  COVER INFORMATION 

 Station:    SHANGHAI  (Code Sh ) 
 Experiment: Probing the innermost regions of AGN jets and their magnetic fields
 Exp. Code:  gl038a  


Schedule Version:       1.10
Processed by SCHED version:  11.10  Version 11.1 Beta of about April 26, 201

PI:       Andrei Lobanov

Address:  MPIfR Bonn
          Auf dem Huegel 69
          53121 Bonn, Germany
 

Phone:    +49 228 525 191
EMAIL:    alobanov@mpifr-bonn.mpg.de
Fax:      +49 228 525 229
Phone during observation: +7 903 661 48 65

Observing mode: L-band, dual-pol

Notes:    L-band, Radioastron-compatible frequency setup
          P-CAL is ON
          Tsys is ON, auto-level (AGC) is ON
          Please, send Mk5 disk packs to MPIfR-Bonn

Schedule for SHANGHAI  (Code Sh )                                   Page   2
               Probing the innermost regions of AGN jets and their magnetic fields
  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
----------------------------------------------------------------------------------------

 --- Thu  24 Oct 2013   Day 297 ---

 ---------- Segment 01: L-band VLBI scans ----------

 Next scan frequencies:  1668.00  1668.00  1668.00  1668.00
 Next BBC frequencies:    632.00   632.00   632.00   632.00
 Next scan bandwidths:     16.00    16.00    16.00    16.00

22 20 00  0836+710     08 38 42  50.3   0.5 -0.1    -178.6     0        0   22 20 00
22 29 30  ---          08 48 14  50.3  -0.7  0.1     178.2   570       18   22 20 01

22 30 00  0836+710     08 48 44  50.3  -0.8  0.1     178.0    28       18   22 30 00
22 39 30  ---          08 58 15  50.2  -2.0  0.3     174.8   570       37   22 30 01

22 40 00  0836+710     08 58 45  50.2  -2.0  0.3     174.7    28       37   22 40 00
22 49 30  ---          09 08 17  50.1  -3.3  0.4     171.5   570       55   22 40 01

22 50 00  0836+710     09 08 47  50.1  -3.3  0.4     171.3    28       55   22 50 00
22 59 30  ---          09 18 19  50.0  -4.5  0.6     168.1   570       73   22 50 01

23 00 00  0836+710     09 18 49  50.0  -4.6  0.6     168.0    28       73   23 00 00
23 10 00  ---          09 28 50  49.8  -5.8  0.8     164.7   600       92   23 00 01

 ---------- GROUND ONLY: L-band VLBI scans: Block 01 ----------

23 10 30  0836+710     09 29 20  49.7  -5.9  0.8     164.5    28       92   23 10 30
23 20 00  ---          09 38 52  49.5  -7.0  0.9     161.4   570      111   23 10 31

23 20 30  0836+710     09 39 22  49.5  -7.1  0.9     161.2    28      111   23 20 30
23 30 00  ---          09 48 54  49.2  -8.2  1.1     158.1   570      129   23 20 31

23 30 30  0836+710     09 49 24  49.2  -8.3  1.1     157.9    28      129   23 30 30
23 40 00  ---          09 58 55  48.9  -9.4  1.3     154.9   570      147   23 30 31

23 40 30  0836+710     09 59 25  48.9  -9.4  1.3     154.7    28      147   23 40 30
23 50 00  ---          10 08 57  48.5 -10.5  1.4     151.7   570      165   23 40 31

23 50 30  0836+710     10 09 27  48.5 -10.5  1.4     151.5    28      165   23 50 30
23 59 59  ---          10 18 59  48.1 -11.6  1.6     148.5   569      184   23 50 31

 --- Fri  25 Oct 2013   Day 298 ---

00 00 30  0836+710     10 19 29  48.1 -11.6  1.6     148.3    28      184   00 00 30
00 10 00  ---          10 29 00  47.7 -12.6  1.8     145.4   570      202   00 00 31

00 10 30  0836+710     10 29 30  47.6 -12.6  1.8     145.2    28      202   00 10 30
00 20 00  ---          10 39 02  47.2 -13.6  1.9     142.3   570      220   00 10 31
Schedule for SHANGHAI  (Code Sh )                                   Page   3
               Probing the innermost regions of AGN jets and their magnetic fields
  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
----------------------------------------------------------------------------------------

