  COVER INFORMATION 

 Station:    SHANGHAI  (Code Sh ) 
 Experiment: Type-2 quasars
 Exp. Code:  EK022B  


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 Gbs 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
----------------------------------------------------------------------------------------

 --- Sun  30 Oct 2005   Day 303 ---

 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 10 00  50.5 -32.8  2.8     116.1     0   1  1      0  09 30 00
09 35 00  =1721+589    20 15 01  49.9 -33.2  2.9     114.7   300   F  1      0  09 30 10

09 35 00  J1722+6105   20 15 01  49.0 -30.2  2.9     117.0    -8   1  1      0  09 35 00
09 41 00  =1722+611    20 21 02  48.3 -30.7  3.0     115.3   352   F  1      0  09 35 10

09 42 00  J1722+5856   20 22 02  49.1 -33.8  3.0     112.8    52   1  1      0  09 42 00
09 45 00  =1721+589    20 25 03  48.7 -34.0  3.0     112.0   180   F  1      0  09 42 10

09 45 00  AMS01        20 25 03  47.3 -33.2  3.2     110.5    -7   1  1      0  09 45 00
09 53 00  ---          20 33 04  46.3 -33.7  3.3     108.4   473   F  1      0  09 45 10

09 54 00  J1722+5856   20 34 04  47.6 -34.6  3.2     109.6    54   1  1      0  09 54 00
09 57 00  =1721+589    20 37 05  47.3 -34.8  3.2     108.8   180   F  1      0  09 54 10

09 57 00  AMS01        20 37 05  45.8 -34.0  3.4     107.4    -7   1  1      0  09 57 00
10 05 00  ---          20 45 06  44.9 -34.4  3.5     105.3   473   F  1      0  09 57 10

10 06 00  J1722+5856   20 46 06  46.2 -35.3  3.4     106.5    54   1  1      0  10 06 00
10 09 00  =1721+589    20 49 07  45.8 -35.5  3.4     105.7   180   F  1      0  10 06 10

10 09 00  AMS06        20 49 07  44.4 -34.5  3.6     104.5    -7   1  1      0  10 09 00
10 17 00  ---          20 57 08  43.5 -34.8  3.7     102.5   473   F  1      0  10 09 10

10 18 00  J1722+5856   20 58 08  44.7 -35.9  3.6     103.5    54   1  1      0  10 18 00
10 21 00  =1721+589    21 01 09  44.3 -36.0  3.6     102.8   180   F  1      0  10 18 10

10 21 00  AMS06        21 01 09  43.0 -35.0  3.8     101.6    -6   1  1      0  10 21 00
10 29 00  ---          21 09 10  42.0 -35.2  3.9      99.7   474   F  1      0  10 21 10

10 30 00  J1722+5856   21 10 10  43.1 -36.3  3.8     100.6    54   1  1      0  10 30 00
10 33 00  =1721+589    21 13 11  42.8 -36.4  3.8      99.9   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
----------------------------------------------------------------------------------------

 --- Sun  30 Oct 2005   Day 303 ---

10 33 00  AMS05        21 13 11  41.5 -35.7  4.0      98.5    -6   1  1      0  10 33 00
10 41 00  ---          21 21 12  40.5 -35.9  4.1      96.6   474   F  1      0  10 33 10

10 42 00  J1722+5856   21 22 12  41.6 -36.7  4.0      97.8    54   1  1      0  10 42 00
10 45 00  =1721+589    21 25 13  41.2 -36.7  4.0      97.1   180   F  1      0  10 42 10

10 45 00  AMS05        21 25 13  40.0 -36.0  4.2      95.7    -6   1  1      0  10 45 00
10 53 00  ---          21 33 14  39.0 -36.1  4.3      93.9   474   F  1      0  10 45 10

