  COVER INFORMATION 

 Station:    SHANGHAI  (Code Sh ) 
 Experiment: EVN Astrometry of PSR J1022+1001
 Exp. Code:  EY010B  


Schedule Version:       1.00
Processed by SCHED version:   9.30  Release near March 23, 2010

PI:       Zhen Yan

Address:  Shanghai Astronomical Observatory
          NO.80 Nandan Road
          Shanghai
          China

Phone:    86-13402136110
EMAIL:    yanzhen@shao.ac.cn,zshen@shao.ac.cn
Fax:      86-21-64281104
Phone during observation: 86-13402136110

Observing mode: Phase-referencing of a source at 18cm (512 Mb/s)

Notes:    Target source: PSR J1022+1001, s=3mJy(1.4GHz)
          Phase calibrator source: J1025+1253, s=0.88Jy(S-band)
          Fringe finder, etc: J0927+3902 (4C39.25), s=4.71Jy(S-band)
          Fringe finder, etc: J1310+3220 (1308+326), s=2.23Jy(S-band)

Schedule for SHANGHAI  (Code Sh )                                   Page   2
               EVN Astrometry of PSR J1022+1001
  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   9 Jun 2010   Day 160 ---

 Next scan frequencies:  1634.49  1634.49  1634.49  1634.49  1650.49  1650.49
                         1650.49  1650.49  1666.49  1666.49  1666.49  1666.49
                         1682.49  1682.49  1682.49  1682.49
 Next BBC frequencies:    665.51   665.51   665.51   665.51   649.51   649.51
                          649.51   649.51   633.51   633.51   633.51   633.51
                          617.51   617.51   617.51   617.51
 Next scan bandwidths:      8.00     8.00     8.00     8.00     8.00     8.00
                            8.00     8.00     8.00     8.00     8.00     8.00
                            8.00     8.00     8.00     8.00

11 30 00  J0927+3902   12 45 43  49.2 -64.8  3.3      85.5     0   1  1      0  11 30 00
11 37 00  =0923+392    12 52 44  47.9 -64.6  3.4      84.5   420   F  1     27  11 30 01

11 42 30  J1025+1253   12 58 15  50.6 251.0  2.5      56.1    10   1  1     27  11 42 30
11 44 30  =1023+131    13 00 15  50.2 251.4  2.6      56.3   120   F  1     35  11 42 31

11 44 30  J1022+1001   13 00 15  48.0 248.4  2.6      54.0    -8   1  1     35  No stop 
11 47 45  ---          13 03 31  47.4 249.1  2.7      54.3   187   F  1     47  11 44 31

11 48 30  J1025+1253   13 04 16  49.4 252.2  2.6      56.8    37   1  1     47  11 48 30
11 50 00  =1023+131    13 05 46  49.1 252.5  2.7      56.9    90   F  1     53  11 48 31

11 50 00  J1022+1001   13 05 46  46.9 249.6  2.7      54.6    -8   1  1     53  No stop 
11 53 15  ---          13 09 01  46.2 250.3  2.8      54.9   187   F  1     66  11 50 01

11 53 15  J1025+1253   13 09 01  48.5 253.2  2.7      57.2    -8   1  1     66  No stop 
11 54 45  =1023+131    13 10 32  48.1 253.5  2.7      57.4    82   F  1     72  11 53 16

11 54 45  J1022+1001   13 10 32  45.9 250.6  2.8      55.1    -8   1  1     72  No stop 
11 58 00  ---          13 13 47  45.3 251.2  2.8      55.4   187   F  1     84  11 54 46

11 58 45  J1025+1253   13 14 32  47.3 254.3  2.8      57.7    37   1  1     84  11 58 45
12 00 15  =1023+131    13 16 03  47.0 254.6  2.8      57.8    90   F  1     90  11 58 46

12 00 15  J1022+1001   13 16 03  44.8 251.7  2.9      55.6    -8   1  1     90  No stop 
12 03 30  ---          13 19 18  44.2 252.3  2.9      55.9   187   F  1    103  12 00 16