 --- Fri  25 Oct 2013   Day 298 ---

 ---------- Segment 02: L-band VLBI scans ----------

00 21 00  0836+710     10 40 02  47.1 -13.7  2.0     142.0    58      220   00 21 00
00 30 30  ---          10 49 34  46.6 -14.5  2.1     139.1   570      238   00 21 01

00 31 00  0836+710     10 50 04  46.6 -14.6  2.1     138.9    28      238   00 31 00
00 40 30  ---          10 59 35  46.1 -15.4  2.3     136.1   570      257   00 31 01

00 41 00  0836+710     11 00 05  46.1 -15.5  2.3     135.9    28      257   00 41 00
00 50 30  ---          11 09 37  45.5 -16.3  2.4     133.1   570      275   00 41 01

00 51 00  0836+710     11 10 07  45.5 -16.3  2.5     133.0    28      275   00 51 00
01 00 30  ---          11 19 39  44.9 -17.0  2.6     130.2   570      293   00 51 01

01 01 00  0836+710     11 20 09  44.9 -17.1  2.6     130.0    28      293   01 01 00
01 11 00  ---          11 30 10  44.2 -17.8  2.8     127.2   600      312   01 01 01

 ---------- GROUND ONLY: L-band VLBI scans: Block 02 ----------

01 11 30  0836+710     11 30 40  44.2 -17.8  2.8     127.0    28      312   01 11 30
01 17 00  ---          11 36 11  43.8 -18.2  2.9     125.5   330      323   01 11 31

01 17 30  0836+710     11 36 41  43.8 -18.2  2.9     125.3    28      323   01 17 30
01 27 00  ---          11 46 13  43.1 -18.8  3.1     122.7   570      341   01 17 31

01 27 30  0836+710     11 46 43  43.1 -18.9  3.1     122.5    28      341   01 27 30
01 37 00  ---          11 56 15  42.4 -19.4  3.2     119.9   570      360   01 27 31

01 37 30  0836+710     11 56 45  42.4 -19.4  3.2     119.8    28      360   01 37 30
01 47 00  ---          12 06 16  41.7 -19.9  3.4     117.2   570      378   01 37 31

01 47 30  0836+710     12 06 46  41.7 -20.0  3.4     117.0    28      378   01 47 30
01 57 00  ---          12 16 18  41.0 -20.4  3.6     114.5   570      396   01 47 31

01 57 30  0836+710     12 16 48  40.9 -20.4  3.6     114.4    28      396   01 57 30
02 07 00  ---          12 26 19  40.2 -20.8  3.7     111.8   570      414   01 57 31

02 07 30  0836+710     12 26 50  40.2 -20.9  3.7     111.7    28      414   02 07 30
02 17 00  ---          12 36 21  39.4 -21.2  3.9     109.2   570      433   02 07 31

 ---------- Segment 03: L-band VLBI scans ----------

02 18 00  0836+710     12 37 21  39.4 -21.3  3.9     109.0    58      433   02 18 00
02 27 30  ---          12 46 53  38.6 -21.6  4.1     106.5   570      451   02 18 01
Schedule for SHANGHAI  (Code Sh )                                   Page   4
               Probing the innermost regions of AGN jets and their magnetic fields
  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
----------------------------------------------------------------------------------------

 --- Fri  25 Oct 2013   Day 298 ---

02 28 00  0836+710     12 47 23  38.6 -21.6  4.1     106.4    28      451   02 28 00
02 37 30  ---          12 56 54  37.8 -21.8  4.2     104.0   570      469   02 28 01

02 38 00  0836+710     12 57 25  37.8 -21.8  4.2     103.9    28      469   02 38 00
02 47 30  ---          13 06 56  37.0 -22.1  4.4     101.5   570      487   02 38 01

02 48 00  0836+710     13 07 26  37.0 -22.1  4.4     101.4    28      487   02 48 00
02 57 30  ---          13 16 58  36.2 -22.2  4.6      99.0   570      506   02 48 01

02 58 00  0836+710     13 17 28  36.2 -22.3  4.6      98.9    28      506   02 58 00
03 08 00  ---          13 27 29  35.4 -22.4  4.7      96.4   600      525   02 58 01

 ---------- GROUND ONLY: L-band VLBI scans: Block 03 ----------

03 08 30  0836+710     13 28 00  35.3 -22.4  4.8      96.3    28      525   03 08 30
03 14 00  ---          13 33 30  34.9 -22.5  4.8      95.0   330      536   03 08 31