10 54 00  J1722+5856   21 34 14  40.1 -36.9  4.2      95.1    54   1  1      0  10 54 00
10 57 00  =1721+589    21 37 14  39.7 -36.9  4.2      94.4   180   F  1      0  10 54 10

10 57 00  AMS03        21 37 14  38.5 -36.4  4.4      92.8    -6   1  1      0  10 57 00
11 05 00  ---          21 45 16  37.5 -36.4  4.5      91.1   474   F  1      0  10 57 10

11 06 00  J1722+5856   21 46 16  38.5 -37.0  4.4      92.4    55   1  1      0  11 06 00
11 09 00  =1721+589    21 49 16  38.1 -37.0  4.4      91.8   180   F  1      0  11 06 10

11 09 00  AMS03        21 49 16  37.0 -36.4  4.6      90.2    -6   1  1      0  11 09 00
11 17 00  ---          21 57 18  36.0 -36.4  4.7      88.5   474   F  1      0  11 09 10

11 18 00  J1722+5856   21 58 18  37.0 -37.1  4.6      89.8    55   1  1      0  11 18 00
11 23 00  =1721+589    22 03 19  36.3 -37.0  4.7      88.7   300   F  1      0  11 18 10

11 23 00  J1722+6105   22 03 19  36.3 -34.4  4.7      90.3    -7   1  1      0  11 23 00
11 29 00  =1722+611    22 09 20  35.6 -34.4  4.8      89.0   353   F  1      0  11 23 10

11 30 00  J1722+5856   22 10 20  35.4 -37.0  4.8      87.3    53   1  1      0  11 30 00
11 33 00  =1721+589    22 13 20  35.0 -37.0  4.8      86.6   180   F  1      0  11 30 10

11 34 00  3C345        22 14 21  24.4 -56.8  5.5      68.9    18   1  1      0  11 34 00
11 45 00  ---          22 25 22  22.4 -56.0  5.7      67.5   660   F  1      0  11 34 10

11 48 00  J1722+5856   22 28 23  33.1 -36.8  5.1      83.5   140   1  1      0  11 48 00
11 51 00  =1721+589    22 31 23  32.7 -36.7  5.1      82.9   180   F  1      0  11 48 10

11 51 00  AMS01        22 31 23  31.7 -35.4  5.3      81.6    -6   1  1      0  11 51 00
11 59 00  ---          22 39 25  30.7 -35.2  5.4      80.0   474   F  1      0  11 51 10

12 00 00  J1722+5856   22 40 25  31.6 -36.5  5.3      81.1    55   1  1      0  12 00 00
12 03 00  =1721+589    22 43 25  31.2 -36.5  5.3      80.5   180   F  1      0  12 00 10

12 03 00  AMS01        22 43 25  30.2 -35.1  5.5      79.2    -5   1  1      0  12 03 00
12 11 00  ---          22 51 27  29.2 -34.8  5.6      77.5   475   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
----------------------------------------------------------------------------------------

 --- Sun  30 Oct 2005   Day 303 ---

12 12 00  J1722+5856   22 52 27  30.0 -36.2  5.5      78.7    55   1  1      0  12 12 00
12 15 00  =1721+589    22 55 27  29.7 -36.1  5.5      78.1   180   F  1      0  12 12 10

12 15 00  AMS06        22 55 27  28.8 -34.7  5.7      76.8    -5   1  1      0  12 15 00
12 23 00  ---          23 03 29  27.8 -34.4  5.8      75.2   475   F  1      0  12 15 10

12 24 00  J1722+5856   23 04 29  28.5 -35.8  5.7      76.3    55   1  1      0  12 24 00
12 27 00  =1721+589    23 07 29  28.1 -35.7  5.7      75.7   180   F  1      0  12 24 10

12 27 00  AMS06        23 07 29  27.3 -34.3  5.9      74.4    -5   1  1      0  12 27 00
12 35 00  ---          23 15 31  26.3 -34.0  6.0      72.8   475   F  1      0  12 27 10

