  COVER INFORMATION 

 Station:    SHANGHAI  (Code Sh ) 
 Experiment: Parsec scale radio nuclei in nearby Seyfert galaxies from a complete sam
 Exp. Code:  EG037B  


Schedule Version:       1.00                                              
Processed by SCHED version:   6.05  June 2006                             

PI:       M. Giroletti                                                    

Address:  INAF Istituto di Radioastronomia                                
          Via Gobetti 101                                                 
          40129 Bologna                                                   
          Italy                                                           

Phone:    +39 051 639 9394                                                
EMAIL:    giroletti@ira.inaf.it                                           
Fax:      +39 051 639 9431                                                
Phone during observation: +39 347 906 6221                                

Observing mode: Phase-referencing of three sources at 18cm (1 Gb/s)       

Notes:                                                                    
                                                                          
                                                                          
                                                                          

Schedule for SHANGHAI  (Code Sh )                                   Page   2
               Parsec scale radio nuclei in nearby Seyfert galaxies from a complete sam
  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.
         For disks, the footages are really the GBytes
  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
----------------------------------------------------------------------------------------

 --- Wed   6 Jun 2007   Day 157 ---

 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

15 00 00  J1221+4411   16 03 23  45.1 -56.8  3.7      87.4     0   1  1      0  15 00 00
15 01 40  =1218+444    16 05 03  44.8 -56.8  3.7      87.1   100   F  1     13  15 00 01

15 01 40  NGC4051      16 05 03  41.6 -56.0  4.0      84.5    -7   1  1     13  15 01 40
15 05 40  ---          16 09 04  40.9 -55.9  4.1      83.9   233   F  1     44  15 01 41

15 05 40  J1221+4411   16 09 04  44.1 -56.8  3.8      86.5    -7   1  1     44  15 05 40
15 07 40  =1218+444    16 11 04  43.8 -56.7  3.8      86.2   113   F  1     59  15 05 41

15 07 40  NGC4051      16 11 04  40.5 -55.9  4.1      83.5    -7   1  1     59  15 07 40
15 11 40  ---          16 15 05  39.8 -55.8  4.2      82.9   233   F  1     90  15 07 41

15 11 40  J1221+4411   16 15 05  43.0 -56.7  3.9      85.5    -7   1  1     90  15 11 40
15 13 40  =1218+444    16 17 05  42.7 -56.6  3.9      85.2   113   F  1    106  15 11 41

15 15 40  J1308+3546   16 19 05  50.4 -70.1  3.2      82.6   105   1  1    106  15 15 40
15 17 20  ---          16 20 46  50.1 -70.0  3.2      82.4   100   F  1    119  15 15 41

15 17 20  NGC5033      16 20 46  51.2 -68.9  3.1      84.0    -4   1  1    119  15 17 20
15 21 20  ---          16 24 46  50.4 -68.8  3.2      83.5   236   F  1    150  15 17 21

15 21 20  J1308+3546   16 24 46  49.3 -69.8  3.3      82.0    -4   1  1    150  15 21 20
15 23 20  ---          16 26 47  48.9 -69.7  3.3      81.7   116   F  1    165  15 21 21

15 23 20  NGC5033      16 26 47  50.0 -68.7  3.2      83.3    -4   1  1    165  15 23 20
15 27 20  ---          16 30 47  49.2 -68.5  3.3      82.8   236   F  1    196  15 23 21

15 27 20  J1308+3546   16 30 47  48.1 -69.6  3.4      81.3    -4   1  1    196  15 27 20
15 29 20  ---          16 32 48  47.6 -69.5  3.4      81.1   116   F  1    212  15 27 21

15 31 20  J1340+3754   16 34 48  53.8 -67.1  2.9      87.4   108   1  1    212  15 31 20
15 33 00  =1338+381    16 36 28  53.5 -67.0  2.9      87.2   100   F  1    225  15 31 21
Schedule for SHANGHAI  (Code Sh )                                   Page   3
               Parsec scale radio nuclei in nearby Seyfert galaxies from a complete sam
  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.
         For disks, the footages are really the GBytes
  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
----------------------------------------------------------------------------------------