12 03 30  J1025+1253   13 19 18  46.3 255.2  2.9      58.1    -8   1  1    103  No stop 
12 05 00  =1023+131    13 20 48  46.0 255.4  2.9      58.2    82   F  1    108  12 03 31

12 05 00  J1022+1001   13 20 48  43.9 252.6  3.0      56.1    -8   1  1    108  No stop 
12 08 15  ---          13 24 04  43.2 253.2  3.0      56.3   187   F  1    121  12 05 01
Schedule for SHANGHAI  (Code Sh )                                   Page   3
               EVN Astrometry of PSR J1022+1001
  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   9 Jun 2010   Day 160 ---

12 09 00  J1025+1253   13 24 49  45.2 256.2  3.0      58.5    38   1  1    121  12 09 00
12 10 30  =1023+131    13 26 19  44.9 256.4  3.0      58.6    90   F  1    127  12 09 01

12 10 30  J1022+1001   13 26 19  42.7 253.6  3.0      56.5    -8   1  1    127  No stop 
12 13 45  ---          13 29 35  42.1 254.2  3.1      56.8   187   F  1    139  12 10 31

12 13 45  J1025+1253   13 29 35  44.2 257.0  3.1      58.9    -8   1  1    139  No stop 
12 15 15  =1023+131    13 31 05  43.9 257.3  3.1      59.0    82   F  1    145  12 13 46

12 15 15  J1022+1001   13 31 05  41.7 254.5  3.1      56.9    -8   1  1    145  No stop 
12 18 30  ---          13 34 21  41.1 255.1  3.2      57.2   187   F  1    158  12 15 16

12 19 15  J1025+1253   13 35 06  43.0 258.0  3.1      59.2    38   1  1    158  12 19 15
12 20 45  =1023+131    13 36 36  42.7 258.2  3.2      59.3    90   F  1    164  12 19 16

12 20 45  J1022+1001   13 36 36  40.6 255.5  3.2      57.3    -8   1  1    164  No stop 
12 24 00  ---          13 39 51  39.9 256.1  3.3      57.5   187   F  1    176  12 20 46

12 24 00  J1025+1253   13 39 51  42.0 258.8  3.2      59.5    -8   1  1    176  No stop 
12 25 30  =1023+131    13 41 22  41.7 259.0  3.2      59.6    82   F  1    182  12 24 01

12 25 30  J1022+1001   13 41 22  39.6 256.3  3.3      57.6    -8   1  1    182  No stop 
12 28 45  ---          13 44 37  38.9 256.9  3.4      57.9   187   F  1    195  12 25 31

12 29 30  J1025+1253   13 45 22  40.9 259.7  3.3      59.8    38   1  1    195  12 29 30
12 31 00  =1023+131    13 46 53  40.6 259.9  3.3      59.9    90   F  1    200  12 29 31

12 31 00  J1022+1001   13 46 53  38.5 257.2  3.4      58.0    -8   1  1    200  No stop 
12 34 15  ---          13 50 08  37.8 257.8  3.4      58.2   187   F  1    213  12 31 01

12 34 15  J1025+1253   13 50 08  39.9 260.5  3.4      60.0    -8   1  1    213  No stop 
12 35 45  =1023+131    13 51 38  39.6 260.7  3.4      60.1    82   F  1    219  12 34 16

12 35 45  J1022+1001   13 51 38  37.5 258.0  3.5      58.3    -8   1  1    219  No stop 
12 39 00  ---          13 54 54  36.8 258.6  3.5      58.4   187   F  1    231  12 35 46

12 39 45  J1025+1253   13 55 39  38.7 261.3  3.5      60.2    38   1  1    231  12 39 45
12 41 15  =1023+131    13 57 09  38.4 261.6  3.5      60.3    90   F  1    237  12 39 46

12 41 15  J1022+1001   13 57 09  36.3 258.9  3.6      58.6    -8   1  1    237  No stop 
12 44 30  ---          14 00 25  35.6 259.4  3.6      58.7   187   F  1    250  12 41 16