12 35 00  J1722+5856   23 15 31  27.1 -35.4  5.9      74.1    -5   1  1      0  12 35 00
12 38 00  =1721+589    23 18 31  26.8 -35.3  5.9      73.5   175   F  1      0  12 35 10

12 39 00  J1722+5856   23 19 31  26.6 -35.3  5.9      73.3    58   1  1      0  12 39 00
12 42 00  =1721+589    23 22 32  26.3 -35.1  6.0      72.7   180   F  1      0  12 39 10

12 42 00  AMS05        23 22 32  25.4 -34.0  6.1      71.3    -5   1  1      0  12 42 00
12 50 00  ---          23 30 33  24.5 -33.6  6.3      69.7   475   F  1      0  12 42 10

12 51 00  J1722+5856   23 31 33  25.2 -34.7  6.1      71.0    56   1  1      0  12 51 00
12 54 00  =1721+589    23 34 34  24.8 -34.6  6.2      70.4   180   F  1      0  12 51 10

12 54 00  AMS05        23 34 34  24.0 -33.4  6.3      69.0    -5   1  1      0  12 54 00
13 02 00  ---          23 42 35  23.0 -33.0  6.5      67.4   475   F  1      0  12 54 10

13 03 00  J1722+5856   23 43 35  23.7 -34.1  6.3      68.6    56   1  1      0  13 03 00
13 06 00  =1721+589    23 46 36  23.4 -34.0  6.4      68.1   180   F  1      0  13 03 10

13 21 00  J2005+7752   00 01 38  36.7 -13.0  3.9     113.7   854   1  1      0  13 21 00
13 32 00  =2007+777    00 12 40  36.1 -13.2  4.1     110.8   660   F  1      0  13 21 10

13 34 00  J1722+5856   00 14 40  20.1 -32.4  6.9      62.7    64   1  1      0  13 34 00
13 37 00  =1721+589    00 17 41  19.7 -32.2  6.9      62.1   180   F  1      0  13 34 10

13 37 00  J1722+6105   00 17 41  20.7 -30.1  6.9      62.8    -6   1  1      0  13 37 00
13 42 00  =1722+611    00 22 42  20.2 -29.8  7.0      61.8   294   F  1      0  13 37 10

13 43 00  J1722+5856   00 23 42  19.0 -31.8  7.0      60.9    54   1  1      0  13 43 00
13 46 00  =1721+589    00 26 42  18.7 -31.6  7.1      60.3   180   F  1      0  13 43 10

13 46 00  AMS03        00 26 42  18.0 -30.5  7.2      58.8    -4   1  1      0  13 46 00
13 54 00  ---          00 34 44  17.1 -29.9  7.4      57.2   476   F  1      0  13 46 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
----------------------------------------------------------------------------------------

 --- Sun  30 Oct 2005   Day 303 ---

13 55 00  J1722+5856   00 35 44  17.7 -31.0  7.2      58.6    56   1  1      0  13 55 00
13 58 00  =1721+589    00 38 44  17.4 -30.7  7.3      58.0   180   F  1      0  13 55 10

13 58 00  AMS03        00 38 44  16.7 -29.6  7.4      56.4    -4   1  1      0  13 58 00
14 06 00  ---          00 46 46  15.8 -29.0  7.6      54.9   476   F  1      0  13 58 10

14 07 00  J1722+5856   00 47 46  16.4 -30.1  7.4      56.3    56   1  1      0  14 07 00
14 10 00  =1721+589    00 50 46  16.1 -29.9  7.5      55.7   180   F  1      0  14 07 10

14 10 00  AMS01        00 50 46  15.7 -28.3  7.6      54.1    -5   1  1      0  14 10 00
14 18 00  ---          00 58 48  14.8 -27.7  7.8      52.5   475   F  1      0  14 10 10

