  COVER INFORMATION 

 Station:    VLBA_FD   (Code Fd ) 
 Experiment: Angular broadening of pulsars
 Exp. Code:  GR024B  


Schedule Version:       1.00                                              
Processed by SCHED version: Release of 18 Sept. 2003                      

PI:       R. Ramachandran                                                 

Address:  Dept of Astronomy,                                              
          University of California at Berkeley                            
          Berkeley, CA 94720                                              
           U.S.A.                                                         

Phone:    510 642 6111                                                    
EMAIL:    ramach@astron.berkeley.edu                                      
Fax:      510 642 3411                                                    
Phone during observation: 510 642 6111                                    

Observing mode: 92cm 256-8-2                                              

Notes:                                                                    
                                                                          
                                                                          
                                                                          


COVER LETTER:


Interference is not a problem

Check BBC settings: desired freqs

Please make sure phase cal is off

Schedule for VLBA_FD   (Code Fd )                                   Page   2
               Angular broadening of pulsars
  UP:  D => Below limits;  H => Below horizon mask.  blank => Up.
  Early: Seconds between end of slew and start.   Dwell: On source seconds. 
  Tapes: Drive, Index, Start footage / Direction, Head Group, End footage.
  TPStart:  Tape motion start time.  Frequencies are LO sum (band edge).
     Automatic tape allocation specified.  Tape positions are just estimates.
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)
----------------------------------------------------------------------------------------

 --- Thu  21 Oct 2004   Day 295 ---

 Next scan frequencies:   311.99   311.99   319.99   319.99   327.99   327.99
                          335.99   335.99
 Next BBC frequencies:    811.99   811.99   819.99   819.99   827.99   827.99
                          835.99   835.99
 Next scan bandwidths:      8.00     8.00     8.00     8.00     8.00     8.00
                            8.00     8.00

21 00 00  J1907+0127   16 06 47  38.3 115.4 -3.0     -51.0     0   1  1      0  21 00 00
21 01 00  =1904+013    16 07 47  38.5 115.6 -3.0     -50.9    60   F  1    800

21 01 00  B1859+03     16 07 47  40.9 114.7 -2.9     -51.5   -11   1  1    800  21 01 00
21 10 05  ---          16 16 54  42.6 116.6 -2.7     -50.4   534   F  1   8067

21 10 05  J1907+0127   16 16 54  40.2 117.5 -2.8     -49.8   -11   1  1   8067  21 10 05
21 11 30  =1904+013    16 18 19  40.5 117.8 -2.8     -49.6    74   F  1   9200

21 11 30  B1859+03     16 18 19  42.9 116.9 -2.7     -50.2   -11   1  1   9200  21 11 30
21 20 35  ---          16 27 26  44.6 119.0 -2.6     -49.0   534   F  1  16467

21 20 35  J1907+0127   16 27 26  42.2 119.8 -2.7     -48.3   -11   1  1  16467  21 20 35
21 22 00  =1904+013    16 28 51  42.5 120.1 -2.6     -48.1    74   F  1  17600

21 27 10  J1904+1536   16 34 02  52.5 105.0 -2.5     -59.7   284   1  2  17600  21 27 10
21 28 20  =1901+155    16 35 12  52.8 105.2 -2.5     -59.6    70   R  1  16667

21 28 20  B1907+10     16 35 12  49.2 110.2 -2.6     -55.4   -13   1  2  16667  21 28 20
21 36 35  ---          16 43 28  50.8 112.0 -2.4     -54.4   482   R  1  10067

21 36 35  J1904+1536   16 43 28  54.5 106.9 -2.3     -58.7   -13   1  2  10067  21 36 35
21 38 45  =1901+155    16 45 39  54.9 107.4 -2.3     -58.5   117   R  1   8333

21 38 45  B1907+10     16 45 39  51.3 112.5 -2.4     -54.1   -13   1  2   8333  21 38 45
21 47 20  ---          16 54 15  53.0 114.5 -2.3     -52.9   502   R  1   1467

21 47 20  J1904+1536   16 54 15  56.7 109.4 -2.2     -57.5   -13   1  3   1467  21 47 20
21 49 15  =1901+155    16 56 10  57.1 109.8 -2.1     -57.2   102   F  1     67

21 54 15  J1935+2031   17 01 11  54.0  97.0 -2.6     -65.8   285   1  3     67  21 54 15
21 55 40  ---          17 02 36  54.3  97.2 -2.5     -65.7    85   F  1   1200

21 55 40  B1929+20     17 02 36  54.9  98.0 -2.5     -65.3    -7   1  3   1200  21 55 40
21 58 40  ---          17 05 37  55.5  98.5 -2.4     -65.2   173   F  1   3600
Schedule for VLBA_FD   (Code Fd )                                   Page   3
               Angular broadening of pulsars
  UP:  D => Below limits;  H => Below horizon mask.  blank => Up.
  Early: Seconds between end of slew and start.   Dwell: On source seconds. 
  Tapes: Drive, Index, Start footage / Direction, Head Group, End footage.
  TPStart:  Tape motion start time.  Frequencies are LO sum (band edge).
     Automatic tape allocation specified.  Tape positions are just estimates.
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)
----------------------------------------------------------------------------------------

