  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: Astrometry for three FAST discovered pulsars
 Exp. Code:  EC069   


Schedule Version:       3.00
Processed by SCHED version:  11.50  Development version 11.5. Started Apr. 2

PI:       Haiyan Zhang

Address:  NAOC
          A20 Datun Road
          Chaoyang District, Beijing
          China

Phone:    +86 10 6483 9807
EMAIL:    hyzhang@bao.ac.cn
Fax:      +86 10 6487 7278
Phone during observation: +86 158 1052 4586

Observing mode: Phase-referencing at 18cm

Notes:
 
 
 

Schedule for HART      (Code Hh )                                   Page   2
               Astrometry for three FAST discovered pulsars
  UP:  D => Below limits;  H => Below horizon mask;  W => still slewing at end;  blank => Up.
  Early: Seconds between end of slew and start.   Dwell: On source seconds. 
  Disk: GBytes recorded to this point.
  TPStart:  Recording start time.  Frequencies are LO sum (band edge).
  SYNC: Time correlator is expected to sync up.
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Disk   TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell   GBytes    SYNC
----------------------------------------------------------------------------------------

 --- Sun   2 Jun 2019   Day 153 ---

 Next scan frequencies:  1610.49  1610.49  1610.49  1610.49  1642.49  1642.49  1642.49  1642.49
                         1674.49  1674.49  1674.49  1674.49  1706.49  1706.49  1706.49  1706.49
 Next BBC frequencies:    100.49   100.49   100.49   100.49   132.49   132.49   132.49   132.49
                          164.49   164.49   164.49   164.49   196.49   196.49   196.49   196.49
 Next scan bandwidths:     16.00    16.00    16.00    16.00    16.00    16.00    16.00    16.00
                           16.00    16.00    16.00    16.00    16.00    16.00    16.00    16.00

20 00 00  J1827+2638   14 34 45  13.1  51.4 -3.9       0.0     0        0   20 00 00
20 02 00  =1825+266    14 36 45  13.4  51.1 -3.9       0.0   120       15   20 00 01

20 02 00  PSRJ1821+26  14 36 45  14.4  50.3 -3.8       0.0   -29       15   No stop 
20 07 00  ---          14 41 46  15.3  49.5 -3.7       0.0   271       54   20 02 01

20 07 00  J1827+2638   14 41 46  14.3  50.3 -3.8       0.0   -29       54   No stop 
20 08 00  =1825+266    14 42 46  14.5  50.2 -3.8       0.0    31       62   20 07 01

20 08 00  PSRJ1821+26  14 42 46  15.5  49.4 -3.7       0.0   -29       62   No stop 
20 13 00  ---          14 47 47  16.3  48.6 -3.6       0.0   271      100   20 08 01

20 13 40  J1827+2638   14 48 27  15.4  49.4 -3.7       0.0    11      100   20 13 40
20 14 40  =1825+266    14 49 27  15.6  49.2 -3.6       0.0    60      108   20 13 41

20 14 40  PSRJ1821+26  14 49 27  16.6  48.4 -3.5       0.0   -29      108   No stop 
20 19 40  ---          14 54 28  17.4  47.6 -3.5       0.0   271      147   20 14 41

20 19 40  J1827+2638   14 54 28  16.5  48.4 -3.6       0.0   -29      147   No stop 
20 20 40  =1825+266    14 55 28  16.6  48.3 -3.5       0.0    31      155   20 19 41

20 20 40  PSRJ1821+26  14 55 28  17.6  47.4 -3.4       0.0   -29      155   No stop 
20 25 40  ---          15 00 29  18.4  46.6 -3.4       0.0   271      193   20 20 41

20 26 20  J1827+2638   15 01 09  17.6  47.4 -3.4       0.0    11      193   20 26 20
20 27 20  =1825+266    15 02 09  17.7  47.2 -3.4       0.0    60      201   20 26 21

20 27 20  PSRJ1821+26  15 02 09  18.7  46.4 -3.3       0.0   -29      201   No stop 
20 32 20  ---          15 07 10  19.5  45.6 -3.3       0.0   271      240   20 27 21

20 32 20  J1827+2638   15 07 10  18.6  46.4 -3.3       0.0   -29      240   No stop 
20 33 20  =1825+266    15 08 10  18.7  46.3 -3.3       0.0    31      247   20 32 21

20 33 20  PSRJ1821+26  15 08 10  19.7  45.4 -3.2       0.0   -29      247   No stop 
20 38 20  ---          15 13 11  20.5  44.6 -3.2       0.0   271      286   20 33 21

20 39 00  J1827+2638   15 13 51  19.6  45.4 -3.2       0.0    11      286   20 39 00
20 40 00  =1825+266    15 14 51  19.8  45.2 -3.2       0.0    60      294   20 39 01
Schedule for HART      (Code Hh )                                   Page   3
               Astrometry for three FAST discovered pulsars
  UP:  D => Below limits;  H => Below horizon mask;  W => still slewing at end;  blank => Up.
  Early: Seconds between end of slew and start.   Dwell: On source seconds. 
  Disk: GBytes recorded to this point.
  TPStart:  Recording start time.  Frequencies are LO sum (band edge).
  SYNC: Time correlator is expected to sync up.
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Disk   TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell   GBytes    SYNC
----------------------------------------------------------------------------------------

