  COVER INFORMATION 

 Station:    SHANGHAI  (Code Sh ) 
 Experiment: IRAS 19312+1950
 Exp. Code:  EB037D  


Schedule Version:       2.00                                              
Processed by SCHED version:   6.05  June 2006                             

PI:       A. Brunthaler                                                   

Address:  MPIfR                                                           
          Auf dem Huegel 69                                               
          53121 Bonn                                                      
          Germany                                                         

Phone:    +49 228 525 377                                                 
EMAIL:    brunthal@mpifr-bonn.mpg.de                                      
Fax:      +49 228 525 229                                                 
Phone during observation: +49 228 525 377                                 

Observing mode: Phase-referencing at 13cm (512 Mb/s)                      

Notes:    TURN PHASE-CAL OFF                                              
                                                                          
                                                                          
                                                                          

Schedule for SHANGHAI  (Code Sh )                                   Page   2
               IRAS 19312+1950
  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
----------------------------------------------------------------------------------------

 --- Thu  30 Oct 2008   Day 304 ---

 Next scan frequencies:  1610.05  1610.05  1627.17  1627.17  1643.17  1643.17
                         1659.17  1659.17
 Next BBC frequencies:    689.95   689.95   672.83   672.83   656.83   656.83
                          640.83   640.83
 Next scan bandwidths:     16.00    16.00    16.00    16.00    16.00    16.00
                           16.00    16.00

10 30 00  3C345        21 11 15  36.0 -60.9  4.5      77.0     0   1  1      0  10 30 00
10 35 00  ---          21 16 16  35.1 -60.7  4.5      76.3   300   F  1     19  10 30 01

10 51 12  1923+210     21 32 31  60.1 258.2  2.1      64.0   652   1  1     19  10 51 12
10 52 42  ---          21 34 01  59.8 258.5  2.1      64.1    90   F  1     25  10 51 13

10 53 12  1932+204     21 34 31  61.3 255.6  2.0      62.3    25   1  1     25  10 53 12
10 54 42  ---          21 36 01  61.0 255.9  2.0      62.5    90   F  1     31  10 53 13

10 54 42  IRAS19312    21 36 01  60.4 255.3  2.0      61.8    -3   1  1     31  10 54 42
10 56 42  ---          21 38 02  60.0 255.7  2.1      62.0   117   F  1     39  10 54 43

10 56 42  1932+204     21 38 02  60.6 256.4  2.0      62.7    -3   1  1     39  10 56 42
10 58 42  ---          21 40 02  60.2 256.8  2.1      62.9   117   F  1     46  10 56 43

10 58 42  IRAS19312    21 40 02  59.6 256.2  2.1      62.2    -3   1  1     46  10 58 42
11 00 42  ---          21 42 02  59.1 256.6  2.1      62.4   117   F  1     54  10 58 43

11 00 42  1932+204     21 42 02  59.8 257.2  2.1      63.1    -3   1  1     54  11 00 42
11 02 42  ---          21 44 03  59.4 257.7  2.1      63.3   117   F  1     62  11 00 43

11 02 42  IRAS19312    21 44 03  58.7 257.0  2.2      62.6    -3   1  1     62  11 02 42
11 04 42  ---          21 46 03  58.3 257.4  2.2      62.8   117   F  1     70  11 02 43

11 04 42  1932+204     21 46 03  58.9 258.1  2.2      63.5    -3   1  1     70  11 04 42
11 06 42  ---          21 48 03  58.5 258.5  2.2      63.6   117   F  1     77  11 04 43

11 07 12  1932+204     21 48 33  58.4 258.6  2.2      63.7    28   1  1     77  11 07 12
11 08 42  ---          21 50 03  58.1 258.9  2.2      63.8    90   F  1     83  11 07 13

11 08 42  IRAS19312    21 50 03  57.5 258.2  2.3      63.1    -3   1  1     83  11 08 42
11 10 42  ---          21 52 04  57.0 258.6  2.3      63.3   117   F  1     91  11 08 43

11 10 42  1932+204     21 52 04  57.7 259.2  2.3      64.0    -3   1  1     91  11 10 42
11 12 42  ---          21 54 04  57.3 259.6  2.3      64.1   117   F  1     99  11 10 43
Schedule for SHANGHAI  (Code Sh )                                   Page   3
               IRAS 19312+1950
  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
----------------------------------------------------------------------------------------

 --- Thu  30 Oct 2008   Day 304 ---

11 12 42  IRAS19312    21 54 04  56.6 259.0  2.3      63.4    -3   1  1     99  11 12 42
11 14 42  ---          21 56 04  56.2 259.4  2.4      63.6   117   F  1    106  11 12 43

11 14 42  1932+204     21 56 04  56.8 260.0  2.3      64.2    -3   1  1    106  11 14 42
11 16 42  ---          21 58 05  56.4 260.4  2.4      64.4   117   F  1    114  11 14 43

