263.1  4.1      59.4   120      194   09 09 09

09 11 08  UGC09555     18 58 10  29.4 263.9  4.1      59.9    -5      194   No stop 
09 20 08  ---          19 07 12  27.5 265.2  4.3      60.1   535      229   09 11 09

09 20 43  J1450+0910   19 07 47  26.8 264.4  4.3      59.7    30      229   09 20 43
09 22 43  =1448+093    19 09 47  26.4 264.7  4.3      59.7   120      237   09 20 44

09 22 43  UGC09555     19 09 47  26.9 265.6  4.3      60.1    -5      237   No stop 
09 31 43  ---          19 18 49  25.0 266.8  4.5      60.3   535      271   09 22 44
Schedule for SHANGHAI  (Code Sh )                                   Page   3
               Observations of the core of the giant radio galaxy J145049+100649
  UP:  D => Below limits;  H => Below horizon mask;  W => still slewing at end;  blank => Up.
  Early: Seconds between end of slew and start.   Dwell: On source seconds. 
  Disk: GBytes recorded to this point.
  TPStart:  Recording start time.  Frequencies are LO sum (band edge).
  SYNC: Time correlator is expected to sync up.
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Disk   TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell   GBytes    SYNC
----------------------------------------------------------------------------------------

 --- Sat  17 Oct 2015   Day 290 ---

09 35 34  3C286        19 22 40  16.9 295.8  5.8      63.4   198      271   09 35 34
09 40 24  ---          19 27 41  16.0 296.3  5.9      62.9   290      290   09 35 35

09 44 13  J1450+0910   19 31 21  21.8 267.6  4.7      60.1   196      290   09 44 13
09 46 03  =1448+093    19 33 21  21.3 267.9  4.7      60.1   110      297   09 44 14

09 46 03  UGC09555     19 33 11  21.9 268.7  4.7      60.4    -5      297   No stop 
09 55 03  ---          19 42 12  20.0 269.9  4.8      60.4   535      331   09 46 04

09 55 38  J1450+0910   19 42 47  19.3 269.1  4.9      60.1    30      331   09 55 38
09 57 38  =1448+093    19 44 48  18.9 269.4  4.9      60.1   120      339   09 55 39

09 57 38  UGC09555     19 44 48  19.4 270.2  4.9      60.4    -5      339   No stop 
10 06 38  ---          19 53 49  17.5 271.4  5.0      60.4   535      374   09 57 39

10 07 15  J1450+0910   19 54 27  16.8 270.6  5.1      60.1    32      374   10 07 15
10 09 05  =1448+093    19 56 27  16.4 270.9  5.1      60.1   110      381   10 07 16

10 09 05  UGC09555     19 56 17  17.0 271.7  5.1      60.4    -5      381   No stop 
10 18 05  ---          20 05 18  15.0 272.8  5.2      60.3   535      415   10 09 06

10 18 40  J1450+0910   20 05 54  14.4 272.1  5.2      60.1    30      415   10 18 40
10 20 40  =1448+093    20 07 54  13.9 272.3  5.3      60.1   120      423   10 18 41

10 20 40  UGC09555     20 07 54  14.5 273.1  5.3      60.3    -5      423   No stop 
10 29 40  ---          20 16 55  12.5 274.3  5.4      60.1   535      458   10 20 41

10 32 42  OQ208        20 19 58  11.8 296.2  6.2      60.9   156      458   10 32 42
10 37 32  ---          20 24 59  10.9 296.7  6.3      60.4   290      476   10 32 43

10 40 35  J1450+0910   20 27 52   9.7 274.9  5.6      59.8   157      476   10 40 35
10 42 25  =1448+093    20 29 52   9.2 275.1  5.6      59.7   110      483   10 40 36

10 42 25  UGC09555     20 29 42   9.8 275.9  5.6      59.9    -5      483   No stop 
10 51 25  ---          20 38 44   7.9 277.0  5.8      59.7   535      518   10 42 26

10 52 00  J1450+0910   20 39 19   7.2 276.3  5.8      59.5    30      518   10 52 00
10 54 00  =1448+093    20 41 19   6.8 276.6  5.8      59.5   120      526   10 52 01

10 54 00  UGC09555     20 41 19   7.3 277.3  5.8      59.6    -5      526   No stop 
11 03 00  ---          20 50 21   5.4 278.5  6.0      59.3   535      560   10 54 01

13 57 44  3C345        23 45 33   8.9 311.5  7.0      56.6 10423      560   13 57 44
14 02 34  ---          23 50 34   8.1 312.0  7.1      55.9   290      579   13 57 45


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


 ======== Setup file: sess315.L512
   Matching groups in /home/guest/rmc/SCHED/sched11.4/catalogs/freq.dat:
     sh18cm          Huang Xinyong 27Sept05

   Setup group:    1         Station: SHANGHAI          Total bit rate:   512
   Format: MARK5B            Bits per sample: 2         Sample rate: 16.000
   Number of channels: 16    DBE type:                  Speedup factor:   1.00

   Disk used to record data.

