  COVER INFORMATION 

 Station:    SHANGHAI  (Code Sh ) 
 Experiment: Type-2 quasars
 Exp. Code:  EK022A  


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

PI:       Hans-Rainer Kloeckner                                           

Address:  University of Oxford                                            
          Keble Road,Oxford OX1 3RH                                       
          United Kingdom                                                  
                                                                          

Phone:    +44 1865 273435                                                 
EMAIL:    hrk@astro.ox.ac.uk                                              
Fax:      +44 1865 273390                                                 
Phone during observation: +44 1865 273435                                 

Observing mode: 1 Gbit at 18cm                                            

Notes:     >>> THANK YOU <<<                                              
                                                                          
                                                                          
                                                                          

Schedule for SHANGHAI  (Code Sh )                                   Page   2
               Type-2 quasars
  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
----------------------------------------------------------------------------------------

 --- Sat  29 Oct 2005   Day 302 ---

 Next scan frequencies:  1610.49  1610.49  1610.49  1610.49  1642.49  1642.49
                         1642.49  1642.49  1674.49  1674.49  1674.49  1674.49
                         1706.49  1706.49  1706.49  1706.49
 Next BBC frequencies:    689.51   689.51   689.51   689.51   657.51   657.51
                          657.51   657.51   625.51   625.51   625.51   625.51
                          593.51   593.51   593.51   593.51
 Next scan bandwidths:     16.00    16.00    16.00    16.00    16.00    16.00
                           16.00    16.00    16.00    16.00    16.00    16.00
                           16.00    16.00    16.00    16.00

09 30 00  J1722+5856   20 06 04  51.0 -32.4  2.7     117.2     0   1  1      0  09 30 00
09 35 00  =1721+589    20 11 04  50.4 -32.9  2.8     115.8   300   F  1      0  09 30 10

09 35 00  J1722+6105   20 11 04  49.4 -29.9  2.8     118.1    -8   1  1      0  09 35 00
09 41 00  =1722+611    20 17 05  48.8 -30.4  2.9     116.4   352   F  1      0  09 35 10

09 42 00  J1722+5856   20 18 06  49.6 -33.4  2.9     113.9    52   1  1      0  09 42 00
09 45 00  =1721+589    20 21 06  49.2 -33.7  3.0     113.0   180   F  1      0  09 42 10

09 45 00  AMS16        20 21 06  48.9 -34.1  3.0     112.1    -3   1  1      0  09 45 00
09 53 00  ---          20 29 07  47.9 -34.7  3.2     109.9   477   F  1      0  09 45 10

09 54 00  J1722+5856   20 30 08  48.1 -34.3  3.1     110.6    57   1  1      0  09 54 00
09 57 00  =1721+589    20 33 08  47.8 -34.5  3.2     109.8   180   F  1      0  09 54 10

09 57 00  AMS16        20 33 08  47.5 -34.9  3.2     108.9    -3   1  1      0  09 57 00
10 05 00  ---          20 41 09  46.5 -35.4  3.4     106.8   477   F  1      0  09 57 10

10 06 00  J1722+5856   20 42 10  46.7 -35.1  3.3     107.5    57   1  1      0  10 06 00
10 09 00  =1721+589    20 45 10  46.3 -35.2  3.4     106.7   180   F  1      0  10 06 10

10 09 00  AMS15        20 45 10  45.8 -35.3  3.4     105.9    -4   1  1      0  10 09 00
10 17 00  ---          20 53 11  44.8 -35.7  3.6     103.9   476   F  1      0  10 09 10

10 18 00  J1722+5856   20 54 12  45.2 -35.7  3.5     104.5    57   1  1      0  10 18 00
10 21 00  =1721+589    20 57 12  44.8 -35.8  3.6     103.7   180   F  1      0  10 18 10

10 21 00  AMS15        20 57 12  44.3 -35.8  3.6     102.9    -4   1  1      0  10 21 00
10 29 00  ---          21 05 13  43.3 -36.1  3.8     101.0   476   F  1      0  10 21 10

10 30 00  J1722+5856   21 06 14  43.6 -36.2  3.7     101.5    57   1  1      0  10 30 00
10 33 00  =1721+589    21 09 14  43.3 -36.3  3.8     100.8   180   F  1      0  10 30 10
Schedule for SHANGHAI  (Code Sh )                                   Page   3
               Type-2 quasars
  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
----------------------------------------------------------------------------------------

 --- Sat  29 Oct 2005   Day 302 ---

10 33 00  AMS17        21 09 14  43.0 -36.4  3.8     100.3    -3   1  1      0  10 33 00
10 41 00  ---          21 17 15  42.0 -36.7  3.9      98.5   477   F  1      0  10 33 10