 --- Thu  21 Oct 2004   Day 295 ---

21 58 40  J1935+2031   17 05 37  54.9  97.7 -2.5     -65.6    -7   1  3   3600  21 58 40
21 59 55  ---          17 06 52  55.2  97.9 -2.5     -65.5    68   F  1   4600

21 59 55  B1929+20     17 06 52  55.8  98.7 -2.4     -65.1    -7   1  3   4600  21 59 55
22 02 55  ---          17 09 53  56.4  99.3 -2.4     -64.9   173   F  1   7000

22 02 55  J1935+2031   17 09 53  55.8  98.4 -2.4     -65.4    -7   1  3   7000  22 02 55
22 04 05  ---          17 11 03  56.1  98.6 -2.4     -65.3    63   F  1   7933

22 04 05  B1929+20     17 11 03  56.7  99.5 -2.4     -64.9    -7   1  3   7933  22 04 05
22 07 05  ---          17 14 03  57.3 100.0 -2.3     -64.7   173   F  1  10333

22 07 05  J1935+2031   17 14 03  56.7  99.2 -2.4     -65.1    -7   1  3  10333  22 07 05
22 08 15  ---          17 15 13  57.0  99.4 -2.3     -65.0    63   F  1  11267

22 08 15  B1929+20     17 15 13  57.5 100.2 -2.3     -64.6    -7   1  3  11267  22 08 15
22 11 15  ---          17 18 14  58.2 100.8 -2.2     -64.3   173   F  1  13667

22 11 15  J1935+2031   17 18 14  57.6  99.9 -2.3     -64.8    -7   1  3  13667  22 11 15
22 12 10  ---          17 19 09  57.8 100.1 -2.3     -64.8    48   F  1  14400

22 12 10  B1929+20     17 19 09  58.4 101.0 -2.2     -64.3    -7   1  3  14400  22 12 10
22 15 10  ---          17 22 10  59.0 101.6 -2.2     -64.0   173   F  1  16800

22 15 10  J1935+2031   17 22 10  58.5 100.7 -2.2     -64.6    -7   1  3  16800  22 15 10
22 16 05  ---          17 23 05  58.6 100.8 -2.2     -64.5    48   F  1  17533

22 19 15  J2047+5343   17 26 15  47.3  42.2 -3.4    -102.0   145   1  4  17533  22 19 15
22 20 15  =2046+535    17 27 15  47.4  42.2 -3.3    -102.2    60   R  1  16733

22 20 15  B2036+53     17 27 15  49.0  42.3 -3.2    -104.1    -9   1  4  16733  22 20 15
22 22 25  ---          17 29 26  49.3  42.2 -3.1    -104.6   121   R  1  15000

22 22 25  J2047+5343   17 29 26  47.8  42.1 -3.3    -102.7    -9   1  4  15000  22 22 25
22 23 15  =2046+535    17 30 16  47.9  42.1 -3.3    -102.9    41   R  1  14333

22 23 15  B2036+53     17 30 16  49.4  42.1 -3.1    -104.8    -9   1  4  14333  22 23 15
22 25 25  ---          17 32 26  49.7  42.0 -3.1    -105.4   121   R  1  12600

22 25 25  J2047+5343   17 32 26  48.2  42.0 -3.3    -103.4    -9   1  4  12600  22 25 25
22 26 15  =2046+535    17 33 16  48.3  41.9 -3.2    -103.6    41   R  1  11933
Schedule for VLBA_FD   (Code Fd )                                   Page   4
               Angular broadening of pulsars
  UP:  D => Below limits;  H => Below horizon mask.  blank => Up.
  Early: Seconds between end of slew and start.   Dwell: On source seconds. 
  Tapes: Drive, Index, Start footage / Direction, Head Group, End footage.
  TPStart:  Tape motion start time.  Frequencies are LO sum (band edge).
     Automatic tape allocation specified.  Tape positions are just estimates.
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)
----------------------------------------------------------------------------------------

 --- Thu  21 Oct 2004   Day 295 ---

22 26 15  B2036+53     17 33 16  49.8  41.9 -3.1    -105.6    -9   1  4  11933  22 26 15
22 28 25  ---          17 35 27  50.1  41.8 -3.0    -106.1   121   R  1  10200

22 28 25  J2047+5343   17 35 27  48.6  41.8 -3.2    -104.2    -9   1  4  10200  22 28 25
22 29 15  =2046+535    17 36 17  48.7  41.7 -3.2    -104.4    41   R  1   9533

22 29 15  B2036+53     17 36 17  50.3  41.8 -3.0    -106.3    -9   1  4   9533  22 29 15
22 31 25  ---          17 38 27  50.6  41.6 -3.0    -106.9   121   R  1   7800

