  COVER INFORMATION 

 Station:    SHANGHAI  (Code Sh ) 
 Experiment: Parsec Emission in Seyfert Galaxies
 Exp. Code:  EL028   


Schedule Version:       4.00                                              
Processed by SCHED version: 16 Oct. 2001                                  

PI:       S. Leon                                                         

Address:  I. Physikalisches Institut d. Uni Koeln                         
          Zuelpicher Strasse 77                                           
          50937 Koeln                                                     
          Germany                                                         

Phone:    0049-221-470-3552                                               
EMAIL:    eckart@ph1.uni-koeln.de                                         
Fax:      0049-0221-470-5162                                              
Phone during observation: 0049-2257-301-155                               

Observing mode: 256-8-2 continuum, LCP only                               

Notes:                                                                    
                                                                          
                                                                          
                                                                          

Schedule for SHANGHAI  (Code Sh )                                   Page   2
               Parsec Emission in Seyfert Galaxies
  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).
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)
----------------------------------------------------------------------------------------

 --- Wed  13 Feb 2002   Day  44 ---

 Next scan frequencies:  1630.49  1630.49  1646.49  1646.49  1662.49  1662.49
                         1684.49  1684.49
 Next BBC frequencies:    810.39   810.39   826.39   826.39   842.39   842.39
                          864.39   864.39
 Next scan bandwidths:      8.00     8.00     8.00     8.00     8.00     8.00
                            8.00     8.00

21 00 00  J1101+7225   14 39 41  40.0 341.3  3.6     114.6     0   1  1      0  21 00 00
21 03 00  =1058+726    14 42 42  39.8 341.2  3.7     113.8   180   F  1   2400

21 04 00  NGC3147      14 43 42  36.3 341.0  4.4     102.7    46   1  1   2400  21 04 00
21 10 30  ---          14 50 13  35.8 340.9  4.6     101.1   390   F  1   7600

21 11 30  J1101+7225   14 51 13  39.2 340.8  3.8     111.6    47   1  1   7600  21 11 30
21 14 30  =1058+726    14 54 13  39.0 340.7  3.9     110.8   180   F  1  10000

21 15 30  NGC3147      14 55 14  35.5 340.8  4.6      99.9    46   1  1  10000  21 15 30
21 22 00  ---          15 01 45  35.0 340.7  4.7      98.2   390   F  1  15200

21 23 00  J1101+7225   15 02 45  38.4 340.5  4.0     108.6    47   1  1  15200  21 23 00
21 26 00  =1058+726    15 05 45  38.2 340.4  4.1     107.8   180   F  1  17600

21 32 00  J1127+5650   15 11 46  44.0 320.9  3.7      99.5   319   1  2  17600  21 32 00
21 35 00  =1124+571    15 14 47  43.6 320.8  3.8      98.8   180   R  1  15200

21 36 00  NGC3718      15 15 47  44.6 315.7  3.7      96.0    48   1  2  15200  21 36 00
21 42 30  ---          15 22 18  43.6 315.6  3.8      94.6   390   R  1  10000

21 43 30  J1127+5650   15 23 18  42.4 320.6  3.9      96.8    48   1  2  10000  21 43 30
21 46 30  =1124+571    15 26 19  42.0 320.6  4.0      96.2   180   R  1   7600

21 47 30  NGC3718      15 27 19  42.9 315.5  3.9      93.6    48   1  2   7600  21 47 30
21 54 00  ---          15 33 50  41.9 315.5  4.0      92.2   390   R  1   2400

21 55 00  J1127+5650   15 34 50  40.8 320.4  4.1      94.3    48   1  2   2400  21 55 00
21 58 00  =1124+571    15 37 51  40.4 320.4  4.2      93.6   180   R  1      0

22 04 00  J1101+7225   15 43 52  35.4 339.6  4.7      98.2   320   1  3      0  22 04 00
22 07 00  =1058+726    15 46 52  35.1 339.5  4.7      97.5   180   F  1   2400