10 42 00  J1722+5856   21 18 15  42.1 -36.6  3.9      98.7    58   1  1      0  10 42 00
10 45 00  =1721+589    21 21 16  41.7 -36.6  4.0      98.0   180   F  1      0  10 42 10

10 45 00  AMS17        21 21 16  41.5 -36.8  4.0      97.5    -3   1  1      0  10 45 00
10 53 00  ---          21 29 17  40.5 -36.9  4.1      95.7   477   F  1      0  10 45 10

10 54 00  J1722+5856   21 30 17  40.6 -36.8  4.1      96.0    58   1  1      0  10 54 00
10 57 00  =1721+589    21 33 18  40.2 -36.9  4.2      95.3   180   F  1      0  10 54 10

10 57 00  AMS12        21 33 18  39.6 -36.8  4.2      94.4    -4   1  1      0  10 57 00
11 05 00  ---          21 41 19  38.6 -36.9  4.4      92.6   476   F  1      0  10 57 10

11 06 00  J1722+5856   21 42 19  39.0 -37.0  4.3      93.3    57   1  1      0  11 06 00
11 09 00  =1721+589    21 45 20  38.6 -37.0  4.4      92.6   180   F  1      0  11 06 10

11 09 00  AMS12        21 45 20  38.1 -36.9  4.4      91.8    -4   1  1      0  11 09 00
11 17 00  ---          21 53 21  37.1 -36.9  4.6      90.0   476   F  1      0  11 09 10

11 18 00  J1722+5856   21 54 21  37.5 -37.1  4.5      90.7    57   1  1      0  11 18 00
11 23 00  =1721+589    21 59 22  36.8 -37.1  4.6      89.6   300   F  1      0  11 18 10

11 23 00  J1722+6105   21 59 22  36.8 -34.4  4.6      91.2    -7   1  1      0  11 23 00
11 29 00  =1722+611    22 05 23  36.1 -34.4  4.7      89.9   353   F  1      0  11 23 10

11 30 00  J1722+5856   22 06 23  35.9 -37.0  4.7      88.1    53   1  1      0  11 30 00
11 33 00  =1721+589    22 09 24  35.5 -37.0  4.8      87.5   180   F  1      0  11 30 10

11 34 00  3C345        22 10 24  25.1 -57.1  5.5      69.4    18   1  1      0  11 34 00
11 45 00  ---          22 21 26  23.1 -56.3  5.6      68.0   660   F  1      0  11 34 10

11 48 00  J1722+5856   22 24 26  33.6 -36.8  5.0      84.3   139   1  1      0  11 48 00
11 51 00  =1721+589    22 27 27  33.2 -36.8  5.1      83.7   180   F  1      0  11 48 10

11 51 00  AMS16        22 27 27  32.8 -36.9  5.1      83.0    -3   1  1      0  11 51 00
11 59 00  ---          22 35 28  31.8 -36.8  5.3      81.4   477   F  1      0  11 51 10

12 00 00  J1722+5856   22 36 28  32.1 -36.6  5.2      81.9    57   1  1      0  12 00 00
12 03 00  =1721+589    22 39 29  31.7 -36.6  5.3      81.3   180   F  1      0  12 00 10

12 03 00  AMS16        22 39 29  31.3 -36.7  5.3      80.6    -3   1  1      0  12 03 00
12 11 00  ---          22 47 30  30.3 -36.5  5.5      79.0   477   F  1      0  12 03 10
Schedule for SHANGHAI  (Code Sh )                                   Page   4
               Type-2 quasars
  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
----------------------------------------------------------------------------------------

 --- Sat  29 Oct 2005   Day 302 ---

12 12 00  J1722+5856   22 48 30  30.5 -36.3  5.4      79.5    57   1  1      0  12 12 00
12 15 00  =1721+589    22 51 31  30.2 -36.2  5.5      78.9   180   F  1      0  12 12 10

12 15 00  AMS15        22 51 31  29.7 -36.0  5.5      78.2    -3   1  1      0  12 15 00
12 23 00  ---          22 59 32  28.7 -35.7  5.7      76.6   477   F  1      0  12 15 10

12 24 00  J1722+5856   23 00 32  29.0 -36.0  5.6      77.1    57   1  1      0  12 24 00
12 27 00  =1721+589    23 03 33  28.6 -35.9  5.7      76.5   180   F  1      0  12 24 10