12 44 30  J1025+1253   14 00 25  37.7 262.1  3.6      60.4    -8   1  1    250  No stop 
12 46 00  =1023+131    14 01 55  37.4 262.3  3.6      60.5    82   F  1    255  12 44 31
Schedule for SHANGHAI  (Code Sh )                                   Page   4
               EVN Astrometry of PSR J1022+1001
  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   9 Jun 2010   Day 160 ---

12 46 00  J1022+1001   14 01 55  35.3 259.7  3.6      58.8    -8   1  1    255  No stop 
12 49 15  ---          14 05 11  34.6 260.2  3.7      58.9   187   F  1    268  12 46 01

12 50 00  J1025+1253   14 05 56  36.5 262.9  3.7      60.6    38   1  1    268  12 50 00
12 51 30  =1023+131    14 07 26  36.2 263.1  3.7      60.7    90   F  1    274  12 50 01

12 51 30  J1022+1001   14 07 26  34.2 260.5  3.7      59.0    -8   1  1    274  No stop 
12 54 45  ---          14 10 42  33.5 261.0  3.8      59.2   187   F  1    286  12 51 31

12 54 45  J1025+1253   14 10 42  35.5 263.6  3.7      60.8    -8   1  1    286  No stop 
12 56 15  =1023+131    14 12 12  35.2 263.8  3.8      60.8    82   F  1    292  12 54 46

12 56 15  J1022+1001   14 12 12  33.1 261.2  3.8      59.2    -8   1  1    292  No stop 
12 59 30  ---          14 15 27  32.5 261.7  3.9      59.4   187   F  1    305  12 56 16

13 00 15  J1025+1253   14 16 12  34.4 264.4  3.8      60.9    38   1  1    305  13 00 15
13 01 45  =1023+131    14 17 43  34.0 264.6  3.9      61.0    90   F  1    311  13 00 16

13 01 45  J1022+1001   14 17 43  32.0 262.1  3.9      59.4    -8   1  1    311  No stop 
13 05 00  ---          14 20 58  31.3 262.5  4.0      59.5   187   F  1    323  13 01 46

13 05 00  J1025+1253   14 20 58  33.3 265.1  3.9      61.0    -8   1  1    323  No stop 
13 06 30  =1023+131    14 22 28  33.0 265.3  3.9      61.1    82   F  1    329  13 05 01

13 06 30  J1022+1001   14 22 28  31.0 262.8  4.0      59.6    -8   1  1    329  No stop 
13 09 45  ---          14 25 44  30.3 263.2  4.0      59.7   187   F  1    342  13 06 31

13 10 30  J1025+1253   14 26 29  32.2 265.8  4.0      61.2    38   1  1    342  13 10 30
13 12 00  =1023+131    14 27 59  31.8 266.0  4.0      61.2    90   F  1    347  13 10 31

13 12 00  J1022+1001   14 27 59  29.8 263.6  4.1      59.8    -8   1  1    347  No stop 
13 15 15  ---          14 31 15  29.1 264.0  4.1      59.8   187   F  1    360  13 12 01

13 15 15  J1025+1253   14 31 15  31.1 266.5  4.1      61.2    -8   1  1    360  No stop 
13 16 45  =1023+131    14 32 45  30.8 266.7  4.1      61.3    82   F  1    366  13 15 16

13 16 45  J1022+1001   14 32 45  28.8 264.2  4.2      59.9    -8   1  1    366  No stop 
13 20 00  ---          14 36 01  28.1 264.7  4.2      60.0   187   F  1    378  13 16 46

13 20 45  J1025+1253   14 36 46  30.0 267.2  4.2      61.3    38   1  1    378  13 20 45
13 22 45  =1023+131    14 38 46  29.5 267.5  4.2      61.3   120   F  1    386  13 20 46

13 26 05  J0927+3902   14 42 07  27.2 301.1  5.2      70.6   162   1  1    386  13 26 05
13 33 40  =0923+392    14 49 43  25.8 301.7  5.4      69.7   455   F  1    415  13 26 06
Schedule for SHANGHAI  (Code Sh )                                   Page   5
               EVN Astrometry of PSR J1022+1001
  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   9 Jun 2010   Day 160 ---