22 08 00  NGC3147      15 47 52  31.7 340.5  5.5      87.1    47   1  3   2400  22 08 00
22 14 30  ---          15 54 23  31.3 340.6  5.6      85.5   390   F  1   7600
Schedule for SHANGHAI  (Code Sh )                                   Page   3
               Parsec Emission in Seyfert Galaxies
  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).
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)
----------------------------------------------------------------------------------------

 --- Wed  13 Feb 2002   Day  44 ---

22 15 30  J1101+7225   15 55 23  34.5 339.4  4.9      95.4    47   1  3   7600  22 15 30
22 18 30  =1058+726    15 58 24  34.3 339.4  4.9      94.7   180   F  1  10000

22 19 30  NGC3147      15 59 24  30.9 340.6  5.7      84.4    47   1  3  10000  22 19 30
22 26 00  ---          16 05 55  30.5 340.7  5.8      82.8   390   F  1  15200

22 27 00  J1101+7225   16 06 55  33.6 339.4  5.1      92.6    47   1  3  15200  22 27 00
22 30 00  =1058+726    16 09 56  33.4 339.4  5.1      91.9   180   F  1  17600

22 37 00  4C39.25      16 16 57  10.5 309.5  6.8      58.3   342   1  4  17600  22 37 00
22 40 00  ---          16 19 57  10.0 309.8  6.9      57.8   180   R  1  15200

22 46 00  J1127+5650   16 25 58  33.9 320.6  5.0      83.7   278   1  4  15200  22 46 00
22 48 00  =1124+571    16 27 59  33.6 320.6  5.0      83.3   120   R  1  13600

22 49 00  NGC3718      16 28 59  33.6 316.0  4.9      81.5    49   1  4  13600  22 49 00
22 55 00  ---          16 35 00  32.8 316.2  5.0      80.4   360   R  1   8800

22 56 00  J1127+5650   16 36 00  32.5 320.8  5.1      81.7    49   1  4   8800  22 56 00
22 58 00  =1124+571    16 38 00  32.2 320.8  5.2      81.3   120   R  1   7200

22 59 00  NGC3718      16 39 01  32.2 316.3  5.1      79.7    49   1  4   7200  22 59 00
23 05 00  ---          16 45 02  31.3 316.5  5.2      78.6   360   R  1   2400

23 06 00  J1127+5650   16 46 02  31.1 321.0  5.3      79.7    49   1  4   2400  23 06 00
23 09 00  =1124+571    16 49 02  30.7 321.1  5.4      79.1   180   R  1      0

23 15 00  J1101+7225   16 55 03  30.0 339.6  5.9      81.3   321   1  5      0  23 15 00
23 18 00  =1058+726    16 58 04  29.8 339.6  5.9      80.6   180   F  1   2400

23 19 00  NGC3147      16 59 04  26.8 341.6  6.7      70.6    48   1  5   2400  23 19 00
23 25 30  ---          17 05 35  26.3 341.8  6.8      69.1   390   F  1   7600

23 26 30  J1101+7225   17 06 35  29.2 339.8  6.1      78.6    49   1  5   7600  23 26 30
23 29 30  =1058+726    17 09 36  28.9 339.8  6.1      77.9   180   F  1  10000

23 30 30  NGC3147      17 10 36  26.0 342.0  6.9      68.0    48   1  5  10000  23 30 30
23 37 00  ---          17 17 07  25.6 342.2  7.0      66.5   390   F  1  15200

23 38 00  J1101+7225   17 18 07  28.3 340.0  6.3      76.0    49   1  5  15200  23 38 00
23 41 00  =1058+726    17 21 07  28.1 340.0  6.3      75.3   180   F  1  17600

23 47 00  J1127+5650   17 27 08  25.7 322.6  6.0      71.9   323   1  6  17600  23 47 00
23 50 00  =1124+571    17 30 09  25.3 322.8  6.0      71.3   180   R  1  15200
Schedule for SHANGHAI  (Code Sh )                                   Page   4
               Parsec Emission in Seyfert Galaxies
  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).
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)
----------------------------------------------------------------------------------------