12 27 00  AMS15        23 03 33  28.2 -35.6  5.7      75.8    -3   1  1      0  12 27 00
12 35 00  ---          23 11 34  27.2 -35.3  5.9      74.2   477   F  1      0  12 27 10

12 36 00  J1722+5856   23 12 34  27.5 -35.5  5.8      74.7    57   1  1      0  12 36 00
12 39 00  =1721+589    23 15 35  27.1 -35.4  5.9      74.1   180   F  1      0  12 36 10

12 39 00  AMS17        23 15 35  26.9 -35.4  5.9      73.7    -3   1  1      0  12 39 00
12 47 00  ---          23 23 36  25.9 -35.1  6.0      72.1   477   F  1      0  12 39 10

12 48 00  J1722+5856   23 24 36  26.0 -35.0  6.0      72.3    58   1  1      0  12 48 00
12 51 00  =1721+589    23 27 37  25.7 -34.9  6.1      71.7   180   F  1      0  12 48 10

12 51 00  AMS17        23 27 37  25.4 -34.9  6.1      71.4    -3   1  1      0  12 51 00
12 59 00  ---          23 35 38  24.4 -34.5  6.2      69.8   477   F  1      0  12 51 10

13 00 00  J1722+5856   23 36 38  24.6 -34.5  6.2      70.0    58   1  1      0  13 00 00
13 03 00  =1721+589    23 39 39  24.2 -34.3  6.3      69.4   180   F  1      0  13 00 10

13 03 00  AMS12        23 39 39  23.7 -34.0  6.4      68.6    -4   1  1      0  13 03 00
13 11 00  ---          23 47 40  22.8 -33.6  6.5      67.1   476   F  1      0  13 03 10

13 12 00  J1722+5856   23 48 40  23.1 -33.9  6.4      67.7    57   1  1      0  13 12 00
13 15 00  =1721+589    23 51 41  22.7 -33.7  6.5      67.1   180   F  1      0  13 12 10

13 15 00  AMS12        23 51 41  22.3 -33.4  6.6      66.3    -4   1  1      0  13 15 00
13 23 00  ---          23 59 42  21.3 -32.9  6.7      64.8   476   F  1      0  13 15 10

13 24 00  J1722+5856   00 00 42  21.7 -33.2  6.6      65.3    57   1  1      0  13 24 00
13 27 00  =1721+589    00 03 43  21.3 -33.0  6.7      64.8   180   F  1      0  13 24 10

13 42 00  J2005+7752   00 18 45  35.8 -13.4  4.2     109.2   850   1  1      0  13 42 00
13 53 00  =2007+777    00 29 47  35.3 -13.6  4.4     106.4   660   F  1      0  13 42 10

13 55 00  J1722+5856   00 31 47  18.1 -31.2  7.2      59.4    61   1  1      0  13 55 00
13 58 00  =1721+589    00 34 48  17.8 -31.0  7.2      58.8   180   F  1      0  13 55 10
Schedule for SHANGHAI  (Code Sh )                                   Page   5
               Type-2 quasars
  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
----------------------------------------------------------------------------------------

 --- Sat  29 Oct 2005   Day 302 ---

13 58 00  J1722+6105   00 34 48  18.9 -29.1  7.2      59.4    -6   1  1      0  13 58 00
14 03 00  =1722+611    00 39 48  18.4 -28.7  7.3      58.4   294   F  1      0  13 58 10

14 04 00  J1722+5856   00 40 49  17.1 -30.6  7.3      57.6    54   1  1      0  14 04 00
14 07 00  =1721+589    00 43 49  16.8 -30.4  7.4      57.0   180   F  1      0  14 04 10

14 07 00  AMS16        00 43 49  16.4 -30.3  7.4      56.4    -3   1  1      0  14 07 00
14 15 00  ---          00 51 50  15.6 -29.7  7.5      54.9   477   F  1      0  14 07 10

14 16 00  J1722+5856   00 52 51  15.8 -29.7  7.5      55.3    57   1  1      0  14 16 00
14 19 00  =1721+589    00 55 51  15.5 -29.5  7.6      54.7   180   F  1      0  14 16 10

14 19 00  AMS16        00 55 51  15.1 -29.4  7.6      54.1    -3   1  1      0  14 19 00
14 27 00  ---          01 03 52  14.3 -28.7  7.7      52.6   477   F  1      0  14 19 10

14 28 00  J1722+5856   01 04 53  14.6 -28.8  7.7      53.0    57   1  1      0  14 28 00
14 31 00  =1721+589    01 07 53  14.3 -28.5  7.8      52.4   180   F  1      0  14 28 10