13 37 00  J1025+1253   14 53 03  26.5 269.4  4.4      61.4   164   1  1    415  13 37 00
13 39 00  =1023+131    14 55 04  26.0 269.7  4.5      61.4   120   F  1    423  13 37 01

13 39 00  J1022+1001   14 55 04  24.0 267.3  4.5      60.3    -8   1  1    423  No stop 
13 42 15  ---          14 58 19  23.3 267.7  4.6      60.3   187   F  1    436  13 39 01

13 43 00  J1025+1253   14 59 04  25.2 270.2  4.5      61.4    38   1  1    436  13 43 00
13 44 30  =1023+131    15 00 35  24.9 270.4  4.6      61.4    90   F  1    442  13 43 01

13 44 30  J1022+1001   15 00 35  22.8 268.0  4.6      60.3    -8   1  1    442  No stop 
13 47 45  ---          15 03 50  22.1 268.5  4.7      60.4   187   F  1    454  13 44 31

13 47 45  J1025+1253   15 03 50  24.2 270.8  4.6      61.4    -8   1  1    454  No stop 
13 49 15  =1023+131    15 05 20  23.8 271.0  4.6      61.4    82   F  1    460  13 47 46

13 49 15  J1022+1001   15 05 20  21.8 268.7  4.7      60.4    -8   1  1    460  No stop 
13 52 30  ---          15 08 36  21.1 269.1  4.8      60.4   187   F  1    473  13 49 16

13 53 15  J1025+1253   15 09 21  23.0 271.5  4.7      61.4    38   1  1    473  13 53 15
13 54 45  =1023+131    15 10 51  22.7 271.7  4.7      61.4    90   F  1    478  13 53 16

13 54 45  J1022+1001   15 10 51  20.6 269.4  4.8      60.4    -8   1  1    478  No stop 
13 58 00  ---          15 14 07  19.9 269.8  4.8      60.4   187   F  1    491  13 54 46

13 58 00  J1025+1253   15 14 07  22.0 272.1  4.8      61.4    -8   1  1    491  No stop 
13 59 30  =1023+131    15 15 37  21.7 272.3  4.8      61.3    82   F  1    497  13 58 01

13 59 30  J1022+1001   15 15 37  19.6 270.0  4.9      60.4    -8   1  1    497  No stop 
14 02 45  ---          15 18 53  18.9 270.4  4.9      60.4   187   F  1    509  13 59 31

14 03 30  J1025+1253   15 19 38  20.8 272.8  4.9      61.3    38   1  1    509  14 03 30
14 05 00  =1023+131    15 21 08  20.5 273.0  4.9      61.3    90   F  1    515  14 03 31

14 05 00  J1022+1001   15 21 08  18.4 270.7  5.0      60.4    -8   1  1    515  No stop 
14 08 15  ---          15 24 24  17.7 271.1  5.0      60.4   187   F  1    528  14 05 01

14 08 15  J1025+1253   15 24 24  19.8 273.4  5.0      61.2    -8   1  1    528  No stop 
14 09 45  =1023+131    15 25 54  19.5 273.6  5.0      61.2    82   F  1    534  14 08 16

14 09 45  J1022+1001   15 25 54  17.4 271.3  5.0      60.4    -8   1  1    534  No stop 
14 13 00  ---          15 29 09  16.7 271.7  5.1      60.3   187   F  1    546  14 09 46

14 13 45  J1025+1253   15 29 55  18.6 274.1  5.1      61.2    38   1  1    546  14 13 45
14 15 15  =1023+131    15 31 25  18.3 274.3  5.1      61.1    90   F  1    552  14 13 46
Schedule for SHANGHAI  (Code Sh )                                   Page   6
               EVN Astrometry of PSR J1022+1001
  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   9 Jun 2010   Day 160 ---

14 15 15  J1022+1001   15 31 25  16.2 272.0  5.1      60.3    -8   1  1    552  No stop 
14 18 30  ---          15 34 40  15.5 272.4  5.2      60.3   187   F  1    564  14 15 16

14 18 30  J1025+1253   15 34 40  17.6 274.7  5.1      61.1    -8   1  1    564  No stop 
14 20 00  =1023+131    15 36 11  17.3 274.8  5.2      61.1    82   F  1    570  14 18 31