03 14 30  0836+710     13 34 01  34.8 -22.5  4.9      94.9    28      536   03 14 30
03 24 00  ---          13 43 32  34.0 -22.5  5.0      92.6   570      554   03 14 31

03 24 30  0836+710     13 44 02  34.0 -22.5  5.0      92.5    28      554   03 24 30
03 34 00  ---          13 53 34  33.2 -22.5  5.2      90.2   570      572   03 24 31

03 34 30  0836+710     13 54 04  33.2 -22.5  5.2      90.1    28      572   03 34 30
03 44 00  ---          14 03 35  32.4 -22.5  5.3      87.8   570      590   03 34 31

03 44 30  0836+710     14 04 05  32.4 -22.5  5.4      87.7    28      590   03 44 30
03 54 00  ---          14 13 37  31.6 -22.5  5.5      85.5   570      609   03 44 31

03 54 30  0836+710     14 14 07  31.5 -22.5  5.5      85.4    28      609   03 54 30
04 04 00  ---          14 23 39  30.8 -22.4  5.7      83.2   570      627   03 54 31

04 04 30  0836+710     14 24 09  30.7 -22.4  5.7      83.1    28      627   04 04 30
04 14 00  ---          14 33 40  29.9 -22.2  5.8      80.9   570      645   04 04 31

 ---------- Segment 04: L-band VLBI scans ----------

04 15 00  0836+710     14 34 40  29.9 -22.2  5.9      80.6    58      645   04 15 00
04 24 30  ---          14 44 12  29.1 -22.1  6.0      78.5   570      663   04 15 01

04 25 00  0836+710     14 44 42  29.0 -22.1  6.0      78.4    28      663   04 25 00
04 34 30  ---          14 54 14  28.3 -21.9  6.2      76.2   570      682   04 25 01

04 35 00  0836+710     14 54 44  28.2 -21.8  6.2      76.1    28      682   04 35 00
04 44 30  ---          15 04 15  27.5 -21.6  6.4      74.0   570      700   04 35 01
Schedule for SHANGHAI  (Code Sh )                                   Page   5
               Probing the innermost regions of AGN jets and their magnetic fields
  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
----------------------------------------------------------------------------------------

 --- Fri  25 Oct 2013   Day 298 ---

04 45 00  0836+710     15 04 45  27.5 -21.6  6.4      73.8    28      700   04 45 00
04 54 30  ---          15 14 17  26.7 -21.3  6.5      71.7   570      718   04 45 01

04 55 00  0836+710     15 14 47  26.7 -21.3  6.5      71.6    28      718   04 55 00
05 05 00  ---          15 24 49  25.9 -21.0  6.7      69.4   600      737   04 55 01

 ---------- GROUND ONLY: L-band VLBI scans: Block 04 ----------

05 05 30  0836+710     15 25 19  25.9 -21.0  6.7      69.3    28      737   05 05 30
05 11 00  ---          15 30 50  25.4 -20.8  6.8      68.0   330      748   05 05 31

05 11 30  0836+710     15 31 20  25.4 -20.8  6.8      67.9    28      748   05 11 30
05 21 00  ---          15 40 51  24.7 -20.5  7.0      65.8   570      766   05 11 31

05 21 30  0836+710     15 41 21  24.6 -20.4  7.0      65.7    28      766   05 21 30
05 31 00  ---          15 50 53  23.9 -20.1  7.1      63.6   570      785   05 21 31

05 31 30  0836+710     15 51 23  23.9 -20.1  7.1      63.5    28      785   05 31 30
05 41 00  ---          16 00 55  23.2 -19.7  7.3      61.4   570      803   05 31 31

05 41 30  0836+710     16 01 25  23.2 -19.6  7.3      61.3    28      803   05 41 30
05 51 00  ---          16 10 56  22.5 -19.2  7.5      59.2   570      821   05 41 31

05 51 30  0836+710     16 11 26  22.4 -19.2  7.5      59.1    28      821   05 51 30
06 01 00  ---          16 20 58  21.8 -18.8  7.6      57.0   570      839   05 51 31

06 01 30  0836+710     16 21 28  21.8 -18.7  7.6      56.9    28      839   06 01 30
06 11 00  ---          16 31 00  21.1 -18.3  7.8      54.8   570      858   06 01 31