11 16 42  IRAS19312    21 58 05  55.8 259.8  2.4      63.7    -3   1  1    114  11 16 42
11 18 42  ---          22 00 05  55.4 260.1  2.4      63.8   117   F  1    122  11 16 43

11 18 42  1932+204     22 00 05  56.0 260.7  2.4      64.5    -3   1  1    122  11 18 42
11 20 42  ---          22 02 05  55.6 261.1  2.4      64.6   117   F  1    130  11 18 43

11 21 12  1932+204     22 02 36  55.5 261.2  2.5      64.6    28   1  1    130  11 21 12
11 22 42  ---          22 04 06  55.1 261.5  2.5      64.7    90   F  1    135  11 21 13

11 22 42  IRAS19312    22 04 06  54.5 260.9  2.5      64.1    -3   1  1    135  11 22 42
11 24 42  ---          22 06 06  54.1 261.2  2.5      64.2   117   F  1    143  11 22 43

11 24 42  1932+204     22 06 06  54.7 261.8  2.5      64.8    -3   1  1    143  11 24 42
11 26 42  ---          22 08 06  54.3 262.1  2.5      64.9   117   F  1    151  11 24 43

11 26 42  IRAS19312    22 08 06  53.7 261.6  2.6      64.3    -3   1  1    151  11 26 42
11 28 42  ---          22 10 07  53.2 261.9  2.6      64.4   117   F  1    159  11 26 43

11 28 42  1932+204     22 10 07  53.9 262.5  2.6      65.0    -3   1  1    159  11 28 42
11 30 42  ---          22 12 07  53.4 262.8  2.6      65.1   117   F  1    166  11 28 43

11 30 42  IRAS19312    22 12 07  52.8 262.2  2.6      64.5    -3   1  1    166  11 30 42
11 32 42  ---          22 14 07  52.4 262.6  2.7      64.6   117   F  1    174  11 30 43

11 32 42  1932+204     22 14 07  53.0 263.1  2.6      65.2    -3   1  1    174  11 32 42
11 34 42  ---          22 16 08  52.6 263.5  2.7      65.3   117   F  1    182  11 32 43

11 35 12  1932+204     22 16 38  52.5 263.6  2.7      65.3    28   1  1    182  11 35 12
11 36 42  ---          22 18 08  52.2 263.8  2.7      65.4    90   F  1    188  11 35 13

11 36 42  IRAS19312    22 18 08  51.5 263.2  2.7      64.8    -3   1  1    188  11 36 42
11 38 42  ---          22 20 08  51.1 263.5  2.8      64.9   117   F  1    195  11 36 43

11 38 42  1932+204     22 20 08  51.7 264.1  2.7      65.5    -3   1  1    195  11 38 42
11 40 42  ---          22 22 09  51.3 264.4  2.8      65.5   117   F  1    203  11 38 43

11 40 42  IRAS19312    22 22 09  50.7 263.9  2.8      64.9    -3   1  1    203  11 40 42
11 42 42  ---          22 24 09  50.3 264.2  2.8      65.0   117   F  1    211  11 40 43
Schedule for SHANGHAI  (Code Sh )                                   Page   4
               IRAS 19312+1950
  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
----------------------------------------------------------------------------------------

 --- Thu  30 Oct 2008   Day 304 ---

11 42 42  1932+204     22 24 09  50.9 264.7  2.8      65.6    -3   1  1    211  11 42 42
11 44 42  ---          22 26 09  50.4 265.0  2.8      65.7   117   F  1    219  11 42 43

11 44 42  IRAS19312    22 26 09  49.8 264.5  2.9      65.1    -3   1  1    219  11 44 42
11 46 42  ---          22 28 10  49.4 264.8  2.9      65.1   117   F  1    226  11 44 43

11 46 42  1932+204     22 28 10  50.0 265.3  2.9      65.7    -3   1  1    226  11 46 42
11 48 42  ---          22 30 10  49.6 265.6  2.9      65.8   117   F  1    234  11 46 43

11 49 12  1923+210     22 30 40  47.8 267.8  3.1      66.5    25   1  1    234  11 49 12
11 50 42  ---          22 32 10  47.4 268.0  3.1      66.6    90   F  1    240  11 49 13

11 50 42  IRAS-B       22 32 10  48.5 265.4  3.0      65.2    -5   1  1    240  11 50 42
11 52 42  ---          22 34 11  48.1 265.7  3.0      65.3   115   F  1    248  11 50 43

11 52 42  1923+210     22 34 11  47.0 268.3  3.1      66.6    -5   1  1    248  11 52 42
11 54 42  ---          22 36 11  46.6 268.6  3.2      66.6   115   F  1    255  11 52 43

11 54 42  IRAS-B       22 36 11  47.7 266.0  3.0      65.3    -5   1  1    255  11 54 42
11 56 42  ---          22 38 11  47.3 266.3  3.1      65.4   115   F  1    263  11 54 43