22 31 25  J2047+5343   17 38 27  49.1  41.6 -3.2    -104.9    -9   1  4   7800  22 31 25
22 32 15  =2046+535    17 39 17  49.2  41.6 -3.1    -105.1    41   R  1   7133

22 32 15  B2036+53     17 39 17  50.7  41.5 -3.0    -107.1    -9   1  4   7133  22 32 15
22 34 15  ---          17 41 18  51.0  41.4 -2.9    -107.6   111   R  1   5533

22 34 15  J2047+5343   17 41 18  49.5  41.5 -3.1    -105.6    -9   1  4   5533  22 34 15
22 35 05  =2046+535    17 42 08  49.6  41.4 -3.1    -105.8    41   R  1   4867

22 35 05  B2036+53     17 42 08  51.1  41.3 -2.9    -107.8    -9   1  4   4867  22 35 05
22 37 05  ---          17 44 08  51.4  41.2 -2.9    -108.3   111   R  1   3267

22 37 05  J2047+5343   17 44 08  49.9  41.3 -3.1    -106.3    -9   1  4   3267  22 37 05
22 37 55  =2046+535    17 44 58  50.0  41.2 -3.1    -106.5    41   R  1   2600

22 37 55  B2036+53     17 44 58  51.5  41.1 -2.9    -108.6    -9   1  4   2600  22 37 55
22 40 05  ---          17 47 09  51.8  41.0 -2.9    -109.1   121   R  1    867

22 40 05  J2047+5343   17 47 09  50.3  41.1 -3.0    -107.1    -9   1  4    867  22 40 05
22 40 55  =2046+535    17 47 59  50.4  41.0 -3.0    -107.3    41   R  1    200

22 41 35  B2036+53     17 48 39  52.0  40.8 -2.8    -109.5    31   1  5    200  22 41 35
22 43 45  ---          17 50 49  52.3  40.7 -2.8    -110.1   130   F  1   1933

22 43 45  J2047+5343   17 50 49  50.8  40.8 -3.0    -108.0    -9   1  5   1933  22 43 45
22 44 35  =2046+535    17 51 39  50.9  40.8 -2.9    -108.2    41   F  1   2600

22 44 35  B2036+53     17 51 39  52.4  40.6 -2.8    -110.3    -9   1  5   2600  22 44 35
22 46 45  ---          17 53 50  52.7  40.4 -2.7    -110.9   121   F  1   4333

22 46 45  J2047+5343   17 53 50  51.2  40.6 -2.9    -108.8    -9   1  5   4333  22 46 45
22 47 35  =2046+535    17 54 40  51.4  40.5 -2.9    -109.0    41   F  1   5000
Schedule for VLBA_FD   (Code Fd )                                   Page   5
               Angular broadening of pulsars
  UP:  D => Below limits;  H => Below horizon mask.  blank => Up.
  Early: Seconds between end of slew and start.   Dwell: On source seconds. 
  Tapes: Drive, Index, Start footage / Direction, Head Group, End footage.
  TPStart:  Tape motion start time.  Frequencies are LO sum (band edge).
     Automatic tape allocation specified.  Tape positions are just estimates.
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)
----------------------------------------------------------------------------------------

 --- Thu  21 Oct 2004   Day 295 ---

22 47 35  B2036+53     17 54 40  52.9  40.3 -2.7    -111.1    -9   1  5   5000  22 47 35
22 49 45  ---          17 56 50  53.2  40.1 -2.7    -111.7   121   F  1   6733

22 49 45  J2047+5343   17 56 50  51.7  40.4 -2.9    -109.6    -9   1  5   6733  22 49 45
22 50 35  =2046+535    17 57 40  51.8  40.3 -2.8    -109.8    41   F  1   7400

22 50 35  B2036+53     17 57 40  53.3  40.1 -2.7    -112.0    -9   1  5   7400  22 50 35
22 52 45  ---          17 59 51  53.6  39.9 -2.6    -112.6   121   F  1   9133

22 52 45  J2047+5343   17 59 51  52.1  40.1 -2.8    -110.4    -9   1  5   9133  22 52 45
22 53 35  =2046+535    18 00 41  52.2  40.0 -2.8    -110.6    41   F  1   9800

22 53 35  J2035+5821   18 00 41  51.8  32.0 -2.6    -119.5   -11   1  5   9800  22 53 35
22 55 05  =2034+581    18 02 11  52.0  31.9 -2.6    -120.0    79   F  1  11000

22 55 05  B2045+56     18 02 11  51.2  34.7 -2.7    -115.3    -8   1  5  11000  22 55 05
22 58 05  ---          18 05 12  51.6  34.4 -2.7    -116.2   172   F  1  13400