 --- Wed   6 Jun 2007   Day 157 ---

15 33 00  NGC5273      16 36 28  53.7 -70.9  2.9      84.4    -6   1  1    225  15 33 00
15 37 00  ---          16 40 29  52.9 -70.7  3.0      83.9   234   F  1    255  15 33 01

15 37 00  J1340+3754   16 40 29  52.7 -67.0  3.0      86.6    -6   1  1    255  15 37 00
15 39 00  =1338+381    16 42 29  52.3 -66.9  3.0      86.4   114   F  1    271  15 37 01

15 39 00  NGC5273      16 42 29  52.5 -70.7  3.0      83.7    -6   1  1    271  15 39 00
15 43 00  ---          16 46 30  51.7 -70.5  3.1      83.2   234   F  1    302  15 39 01

15 43 00  J1340+3754   16 46 30  51.5 -66.8  3.1      85.8    -6   1  1    302  15 43 00
15 45 00  =1338+381    16 48 30  51.1 -66.8  3.1      85.5   114   F  1    317  15 43 01

15 47 00  J1221+4411   16 50 30  36.7 -55.6  4.5      80.0    94   1  1    317  15 47 00
15 48 40  =1218+444    16 52 11  36.4 -55.5  4.5      79.7   100   F  1    330  15 47 01

15 48 40  NGC4051      16 52 11  33.3 -54.3  4.8      77.2    -7   1  1    330  15 48 40
15 52 40  ---          16 56 11  32.6 -54.1  4.9      76.6   233   F  1    361  15 48 41

15 52 40  J1221+4411   16 56 11  35.7 -55.4  4.6      79.1    -7   1  1    361  15 52 40
15 54 40  =1218+444    16 58 12  35.4 -55.3  4.6      78.8   113   F  1    377  15 52 41

15 54 40  NGC4051      16 58 12  32.3 -54.0  4.9      76.3    -7   1  1    377  15 54 40
15 58 40  ---          17 02 12  31.6 -53.8  5.0      75.8   233   F  1    408  15 54 41

15 58 40  J1221+4411   17 02 12  34.7 -55.1  4.7      78.2    -7   1  1    408  15 58 40
16 00 40  =1218+444    17 04 13  34.3 -55.0  4.7      77.9   113   F  1    423  15 58 41

16 02 40  J1308+3546   17 06 13  41.0 -67.7  4.0      77.4   105   1  1    423  16 02 40
16 04 20  ---          17 07 53  40.7 -67.6  4.0      77.2   100   F  1    436  16 02 41

16 04 20  NGC5033      17 07 53  41.8 -66.8  3.9      78.5    -4   1  1    436  16 04 20
16 08 20  ---          17 11 54  41.0 -66.6  4.0      78.0   236   F  1    467  16 04 21

16 08 20  J1308+3546   17 11 54  39.9 -67.4  4.1      76.8    -4   1  1    467  16 08 20
16 10 20  ---          17 13 54  39.5 -67.2  4.1      76.6   116   F  1    483  16 08 21

16 10 20  NGC5033      17 13 54  40.6 -66.5  4.0      77.8    -4   1  1    483  16 10 20
16 14 20  ---          17 17 55  39.9 -66.3  4.1      77.4   236   F  1    514  16 10 21

16 14 20  J1308+3546   17 17 55  38.7 -67.0  4.2      76.2    -4   1  1    514  16 14 20
16 16 20  ---          17 19 55  38.3 -66.9  4.2      76.0   116   F  1    529  16 14 21

16 18 20  J1340+3754   17 21 56  44.6 -65.7  3.7      81.2   107   1  1    529  16 18 20
16 20 00  =1338+381    17 23 36  44.3 -65.6  3.7      81.0   100   F  1    542  16 18 21
Schedule for SHANGHAI  (Code Sh )                                   Page   4
               Parsec scale radio nuclei in nearby Seyfert galaxies from a complete sam
  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.
         For disks, the footages are really the GBytes
  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
----------------------------------------------------------------------------------------

 --- Wed   6 Jun 2007   Day 157 ---

16 20 00  NGC5273      17 23 36  44.2 -68.8  3.7      79.1    -5   1  1    542  16 20 00
16 24 00  ---          17 27 37  43.4 -68.6  3.8      78.6   235   F  1    573  16 20 01