11 56 42  1923+210     22 38 11  46.1 268.8  3.2      66.6    -5   1  1    263  11 56 42
11 58 42  ---          22 40 12  45.7 269.1  3.2      66.6   115   F  1    271  11 56 43

11 58 42  IRAS-B       22 40 12  46.8 266.6  3.1      65.4    -5   1  1    271  11 58 42
12 00 42  ---          22 42 12  46.4 266.8  3.1      65.5   115   F  1    279  11 58 43

12 00 42  1923+210     22 42 12  45.3 269.4  3.3      66.6    -5   1  1    279  12 00 42
12 02 42  ---          22 44 12  44.9 269.6  3.3      66.6   115   F  1    286  12 00 43

12 03 12  1923+210     22 44 42  44.8 269.7  3.3      66.6    28   1  1    286  12 03 12
12 04 42  ---          22 46 13  44.4 269.9  3.3      66.6    90   F  1    292  12 03 13

12 04 42  IRAS-B       22 46 13  45.5 267.4  3.2      65.5    -4   1  1    292  12 04 42
12 06 42  ---          22 48 13  45.1 267.7  3.2      65.5   116   F  1    300  12 04 43

12 06 42  1923+210     22 48 13  44.0 270.2  3.4      66.6    -4   1  1    300  12 06 42
12 08 42  ---          22 50 13  43.6 270.4  3.4      66.6   116   F  1    308  12 06 43

12 08 42  IRAS-B       22 50 13  44.7 268.0  3.3      65.6    -4   1  1    308  12 08 42
12 10 42  ---          22 52 14  44.3 268.2  3.3      65.6   116   F  1    315  12 08 43

12 10 42  1923+210     22 52 14  43.1 270.7  3.4      66.6    -4   1  1    315  12 10 42
12 12 42  ---          22 54 14  42.7 270.9  3.5      66.6   116   F  1    323  12 10 43
Schedule for SHANGHAI  (Code Sh )                                   Page   5
               IRAS 19312+1950
  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
----------------------------------------------------------------------------------------

 --- Thu  30 Oct 2008   Day 304 ---

12 12 42  IRAS-B       22 54 14  43.8 268.5  3.3      65.6    -4   1  1    323  12 12 42
12 14 42  ---          22 56 14  43.4 268.8  3.4      65.6   116   F  1    331  12 12 43

12 14 42  1923+210     22 56 14  42.3 271.2  3.5      66.6    -4   1  1    331  12 14 42
12 16 42  ---          22 58 15  41.9 271.4  3.5      66.6   116   F  1    339  12 14 43

12 17 12  1932+204     22 58 45  43.5 269.6  3.4      66.1    25   1  1    339  12 17 12
12 18 42  ---          23 00 15  43.2 269.8  3.4      66.1    90   F  1    344  12 17 13

12 18 42  IRAS19312    23 00 15  42.5 269.3  3.4      65.6    -3   1  1    344  12 18 42
12 20 42  ---          23 02 15  42.1 269.6  3.5      65.6   117   F  1    352  12 18 43

12 20 42  1932+204     23 02 15  42.7 270.1  3.4      66.1    -3   1  1    352  12 20 42
12 22 42  ---          23 04 16  42.3 270.3  3.5      66.1   117   F  1    360  12 20 43

12 22 42  IRAS19312    23 04 16  41.7 269.8  3.5      65.7    -3   1  1    360  12 22 42
12 24 42  ---          23 06 16  41.3 270.1  3.5      65.7   117   F  1    368  12 22 43

12 24 42  1932+204     23 06 16  41.9 270.6  3.5      66.1    -3   1  1    368  12 24 42
12 26 42  ---          23 08 16  41.4 270.8  3.5      66.1   117   F  1    375  12 24 43

12 26 42  IRAS19312    23 08 16  40.8 270.3  3.6      65.6    -3   1  1    375  12 26 42
12 28 42  ---          23 10 17  40.4 270.6  3.6      65.6   117   F  1    383  12 26 43

12 28 42  1932+204     23 10 17  41.0 271.1  3.6      66.1    -3   1  1    383  12 28 42
12 30 42  ---          23 12 17  40.6 271.3  3.6      66.1   117   F  1    391  12 28 43

12 31 12  1932+204     23 12 47  40.5 271.4  3.6      66.1    28   1  1    391  12 31 12
12 32 42  ---          23 14 17  40.2 271.6  3.6      66.1    90   F  1    397  12 31 13

12 32 42  IRAS19312    23 14 17  39.5 271.1  3.7      65.6    -3   1  1    397  12 32 42
12 34 42  ---          23 16 18  39.1 271.4  3.7      65.6   117   F  1    404  12 32 43

12 34 42  1932+204     23 16 18  39.7 271.8  3.7      66.1    -3   1  1    404  12 34 42
12 36 42  ---          23 18 18  39.3 272.1  3.7      66.0   117   F  1    412  12 34 43