22 58 05  J2035+5821   18 05 12  52.3  31.5 -2.5    -120.9    -8   1  5  13400  22 58 05
22 59 15  =2034+581    18 06 22  52.5  31.4 -2.5    -121.2    62   F  1  14333

22 59 15  B2045+56     18 06 22  51.7  34.3 -2.7    -116.5    -8   1  5  14333  22 59 15
23 02 25  ---          18 09 32  52.1  34.0 -2.6    -117.4   182   F  1  16867

23 02 25  J2035+5821   18 09 32  52.8  31.1 -2.4    -122.2    -8   1  6  16867  23 02 25
23 03 35  =2034+581    18 10 42  52.9  30.9 -2.4    -122.5    62   R  1  17400

23 04 15  B2045+56     18 11 23  52.3  33.8 -2.6    -117.9    32   1  6  17400  23 04 15
23 07 15  ---          18 14 23  52.7  33.5 -2.5    -118.8   180   R  1  15000

23 07 15  J2035+5821   18 14 23  53.3  30.5 -2.4    -123.7    -8   1  6  15000  23 07 15
23 08 25  =2034+581    18 15 33  53.5  30.3 -2.3    -124.0    62   R  1  14067

23 08 25  B2045+56     18 15 33  52.8  33.4 -2.5    -119.2    -8   1  6  14067  23 08 25
23 11 35  ---          18 18 44  53.2  33.0 -2.5    -120.1   182   R  1  11533

23 11 35  J2035+5821   18 18 44  53.8  29.9 -2.3    -125.0    -8   1  6  11533  23 11 35
23 12 45  =2034+581    18 19 54  53.9  29.8 -2.3    -125.4    62   R  1  10600

23 12 45  B2045+56     18 19 54  53.3  32.9 -2.4    -120.5    -8   1  6  10600  23 12 45
23 16 05  ---          18 23 15  53.7  32.5 -2.4    -121.5   192   R  1   7933
Schedule for VLBA_FD   (Code Fd )                                   Page   6
               Angular broadening of pulsars
  UP:  D => Below limits;  H => Below horizon mask.  blank => Up.
  Early: Seconds between end of slew and start.   Dwell: On source seconds. 
  Tapes: Drive, Index, Start footage / Direction, Head Group, End footage.
  TPStart:  Tape motion start time.  Frequencies are LO sum (band edge).
     Automatic tape allocation specified.  Tape positions are just estimates.
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)
----------------------------------------------------------------------------------------

 --- Thu  21 Oct 2004   Day 295 ---

23 16 05  J2035+5821   18 23 15  54.3  29.4 -2.2    -126.5    -8   1  6   7933  23 16 05
23 17 15  =2034+581    18 24 25  54.4  29.2 -2.2    -126.8    62   R  1   7000

23 17 15  B2045+56     18 24 25  53.8  32.4 -2.4    -121.9    -8   1  6   7000  23 17 15
23 20 35  ---          18 27 45  54.2  31.9 -2.3    -122.9   192   R  1   4333

23 20 35  J2035+5821   18 27 45  54.8  28.7 -2.1    -127.9    -8   1  6   4333  23 20 35
23 21 45  =2034+581    18 28 55  54.9  28.6 -2.1    -128.3    62   R  1   3400

23 21 45  B2045+56     18 28 55  54.4  31.8 -2.3    -123.3    -8   1  6   3400  23 21 45
23 25 05  ---          18 32 16  54.7  31.4 -2.2    -124.3   192   R  1    733

23 25 05  J2035+5821   18 32 16  55.2  28.1 -2.1    -129.4    -8   1  7    733  23 25 05
23 26 15  =2034+581    18 33 26  55.3  27.9 -2.0    -129.8    62   F  1    200

23 26 55  J2120+4434   18 34 06  54.6  54.9 -2.8     -98.8    16   1  7    200  23 26 55
23 28 25  =2118+443    18 35 37  54.9  54.8 -2.8     -99.1    90   F  1   1400

23 28 25  B2106+44     18 35 37  57.0  53.9 -2.5    -102.0   -10   1  7   1400  23 28 25
23 30 55  ---          18 38 07  57.5  53.7 -2.5    -102.6   140   F  1   3400

23 30 55  J2120+4434   18 38 07  55.3  54.7 -2.7     -99.7   -10   1  7   3400  23 30 55
23 31 55  =2118+443    18 39 07  55.5  54.6 -2.7     -99.9    50   F  1   4200

23 31 55  B2106+44     18 39 07  57.6  53.6 -2.5    -102.9   -10   1  7   4200  23 31 55
23 34 25  ---          18 41 38  58.1  53.4 -2.4    -103.5   140   F  1   6200

23 34 25  J2120+4434   18 41 38  56.0  54.5 -2.7    -100.5   -10   1  7   6200  23 34 25
23 35 25  =2118+443    18 42 38  56.1  54.4 -2.6    -100.7    50   F  1   7000