16 24 00  J1340+3754   17 27 37  43.5 -65.4  3.8      80.5    -5   1  1    573  16 24 00
16 26 00  =1338+381    17 29 37  43.1 -65.3  3.8      80.3   115   F  1    588  16 24 01

16 26 00  NGC5273      17 29 37  43.0 -68.4  3.8      78.4    -5   1  1    588  16 26 00
16 30 00  ---          17 33 38  42.2 -68.2  3.9      78.0   235   F  1    619  16 26 01

16 30 00  J1340+3754   17 33 38  42.3 -65.1  3.9      79.8    -5   1  1    619  16 30 00
16 32 00  =1338+381    17 35 38  41.9 -65.0  3.9      79.6   115   F  1    635  16 30 01

16 34 00  J1221+4411   17 37 38  28.5 -53.3  5.3      73.0    96   1  1    635  16 34 00
16 35 40  =1218+444    17 39 18  28.2 -53.2  5.3      72.8   100   F  1    648  16 34 01

16 35 40  NGC4051      17 39 18  25.2 -51.7  5.6      70.3    -7   1  1    648  16 35 40
16 39 40  ---          17 43 19  24.6 -51.4  5.7      69.7   233   F  1    679  16 35 41

16 39 40  J1221+4411   17 43 19  27.6 -52.9  5.4      72.2    -7   1  1    679  16 39 40
16 41 40  =1218+444    17 45 19  27.2 -52.8  5.4      71.9   113   F  1    694  16 39 41

16 41 40  NGC4051      17 45 19  24.2 -51.2  5.7      69.4    -7   1  1    694  16 41 40
16 45 40  ---          17 49 20  23.6 -51.0  5.8      68.8   233   F  1    725  16 41 41

16 45 40  J1221+4411   17 49 20  26.5 -52.5  5.5      71.3    -7   1  1    725  16 45 40
16 47 40  =1218+444    17 51 20  26.2 -52.4  5.5      71.0   113   F  1    741  16 45 41

16 49 40  J1308+3546   17 53 21  31.8 -64.6  4.7      72.4   106   1  1    741  16 49 40
16 51 20  ---          17 55 01  31.4 -64.5  4.8      72.2   100   F  1    754  16 49 41

16 51 20  NGC5033      17 55 01  32.7 -63.9  4.7      73.2    -4   1  1    754  16 51 20
16 55 20  ---          17 59 02  31.9 -63.6  4.8      72.8   236   F  1    784  16 51 21

16 55 20  J1308+3546   17 59 02  30.7 -64.2  4.8      71.7    -4   1  1    784  16 55 20
16 57 20  ---          18 01 02  30.3 -64.0  4.9      71.5   116   F  1    800  16 55 21

16 57 20  NGC5033      18 01 02  31.5 -63.5  4.8      72.6    -4   1  1    800  16 57 20
17 01 20  ---          18 05 03  30.7 -63.2  4.9      72.1   236   F  1    831  16 57 21

17 01 20  J1308+3546   18 05 03  29.5 -63.7  4.9      71.1    -4   1  1    831  17 01 20
17 03 20  ---          18 07 03  29.1 -63.6  5.0      70.9   116   F  1    846  17 01 21

17 05 20  J1340+3754   18 09 03  35.5 -63.2  4.5      75.6   107   1  1    846  17 05 20
17 07 00  =1338+381    18 10 44  35.2 -63.1  4.5      75.4   100   F  1    859  17 05 21
Schedule for SHANGHAI  (Code Sh )                                   Page   5
               Parsec scale radio nuclei in nearby Seyfert galaxies from a complete sam
  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.
         For disks, the footages are really the GBytes
  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
----------------------------------------------------------------------------------------

 --- Wed   6 Jun 2007   Day 157 ---

17 07 00  NGC5273      18 10 44  34.9 -65.9  4.5      74.0    -5   1  1    859  17 07 00
17 11 00  ---          18 14 44  34.1 -65.6  4.5      73.6   235   F  1    890  17 07 01

17 11 00  J1340+3754   18 14 44  34.4 -62.9  4.6      74.9    -5   1  1    890  17 11 00
17 13 00  =1338+381    18 16 45  34.0 -62.7  4.6      74.7   115   F  1    906  17 11 01