12 36 42  IRAS19312    23 18 18  38.7 271.6  3.7      65.6    -3   1  1    412  12 36 42
12 38 42  ---          23 20 18  38.3 271.9  3.8      65.6   117   F  1    420  12 36 43

12 38 42  1932+204     23 20 18  38.9 272.3  3.7      66.0    -3   1  1    420  12 38 42
12 40 42  ---          23 22 19  38.4 272.6  3.8      66.0   117   F  1    428  12 38 43

12 40 42  IRAS19312    23 22 19  37.8 272.1  3.8      65.6    -3   1  1    428  12 40 42
12 42 42  ---          23 24 19  37.4 272.3  3.8      65.5   117   F  1    435  12 40 43
Schedule for SHANGHAI  (Code Sh )                                   Page   6
               IRAS 19312+1950
  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
----------------------------------------------------------------------------------------

 --- Thu  30 Oct 2008   Day 304 ---

12 42 42  1932+204     23 24 19  38.0 272.8  3.8      66.0    -3   1  1    435  12 42 42
12 44 42  ---          23 26 19  37.6 273.0  3.8      66.0   117   F  1    443  12 42 43

12 45 12  1932+204     23 26 49  37.5 273.1  3.9      65.9    28   1  1    443  12 45 12
12 46 42  ---          23 28 20  37.2 273.3  3.9      65.9    90   F  1    449  12 45 13

12 46 42  IRAS19312    23 28 20  36.5 272.8  3.9      65.5    -3   1  1    449  12 46 42
12 48 42  ---          23 30 20  36.1 273.1  3.9      65.5   117   F  1    457  12 46 43

12 48 42  1932+204     23 30 20  36.7 273.5  3.9      65.9    -3   1  1    457  12 48 42
12 50 42  ---          23 32 20  36.3 273.8  3.9      65.9   117   F  1    464  12 48 43

12 50 42  IRAS19312    23 32 20  35.7 273.3  4.0      65.4    -3   1  1    464  12 50 42
12 52 42  ---          23 34 21  35.2 273.6  4.0      65.4   117   F  1    472  12 50 43

12 52 42  1932+204     23 34 21  35.9 274.0  4.0      65.8    -3   1  1    472  12 52 42
12 54 42  ---          23 36 21  35.4 274.2  4.0      65.8   117   F  1    480  12 52 43

12 54 42  IRAS19312    23 36 21  34.8 273.8  4.0      65.4    -3   1  1    480  12 54 42
12 56 42  ---          23 38 21  34.4 274.0  4.1      65.3   117   F  1    488  12 54 43

12 56 42  1932+204     23 38 21  35.0 274.5  4.0      65.7    -3   1  1    488  12 56 42
12 58 42  ---          23 40 22  34.6 274.7  4.1      65.7   117   F  1    495  12 56 43

12 59 12  1932+204     23 40 52  34.5 274.8  4.1      65.7    28   1  1    495  12 59 12
13 00 42  ---          23 42 22  34.2 274.9  4.1      65.7    90   F  1    501  12 59 13

13 00 42  IRAS19312    23 42 22  33.5 274.5  4.1      65.3    -3   1  1    501  13 00 42
13 02 42  ---          23 44 22  33.1 274.8  4.2      65.2   117   F  1    509  13 00 43

13 02 42  1932+204     23 44 22  33.7 275.2  4.1      65.6    -3   1  1    509  13 02 42
13 04 42  ---          23 46 23  33.3 275.4  4.2      65.6   117   F  1    517  13 02 43

13 04 42  IRAS19312    23 46 23  32.7 275.0  4.2      65.2    -3   1  1    517  13 04 42
13 06 42  ---          23 48 23  32.3 275.2  4.2      65.1   117   F  1    524  13 04 43

13 06 42  1932+204     23 48 23  32.9 275.6  4.2      65.5    -3   1  1    524  13 06 42
13 08 42  ---          23 50 23  32.4 275.9  4.2      65.5   117   F  1    532  13 06 43

13 08 42  IRAS19312    23 50 23  31.8 275.5  4.3      65.1    -3   1  1    532  13 08 42
13 10 42  ---          23 52 24  31.4 275.7  4.3      65.0   117   F  1    540  13 08 43

13 10 42  1932+204     23 52 24  32.0 276.1  4.3      65.4    -3   1  1    540  13 10 42
13 12 42  ---          23 54 24  31.6 276.3  4.3      65.4   117   F  1    548  13 10 43
Schedule for SHANGHAI  (Code Sh )                                   Page   7
               IRAS 19312+1950
  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
----------------------------------------------------------------------------------------

 --- Thu  30 Oct 2008   Day 304 ---

13 13 14  1923+210     23 54 56  29.8 278.0  4.5      65.4    27   1  1    548  13 13 14
13 14 44  ---          23 56 26  29.4 278.2  4.5      65.3    90   F  1    554  13 13 15