23 35 25  B2106+44     18 42 38  58.2  53.3 -2.4    -103.7   -10   1  7   7000  23 35 25
23 37 55  ---          18 45 08  58.7  53.1 -2.4    -104.3   140   F  1   9000

23 37 55  J2120+4434   18 45 08  56.6  54.3 -2.6    -101.2   -10   1  7   9000  23 37 55
23 38 55  =2118+443    18 46 08  56.8  54.2 -2.6    -101.5    50   F  1   9800

23 38 55  B2106+44     18 46 08  58.8  53.1 -2.4    -104.6   -10   1  7   9800  23 38 55
23 41 25  ---          18 48 39  59.3  52.8 -2.3    -105.2   140   F  1  11800

23 41 25  J2120+4434   18 48 39  57.2  54.0 -2.5    -102.1   -10   1  7  11800  23 41 25
23 42 25  =2118+443    18 49 39  57.4  54.0 -2.5    -102.3    50   F  1  12600
Schedule for VLBA_FD   (Code Fd )                                   Page   7
               Angular broadening of pulsars
  UP:  D => Below limits;  H => Below horizon mask.  blank => Up.
  Early: Seconds between end of slew and start.   Dwell: On source seconds. 
  Tapes: Drive, Index, Start footage / Direction, Head Group, End footage.
  TPStart:  Tape motion start time.  Frequencies are LO sum (band edge).
     Automatic tape allocation specified.  Tape positions are just estimates.
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)
----------------------------------------------------------------------------------------

 --- Thu  21 Oct 2004   Day 295 ---

23 42 25  B2106+44     18 49 39  59.4  52.7 -2.3    -105.5   -10   1  7  12600  23 42 25
23 44 55  ---          18 52 09  59.9  52.5 -2.3    -106.1   140   F  1  14600

23 44 55  J2120+4434   18 52 09  57.8  53.8 -2.5    -102.9   -10   1  7  14600  23 44 55
23 45 55  =2118+443    18 53 09  58.0  53.7 -2.5    -103.1    50   F  1  15400

23 45 55  B2106+44     18 53 09  60.0  52.4 -2.3    -106.4   -10   1  7  15400  23 45 55
23 47 55  ---          18 55 10  60.4  52.2 -2.2    -106.9   110   F  1  17000

23 47 55  J2120+4434   18 55 10  58.3  53.5 -2.4    -103.6   -10   1  8  17000  23 47 55
23 48 55  =2118+443    18 56 10  58.5  53.5 -2.4    -103.9    50   R  1  17400

23 49 35  J2123+4614   18 56 50  57.7  50.6 -2.4    -105.9    32   1  8  17400  23 49 35
23 50 35  =2121+460    18 57 50  57.8  50.5 -2.4    -106.1    60   R  1  16600

23 50 35  B2111+46     18 57 50  59.3  48.6 -2.3    -109.6    -9   1  8  16600  23 50 35
23 59 35  ---          19 06 52  60.8  47.5 -2.1    -112.2   531   R  1   9400

 --- Start: Thu  21 Oct 2004   Day 295 -- Stop: Fri  22 Oct 2004   Day 296 ---

23 59 35  J2123+4614   19 06 52  59.3  49.6 -2.3    -108.5    -9   1  8   9400  23 59 35
00 01 05  =2121+460    19 08 22  59.6  49.5 -2.3    -108.9    81   R  1   8200

00 01 05  B2111+46     19 08 22  61.0  47.3 -2.1    -112.6    -9   1  8   8200  00 01 05
00 10 05  ---          19 17 23  62.4  46.0 -1.9    -115.5   531   R  1   1000

00 10 05  J2123+4614   19 17 23  61.0  48.4 -2.1    -111.5    -9   1  9   1000  00 10 05
00 11 35  =2121+460    19 18 54  61.3  48.2 -2.1    -111.9    81   F  1    200

00 12 15  J2202+4216   19 19 34  55.5  58.7 -2.7     -96.2    22   1  9    200  00 12 15
00 13 35  =2200+420    19 20 54  55.8  58.7 -2.7     -96.5    80   F  1   1267

00 13 35  B2154+40     19 20 54  57.0  62.0 -2.6     -94.6    -9   1  9   1267  00 13 35
00 22 35  ---          19 29 55  58.7  61.7 -2.5     -96.3   531   F  1   8467

00 22 35  J2202+4216   19 29 55  57.4  58.3 -2.5     -98.3    -9   1  9   8467  00 22 35
00 23 55  =2200+420    19 31 16  57.7  58.2 -2.5     -98.6    71   F  1   9533

00 23 55  B2154+40     19 31 16  59.0  61.7 -2.4     -96.6    -9   1  9   9533  00 23 55
00 32 55  ---          19 40 17  60.7  61.2 -2.3     -98.4   531   F  1  16733