17 13 00  NGC5273      18 16 45  33.7 -65.5  4.6      73.4    -5   1  1    906  17 13 00
17 17 00  ---          18 20 45  32.9 -65.2  4.6      73.0   235   F  1    937  17 13 01

17 17 00  J1340+3754   18 20 45  33.2 -62.5  4.7      74.2    -5   1  1    937  17 17 00
17 19 00  =1338+381    18 22 46  32.9 -62.4  4.7      73.9   115   F  1    952  17 17 01

17 23 00  3C345        18 26 46  67.3 -60.3  1.7     104.4   181   1  1    952  17 23 00
17 33 00  ---          18 36 48  65.4 -61.4  1.9     101.8   600   F  1   1030  17 23 01

17 37 00  J1221+4411   18 40 49  18.0 -48.7  6.3      63.8   159   1  1   1030  17 37 00
17 39 00  =1218+444    18 42 49  17.7 -48.6  6.3      63.5   120   F  1   1045  17 37 01

17 39 00  NGC4051      18 42 49  14.9 -46.7  6.7      60.8    -7   1  1   1045  17 39 00
17 43 00  ---          18 46 50  14.3 -46.3  6.7      60.2   233   F  1   1076  17 39 01

17 43 00  J1221+4411   18 46 50  17.0 -48.2  6.4      62.9    -7   1  1   1076  17 43 00
17 45 00  =1218+444    18 48 50  16.7 -48.1  6.4      62.6   113   F  1   1092  17 43 01

17 45 00  NGC4051      18 48 50  14.0 -46.1  6.8      59.9    -7   1  1   1092  17 45 00
17 49 00  ---          18 52 51  13.4 -45.8  6.8      59.3   233   F  1   1123  17 45 01

17 49 00  J1221+4411   18 52 51  16.1 -47.7  6.5      62.0    -6   1  1   1123  17 49 00
17 51 00  =1218+444    18 54 51  15.8 -47.5  6.6      61.7   114   F  1   1138  17 49 01

17 53 00  J1308+3546   18 56 51  19.7 -59.5  5.8      65.3   106   1  1   1138  17 53 00
17 54 40  ---          18 58 31  19.4 -59.3  5.8      65.1   100   F  1   1151  17 53 01

17 54 40  NGC5033      18 58 31  20.7 -59.0  5.7      66.0    -4   1  1   1151  17 54 40
17 58 40  ---          19 02 32  20.0 -58.6  5.8      65.5   236   F  1   1182  17 54 41

17 58 40  J1308+3546   19 02 32  18.7 -58.9  5.9      64.6    -4   1  1   1182  17 58 40
18 00 40  ---          19 04 32  18.3 -58.8  5.9      64.4   116   F  1   1197  17 58 41

18 00 40  NGC5033      19 04 32  19.6 -58.4  5.8      65.3    -4   1  1   1197  18 00 40
18 04 40  ---          19 08 33  18.9 -58.1  5.9      64.8   236   F  1   1228  18 00 41

18 04 40  J1308+3546   19 08 33  17.6 -58.4  6.0      63.9    -4   1  1   1228  18 04 40
18 06 40  ---          19 10 33  17.2 -58.2  6.0      63.7   116   F  1   1244  18 04 41
Schedule for SHANGHAI  (Code Sh )                                   Page   6
               Parsec scale radio nuclei in nearby Seyfert galaxies from a complete sam
  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.
         For disks, the footages are really the GBytes
  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
----------------------------------------------------------------------------------------

 --- Wed   6 Jun 2007   Day 157 ---

18 08 40  J1340+3754   19 12 34  23.6 -58.7  5.5      68.0   107   1  1   1244  18 08 40
18 10 20  =1338+381    19 14 14  23.3 -58.6  5.6      67.8   100   F  1   1257  18 08 41

18 10 20  NGC5273      19 14 14  22.7 -61.0  5.5      67.1    -4   1  1   1257  18 10 20
18 14 20  ---          19 18 15  22.0 -60.7  5.6      66.7   236   F  1   1288  18 10 21

18 14 20  J1340+3754   19 18 15  22.5 -58.3  5.6      67.3    -4   1  1   1288  18 14 20
18 16 20  =1338+381    19 20 15  22.2 -58.1  5.7      67.1   116   F  1   1303  18 14 21