13 15 14  1932+204     23 56 56  31.1 276.6  4.4      65.3    25   1  1    554  13 15 14
13 16 44  ---          23 58 26  30.7 276.8  4.4      65.2    90   F  1    559  13 15 15

13 16 44  IRAS19312    23 58 26  30.1 276.4  4.4      64.9    -3   1  1    559  13 16 44
13 18 44  ---          00 00 27  29.7 276.6  4.4      64.8   117   F  1    567  13 16 45

13 18 44  1932+204     00 00 27  30.3 277.0  4.4      65.2    -3   1  1    567  13 18 44
13 20 44  ---          00 02 27  29.9 277.3  4.4      65.1   117   F  1    575  13 18 45

13 20 44  IRAS19312    00 02 27  29.3 276.8  4.5      64.8    -3   1  1    575  13 20 44
13 22 44  ---          00 04 27  28.8 277.1  4.5      64.7   117   F  1    583  13 20 45

13 22 44  1932+204     00 04 27  29.5 277.5  4.5      65.1    -3   1  1    583  13 22 44
13 24 44  ---          00 06 28  29.0 277.7  4.5      65.0   117   F  1    590  13 22 45

13 24 44  IRAS19312    00 06 28  28.4 277.3  4.5      64.6    -3   1  1    590  13 24 44
13 26 44  ---          00 08 28  28.0 277.5  4.6      64.6   117   F  1    598  13 24 45

13 26 44  1932+204     00 08 28  28.6 277.9  4.5      64.9    -3   1  1    598  13 26 44
13 28 44  ---          00 10 28  28.2 278.2  4.6      64.9   117   F  1    606  13 26 45

13 29 14  1932+204     00 10 58  28.1 278.2  4.6      64.8    28   1  1    606  13 29 14
13 30 44  ---          00 12 29  27.8 278.4  4.6      64.8    90   F  1    612  13 29 15

13 30 44  IRAS19312    00 12 29  27.1 278.0  4.6      64.4    -3   1  1    612  13 30 44
13 32 44  ---          00 14 29  26.7 278.2  4.7      64.4   117   F  1    619  13 30 45

13 32 44  1932+204     00 14 29  27.3 278.6  4.6      64.7    -3   1  1    619  13 32 44
13 34 44  ---          00 16 29  26.9 278.8  4.7      64.6   117   F  1    627  13 32 45

13 34 44  IRAS19312    00 16 29  26.3 278.5  4.7      64.3    -3   1  1    627  13 34 44
13 36 44  ---          00 18 29  25.9 278.7  4.7      64.2   117   F  1    635  13 34 45

13 36 44  1932+204     00 18 29  26.5 279.1  4.7      64.6    -3   1  1    635  13 36 44
13 38 44  ---          00 20 30  26.1 279.3  4.7      64.5   117   F  1    643  13 36 45

13 38 44  IRAS19312    00 20 30  25.4 278.9  4.8      64.2    -3   1  1    643  13 38 44
13 40 44  ---          00 22 30  25.0 279.1  4.8      64.1   117   F  1    650  13 38 45

13 40 44  1932+204     00 22 30  25.6 279.5  4.8      64.4    -3   1  1    650  13 40 44
13 42 44  ---          00 24 30  25.2 279.7  4.8      64.3   117   F  1    658  13 40 45
Schedule for SHANGHAI  (Code Sh )                                   Page   8
               IRAS 19312+1950
  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
----------------------------------------------------------------------------------------

 --- Thu  30 Oct 2008   Day 304 ---

13 43 14  1932+204     00 25 01  25.1 279.8  4.8      64.3    28   1  1    658  13 43 14
13 44 44  ---          00 26 31  24.8 280.0  4.8      64.2    90   F  1    664  13 43 15

13 44 44  IRAS19312    00 26 31  24.2 279.6  4.9      63.9    -3   1  1    664  13 44 44
13 46 44  ---          00 28 31  23.7 279.8  4.9      63.9   117   F  1    672  13 44 45

13 46 44  1932+204     00 28 31  24.4 280.2  4.9      64.2    -3   1  1    672  13 46 44
13 48 44  ---          00 30 31  23.9 280.4  4.9      64.1   117   F  1    679  13 46 45

13 48 44  IRAS19312    00 30 31  23.3 280.0  4.9      63.8    -3   1  1    679  13 48 44
13 50 44  ---          00 32 32  22.9 280.3  5.0      63.7   117   F  1    687  13 48 45

13 50 44  1932+204     00 32 32  23.5 280.6  4.9      64.0    -3   1  1    687  13 50 44
13 52 44  ---          00 34 32  23.1 280.9  5.0      63.9   117   F  1    695  13 50 45

13 52 44  IRAS19312    00 34 32  22.5 280.5  5.0      63.6    -3   1  1    695  13 52 44
13 54 44  ---          00 36 32  22.0 280.7  5.0      63.5   117   F  1    703  13 52 45