 --- Wed  13 Feb 2002   Day  44 ---

23 51 00  NGC3718      17 31 09  24.6 318.6  6.0      70.3    50   1  6  15200  23 51 00
23 57 30  ---          17 37 40  23.7 319.0  6.1      69.2   390   R  1  10000

 --- Start: Wed  13 Feb 2002   Day  44 -- Stop: Thu  14 Feb 2002   Day  45 ---

23 58 30  J1127+5650   17 38 40  24.2 323.2  6.2      69.7    50   1  6  10000  23 58 30
00 01 30  =1124+571    17 41 41  23.8 323.3  6.2      69.1   180   R  1   7600

00 02 30  NGC3718      17 42 41  23.0 319.3  6.2      68.3    50   1  6   7600  00 02 30
00 09 00  ---          17 49 12  22.1 319.7  6.3      67.2   390   R  1   2400

00 10 00  J1127+5650   17 50 12  22.7 323.8  6.4      67.5    50   1  6   2400  00 10 00
00 13 00  =1124+571    17 53 13  22.4 324.0  6.4      67.0   180   R  1      0

00 19 00  J1101+7225   17 59 14  25.4 341.1  7.0      66.7   324   1  7      0  00 19 00
00 22 00  =1058+726    18 02 14  25.2 341.2  7.0      66.0   180   F  1   2400

00 23 00  NGC3147      18 03 14  22.7 343.9  7.8      56.1    50   1  7   2400  00 23 00
00 29 30  ---          18 09 45  22.3 344.2  7.9      54.7   390   F  1   7600

00 30 30  J1101+7225   18 10 46  24.6 341.5  7.1      64.1    50   1  7   7600  00 30 30
00 33 30  =1058+726    18 13 46  24.4 341.6  7.2      63.4   180   F  1  10000

00 34 30  NGC3147      18 14 46  22.0 344.4  8.0      53.6    50   1  7  10000  00 34 30
00 41 00  ---          18 21 17  21.6 344.7  8.1      52.1   390   F  1  15200

00 42 00  J1101+7225   18 22 17  23.8 341.9  7.3      61.5    51   1  7  15200  00 42 00
00 45 00  =1058+726    18 25 18  23.6 342.1  7.4      60.9   180   F  1  17600

00 51 00  J1127+5650   18 31 19  17.7 326.5  7.1      59.8   327   1  8  17600  00 51 00
00 54 00  =1124+571    18 34 19  17.4 326.7  7.1      59.3   180   R  1  15200

00 55 00  NGC3718      18 35 20  15.9 323.0  7.0      59.0    51   1  8  15200  00 55 00
01 01 30  ---          18 41 51  15.1 323.5  7.2      57.9   390   R  1  10000

01 02 30  J1127+5650   18 42 51  16.4 327.3  7.3      57.7    50   1  8  10000  01 02 30
01 05 30  =1124+571    18 45 51  16.0 327.5  7.3      57.1   180   R  1   7600

01 06 30  NGC3718      18 46 52  14.4 324.0  7.2      57.0    51   1  8   7600  01 06 30
01 13 00  ---          18 53 23  13.6 324.5  7.3      55.8   390   R  1   2400

01 14 00  J1127+5650   18 54 23  15.0 328.2  7.4      55.5    51   1  8   2400  01 14 00
01 17 00  =1124+571    18 57 23  14.7 328.5  7.5      54.9   180   R  1      0
Schedule for SHANGHAI  (Code Sh )                                   Page   5
               Parsec Emission in Seyfert Galaxies
  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).
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)
----------------------------------------------------------------------------------------

 --- Thu  14 Feb 2002   Day  45 ---

01 23 00  J1127+5650   19 03 24  14.0 329.0  7.6      53.8   356   1  9      0  01 23 00
01 25 30  =1124+571    19 05 55  13.8 329.2  7.6      53.3   150   F  1   2000

01 26 30  NGC3718      19 06 55  12.0 325.7  7.6      53.4    51   1  9   2000  01 26 30
01 32 30  ---          19 12 56  11.2 326.3  7.7      52.3   360   F  1   6800