14 31 00  AMS15        01 07 53  14.0 -28.1  7.8      51.7    -3   1  1      0  14 31 00
14 39 00  ---          01 15 54  13.2 -27.4  7.9      50.1   477   F  1      0  14 31 10

14 40 00  J1722+5856   01 16 55  13.4 -27.8  7.9      50.6    57   1  1      0  14 40 00
14 43 00  =1721+589    01 19 55  13.1 -27.5  8.0      50.0   180   F  1      0  14 40 10

14 43 00  AMS15        01 19 55  12.8 -27.1  8.0      49.3    -3   1  1      0  14 43 00
14 51 00  ---          01 27 56  12.0 -26.4  8.1      47.8   477   F  1      0  14 43 10

14 52 00  J1722+5856   01 28 57  12.2 -26.7  8.1      48.3    57   1  1      0  14 52 00
14 55 00  =1721+589    01 31 57  11.9 -26.5  8.2      47.7   180   F  1      0  14 52 10

14 55 00  AMS17        01 31 57  11.7 -26.3  8.2      47.3    -3   1  1      0  14 55 00
15 03 00  ---          01 39 58  10.9 -25.6  8.3      45.7   477   F  1      0  14 55 10

15 04 00  J1722+5856   01 40 59  11.1 -25.7  8.3      45.9    58   1  1      0  15 04 00
15 07 00  =1721+589    01 43 59  10.8 -25.4  8.4      45.3   180   F  1      0  15 04 10

15 07 00  AMS17        01 43 59  10.6 -25.3  8.4      45.0    -3   1  1      0  15 07 00
15 15 00  ---          01 52 00   9.8 -24.5  8.5      43.4   477   F  1      0  15 07 10

15 16 00  J1722+5856   01 53 00  10.0 -24.5  8.5      43.5    58   1  1      0  15 16 00
15 19 00  =1721+589    01 56 01   9.7 -24.2  8.6      43.0   180   F  1      0  15 16 10

15 19 00  AMS12        01 56 01   9.4 -23.8  8.6      42.1    -3   1  1      0  15 19 00
15 27 00  ---          02 04 02   8.7 -23.0  8.8      40.5   477   F  1      0  15 19 10
Schedule for SHANGHAI  (Code Sh )                                   Page   6
               Type-2 quasars
  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
----------------------------------------------------------------------------------------

 --- Sat  29 Oct 2005   Day 302 ---

15 28 00  J1722+5856   02 05 02   8.9 -23.4  8.7      41.2    57   1  1      0  15 28 00
15 31 00  =1721+589    02 08 03   8.7 -23.1  8.8      40.6   180   F  1      0  15 28 10

15 31 00  AMS12        02 08 03   8.4 -22.6  8.8      39.7    -3   1  1      0  15 31 00
15 39 00  ---          02 16 04   7.7 -21.8  9.0      38.1   477   F  1      0  15 31 10

15 40 00  J1722+5856   02 17 04   7.9 -22.2  8.9      38.8    57   1  1      0  15 40 00
15 45 00  =1721+589    02 22 05   7.5 -21.7  9.0      37.8   300   F  1      0  15 40 10

15 45 00  J1722+6105   02 22 05   9.2 -20.3  9.0      38.0    -8   1  1      0  15 45 00
15 51 00  =1722+611    02 28 06   8.8 -19.7  9.1      36.7   352   F  1      0  15 45 10

15 52 00  J1722+5856   02 29 06   7.0 -20.9  9.1      36.3    52   1  1      0  15 52 00
15 55 00  =1721+589    02 32 07   6.7 -20.6  9.2      35.7   180   F  1      0  15 52 10

15 55 00  AMS16        02 32 07   6.4 -20.4  9.2      35.1    -3   1  1      0  15 55 00
16 03 00  ---          02 40 08   5.8 -19.5  9.3      33.5   477   F  1      0  15 55 10

16 04 00  J1722+5856   02 41 08   6.1 -19.6  9.3      33.9    57   1  1      0  16 04 00
16 07 00  =1721+589    02 44 09   5.9 -19.3  9.4      33.3   180   F  1      0  16 04 10

16 16 00  J1722+5856   02 53 10   5.2 -18.3  9.5      31.5   536   1  1      0  16 16 00
16 19 00  =1721+589    02 56 11   5.0 -18.0  9.6      30.8   180   F  1      0  16 16 10


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


 Setup file: 1Gbs.18cm
   Matches group sh18cm in ./hrkfreq.dat
    Huang Xinyong 27Sept05

   Setup group:    9         Station: SHANGHAI          Total bit rate: 1024
   Format: MKIV1:2           Bits per sample: 2         Sample rate: 32.000
   Number of channels: 16                               Speedup factor:   0.50

   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
   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 this setup were used.