13 54 44  1932+204     00 36 32  22.7 281.1  5.0      63.8    -3   1  1    703  13 54 44
13 56 44  ---          00 38 33  22.3 281.3  5.0      63.7   117   F  1    710  13 54 45

13 57 14  1932+204     00 39 03  22.2 281.4  5.1      63.7    28   1  1    710  13 57 14
13 58 44  ---          00 40 33  21.8 281.5  5.1      63.6    90   F  1    716  13 57 15

13 58 44  IRAS19312    00 40 33  21.2 281.2  5.1      63.4    -3   1  1    716  13 58 44
14 00 44  ---          00 42 33  20.8 281.4  5.1      63.3   117   F  1    724  13 58 45

14 00 44  1932+204     00 42 33  21.4 281.8  5.1      63.5    -3   1  1    724  14 00 44
14 02 44  ---          00 44 34  21.0 282.0  5.2      63.5   117   F  1    732  14 00 45

14 02 44  IRAS19312    00 44 34  20.4 281.6  5.2      63.2    -3   1  1    732  14 02 44
14 04 44  ---          00 46 34  19.9 281.9  5.2      63.1   117   F  1    739  14 02 45

14 04 44  1932+204     00 46 34  20.6 282.2  5.2      63.4    -3   1  1    739  14 04 44
14 06 44  ---          00 48 34  20.2 282.4  5.2      63.3   117   F  1    747  14 04 45

14 06 44  IRAS19312    00 48 34  19.5 282.1  5.2      63.0    -3   1  1    747  14 06 44
14 08 44  ---          00 50 35  19.1 282.3  5.3      62.9   117   F  1    755  14 06 45

14 08 44  1932+204     00 50 35  19.7 282.7  5.3      63.2    -3   1  1    755  14 08 44
14 10 44  ---          00 52 35  19.3 282.9  5.3      63.1   117   F  1    763  14 08 45

14 11 16  1923+210     00 53 07  17.6 284.5  5.4      62.7    27   1  1    763  14 11 16
14 12 46  ---          00 54 37  17.2 284.7  5.5      62.6    90   F  1    768  14 11 17
Schedule for SHANGHAI  (Code Sh )                                   Page   9
               IRAS 19312+1950
  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
----------------------------------------------------------------------------------------

 --- Thu  30 Oct 2008   Day 304 ---

14 13 16  1932+204     00 55 07  18.8 283.2  5.3      62.9    25   1  1    768  14 13 16
14 14 46  ---          00 56 37  18.5 283.3  5.4      62.8    90   F  1    774  14 13 17

14 14 46  IRAS19312    00 56 37  17.8 283.0  5.4      62.6    -3   1  1    774  14 14 46
14 16 46  ---          00 58 38  17.4 283.2  5.4      62.5   117   F  1    782  14 14 47

14 16 46  1932+204     00 58 38  18.1 283.6  5.4      62.7    -3   1  1    782  14 16 46
14 18 46  ---          01 00 38  17.6 283.8  5.4      62.6   117   F  1    790  14 16 47

14 18 46  IRAS19312    01 00 38  17.0 283.5  5.4      62.4    -3   1  1    790  14 18 46
14 20 46  ---          01 02 38  16.6 283.7  5.5      62.3   117   F  1    797  14 18 47

14 20 46  1932+204     01 02 38  17.2 284.0  5.5      62.5    -3   1  1    797  14 20 46
14 22 46  ---          01 04 39  16.8 284.2  5.5      62.4   117   F  1    805  14 20 47

14 22 46  IRAS19312    01 04 39  16.2 283.9  5.5      62.2    -3   1  1    805  14 22 46
14 24 46  ---          01 06 39  15.8 284.1  5.5      62.1   117   F  1    813  14 22 47

14 24 46  1932+204     01 06 39  16.4 284.5  5.5      62.3    -3   1  1    813  14 24 46
14 26 46  ---          01 08 39  16.0 284.7  5.6      62.2   117   F  1    821  14 24 47

14 27 16  1932+204     01 09 09  15.9 284.8  5.6      62.2    28   1  1    821  14 27 16
14 28 46  ---          01 10 40  15.6 284.9  5.6      62.1    90   F  1    826  14 27 17

14 28 46  IRAS19312    01 10 40  14.9 284.6  5.6      61.8    -3   1  1    826  14 28 46
14 30 46  ---          01 12 40  14.5 284.8  5.6      61.7   117   F  1    834  14 28 47

14 30 46  1932+204     01 12 40  15.1 285.2  5.6      62.0    -3   1  1    834  14 30 46
14 32 46  ---          01 14 40  14.7 285.4  5.7      61.8   117   F  1    842  14 30 47

14 32 46  IRAS19312    01 14 40  14.1 285.1  5.7      61.6    -3   1  1    842  14 32 46
14 34 46  ---          01 16 41  13.7 285.3  5.7      61.5   117   F  1    850  14 32 47