00 32 55  J2202+4216   19 40 17  59.3  57.7 -2.4    -100.6    -9   1 10  16733  00 32 55
00 34 15  =2200+420    19 41 37  59.6  57.6 -2.4    -100.9    71   R  1  17400
Schedule for VLBA_FD   (Code Fd )                                   Page   8
               Angular broadening of pulsars
  UP:  D => Below limits;  H => Below horizon mask.  blank => Up.
  Early: Seconds between end of slew and start.   Dwell: On source seconds. 
  Tapes: Drive, Index, Start footage / Direction, Head Group, End footage.
  TPStart:  Tape motion start time.  Frequencies are LO sum (band edge).
     Automatic tape allocation specified.  Tape positions are just estimates.
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)
----------------------------------------------------------------------------------------

 --- Fri  22 Oct 2004   Day 296 ---

00 34 55  J2120+6642   19 42 17  51.0  15.2 -1.6    -145.3     6   1 10  17400  00 34 55
00 36 15  =2119+664    19 43 38  51.1  15.0 -1.6    -145.7    80   R  1  16333

00 36 15  B2148+63     19 43 38  51.5  22.1 -2.1    -133.5   -11   1 10  16333  00 36 15
00 45 15  ---          19 52 39  52.2  20.9 -2.0    -136.5   529   R  1   9133

00 45 15  J2120+6642   19 52 39  51.6  13.8 -1.5    -148.7   -11   1 10   9133  00 45 15
00 46 35  =2119+664    19 53 59  51.6  13.6 -1.4    -149.2    69   R  1   8067

00 46 35  B2148+63     19 53 59  52.3  20.7 -1.9    -136.9   -11   1 10   8067  00 46 35
00 55 35  ---          20 03 01  53.0  19.5 -1.8    -139.9   529   R  1    867

00 55 35  J2120+6642   20 03 01  52.1  12.4 -1.3    -152.2   -11   1 11    867  00 55 35
00 56 55  =2119+664    20 04 21  52.1  12.2 -1.3    -152.7    69   F  1    200

00 57 35  J2302+6405   20 05 01  46.6  26.4 -3.0    -118.7    23   1 11    200  00 57 35
00 59 15  =2300+638    20 06 41  46.7  26.3 -2.9    -119.2   100   F  1   1533

00 59 15  B2227+61     20 06 41  51.0  25.7 -2.4    -127.0   -14   1 11   1533  00 59 15
01 02 05  ---          20 09 32  51.2  25.4 -2.3    -127.8   156   F  1   3800

01 02 05  J2302+6405   20 09 32  47.0  26.1 -2.9    -120.0   -14   1 11   3800  01 02 05
01 03 15  =2300+638    20 10 42  47.1  26.0 -2.9    -120.3    56   F  1   4733

01 03 15  B2227+61     20 10 42  51.3  25.3 -2.3    -128.2   -14   1 11   4733  01 03 15
01 06 05  ---          20 13 33  51.6  25.0 -2.3    -129.1   156   F  1   7000

01 06 05  J2302+6405   20 13 33  47.4  25.7 -2.8    -121.1   -14   1 11   7000  01 06 05
01 07 15  =2300+638    20 14 43  47.5  25.6 -2.8    -121.5    56   F  1   7933

01 07 15  B2227+61     20 14 43  51.7  24.8 -2.3    -129.5   -14   1 11   7933  01 07 15
01 10 05  ---          20 17 33  52.0  24.5 -2.2    -130.4   156   F  1  10200

01 10 05  J2302+6405   20 17 33  47.8  25.4 -2.8    -122.3   -14   1 11  10200  01 10 05
01 11 15  =2300+638    20 18 43  47.9  25.3 -2.7    -122.6    56   F  1  11133

01 11 15  B2227+61     20 18 43  52.1  24.3 -2.2    -130.7   -14   1 11  11133  01 11 15
01 14 15  ---          20 21 44  52.3  23.9 -2.1    -131.7   166   F  1  13533

01 14 15  J2302+6405   20 21 44  48.2  25.0 -2.7    -123.5   -14   1 11  13533  01 14 15
01 15 25  =2300+638    20 22 54  48.3  24.9 -2.7    -123.8    56   F  1  14467
Schedule for VLBA_FD   (Code Fd )                                   Page   9
               Angular broadening of pulsars
  UP:  D => Below limits;  H => Below horizon mask.  blank => Up.
  Early: Seconds between end of slew and start.   Dwell: On source seconds. 
  Tapes: Drive, Index, Start footage / Direction, Head Group, End footage.
  TPStart:  Tape motion start time.  Frequencies are LO sum (band edge).
     Automatic tape allocation specified.  Tape positions are just estimates.
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)
----------------------------------------------------------------------------------------

 --- Fri  22 Oct 2004   Day 296 ---

01 15 25  B2227+61     20 22 54  52.4  23.8 -2.1    -132.1   -14   1 11  14467  01 15 25
01 18 25  ---          20 25 55  52.7  23.4 -2.1    -133.0   166   F  1  16867