01 33 30  J1127+5650   19 13 56  12.9 329.9  7.8      51.8    51   1  9   6800  01 33 30
01 35 30  =1124+571    19 15 56  12.7 330.0  7.8      51.4   120   F  1   8400

01 36 30  NGC3718      19 16 56  10.8 326.7  7.7      51.5    51   1  9   8400  01 36 30
01 42 30  ---          19 22 57  10.1 327.2  7.8      50.4   360   F  1  13200

01 43 30  J1127+5650   19 23 58  11.8 330.7  7.9      49.9    51   1  9  13200  01 43 30
01 45 30  =1124+571    19 25 58  11.6 330.9  8.0      49.5   120   F  1  14800

01 53 30  1803+784     19 33 59  41.6 353.9  1.6     153.0   378   1  9  14800  01 53 30
01 57 00  ---          19 37 30  41.5 353.7  1.6     152.0   210   F  1  17600

02 03 00  J1101+7225   19 43 31  19.0 345.9  8.7      43.6   283   1 10  17600  02 03 00
02 06 00  =1058+726    19 46 31  18.8 346.1  8.7      42.9   180   R  1  15200

02 07 00  NGC3147      19 47 31  17.5 349.5  9.5      33.0    51   1 10  15200  02 07 00
02 13 30  ---          19 54 03  17.2 349.9  9.6      31.6   390   R  1  10000

02 14 30  J1101+7225   19 55 03  18.4 346.6  8.9      41.1    51   1 10  10000  02 14 30
02 17 30  =1058+726    19 58 03  18.2 346.8  8.9      40.4   180   R  1   7600

02 18 30  NGC3147      19 59 03  17.1 350.2  9.7      30.5    51   1 10   7600  02 18 30
02 25 00  ---          20 05 34  16.8 350.7  9.8      29.1   390   R  1   2400

02 26 00  J1101+7225   20 06 35  17.8 347.3  9.1      38.5    51   1 10   2400  02 26 00
02 29 00  =1058+726    20 09 35  17.7 347.5  9.1      37.9   180   R  1      0

02 35 00  J1101+7225   20 15 36  17.4 347.9  9.2      36.6   357   1 11      0  02 35 00
02 38 00  =1058+726    20 18 37  17.3 348.1  9.3      35.9   180   F  1   2400

02 39 00  NGC3147      20 19 37  16.4 351.6 10.0      26.0    51   1 11   2400  02 39 00
02 45 30  ---          20 26 08  16.2 352.0 10.2      24.5   390   F  1   7600

02 46 30  J1101+7225   20 27 08  16.9 348.6  9.4      34.0    51   1 11   7600  02 46 30
02 49 30  =1058+726    20 30 08  16.8 348.8  9.5      33.4   180   F  1  10000

02 50 30  NGC3147      20 31 09  16.0 352.4 10.2      23.4    51   1 11  10000  02 50 30
02 57 00  ---          20 37 40  15.8 352.8 10.3      22.0   390   F  1  15200
Schedule for SHANGHAI  (Code Sh )                                   Page   6
               Parsec Emission in Seyfert Galaxies
  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).
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)
----------------------------------------------------------------------------------------

 --- Thu  14 Feb 2002   Day  45 ---

02 58 00  J1101+7225   20 38 40  16.4 349.4  9.6      31.5    51   1 11  15200  02 58 00
03 01 00  =1058+726    20 41 40  16.3 349.6  9.7      30.8   180   F  1  17600

03 07 00  J1127+5650   20 47 41   4.2 339.3  9.3  D   33.5   320   1 12  17600  03 07 00
03 10 00  =1124+571    20 50 42   4.0 339.7  9.4  D   32.9     0   R  1  15200

03 11 00  NGC3718      20 51 42   1.1 337.1  9.3  D   33.6    53   1 12  15200  03 11 00
03 17 30  ---          20 58 13   0.6 338.0  9.4  D   32.3     0   R  1  10000

03 18 30  J1127+5650   20 59 13   3.4 340.7  9.5  D   31.2    53   1 12  10000  03 18 30
03 21 30  =1124+571    21 02 14   3.2 341.0  9.6  D   30.6     0   R  1   7600