14 34 46  1932+204     01 16 41  14.3 285.6  5.7      61.7    -3   1  1    850  14 34 46
14 36 46  ---          01 18 41  13.9 285.8  5.7      61.6   117   F  1    857  14 34 47

14 36 46  IRAS19312    01 18 41  13.3 285.5  5.7      61.4    -3   1  1    857  14 36 46
14 38 46  ---          01 20 41  12.8 285.8  5.8      61.3   117   F  1    865  14 36 47

14 38 46  1932+204     01 20 41  13.5 286.1  5.8      61.5    -3   1  1    865  14 38 46
14 40 46  ---          01 22 42  13.1 286.3  5.8      61.4   117   F  1    873  14 38 47

14 41 16  1932+204     01 23 12  13.0 286.4  5.8      61.3    28   1  1    873  14 41 16
14 42 46  ---          01 24 42  12.7 286.5  5.8      61.2    90   F  1    879  14 41 17
Schedule for SHANGHAI  (Code Sh )                                   Page  10
               IRAS 19312+1950
  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
----------------------------------------------------------------------------------------

 --- Thu  30 Oct 2008   Day 304 ---

14 42 46  IRAS19312    01 24 42  12.0 286.2  5.8      61.0    -3   1  1    879  14 42 46
14 44 46  ---          01 26 42  11.6 286.5  5.9      60.9   117   F  1    886  14 42 47

14 44 46  1932+204     01 26 42  12.3 286.8  5.9      61.1    -3   1  1    886  14 44 46
14 46 46  ---          01 28 43  11.8 287.0  5.9      61.0   117   F  1    894  14 44 47

14 46 46  IRAS19312    01 28 43  11.2 286.7  5.9      60.8    -3   1  1    894  14 46 46
14 48 46  ---          01 30 43  10.8 286.9  5.9      60.6   117   F  1    902  14 46 47

14 48 46  1932+204     01 30 43  11.4 287.2  5.9      60.9    -3   1  1    902  14 48 46
14 50 46  ---          01 32 43  11.0 287.5  6.0      60.7   117   F  1    910  14 48 47

14 50 46  IRAS19312    01 32 43  10.4 287.2  6.0      60.5    -3   1  1    910  14 50 46
14 52 46  ---          01 34 44  10.0 287.4  6.0      60.4   117   F  1    917  14 50 47

14 52 46  1932+204     01 34 44  10.6 287.7  6.0      60.6    -3   1  1    917  14 52 46
14 54 46  ---          01 36 44  10.2 287.9  6.0      60.5   117   F  1    925  14 52 47

14 55 16  1932+204     01 37 14  10.1 288.0  6.0      60.4    28   1  1    925  14 55 16
14 56 46  ---          01 38 44   9.8 288.2  6.1      60.3    90   F  1    931  14 55 17

14 56 46  IRAS19312    01 38 44   9.2 287.9  6.1      60.1    -3   1  1    931  14 56 46
14 58 46  ---          01 40 45   8.7 288.1  6.1      60.0   117   F  1    939  14 56 47

14 58 46  1932+204     01 40 45   9.4 288.4  6.1      60.2    -3   1  1    939  14 58 46
15 00 46  ---          01 42 45   9.0 288.6  6.1      60.1   117   F  1    946  14 58 47

15 00 46  IRAS19312    01 42 45   8.3 288.3  6.1      59.9    -3   1  1    946  15 00 46
15 02 46  ---          01 44 45   7.9 288.6  6.2      59.7   117   F  1    954  15 00 47

15 02 46  1932+204     01 44 45   8.6 288.9  6.2      59.9    -3   1  1    954  15 02 46
15 04 46  ---          01 46 46   8.2 289.1  6.2      59.8   117   F  1    962  15 02 47

15 04 46  IRAS19312    01 46 46   7.5 288.8  6.2      59.6    -3   1  1    962  15 04 46
15 06 46  ---          01 48 46   7.1 289.1  6.2      59.4   117   F  1    970  15 04 47

15 06 46  1932+204     01 48 46   7.8 289.4  6.2      59.6    -3   1  1    970  15 06 46
15 08 46  ---          01 50 46   7.4 289.6  6.3      59.5   117   F  1    977  15 06 47

15 20 31  2007+777     02 02 33  30.5 345.9  6.0      83.4   647   1  1    977  15 20 31
15 25 31  ---          02 07 34  30.2 346.0  6.0      82.2   300   F  1    997  15 20 32

19 47 33  3C84         06 30 19  50.9 299.1  3.2      89.8 15673   1  1    997  19 47 33
19 52 33  ---          06 35 20  49.9 299.1  3.2      88.9   300   F  1   1016  19 47 34


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


 Setup file: eb037a.set
   Matches group sh18cm in /home/brunthal/Soft/Astronomy/sched/catalogs/freq.dat
    Huang Xinyong 27Sept05

   Setup group:   10         Station: SHANGHAI          Total bit rate:  512
   Format: MKIV1:4           Bits per sample: 2         Sample rate: 32.000
   Number of channels:  8                               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
   Net SB=         U         U         U         U         U         U         U         U
   Pol.  =      RCP       LCP       RCP       LCP       RCP       LCP       RCP       LCP 
   BBC   =         1         2         3         4         5         6         7         8
   BBC SB=         L         L         L         L         L         L         L         L
   IF    =        C         A         C         A         C         A         C         A 

  The following frequency sets based on this setup were used.