 ---------- Segment 05: L-band VLBI scans ----------

06 12 00  0836+710     16 32 00  21.0 -18.2  7.8      54.6    58      858   06 12 00
06 21 30  ---          16 41 31  20.4 -17.7  8.0      52.5   570      876   06 12 01

06 22 00  0836+710     16 42 01  20.4 -17.7  8.0      52.4    28      876   06 22 00
06 31 30  ---          16 51 33  19.8 -17.2  8.1      50.4   570      894   06 22 01

06 32 00  0836+710     16 52 03  19.7 -17.1  8.2      50.2    28      894   06 32 00
06 41 30  ---          17 01 35  19.1 -16.6  8.3      48.2   570      912   06 32 01

06 42 00  0836+710     17 02 05  19.1 -16.6  8.3      48.1    28      912   06 42 00
06 51 30  ---          17 11 36  18.5 -16.0  8.5      46.0   570      931   06 42 01

06 52 00  0836+710     17 12 06  18.5 -16.0  8.5      45.9    28      931   06 52 00
07 02 00  ---          17 22 08  17.9 -15.4  8.7      43.7   600      950   06 52 01
Schedule for SHANGHAI  (Code Sh )                                   Page   6
               Probing the innermost regions of AGN jets and their magnetic fields
  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
----------------------------------------------------------------------------------------

 --- Fri  25 Oct 2013   Day 298 ---

 ---------- GROUND ONLY: L-band VLBI scans: Block 05 ----------

07 02 30  0836+710     17 22 38  17.9 -15.3  8.7      43.6    28      950   07 02 30
07 08 00  ---          17 28 09  17.6 -15.0  8.8      42.4   330      961   07 02 31

07 08 30  0836+710     17 28 39  17.6 -15.0  8.8      42.3    28      961   07 08 30
07 18 00  ---          17 38 11  17.0 -14.3  8.9      40.2   570      979   07 08 31

07 18 30  0836+710     17 38 41  17.0 -14.3  8.9      40.1    28      979   07 18 30
07 28 00  ---          17 48 12  16.5 -13.7  9.1      38.1   570      997   07 18 31

07 28 30  0836+710     17 48 42  16.5 -13.6  9.1      38.0    28      997   07 28 30
07 38 00  ---          17 58 14  16.0 -13.0  9.3      35.9   570     1015   07 28 31

07 38 30  0836+710     17 58 44  16.0 -12.9  9.3      35.8    28     1015   07 38 30
07 48 00  ---          18 08 15  15.6 -12.3  9.4      33.7   570     1034   07 38 31

07 48 30  0836+710     18 08 46  15.5 -12.2  9.4      33.6    28     1034   07 48 30
07 58 00  ---          18 18 17  15.1 -11.6  9.6      31.5   570     1052   07 48 31

07 58 30  0836+710     18 18 47  15.1 -11.5  9.6      31.4    28     1052   07 58 30
08 08 00  ---          18 28 19  14.7 -10.8  9.8      29.3   570     1070   07 58 31

 ---------- Segment 06: L-band VLBI scans ----------

08 09 00  0836+710     18 29 19  14.7 -10.8  9.8      29.1    58     1070   08 09 00
08 18 30  ---          18 38 50  14.3 -10.0  9.9      27.1   570     1088   08 09 01

08 19 00  0836+710     18 39 21  14.3 -10.0  9.9      27.0    28     1088   08 19 00
08 28 30  ---          18 48 52  13.9  -9.3 10.1      24.9   570     1107   08 19 01

08 29 00  0836+710     18 49 22  13.9  -9.2 10.1      24.8    28     1107   08 29 00
08 38 30  ---          18 58 54  13.6  -8.5 10.3      22.7   570     1125   08 29 01

08 39 00  0836+710     18 59 24  13.6  -8.5 10.3      22.6    28     1125   08 39 00
08 48 30  ---          19 08 55  13.3  -7.7 10.4      20.5   570     1143   08 39 01

08 49 00  0836+710     19 09 25  13.3  -7.7 10.4      20.4    28     1143   08 49 00
08 59 00  ---          19 19 27  13.0  -6.9 10.6      18.2   600     1162   08 49 01