03 22 30  NGC3718      21 03 14   0.2 338.6  9.5  D   31.3    53   1 12   7600  03 22 30
03 29 00  ---          21 09 45  -0.3 339.4  9.6  D   30.0     0   R  1   2400

03 30 00  J1127+5650   21 10 45   2.6 342.0  9.7  D   28.9    53   1 12   2400  03 30 00
03 33 00  =1124+571    21 13 46   2.4 342.4  9.8  D   28.2     0   R  1      0

03 39 00  J1101+7225   21 19 47  15.0 352.2 10.3      22.5   325   1 13      0  03 39 00
03 42 00  =1058+726    21 22 47  14.9 352.5 10.3      21.8   180   F  1   2400

03 43 00  NGC3147      21 23 47  14.9 356.1 11.1      11.8    51   1 13   2400  03 43 00
03 49 30  ---          21 30 18  14.8 356.6 11.2      10.3   390   F  1   7600

03 50 30  J1101+7225   21 31 18  14.7 353.1 10.5      20.0    51   1 13   7600  03 50 30
03 53 30  =1058+726    21 34 19  14.6 353.3 10.5      19.3   180   F  1  10000

03 54 30  NGC3147      21 35 19  14.7 356.9 11.3       9.2    51   1 13  10000  03 54 30
04 01 00  ---          21 41 50  14.7 357.4 11.4       7.8   390   F  1  15200

04 02 00  J1101+7225   21 42 50  14.4 353.9 10.7      17.4    51   1 13  15200  04 02 00
04 05 00  =1058+726    21 45 51  14.3 354.2 10.7      16.8   180   F  1  17600

04 11 00  J1127+5650   21 51 52   0.2 347.1 10.4  D   20.4   327   1 14  17600  04 11 00
04 15 00  =1124+571    21 55 52   0.1 347.7 10.5  D   19.5     0   R  1  14400

04 15 00  NGC3718      21 55 52  -3.2 345.7 10.4  D   20.6    -6   1 14  14400  04 15 00
04 29 00  ---          22 09 55  -3.9 347.7 10.6  D   17.7     0   R  1   3200

04 29 00  J1127+5650   22 09 55  -0.5 349.5 10.7  D   16.6    -6   1 14   3200  04 29 00
04 33 00  =1124+571    22 13 55  -0.7 350.0 10.8  D   15.7     0   R  1      0
Schedule for SHANGHAI  (Code Sh )                                   Page   7
               Parsec Emission in Seyfert Galaxies
  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).
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)
----------------------------------------------------------------------------------------

 --- Thu  14 Feb 2002   Day  45 ---

-----------  Tape Change ------------

04 48 00  J1101+7225   22 28 58  13.7 357.4 11.4       7.3   869   1  1      0  04 48 00
04 51 00  =1058+726    22 31 58  13.6 357.7 11.5       6.6   180   F  1   2400

04 52 00  NGC3147      22 32 59  14.5 361.2-11.7      -3.5    51   1  1   2400  04 52 00
04 58 30  ---          22 39 30  14.6 361.6-11.6      -4.9   390   F  1   7600

04 59 30  J1101+7225   22 40 30  13.6 358.3 11.6       4.7    51   1  1   7600  04 59 30
05 02 30  =1058+726    22 43 30  13.6 358.6 11.7       4.1   180   F  1  10000

05 03 30  NGC3147      22 44 30  14.6 362.0-11.5      -6.1    51   1  1  10000  05 03 30
05 10 00  ---          22 51 02  14.6 362.5-11.4      -7.5   390   F  1  15200

05 11 00  J1101+7225   22 52 02  13.5 359.2 11.8       2.2    51   1  1  15200  05 11 00
05 14 00  =1058+726    22 55 02  13.5 359.5 11.9       1.5   180   F  1  17600

05 20 00  J1127+5650   23 01 03  -1.9 356.3 11.6  D    5.7   330   1  2  17600  05 20 00
05 23 00  =1124+571    23 04 04  -1.9 356.8 11.6  D    5.1     0   R  1  15200