14 20 00  J1022+1001   15 36 11  15.2 272.6  5.2      60.3    -8   1  1    570  No stop 
14 23 15  ---          15 39 26  14.5 273.0  5.3      60.3   187   F  1    583  14 20 01

14 24 00  J1025+1253   15 40 11  16.4 275.3  5.2      61.0    38   1  1    583  14 24 00
14 25 30  =1023+131    15 41 41  16.1 275.5  5.3      60.9    90   F  1    589  14 24 01

14 25 30  J1022+1001   15 41 41  14.0 273.3  5.3      60.2    -8   1  1    589  No stop 
14 28 45  ---          15 44 57  13.3 273.7  5.4      60.2   187   F  1    601  14 25 31

14 28 45  J1025+1253   15 44 57  15.4 275.9  5.3      60.9    -8   1  1    601  No stop 
14 30 15  =1023+131    15 46 27  15.1 276.1  5.3      60.8    82   F  1    607  14 28 46

14 30 15  J1022+1001   15 46 27  13.0 273.9  5.4      60.2    -8   1  1    607  No stop 
14 33 30  ---          15 49 43  12.3 274.3  5.4      60.1   187   F  1    620  14 30 16

14 34 15  J1025+1253   15 50 28  14.2 276.6  5.4      60.7    38   1  1    620  14 34 15
14 35 45  =1023+131    15 51 58  13.9 276.8  5.4      60.7    90   F  1    625  14 34 16

14 35 45  J1022+1001   15 51 58  11.8 274.6  5.5      60.1    -8   1  1    625  No stop 
14 39 00  ---          15 55 14  11.1 275.0  5.5      60.0   187   F  1    638  14 35 46

14 39 00  J1025+1253   15 55 14  13.2 277.2  5.5      60.6    -8   1  1    638  No stop 
14 40 30  =1023+131    15 56 44  12.9 277.4  5.5      60.6    82   F  1    644  14 39 01

14 40 30  J1022+1001   15 56 44  10.8 275.2  5.6      60.0    -8   1  1    644  No stop 
14 43 45  ---          15 59 59  10.1 275.6  5.6      59.9   187   F  1    656  14 40 31

14 44 30  J1025+1253   16 00 45  12.0 277.9  5.6      60.5    38   1  1    656  14 44 30
14 46 00  =1023+131    16 02 15  11.7 278.1  5.6      60.4    90   F  1    662  14 44 31

14 46 00  J1022+1001   16 02 15   9.7 275.9  5.6      59.9    -8   1  1    662  No stop 
14 49 15  ---          16 05 30   9.0 276.3  5.7      59.8   187   F  1    675  14 46 01

14 49 15  J1025+1253   16 05 30  11.0 278.5  5.6      60.3    -8   1  1    675  No stop 
14 50 45  =1023+131    16 07 01  10.7 278.6  5.7      60.3    82   F  1    681  14 49 16

14 50 45  J1022+1001   16 07 01   8.6 276.5  5.7      59.8    -8   1  1    681  No stop 
14 54 00  ---          16 10 16   7.9 276.9  5.8      59.7   187   F  1    693  14 50 46
Schedule for SHANGHAI  (Code Sh )                                   Page   7
               EVN Astrometry of PSR J1022+1001
  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   9 Jun 2010   Day 160 ---

14 54 45  J1025+1253   16 11 01   9.9 279.1  5.7      60.1    38   1  1    693  14 54 45
14 56 15  =1023+131    16 12 31   9.5 279.3  5.8      60.1    90   F  1    699  14 54 46

14 56 15  J1022+1001   16 12 31   7.5 277.2  5.8      59.6    -8   1  1    699  No stop 
14 59 30  ---          16 15 47   6.8 277.6  5.9      59.5   187   F  1    712  14 56 16

14 59 30  J1025+1253   16 15 47   8.9 279.7  5.8      60.0    -8   1  1    712  No stop 
15 01 00  =1023+131    16 17 17   8.5 279.9  5.8      59.9    82   F  1    717  14 59 31