 ---------- GROUND ONLY: L-band VLBI scans: Block 06 ----------

08 59 30  0836+710     19 19 57  13.0  -6.8 10.6      18.1    28     1162   08 59 30
09 05 00  ---          19 25 28  12.9  -6.4 10.7      16.9   330     1173   08 59 31
Schedule for SHANGHAI  (Code Sh )                                   Page   7
               Probing the innermost regions of AGN jets and their magnetic fields
  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
----------------------------------------------------------------------------------------

 --- Fri  25 Oct 2013   Day 298 ---

09 05 30  0836+710     19 25 58  12.9  -6.4 10.7      16.8    28     1173   09 05 30
09 15 00  ---          19 35 30  12.6  -5.6 10.9      14.7   570     1191   09 05 31

09 15 30  0836+710     19 36 00  12.6  -5.5 10.9      14.6    28     1191   09 15 30
09 25 00  ---          19 45 31  12.4  -4.8 11.0      12.5   570     1210   09 15 31

09 25 30  0836+710     19 46 01  12.4  -4.7 11.1      12.4    28     1210   09 25 30
09 35 00  ---          19 55 33  12.3  -3.9 11.2      10.3   570     1228   09 25 31

09 35 30  0836+710     19 56 03  12.3  -3.9 11.2      10.2    28     1228   09 35 30
09 45 00  ---          20 05 35  12.2  -3.1 11.4       8.1   570     1246   09 35 31

09 45 30  0836+710     20 06 05  12.1  -3.1 11.4       8.0    28     1246   09 45 30
09 55 00  ---          20 15 36  12.1  -2.3 11.5       5.9   570     1264   09 45 31

09 55 30  0836+710     20 16 06  12.0  -2.2 11.6       5.8    28     1264   09 55 30
10 05 00  ---          20 25 38  12.0  -1.4 11.7       3.8   570     1283   09 55 31

 ---------- Segment 07: L-band VLBI scans ----------

10 06 00  0836+710     20 26 38  12.0  -1.4 11.7       3.5    58     1283   10 06 00
10 15 30  ---          20 36 10  11.9  -0.6 11.9       1.4   570     1301   10 06 01

10 16 00  0836+710     20 36 40  11.9  -0.5 11.9       1.3    28     1301   10 16 00
10 25 30  ---          20 46 11  11.9   0.3-11.9      -0.7   570     1319   10 16 01

10 26 00  0836+710     20 46 41  11.9   0.3-11.9      -0.9    28     1319   10 26 00
10 35 30  ---          20 56 13  12.0   1.1-11.8      -2.9   570     1337   10 26 01

10 36 00  0836+710     20 56 43  12.0   1.2-11.8      -3.0    28     1337   10 36 00
10 45 30  ---          21 06 15  12.0   2.0-11.6      -5.1   570     1356   10 36 01

10 46 00  0836+710     21 06 45  12.0   2.0-11.6      -5.2    28     1356   10 46 00
10 56 00  ---          21 16 46  12.1   2.8-11.4      -7.4   600     1375   10 46 01

 ---------- GROUND ONLY: L-band VLBI scans: Block 07 ----------

10 56 30  0836+710     21 17 16  12.1   2.9-11.4      -7.5    28     1375   10 56 30
11 02 00  ---          21 22 47  12.2   3.3-11.3      -8.8   330     1386   10 56 31

11 02 30  0836+710     21 23 17  12.2   3.4-11.3      -8.9    28     1386   11 02 30
11 12 00  ---          21 32 49  12.3   4.2-11.2     -10.9   570     1404   11 02 31

11 12 30  0836+710     21 33 19  12.3   4.2-11.2     -11.1    28     1404   11 12 30
11 22 00  ---          21 42 51  12.5   5.0-11.0     -13.1   570     1422   11 12 31
Schedule for SHANGHAI  (Code Sh )                                   Page   8
               Probing the innermost regions of AGN jets and their magnetic fields
  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
----------------------------------------------------------------------------------------

 --- Fri  25 Oct 2013   Day 298 ---

11 22 30  0836+710     21 43 21  12.5   5.0-11.0     -13.2    28     1422   11 22 30
11 32 00  ---          21 52 52  12.7   5.8-10.8     -15.3   570     1440   11 22 31

11 32 30  0836+710     21 53 22  12.7   5.9-10.8     -15.4    28     1440   11 32 30
11 42 00  ---          22 02 54  12.9   6.6-10.7     -17.5   570     1459   11 32 31

11 42 30  0836+710     22 03 24  12.9   6.7-10.7     -17.6    28     1459   11 42 30
11 52 00  ---          22 12 56  13.2   7.4-10.5     -19.7   570     1477   11 42 31