14 19 00  J1722+5856   00 59 48  15.1 -29.2  7.6      53.9    55   1  1      0  14 19 00
14 22 00  =1721+589    01 02 48  14.8 -28.9  7.7      53.4   180   F  1      0  14 19 10

14 22 00  AMS01        01 02 48  14.5 -27.4  7.8      51.7    -5   1  1      0  14 22 00
14 30 00  ---          01 10 49  13.7 -26.7  8.0      50.2   475   F  1      0  14 22 10

14 31 00  J1722+5856   01 11 50  13.9 -28.2  7.8      51.6    55   1  1      0  14 31 00
14 34 00  =1721+589    01 14 50  13.6 -27.9  7.9      51.0   180   F  1      0  14 31 10

14 34 00  AMS06        01 14 50  13.4 -26.4  8.0      49.5    -5   1  1      0  14 34 00
14 42 00  ---          01 22 51  12.6 -25.7  8.2      47.9   475   F  1      0  14 34 10

14 43 00  J1722+5856   01 23 52  12.7 -27.2  8.0      49.3    55   1  1      0  14 43 00
14 46 00  =1721+589    01 26 52  12.4 -26.9  8.1      48.7   180   F  1      0  14 43 10

14 46 00  AMS06        01 26 52  12.2 -25.4  8.2      47.1    -5   1  1      0  14 46 00
14 54 00  ---          01 34 53  11.5 -24.7  8.4      45.5   475   F  1      0  14 46 10

14 55 00  J1722+5856   01 35 54  11.5 -26.1  8.2      46.9    55   1  1      0  14 55 00
14 58 00  =1721+589    01 38 54  11.2 -25.8  8.3      46.3   180   F  1      0  14 55 10

14 58 00  AMS05        01 38 54  10.9 -24.5  8.4      44.7    -5   1  1      0  14 58 00
15 06 00  ---          01 46 55  10.2 -23.8  8.6      43.1   475   F  1      0  14 58 10

15 07 00  J1722+5856   01 47 56  10.4 -25.0  8.4      44.5    56   1  1      0  15 07 00
15 10 00  =1721+589    01 50 56  10.1 -24.7  8.5      44.0   180   F  1      0  15 07 10

15 10 00  AMS05        01 50 56   9.9 -23.4  8.6      42.3    -5   1  1      0  15 10 00
15 18 00  ---          01 58 57   9.2 -22.6  8.8      40.7   475   F  1      0  15 10 10

15 19 00  J1722+5856   01 59 58   9.3 -23.9  8.6      42.2    56   1  1      0  15 19 00
15 22 00  =1721+589    02 02 58   9.1 -23.6  8.7      41.6   180   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
----------------------------------------------------------------------------------------

 --- Sun  30 Oct 2005   Day 303 ---

15 22 00  AMS03        02 02 58   8.7 -22.3  8.8      39.8    -4   1  1      0  15 22 00
15 30 00  ---          02 10 59   8.1 -21.5  9.0      38.2   476   F  1      0  15 22 10

15 31 00  J1722+5856   02 12 00   8.3 -22.7  8.8      39.8    56   1  1      0  15 31 00
15 34 00  =1721+589    02 15 00   8.1 -22.4  8.9      39.2   180   F  1      0  15 31 10

15 34 00  AMS03        02 15 00   7.8 -21.1  9.0      37.4    -4   1  1      0  15 34 00
15 42 00  ---          02 23 01   7.2 -20.3  9.2      35.8   476   F  1      0  15 34 10

15 43 00  J1722+5856   02 24 01   7.4 -21.5  9.0      37.4    56   1  1      0  15 43 00
15 48 00  =1721+589    02 29 02   7.0 -20.9  9.1      36.4   300   F  1      0  15 43 10

15 48 00  J1722+6105   02 29 02   8.7 -19.6  9.1      36.5    -8   1  1      0  15 48 00
15 54 00  =1722+611    02 35 03   8.3 -19.0  9.2      35.3   352   F  1      0  15 48 10