15 01 00  J1022+1001   16 17 17   6.5 277.8  5.9      59.5    -8   1  1    717  No stop 
15 04 15  ---          16 20 33   5.8 278.2  6.0      59.4   187   F  1    730  15 01 01

15 05 00  J1025+1253   16 21 18   7.7 280.4  5.9      59.7    38   1  1    730  15 05 00
15 06 30  =1023+131    16 22 48   7.4 280.6  5.9      59.7    90   F  1    736  15 05 01

15 06 30  J1022+1001   16 22 48   5.3 278.5  6.0      59.3    -8   1  1    736  No stop 
15 09 45  ---          16 26 04   4.6 278.9  6.0  D   59.2     0   F  1    748  15 06 31

15 09 45  J1025+1253   16 26 04   6.7 281.0  6.0      59.6    -7   1  1    748  No stop 
15 11 15  =1023+131    16 27 34   6.4 281.2  6.0      59.5    83   F  1    754  15 09 46

15 15 15  J1025+1253   16 31 35   5.5 281.7  6.1      59.3   235   1  1    754  15 15 15
15 17 15  =1023+131    16 33 35   5.1 281.9  6.1      59.2   120   F  1    762  15 15 16

15 22 00  J1310+3220   16 38 21  46.3 285.8  3.5      77.1   212   1  1    762  15 22 00
15 30 00  =1308+326    16 46 22  44.7 286.3  3.6      76.4   480   F  1    793  15 22 01


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


 Setup file: eyan.18cm
   Matching groups in /usr/local/sched9.3/catalogs/freq.dat:
     sh18cm          Huang Xinyong 27Sept05

   Setup group:    7         Station: SHANGHAI          Total bit rate:  512
   Format: MKIV1:2           Bits per sample: 2         Sample rate: 16.000
   Number of channels: 16                               Speedup factor:   1.00

   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=    1634.49   1634.49   1634.49   1634.49   1650.49   1650.49   1650.49   1650.49
              1666.49   1666.49   1666.49   1666.49   1682.49   1682.49   1682.49   1682.49
   BBC fr=     665.51    665.51    665.51    665.51    649.51    649.51    649.51    649.51
               633.51    633.51    633.51    633.51    617.51    617.51    617.51    617.51
   Bandwd=      8.000     8.000     8.000     8.000     8.000     8.000     8.000     8.000
                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    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 -- EVN Astrometry of PSR J1022+1001
     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)

 * J1022+1001        10 20 19.263127   * 10 22 57.995628     10 23 31.806306       0.00
                     10 17 03.79035    * 10 01 52.61483      09 58 38.47674        0.00
                     From catalog imbedded in main SCHED input file.
                        2.058 scan hours,     50.059 baseline hours above horizon.

 * J0927+3902        09 23 55.319214   * 09 27 03.013935     09 27 42.553590       0.26
   0923+392          39 15 23.56647    * 39 02 20.85187      38 59 42.39877        0.40
   4C39.25           From catalog imbedded in main SCHED input file.
   J0927+39          VLBA Calib Survey - GSFC sols. - created L.Petrov 2008a_astro
                        0.243 scan hours,      6.806 baseline hours above horizon.

 * J1025+1253        10 23 16.285228   * 10 25 56.285369     10 26 30.383251       0.31
   1023+131          13 09 05.49493    * 12 53 49.02205      12 50 34.72496        0.21
                     From catalog imbedded in main SCHED input file.
                     VLBA Calib Survey - GSFC sols. - created L.Petrov 2008a_astro
                        1.033 scan hours,     23.362 baseline hours above horizon.

 * J1310+3220        13 08 07.560131   * 13 10 28.663850     13 10 59.796745       0.24
   1308+326          32 36 40.23883    * 32 20 43.78290      32 17 25.99264        0.40
   J1310+32          From catalog imbedded in main SCHED input file.
                     VLBA Calib Survey - GSFC sols. - created L.Petrov 2008a_astro
                        0.133 scan hours,      3.733 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) 
   J1022+1001          75.4
   J0927+3902          56.2
   J1025+1253          75.1
   J1310+3220         100.5

  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 