18 16 20  NGC5273      19 20 15  21.6 -60.5  5.6      66.4    -4   1  1   1303  18 16 20
18 20 20  ---          19 24 16  20.9 -60.1  5.7      66.0   236   F  1   1334  18 16 21

18 20 20  J1340+3754   19 24 16  21.4 -57.8  5.7      66.6    -4   1  1   1334  18 20 20
18 22 20  =1338+381    19 26 16  21.1 -57.6  5.8      66.3   116   F  1   1350  18 20 21

18 24 20  J1308+3546   19 28 16  14.0 -56.5  6.3      61.6   106   1  1   1350  18 24 20
18 26 00  ---          19 29 57  13.7 -56.3  6.4      61.4   100   F  1   1362  18 24 21

18 26 00  NGC5033      19 29 57  15.0 -56.1  6.3      62.2    -4   1  1   1362  18 26 00
18 30 00  ---          19 33 57  14.3 -55.7  6.3      61.7   236   F  1   1393  18 26 01

18 30 00  J1308+3546   19 33 57  13.0 -55.9  6.4      60.9    -4   1  1   1393  18 30 00
18 32 00  ---          19 35 58  12.7 -55.7  6.5      60.6   116   F  1   1409  18 30 01

18 32 00  NGC5033      19 35 58  14.0 -55.5  6.4      61.4    -4   1  1   1409  18 32 00
18 36 00  ---          19 39 58  13.3 -55.1  6.4      60.9   236   F  1   1440  18 32 01

18 36 00  J1308+3546   19 39 58  12.0 -55.3  6.5      60.1    -4   1  1   1440  18 36 00
18 38 00  ---          19 41 59  11.6 -55.1  6.6      59.9   116   F  1   1455  18 36 01

18 40 00  J1340+3754   19 43 59  17.9 -56.0  6.1      64.1   108   1  1   1455  18 40 00
18 41 40  =1338+381    19 45 39  17.6 -55.9  6.1      63.9   100   F  1   1468  18 40 01

18 41 40  NGC5273      19 45 39  16.9 -58.2  6.1      63.5    -4   1  1   1468  18 41 40
18 45 40  ---          19 49 40  16.2 -57.8  6.1      63.0   236   F  1   1499  18 41 41

18 45 40  J1340+3754   19 49 40  16.9 -55.5  6.1      63.4    -4   1  1   1499  18 45 40
18 47 40  =1338+381    19 51 40  16.6 -55.3  6.2      63.2   116   F  1   1515  18 45 41

18 47 40  NGC5273      19 51 40  15.8 -57.6  6.2      62.8    -4   1  1   1515  18 47 40
18 51 40  ---          19 55 41  15.1 -57.2  6.2      62.3   236   F  1   1546  18 47 41

18 51 40  J1340+3754   19 55 41  15.8 -55.0  6.2      62.6    -4   1  1   1546  18 51 40
18 53 40  =1338+381    19 57 41  15.5 -54.8  6.3      62.4   116   F  1   1561  18 51 41
Schedule for SHANGHAI  (Code Sh )                                   Page   7
               Parsec scale radio nuclei in nearby Seyfert galaxies from a complete sam
  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.
         For disks, the footages are really the GBytes
  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
----------------------------------------------------------------------------------------

 --- Wed   6 Jun 2007   Day 157 ---

18 57 40  3C345        20 01 42  49.2 -63.6  3.3      86.3   182   1  1   1561  18 57 40
19 07 40  ---          20 11 43  47.3 -63.3  3.5      84.9   600   F  1   1639  18 57 41

19 10 40  J1308+3546   20 14 44   6.0 -51.5  7.1      55.6   109   1  1   1639  19 10 40
19 12 40  ---          20 16 44   5.7 -51.3  7.1      55.4   120   F  1   1654  19 10 41

19 12 40  NGC5033      20 16 44   7.0 -51.2  7.0      56.1    -4   1  1   1654  19 12 40
19 16 40  ---          20 20 45   6.3 -50.7  7.1      55.6   236   F  1   1685  19 12 41

19 18 40  NGC5033      20 22 45   6.0 -50.5  7.1      55.3   117   1  1   1685  19 18 40
19 22 40  ---          20 26 46   5.3 -50.0  7.2      54.8   240   F  1   1716  19 18 41