15 55 00  J1722+5856   02 36 03   6.4 -20.2  9.2      34.9    52   1  1      0  15 55 00
15 58 00  =1721+589    02 39 04   6.2 -19.9  9.3      34.3   180   F  1      0  15 55 10

15 58 00  AMS01        02 39 04   6.4 -18.3  9.4      32.5    -5   1  1      0  15 58 00
16 06 00  ---          02 47 05   5.9 -17.5  9.6      30.8   475   F  1      0  15 58 10

16 07 00  J1722+5856   02 48 05   5.6 -18.9  9.4      32.5    55   1  1      0  16 07 00
16 10 00  =1721+589    02 51 06   5.4 -18.6  9.5      31.9   180   F  1      0  16 07 10

16 10 00  AMS01        02 51 06   5.6 -17.0  9.6      30.0    -5   1  1      0  16 10 00
16 18 00  ---          02 59 07   5.1 -16.1  9.8      28.4   475   F  1      0  16 10 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)

 * AMS01             17 12 30.450877   * 17 13 11.167000     17 13 13.994101       0.00
                     59 59 16.13269    * 59 55 51.53000      59 55 32.97432        0.00
                     From catalog imbedded in main SCHED input file.
                        1.067 scan hours,     36.295 baseline hours above horizon.

 * AMS03             17 12 57.418009   * 17 13 40.191000     17 13 43.278870       0.00
                     59 31 08.36688    * 59 27 45.76100      59 27 27.46397        0.00
                     From catalog imbedded in main SCHED input file.
                        0.933 scan hours,     30.857 baseline hours above horizon.

 * AMS05             17 13 00.857297   * 17 13 42.766000     17 13 45.745146       0.00
                     59 42 42.61119    * 59 39 20.22000      59 39 01.94751        0.00
                     From catalog imbedded in main SCHED input file.
                        1.067 scan hours,     34.366 baseline hours above horizon.

 * AMS06             17 13 03.349588   * 17 13 43.906000     17 13 46.714832       0.00
                     60 00 36.88942    * 59 57 14.62800      59 56 56.36754        0.00
                     From catalog imbedded in main SCHED input file.
                        1.067 scan hours,     34.240 baseline hours above horizon.

   J1642+3948        16 41 17.606231   * 16 42 58.809968     16 43 09.101504       0.26
   1641+399          39 54 10.81493    * 39 48 36.99399      39 48 01.86785        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,      5.874 baseline hours above horizon.

 * J1722+5856        17 21 52.440263   * 17 22 36.726557     17 22 40.035279       0.62
   1721+589          58 59 06.49428    * 58 56 22.26066      58 56 08.80603        0.49
                     /data/soay/hrk/HRKSOFTWAREBOX/SCHED_6.02/catalogs/sources.vlba
                     VLBA Calib Srcs - GSFC sols. - catalog 2004f_astro
                        2.083 scan hours,     71.793 baseline hours above horizon.

 * J1722+6105        17 22 05.759508   * 17 22 40.059358     17 22 42.110691       0.52
   1722+611          61 08 43.42140    * 61 05 59.78729      61 05 46.38463        0.45
                     /data/soay/hrk/HRKSOFTWAREBOX/SCHED_6.02/catalogs/sources.vlba
                     VLBA Calib Srcs - GSFC sols. - catalog 2004f_astro
                        0.483 scan hours,     15.142 baseline hours above horizon.

 * J2005+7752        20 07 20.430184   * 20 05 30.998512     20 05 15.699597       0.96
   2007+777          77 43 58.12306    * 77 52 43.24759      77 53 55.43800        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,      6.318 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) 
   AMS01               81.7
   AMS03               81.4
   AMS05               81.5
   AMS06               81.7
   3C345               63.3
   J1722+5856          81.8
   J1722+6105          83.3
   J2005+7752         102.9

  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 