05 24 00  NGC3718      23 05 04  -5.6 355.8 11.5  D    5.9    56   1  2  15200  05 24 00
05 30 30  ---          23 11 35  -5.7 356.8 11.6  D    4.5     0   R  1  10000

05 31 30  J1127+5650   23 12 35  -2.0 357.9 11.7  D    3.3    56   1  2  10000  05 31 30
05 34 30  =1124+571    23 15 36  -2.0 358.3 11.8  D    2.6     0   R  1   7600

05 35 30  NGC3718      23 16 36  -5.8 357.6 11.7  D    3.5    56   1  2   7600  05 35 30
05 42 00  ---          23 23 07  -5.8 358.6 11.8  D    2.1     0   R  1   2400

05 43 00  J1127+5650   23 24 07  -2.1 359.5 11.9  D    0.8    56   1  2   2400  05 43 00
05 46 00  =1124+571    23 27 07  -2.1 359.9 12.0  D    0.1     0   R  1      0

05 52 00  J1101+7225   23 33 08  13.7 362.4-11.5      -6.9   329   1  3      0  05 52 00
05 55 00  =1058+726    23 36 09  13.7 362.6-11.4      -7.5   180   F  1   2400

05 56 00  NGC3147      23 37 09  15.4 365.8-10.7     -17.7    52   1  3   2400  05 56 00
06 02 30  ---          23 43 40  15.5 366.3-10.6     -19.1   390   F  1   7600

06 03 30  J1101+7225   23 44 40  13.8 363.3-11.3      -9.4    52   1  3   7600  06 03 30
06 06 30  =1058+726    23 47 41  13.8 363.5-11.2     -10.1   180   F  1  10000

06 07 30  NGC3147      23 48 41  15.6 366.6-10.5     -20.2    52   1  3  10000  06 07 30
06 14 00  ---          23 55 12  15.8 367.1-10.4     -21.7   390   F  1  15200
Schedule for SHANGHAI  (Code Sh )                                   Page   8
               Parsec Emission in Seyfert Galaxies
  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).
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)
----------------------------------------------------------------------------------------

 --- Thu  14 Feb 2002   Day  45 ---

06 15 00  J1101+7225   23 56 12  13.9 364.2-11.1     -11.9    52   1  3  15200  06 15 00
06 18 00  =1058+726    23 59 13  14.0 364.4-11.0     -12.6   180   F  1  17600

06 24 00  J1127+5650   00 05 14  -1.7 365.1-11.4  D   -8.0   328   1  4  17600  06 24 00
06 27 00  =1124+571    00 08 14  -1.7 365.5-11.3  D   -8.6     0   R  1  15200

06 28 00  NGC3718      00 09 14  -5.5 365.5-11.4  D   -7.8    58   1  4  15200  06 28 00
06 34 30  ---          00 15 45  -5.3 366.5-11.3  D   -9.2     0   R  1  10000

06 35 30  J1127+5650   00 16 46  -1.5 366.7-11.2  D  -10.5    58   1  4  10000  06 35 30
06 38 30  =1124+571    00 19 46  -1.4 367.1-11.1  D  -11.1     0   R  1   7600

06 39 30  NGC3718      00 20 46  -5.2 367.2-11.2  D  -10.3    58   1  4   7600  06 39 30
06 46 00  ---          00 27 17  -5.0 368.2-11.1  D  -11.7     0   R  1   2400

06 47 00  J1127+5650   00 28 17  -1.1 368.2-11.0  D  -12.9    58   1  4   2400  06 47 00
06 50 00  =1124+571    00 31 18  -1.1 368.6-10.9  D  -13.5     0   R  1      0

06 56 00  J1101+7225   00 37 19  14.8 367.3-10.4     -21.0   325   1  5      0  06 56 00
06 59 00  =1058+726    00 40 19  14.9 367.5-10.4     -21.6   180   F  1   2400

07 00 00  NGC3147      00 41 20  17.3 370.1 -9.6     -31.9    50   1  5   2400  07 00 00
07 06 30  ---          00 47 51  17.5 370.6 -9.5     -33.3   390   F  1   7600