01 18 25  J2302+6405   20 25 55  48.5  24.6 -2.6    -124.7   -14   1 12  16867  01 18 25
01 19 35  =2300+638    20 27 05  48.6  24.5 -2.6    -125.1    56   R  1  17400

01 20 15  B2227+61     20 27 45  52.8  23.2 -2.0    -133.6    26   1 12  17400  01 20 15
01 23 15  ---          20 30 45  53.1  22.8 -2.0    -134.6   180   R  1  15000

01 23 15  J2302+6405   20 30 45  49.0  24.2 -2.5    -126.2   -14   1 12  15000  01 23 15
01 24 25  =2300+638    20 31 56  49.1  24.1 -2.5    -126.5    56   R  1  14067

01 24 25  B2227+61     20 31 56  53.2  22.6 -2.0    -135.0   -14   1 12  14067  01 24 25
01 27 25  ---          20 34 56  53.4  22.2 -1.9    -136.0   166   R  1  11667

01 27 25  J2302+6405   20 34 56  49.3  23.8 -2.5    -127.4   -14   1 12  11667  01 27 25
01 28 35  =2300+638    20 36 06  49.4  23.6 -2.4    -127.8    56   R  1  10733


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


 Setup file: gr024set
   Matches group v5090n in /juno1/ramach/sched/catalogs/freq.dat

   Setup group:    1         Station: VLBA              Total bit rate:  256
   Format: VLBA1:2           Bits per sample: 2         Sample rate: 16.000
   Number of channels:  8    Passes/head pos:   1       Speedup factor:   1.00

   Tape speeds: Low density - 266.660 ips,  High density - 160.00 ips
   Time per pass for  17600 ft, High density tapes is: 00:22:00

   1st LO=   -500.00   -500.00   -500.00   -500.00   -500.00   -500.00   -500.00   -500.00
   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=         U         U         U         U         U         U         U         U
   IF    =        B         D         B         D         B         D         B         D 

   VLBA FE=     omit     90cm     omit     90cm
   VLBA Synth=  15.4     15.4     15.4

  The following frequency sets based on this setup were used.

   Frequency Set:   1  Setup file default.  Used pcal sets:   1
   LO sum=     311.99    311.99    319.99    319.99    327.99    327.99    335.99    335.99
   BBC fr=     811.99    811.99    819.99    819.99    827.99    827.99    835.99    835.99
   Bandwd=      8.000     8.000     8.000     8.000     8.000     8.000     8.000     8.000

  The following pulse cal sets were used with this setup:

   Pulse cal detection set:   1  PCAL = 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, 10, 18, 26,  3, 11, 19, 27
    barrel=roll_auto
 SOURCE LIST -- Angular broadening of pulsars
     Catalog positions marked with *. 
     Precession of date coordinates is based on stop time of first scan.
     Names used in schedule marked with *. 
     Short names used in VLA and SNAP files marked with +. 
     Observation date used in B1950/J2000 coordinate conversion (PRECDATE):  1979.900
     No adjustments are made for rates (DRA, DDEC).

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

 * B1859+03          18 59 01.920282   * 19 01 31.782760     19 01 45.215469 
                     03 26 45.66806    * 03 31 06.25250      03 31 31.30321 
                     From catalog imbedded in main SCHED input file.

 * B1907+10          19 07 27.308346   * 19 09 48.696240     19 10 01.365206 
                     10 57 07.63220    * 11 02 03.29660      11 02 33.95662 
                     From catalog imbedded in main SCHED input file.

 * B1929+20          19 29 57.020134   * 19 32 08.029650     19 32 19.811755 
                     20 14 18.59562    * 20 20 46.30490      20 21 28.41646 
                     From catalog imbedded in main SCHED input file.

 * B2036+53          20 36 38.669181   * 20 38 03.316890     20 38 10.939007 
                     53 08 37.09371    * 53 19 12.22340      53 20 24.44737 
                     From catalog imbedded in main SCHED input file.

 * B2045+56          20 45 30.046546   * 20 46 46.687790     20 46 53.592261 
                     56 57 33.01187    * 57 08 37.37590      57 09 52.71040 
                     From catalog imbedded in main SCHED input file.

 * B2106+44          21 06 31.729985   * 21 08 20.478230     21 08 30.589287 
                     44 29 37.68074    * 44 41 48.78940      44 43 09.18620 
                     From catalog imbedded in main SCHED input file.

 * B2111+46          21 11 37.710562   * 21 13 24.294900     21 13 34.227230 
                     46 31 42.57014    * 46 44 08.68190      46 45 30.77918 
                     From catalog imbedded in main SCHED input file.

 * B2148+63          21 48 36.754875   * 21 49 58.594090     21 50 06.472562 
                     63 15 40.20571    * 63 29 43.53030      63 31 15.91495 
                     From catalog imbedded in main SCHED input file.

 * B2154+40          21 54 57.091107   * 21 57 01.820500     21 57 13.711504 
                     40 03 27.04649    * 40 17 45.88060      40 19 17.73115 
                     From catalog imbedded in main SCHED input file.