   Frequency Set:   9  Setup file default.  Used pcal sets:   1
   LO sum=    1610.49   1610.49   1610.49   1610.49   1642.49   1642.49   1642.49   1642.49
              1674.49   1674.49   1674.49   1674.49   1706.49   1706.49   1706.49   1706.49
   BBC fr=     689.51    689.51    689.51    689.51    657.51    657.51    657.51    657.51
               625.51    625.51    625.51    625.51    593.51    593.51    593.51    593.51
   Bandwd=     16.000    16.000    16.000    16.000    16.000    16.000    16.000    16.000
               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    S9    S11   S13   S15
    PCALXB2=   S2    S4    S6    S8    S10   S12   S14   S16
    PCALFR1=   490   510   490   510   490   510   490   510
    PCALFR2=   490   510   490   510   490   510   490   510

   Track assignments are: 
    track1=   2, 10, 18, 26,  3, 11, 19, 27, 66, 74, 82, 90, 67, 75, 83, 91
    barrel=roll_off 
 SOURCE LIST -- Type-2 quasars
     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)

 * AMS12             17 17 38.418600   * 17 18 22.650000     17 18 25.969615       0.00
                     59 04 56.72127    * 59 01 54.25800      59 01 38.74536        0.00
                     From catalog imbedded in main SCHED input file.
                        1.000 scan hours,     32.948 baseline hours above horizon.

 * AMS15             17 18 12.853809   * 17 18 56.927000     17 19 00.228742       0.00
                     59 06 24.95149    * 59 03 24.95000      59 03 09.74694        0.00
                     From catalog imbedded in main SCHED input file.
                        1.067 scan hours,     34.855 baseline hours above horizon.

 * AMS16             17 18 56.894176   * 17 19 42.074000     17 19 45.517372       0.00
                     58 50 05.71563    * 58 47 08.91100      58 46 54.11159        0.00
                     From catalog imbedded in main SCHED input file.
                        1.067 scan hours,     35.948 baseline hours above horizon.

 * AMS17             17 20 00.448488   * 17 20 45.170000     17 20 48.559501       0.00
                     58 55 13.59647    * 58 52 21.33500      58 52 07.10658        0.00
                     From catalog imbedded in main SCHED input file.
                        1.067 scan hours,     35.053 baseline hours above horizon.

   J1642+3948        16 41 17.606231   * 16 42 58.809968     16 43 09.119068       0.26
   1641+399          39 54 10.81493    * 39 48 36.99399      39 48 02.10034        0.40
 * 3C345             /data/soay/hrk/HRKSOFTWAREBOX/SCHED_6.02/catalogs/sources.vlba
   J1642+39          VLBA Calib Srcs - GSFC sols. - catalog 2004f_astro
                        0.183 scan hours,      5.893 baseline hours above horizon.

 * J1722+5856        17 21 52.440263   * 17 22 36.726557     17 22 40.067948       0.62
   1721+589          58 59 06.49428    * 58 56 22.26066      58 56 09.04151        0.49
                     /data/soay/hrk/HRKSOFTWAREBOX/SCHED_6.02/catalogs/sources.vlba
                     VLBA Calib Srcs - GSFC sols. - catalog 2004f_astro
                        2.050 scan hours,     71.221 baseline hours above horizon.

 * J1722+6105        17 22 05.759508   * 17 22 40.059358     17 22 42.145684       0.52
   1722+611          61 08 43.42140    * 61 05 59.78729      61 05 46.62183        0.45
                     /data/soay/hrk/HRKSOFTWAREBOX/SCHED_6.02/catalogs/sources.vlba
                     VLBA Calib Srcs - GSFC sols. - catalog 2004f_astro
                        0.433 scan hours,     13.733 baseline hours above horizon.

 * J2005+7752        20 07 20.430184   * 20 05 30.998512     20 05 15.808903       0.96
   2007+777          77 43 58.12306    * 77 52 43.24759      77 53 55.45504        0.40
   J2005+77          /data/soay/hrk/HRKSOFTWAREBOX/SCHED_6.02/catalogs/sources.vlba
                     VLBA Calib Srcs - GSFC sols. - catalog 2004f_astro
                        0.183 scan hours,      6.283 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) 
   AMS12               81.5
   AMS15               81.6
   AMS16               81.4
   AMS17               81.6
   3C345               63.5
   J1722+5856          81.8
   J1722+6105          83.3
   J2005+7752         102.7

  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 