07 07 30  J1101+7225   00 48 51  15.1 368.1-10.2     -23.5    50   1  5   7600  07 07 30
07 10 30  =1058+726    00 51 51  15.2 368.3-10.2     -24.2   180   F  1  10000

07 11 30  NGC3147      00 52 51  17.7 370.9 -9.4     -34.4    50   1  5  10000  07 11 30
07 18 00  ---          00 59 23  18.0 371.3 -9.3     -35.8   390   F  1  15200

07 19 00  J1101+7225   01 00 23  15.5 368.9-10.0     -26.0    50   1  5  15200  07 19 00
07 22 00  =1058+726    01 03 23  15.6 369.1-10.0     -26.7   180   F  1  17600

07 28 00  J1127+5650   01 09 24   0.5 373.6-10.3  D  -21.5   323   1  6  17600  07 28 00
07 31 00  =1124+571    01 12 25   0.7 374.0-10.3  D  -22.2     0   R  1  15200

07 32 00  NGC3718      01 13 25  -3.0 374.8-10.3  D  -21.4    56   1  6  15200  07 32 00
07 38 30  ---          01 19 56  -2.7 375.7-10.2  D  -22.7     0   R  1  10000

07 39 30  J1127+5650   01 20 56   1.1 375.0-10.1  D  -23.9    57   1  6  10000  07 39 30
07 42 30  =1124+571    01 23 57   1.3 375.4-10.1  D  -24.6     0   R  1   7600

07 43 30  NGC3718      01 24 57  -2.4 376.4-10.1  D  -23.8    56   1  6   7600  07 43 30
07 50 00  ---          01 31 28  -2.0 377.3-10.0  D  -25.1     0   R  1   2400
Schedule for SHANGHAI  (Code Sh )                                   Page   9
               Parsec Emission in Seyfert Galaxies
  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).
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)
----------------------------------------------------------------------------------------

 --- Thu  14 Feb 2002   Day  45 ---

07 51 00  J1127+5650   01 32 28   1.8 376.5 -9.9  D  -26.3    56   1  6   2400  07 51 00
07 54 00  =1124+571    01 35 28   2.0 376.8 -9.9  D  -26.9     0   R  1      0

08 00 00  J1101+7225   01 41 29  17.1 371.7 -9.3     -35.0   318   1  7      0  08 00 00
08 03 00  =1058+726    01 44 30  17.2 371.9 -9.3     -35.7   180   F  1   2400

08 04 00  NGC3147      01 45 30  20.2 373.9 -8.5     -46.0    48   1  7   2400  08 04 00
08 10 30  ---          01 52 01  20.5 374.2 -8.4     -47.5   390   F  1   7600

08 11 30  J1101+7225   01 53 01  17.6 372.4 -9.1     -37.6    48   1  7   7600  08 11 30
08 14 30  =1058+726    01 56 02  17.7 372.6 -9.1     -38.2   180   F  1  10000

08 15 30  NGC3147      01 57 02  20.8 374.5 -8.3     -48.6    48   1  7  10000  08 15 30
08 22 00  ---          02 03 33  21.1 374.8 -8.2     -50.0   390   F  1  15200

08 23 00  J1101+7225   02 04 33  18.1 373.1 -9.0     -40.1    48   1  7  15200  08 23 00
08 26 00  =1058+726    02 07 34  18.3 373.3 -8.9     -40.8   180   F  1  17600

08 31 00  J1127+5650   02 12 35   4.6 381.2 -9.3  D  -34.5   254   1  8  17600  08 31 00
08 34 00  =1124+571    02 15 35   4.8 381.5 -9.2  D  -35.1     0   R  1  15200

08 35 00  NGC3718      02 16 35   1.4 383.2 -9.3  D  -34.2    55   1  8  15200  08 35 00
08 44 00  ---          02 25 37   2.2 384.3 -9.1  D  -35.9     0   R  1   8000

08 45 00  J1127+5650   02 26 37   5.7 382.8 -9.0     -37.3    55   1  8   8000  08 45 00
08 48 00  =1124+571    02 29 37   5.9 383.1 -9.0     -37.8   180   R  1   5600