11 52 30  0836+710     22 13 26  13.2   7.5-10.5     -19.8    28     1477   11 52 30
12 02 00  ---          22 22 57  13.5   8.2-10.3     -21.9   570     1495   11 52 31

 ---------- Segment 08: L-band VLBI scans ----------

12 03 00  0836+710     22 23 57  13.5   8.3-10.3     -22.1    58     1495   12 03 00
12 12 30  ---          22 33 29  13.8   9.0-10.2     -24.2   570     1513   12 03 01

12 13 00  0836+710     22 33 59  13.8   9.1-10.1     -24.3    28     1513   12 13 00
12 22 30  ---          22 43 31  14.2   9.8-10.0     -26.4   570     1532   12 13 01

12 23 00  0836+710     22 44 01  14.2   9.8-10.0     -26.5    28     1532   12 23 00
12 32 30  ---          22 53 32  14.6  10.6 -9.8     -28.5   570     1550   12 23 01

12 33 00  0836+710     22 54 02  14.6  10.6 -9.8     -28.6    28     1550   12 33 00
12 42 30  ---          23 03 34  15.0  11.3 -9.7     -30.7   570     1568   12 33 01

12 43 00  0836+710     23 04 04  15.0  11.3 -9.6     -30.8    28     1568   12 43 00
12 53 00  ---          23 14 06  15.4  12.1 -9.5     -33.0   600     1587   12 43 01

 ---------- GROUND ONLY: L-band VLBI scans: Block 08 ----------

12 53 30  0836+710     23 14 36  15.4  12.1 -9.5     -33.1    28     1587   12 53 30
12 59 00  ---          23 20 07  15.7  12.5 -9.4     -34.3   330     1598   12 53 31


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


 ======== Setup file: ra18cm2.set
   Matching groups in ./gl038a.freq.sess313rdbe.dat:
     sh18cm          Huang Xinyong 27Sept05

   Setup group:   18         Station: SHANGHAI          Total bit rate:   256
   Format: MARK5B            Bits per sample: 2         Sample rate: 32.000
   Number of channels:  4    DBE type:                  Speedup factor:   1.00

   Disk used to record data.

   1st LO=   2300.00   2300.00   2300.00   2300.00
   Net SB=         L         L         U         U
   IF SB =         L         L         L         L
   Pol.  =      RCP       LCP       RCP       LCP 
   BBC   =         1         2         1         2
   BBC SB=         U         U         L         L
   IF    =        C         A         C         A 

  The following frequency sets based on these setups were used.

   Frequency Set:  12  Setup file default.  Used pcal sets:   1
   LO sum=   1668.00  1668.00  1668.00  1668.00
   BBC fr=    632.00   632.00   632.00   632.00
   Bandwd=     16.00    16.00    16.00    16.00
    Matching frequency sets:  12

  The following pulse cal sets were used with this setup:

   Pulse cal detection set:   1  PCAL = 1MHZ
    PCALXB1=   S1    S3    S1    S3    S1    S2    S3    S4 
    PCALXB2=   S2    S4    S2    S4    M1    M2    M3    M4 
    PCALFR1=  1000  1000 13000 13000     0     0     0     0
    PCALFR2=  1000  1000 13000 13000     0     0     0     0

   Track assignments are: 
    track1=   2,  4,  6,  8
    barrel=roll_off 

 POSITIONS OF SOURCES USED IN RECORDING SCANS

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

 * FAKERA            11 57 21.769299   * 12 00 00.000000     12 00 25.374091       0.00
                     85 16 41.77889    * 85 00 00.00000      84 55 09.02682        0.00
                     From catalog imbedded in main SCHED input file.
                     fake circumpolar target for a TS to look at

   J0841+7053        08 36 21.556645   * 08 41 24.365283     08 42 47.118679       0.31
 * 0836+710          71 04 22.42740    * 70 53 42.17302      70 50 18.47640        0.10
   J0841+70          ./gl038a.sources.vlba
                     rfc_2012b Petrov, 2012, unpublished 4322 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
  FAKERA     ra18cm2.set           22                                6.883     0.000
  0836+710   ra18cm2.set           1 2 3 4 5 6 7 8 11 12 13 22 +    14.333  3318.856


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) 
   FAKERA              97.7
   0836+710            98.0

  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 