 * B2227+61          22 27 56.714701   * 22 29 41.898790     22 29 52.276557 
                     61 50 12.21440    * 62 05 35.84520      62 07 15.31075 
                     From catalog imbedded in main SCHED input file.

 * J1935+2031        19 32 59.558226   * 19 35 10.472879     19 35 22.260828 
                     20 25 14.21753    * 20 31 54.15430      20 32 37.49602 
                     From catalog imbedded in main SCHED input file.

 * J1904+1536        19 01 58.490214   * 19 04 14.361251     19 04 26.474493 
   1901+155          15 32 05.95927    * 15 36 38.45017      15 37 08.19222 
                     /juno1/ramach/sched/catalogs/sources.vlba
                     VLBA Calib. Survey - ICRF Frame - reduced by GSFC group - Aug 2001

 * J1907+0127        19 04 39.789625   * 19 07 11.997374     19 07 25.681753 
   1904+013          01 22 24.62716    * 01 27 08.98922      01 27 35.63859 
                     /juno1/ramach/sched/catalogs/sources.vlba
                     VLBA Calib. Survey - ICRF Frame - reduced by GSFC group - Aug 2001

 * J2035+5821        20 34 14.260199   * 20 35 23.752163     20 35 29.893402 
   2034+581          58 10 52.22826    * 58 21 18.74634      58 22 30.52822 
                     /juno1/ramach/sched/catalogs/sources.vlba
                     VLBA Calib. Survey - ICRF Frame - reduced by GSFC group - Aug 2001

 * J2047+5343        20 46 27.637630   * 20 47 53.795933     20 48 01.622770 
   2046+535          53 32 24.63403    * 53 43 32.39810      53 44 47.78919 
                     /juno1/ramach/sched/catalogs/sources.vlba
                     VLBA Calib. Survey - ICRF Frame - reduced by GSFC group - Aug 2001

 * J2120+4434        21 18 40.226913   * 21 20 31.773230     21 20 42.218225 
   2118+443          44 21 47.83700    * 44 34 34.26192      44 35 58.00147 
                     /juno1/ramach/sched/catalogs/sources.vlba
                     VLBA Calib. Survey - ICRF Frame - reduced by GSFC group - Aug 2001

 * J2120+6642        21 19 51.459944   * 21 20 46.199501     21 20 51.279883 
   2119+664          66 29 31.82912    * 66 42 20.20874      66 43 45.71809 
                     /juno1/ramach/sched/catalogs/sources.vlba
                     VLBA Calib. Survey - ICRF Frame - reduced by GSFC group - Aug 2001

 * J2123+4614        21 21 42.102521   * 21 23 31.828487     21 23 42.117037 
   2121+460          46 01 28.11520    * 46 14 22.96096      46 15 47.71867 
                     /juno1/ramach/sched/catalogs/sources.vlba
                     VLBA Calib. Survey - ICRF Frame - reduced by GSFC group - Aug 2001

 * J2202+4216        22 00 39.362511   * 22 02 43.291378     22 02 55.137851 
   2200+420          42 02 08.59080    * 42 16 39.97994      42 18 13.28154 
   BLLAC             /juno1/ramach/sched/catalogs/sources.vlba
   J2202+42          ICRF - Ext.1 Source - 1998 IERS Annual Report
   VR42220     

 * J2302+6405        23 00 41.945128   * 23 02 41.315205     23 02 53.327062 
   2300+638          63 49 43.23851    * 64 05 52.85125      64 07 36.04362 
                     /juno1/ramach/sched/catalogs/sources.vlba
                     VLBA Calib. Survey - ICRF Frame - reduced by GSFC group - Aug 2001



  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) 
   B1859+03            79.5
   B1907+10            83.1
   B1929+20            90.4
   B2036+53           106.4
   B2045+56           107.3
   B2106+44           112.1
   B2111+46           112.8
   B2148+63           113.3
   B2154+40           121.7
   B2227+61           117.9
   J1935+2031          91.1
   J1904+1536          82.8
   J1907+0127          80.5
   J2035+5821         105.7
   J2047+5343         107.9
   J2120+4434         114.3
   J2120+6642         109.3
   J2123+4614         114.6
   J2202+4216         122.3
   J2302+6405         119.7

  Barry Clark estimates from predictions by Ketan Desai of IPM scattering sizes 
  that the Sun will cause amplitude reductions on the  longest VLBA baselines 
  at a solar distance of 60deg F^(-0.6) where F is in GHz. 
  For common VLBI bands, this is: 
       327 MHz        117. deg 
       610 MHz         81. deg 
       1.6 GHz         45. deg 
       2.3 GHz         36. deg 
       5.0 GHz         23. deg 
       8.4 GHz         17. deg 
      15.0 GHz         12. deg 
      22.0 GHz          9. deg 
      43.0 GHz          6. deg 