   1st LO=   2300.00   2300.00   2300.00   2300.00   2300.00   2300.00   2300.00   2300.00
             2300.00   2300.00   2300.00   2300.00   2300.00   2300.00   2300.00   2300.00
   Net SB=         L         L         U         U         L         L         U         U
                   L         L         U         U         L         L         U         U
   IF SB =         L         L         L         L         L         L         L         L
                   L         L         L         L         L         L         L         L
   Pol.  =      RCP       LCP       RCP       LCP       RCP       LCP       RCP       LCP 
                RCP       LCP       RCP       LCP       RCP       LCP       RCP       LCP 
   BBC   =         1         2         1         2         3         4         3         4
                   5         6         5         6         7         8         7         8
   BBC SB=         U         U         L         L         U         U         L         L
                   U         U         L         L         U         U         L         L
   IF    =        C         A         C         A         C         A         C         A 
                  C         A         C         A         C         A         C         A 

  The following frequency sets based on these setups were used.

   Frequency Set:  14  Setup file default.  Used with PCAL = off
   LO sum=   1634.49  1634.49  1634.49  1634.49  1650.49  1650.49  1650.49  1650.49
             1666.49  1666.49  1666.49  1666.49  1682.49  1682.49  1682.49  1682.49
   BBC fr=    665.51   665.51   665.51   665.51   649.51   649.51   649.51   649.51
              633.51   633.51   633.51   633.51   617.51   617.51   617.51   617.51
   Bandwd=      8.00     8.00     8.00     8.00     8.00     8.00     8.00     8.00
                8.00     8.00     8.00     8.00     8.00     8.00     8.00     8.00
    Matching frequency sets:  14

   Track assignments are: 
    track1=   2,  4, 18, 20,  6,  8, 22, 24, 10, 12, 26, 28, 14, 16, 30, 32
    barrel=roll_off 

 POSITIONS OF SOURCES USED IN RECORDING SCANS

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

 * UGC09555          14 48 23.739225   * 14 50 49.397000     14 51 33.998406       0.00
                     10 19 09.23120    * 10 06 49.31000      10 03 11.91829        0.00
                     From catalog imbedded in main SCHED input file.

 * 4C39.25           09 23 55.319215   * 09 27 03.013936     09 28 00.920337       0.30
   J0927+3902        39 15 23.56645    * 39 02 20.85186      38 58 01.68818        0.16
   0923+392          /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc
   J0927+39          GSFC 2015a astro solution, unpublished 245753 observations.

 * 3C286             13 28 49.657758   * 13 31 08.288051     13 31 50.136426       0.18
   J1331+3030        30 45 58.64059    * 30 30 32.95924      30 25 51.23204        0.17
   1328+307          /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc
   J1331+30          GSFC 2015a astro solution, unpublished    225 observations.

 * OQ208             14 04 45.615156   * 14 07 00.394414     14 07 41.130297       0.24
   J1407+2827        28 41 29.23518    * 28 27 14.69022      28 22 58.48911        0.34
   1404+286          /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc
   J1407+28          GSFC 2015a astro solution, unpublished  67871 observations.

   1448+093          14 48 04.740055   * 14 50 31.168932     14 51 16.025239       0.13
 * J1450+0910        09 22 48.79490    * 09 10 27.95504      09 06 50.20130        0.27
                     /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc
                     GSFC 2015a astro solution, unpublished    138 observations.

 * 3C345             16 41 17.606228   * 16 42 58.809966     16 43 29.356876       0.76
   J1642+3948        39 54 10.81496    * 39 48 36.99402      39 47 15.94486        0.52
   1641+399          /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc
   J1642+39          GSFC 2015a astro solution, unpublished  53430 observations.



SOURCE SCAN SUMMARY FOR SOURCES LISTED ABOVE

     Scan hours are for recording scans only. 
     Baseline hours are only counted for scans above horizon at both ends.
  Source       Setup file             Frequency sets                  Observing hours
                                   (duplicates not shown)              Scan  Baseline
  UGC09555   sess315.L512          1 2 3 4 5 6 7 8 11 12 13 14 +     4.800   365.796
  4C39.25    sess315.L512          1 2 3 4 5 6 7 8 11 12 13          0.083     6.500
  3C286      sess315.L512          1 2 3 4 5 6 7 8 11 12 13 14 +     0.322    23.683
  OQ208      sess315.L512          1 2 3 4 5 6 7 8 11 12 13 14 +     0.322    27.631
  J1450+0910 sess315.L512          1 2 3 4 5 6 7 8 11 12 13 14 +     1.067    83.114
  3C345      sess315.L512          1 2 3 4 5 6 7 8 11 13 14 15       0.081     7.331


EFFECT OF SOLAR CORONA

  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) 
   UGC09555            28.3
   4C39.25             73.6
   3C286               39.7
   OQ208               38.8
   J1450+0910          27.7
   3C345               66.6

  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 