  Frequency Set:  10  Based on FREQ, BW, and/or DOPPLER in schedule.  Used pcal sets:   1
   LO sum=    1610.05   1610.05   1627.17   1627.17   1643.17   1643.17   1659.17   1659.17
   BBC fr=     689.95    689.95    672.83    672.83    656.83    656.83    640.83    640.83
   Bandwd=     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 = OFF 
    PCALXB1=   S1    S2    S3    S4    S5    S6    S7    S8 
    PCALXB2=   M1    M2    M3    M4    M5    M6    M7    M8 
    PCALFR1=     0     0     0     0     0     0     0     0
    PCALFR2=     0     0     0     0     0     0     0     0

   Track assignments are: 
    track1=   2, 18,  3, 19, 66, 82, 67, 83
    barrel=roll_off 
 SOURCE LIST -- IRAS 19312+1950
     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)

 * IRAS19312         19 31 12.699233   * 19 33 24.246000     19 33 47.538911       0.00
                     19 50 22.88294    * 19 56 55.69000      19 58 14.09349        0.00
                     From catalog imbedded in main SCHED input file.
                     Doppler based on LSR frame and radio definition.  Velocities:
                         30.00    30.00    30.00    30.00    30.00    30.00    30.00    30.00
                        3.100 scan hours,    127.477 baseline hours above horizon.

 * IRAS-B            19 31 12.699233   * 19 33 24.246000     19 33 47.538911       0.00
                     19 50 22.88294    * 19 56 55.69000      19 58 14.09349        0.00
                     From catalog imbedded in main SCHED input file.
                     Doppler based on other sources.
                        0.600 scan hours,     20.190 baseline hours above horizon.

   J0319+4130        03 16 29.567289   * 03 19 48.160119     03 20 25.624714       0.28
   0316+413          41 19 51.91677    * 41 30 42.10389      41 32 46.19186        0.41
 * 3C84              /home/brunthal/Soft/Astronomy/sched/catalogs/sources.vlba
   J0319+41          VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro
                     Doppler based on other sources.
                        0.083 scan hours,      4.583 baseline hours above horizon.

   J1331+3030        13 28 49.657756   * 13 31 08.288048     13 31 32.113351       0.37
   1328+307          30 45 58.64060    * 30 30 32.95924      30 27 45.99897        0.47
 * 3C286             /home/brunthal/Soft/Astronomy/sched/catalogs/sources.vlba
   J1331+30          VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro
                     Doppler based on other sources.
                        0.083 scan hours,      3.749 baseline hours above horizon.

   J1642+3948        16 41 17.606231   * 16 42 58.809968     16 43 15.748946       0.26
   1641+399          39 54 10.81494    * 39 48 36.99400      39 47 42.45732        0.40
 * 3C345             /home/brunthal/Soft/Astronomy/sched/catalogs/sources.vlba
   J1642+39          VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro
                     Doppler based on other sources.
                        0.083 scan hours,      4.583 baseline hours above horizon.

   J1925+2106        19 23 49.792391   * 19 25 59.605354     19 26 22.540029       0.22
 * 1923+210          21 00 23.30492    * 21 06 26.16200      21 07 39.30763        0.40
   J1925+21          /home/brunthal/Soft/Astronomy/sched/catalogs/sources.vlba
                     VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro
                     Doppler based on other sources.
                        0.947 scan hours,     34.199 baseline hours above horizon.

   J1935+2031        19 32 59.558257   * 19 35 10.472910     19 35 33.657269       0.22
 * 1932+204          20 25 14.21757    * 20 31 54.15434      20 33 14.03119        0.41
   J1935+20          /home/brunthal/Soft/Astronomy/sched/catalogs/sources.vlba
                     VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro
                     Doppler based on other sources.
                        3.900 scan hours,    165.375 baseline hours above horizon.

   J2005+7752        20 07 20.430185   * 20 05 30.998513     20 05 08.636603       0.96
 * 2007+777          77 43 58.12307    * 77 52 43.24760      77 54 32.14134        0.40
   J2005+77          /home/brunthal/Soft/Astronomy/sched/catalogs/sources.vlba
                     VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro
                     Doppler based on other sources.
                        0.083 scan hours,      3.750 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) 
   IRAS19312           84.1
   IRAS-B              84.1
   3C84               149.6
   3C286               46.1
   3C345               63.2
   1923+210            82.8
   1932+204            84.6
   2007+777           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 