19 26 40  J1340+3754   20 30 47   9.8 -51.5  6.8      58.0   230   1  1   1716  19 26 40
19 28 40  =1338+381    20 32 47   9.5 -51.2  6.9      57.8   120   F  1   1732  19 26 41

19 28 40  NGC5273      20 32 47   8.6 -53.4  6.8      57.7    -4   1  1   1732  19 28 40
19 32 40  ---          20 36 48   7.9 -52.9  6.9      57.2   236   F  1   1762  19 28 41

19 32 40  J1340+3754   20 36 48   8.8 -50.8  6.9      57.2    -4   1  1   1762  19 32 40
19 34 40  =1338+381    20 38 48   8.5 -50.6  7.0      56.9   116   F  1   1778  19 32 41

19 34 40  NGC5273      20 38 48   7.6 -52.7  6.9      56.9    -4   1  1   1778  19 34 40
19 38 40  ---          20 42 49   6.9 -52.2  7.0      56.4   236   F  1   1809  19 34 41

19 38 40  J1340+3754   20 42 49   7.8 -50.2  7.0      56.4    -4   1  1   1809  19 38 40
19 40 40  =1338+381    20 44 49   7.5 -49.9  7.1      56.1   116   F  1   1824  19 38 41


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


 Setup file: eg037b.18cm
   Matches group sh18cm in /irasoft/sched/catalogs/freq.dat
    Huang Xinyong 27Sept05
    ****** Only  244.98 of  256.00 MHz total bandwidth is within the IFs
           in the setup file before any FREQ or DOPPLER shifts.

   Setup group:    7         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:   7  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 -- Parsec scale radio nuclei in nearby Seyfert galaxies from a complete sam
     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)

 * NGC4051           12 00 36.396526   * 12 03 09.613000     12 03 33.626574       0.00
                     44 48 34.49046    * 44 31 52.65000      44 29 33.80749        0.00
                     From catalog imbedded in main SCHED input file.
                        1.417 scan hours,     34.420 baseline hours above horizon.

 * NGC5033           13 11 09.172609   * 13 13 27.475000     13 13 49.537974       0.00
                     36 51 30.38369    * 36 35 37.94000      36 33 20.65276        0.00
                     From catalog imbedded in main SCHED input file.
                        1.467 scan hours,     42.747 baseline hours above horizon.

 * NGC5273           13 39 55.142349   * 13 42 08.370000     13 42 29.801814       0.00
                     35 54 21.44090    * 35 39 15.33000      35 37 03.05795        0.00
                     From catalog imbedded in main SCHED input file.
                        1.467 scan hours,     41.660 baseline hours above horizon.

 * J1221+4411        12 18 59.032728   * 12 21 27.044650     12 21 50.412648       0.42
   1218+444          44 28 07.64767    * 44 11 29.67155      44 09 10.41670        0.60
                     /irasoft/sched/catalogs/sources.vlba
                     VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro
                        0.872 scan hours,     18.128 baseline hours above horizon.

 * J1308+3546        13 06 03.930616   * 13 08 23.709146     13 08 45.945009       0.27
                     36 02 36.26229    * 35 46 37.16399      35 44 18.95445        0.45
                     /irasoft/sched/catalogs/sources.vlba
                     VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro
                        1.072 scan hours,     26.965 baseline hours above horizon.

 * J1340+3754        13 38 11.121586   * 13 40 22.951814     13 40 44.223944       0.33
   1338+381          38 09 53.16408    * 37 54 43.83329      37 52 31.72082        0.49
   J1340+37          /irasoft/sched/catalogs/sources.vlba
                     VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro
                        1.072 scan hours,     26.725 baseline hours above horizon.

   J1642+3948        16 41 17.606231   * 16 42 58.809968     16 43 15.927328       0.26
   1641+399          39 54 10.81494    * 39 48 36.99400      39 47 39.20818        0.40
 * 3C345             /irasoft/sched/catalogs/sources.vlba
   J1642+39          VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro
                        0.333 scan hours,     11.850 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) 
   NGC4051             85.2
   NGC5033            100.6
   NGC5273            105.6
   J1221+4411          88.2
   J1308+3546         100.3
   J1340+3754         103.8
   3C345              117.4

  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 