08 53 00  1803+784     02 34 38  23.5 350.2  8.6      47.0   232   1  8   5600  08 53 00
09 00 00  ---          02 41 39  23.3 350.4  8.7      45.3   420   R  1      0


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


 Setup file: e18cm-256-8-2-L-UL.set
   Matches group sh18cmo in /home/krips/SCHED/catalogs/freq.dat
    Huang Xinyong 231198, old (obsolete?) configuration

   Setup group:    6         Station: SHANGHAI          Total bit rate:  256
   Format: MKIV1:2           Bits per sample: 2         Sample rate: 16.000
   Number of channels:  8    Passes/head pos:   1       Speedup factor:   1.00

   Tape speeds: Low density - 270.000 ips,  High density - 160.00 ips
   Time per pass for  17600 ft, High density tapes is: 00:22:00

   1st LO=    820.10    820.10    820.10    820.10    820.10    820.10    820.10    820.10
   Net SB=         L         U         L         U         L         U         L         U
   Pol.  =      LCP       LCP       LCP       LCP       LCP       LCP       LCP       LCP 
   BBC   =         1         1         2         2         3         3         4         4
   BBC SB=         L         U         L         U         L         U         L         U
   IF    =        A         A         A         A         A         A         A         A 

  The following frequency sets based on this setup were used.

   Frequency Set:   6  Setup file default.  Used pcal sets:   1
   LO sum=    1630.49   1630.49   1646.49   1646.49   1662.49   1662.49   1684.49   1684.49
   BBC fr=     810.39    810.39    826.39    826.39    842.39    842.39    864.39    864.39
   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=   490   490   490   490  6490  6490  6490  6490
    PCALFR2=   510   510   510   510  6510  6510  6510  6510

   Track assignments are: 
    track1=   2, 10, 18, 26,  3, 11, 19, 27
    barrel=roll_off 
 SOURCE LIST -- Parsec Emission in Seyfert Galaxies
     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).

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

 * NGC3147           10 12 39.434759   * 10 16 53.270000     10 17 07.104619 
                     73 39 00.48245    * 73 24 02.40000      73 23 24.36217 
                     From catalog imbedded in main SCHED input file.

 * NGC3718           11 29 49.934168   * 11 32 34.880000     11 32 42.810315 
                     53 20 37.85586    * 53 04 03.90000      53 03 15.85824 
                     From catalog imbedded in main SCHED input file.

   J0927+3902        09 23 55.319195   * 09 27 03.013916     09 27 11.536382 
   0923+392          39 15 23.56655    * 39 02 20.85195      39 01 47.98013 
 * 4C39.25           /home/krips/SCHED/catalogs/sources.vlba
   4C39.25           ICRF - Ext.1 Source - 1998 IERS Annual Report
   J0927+39    

 * J1101+7225        10 58 20.093294   * 11 01 48.805363     11 02 00.531596 
   1058+726          72 41 44.88774    * 72 25 37.11828      72 24 52.82024 
   1058+726          /home/krips/SCHED/catalogs/sources.vlba
                     VLBA Calib. Survey - ICRF Frame - reduced by GSFC group - Aug 2001

 * J1127+5650        11 24 51.308501   * 11 27 40.135071     11 27 48.428201 
   1124+571          57 06 45.80099    * 56 50 14.79405      56 49 27.16161 
   1124+571          /home/krips/SCHED/catalogs/sources.vlba
                     VLBA Calib. Survey - ICRF Frame - reduced by GSFC group - Aug 2001

   J1800+7828        18 03 39.193542   * 18 00 45.683918     18 00 35.344819 
 * 1803+784          78 27 54.29757    * 78 28 04.01851      78 27 46.34371 
   1803+784          /home/krips/SCHED/catalogs/sources.vlba
   J1800+78          ICRF - Ext.1 Source - 1998 IERS Annual Report



  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) 
   NGC3147            119.6
   NGC3718            135.1
   4C39.25            153.6
   J1101+7225         119.7
   J1127+5650         132.5
   1803+784            96.7

  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 