 --- Sun   2 Jun 2019   Day 153 ---

20 40 00  PSRJ1821+26  15 14 51  20.7  44.3 -3.1       0.0   -29      294   No stop 
20 45 00  ---          15 19 52  21.5  43.4 -3.0       0.0   271      332   20 40 01

20 45 00  J1827+2638   15 19 52  20.6  44.3 -3.1       0.0   -29      332   No stop 
20 46 00  =1825+266    15 20 52  20.8  44.2 -3.1       0.0    31      340   20 45 01

20 46 00  PSRJ1821+26  15 20 52  21.7  43.2 -3.0       0.0   -29      340   No stop 
20 51 00  ---          15 25 53  22.4  42.3 -2.9       0.0   271      379   20 46 01

20 51 40  J1827+2638   15 26 33  21.6  43.2 -3.0       0.0    11      379   20 51 40
20 52 40  =1825+266    15 27 33  21.8  43.0 -3.0       0.0    60      386   20 51 41

20 52 40  PSRJ1821+26  15 27 33  22.7  42.1 -2.9       0.0   -29      386   No stop 
20 57 40  ---          15 32 34  23.4  41.1 -2.8       0.0   271      425   20 52 41

20 57 40  J1827+2638   15 32 34  22.6  42.1 -2.9       0.0   -29      425   No stop 
20 58 40  =1825+266    15 33 34  22.7  42.0 -2.9       0.0    31      433   20 57 41

20 58 40  PSRJ1821+26  15 33 34  23.6  41.0 -2.8       0.0   -29      433   No stop 
21 03 40  ---          15 38 35  24.3  40.0 -2.7       0.0   271      471   20 58 41

21 04 20  J1827+2638   15 39 15  23.6  40.9 -2.8       0.0    11      471   21 04 20
21 05 20  =1825+266    15 40 15  23.7  40.7 -2.8       0.0    60      479   21 04 21

21 05 20  PSRJ1821+26  15 40 15  24.6  39.7 -2.7       0.0   -29      479   No stop 
21 10 20  ---          15 45 16  25.3  38.8 -2.6       0.0   271      518   21 05 21

21 10 20  J1827+2638   15 45 16  24.4  39.8 -2.7       0.0   -29      518   No stop 
21 11 20  =1825+266    15 46 16  24.6  39.6 -2.7       0.0    31      526   21 10 21

21 11 20  PSRJ1821+26  15 46 16  25.4  38.6 -2.6       0.0   -29      526   No stop 
21 16 20  ---          15 51 17  26.1  37.6 -2.5       0.0   271      564   21 11 21

21 17 00  J1827+2638   15 51 57  25.4  38.5 -2.6       0.0    11      564   21 17 00
21 18 00  =1825+266    15 52 57  25.5  38.4 -2.6       0.0    60      572   21 17 01

21 18 00  PSRJ1821+26  15 52 57  26.3  37.3 -2.5       0.0   -29      572   No stop 
21 23 00  ---          15 57 58  27.0  36.3 -2.4       0.0   271      611   21 18 01

21 23 00  J1827+2638   15 57 58  26.2  37.4 -2.5       0.0   -29      611   No stop 
21 24 00  =1825+266    15 58 58  26.3  37.2 -2.5       0.0    31      618   21 23 01

21 24 00  PSRJ1821+26  15 58 58  27.2  36.1 -2.4       0.0   -29      618   No stop 
21 29 00  ---          16 03 59  27.8  35.0 -2.3       0.0   271      657   21 24 01
Schedule for HART      (Code Hh )                                   Page   4
               Astrometry for three FAST discovered pulsars
  UP:  D => Below limits;  H => Below horizon mask;  W => still slewing at end;  blank => Up.
  Early: Seconds between end of slew and start.   Dwell: On source seconds. 
  Disk: GBytes recorded to this point.
  TPStart:  Recording start time.  Frequencies are LO sum (band edge).
  SYNC: Time correlator is expected to sync up.
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Disk   TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell   GBytes    SYNC
----------------------------------------------------------------------------------------

 --- Sun   2 Jun 2019   Day 153 ---

21 29 40  J1827+2638   16 04 39  27.1  36.0 -2.4       0.0    11      657   21 29 40
21 30 40  =1825+266    16 05 39  27.2  35.8 -2.4       0.0    60      665   21 29 41

21 30 40  PSRJ1821+26  16 05 39  28.0  34.7 -2.3       0.0   -29      665   No stop 
21 35 40  ---          16 10 40  28.7  33.6 -2.2       0.0   271      703   21 30 41

21 35 40  J1827+2638   16 10 40  27.9  34.8 -2.3       0.0   -29      703   No stop 
21 36 40  =1825+266    16 11 40  28.0  34.6 -2.3       0.0    31      711   21 35 41

21 36 40  PSRJ1821+26  16 11 40  28.8  33.4 -2.2       0.0   -29      711   No stop 
21 41 40  ---          16 16 41  29.4  32.4 -2.1       0.0   271      750   21 36 41

21 42 20  J1827+2638   16 17 21  28.7  33.4 -2.2       0.0    11      750   21 42 20
21 43 20  =1825+266    16 18 22  28.9  33.2 -2.2       0.0    60      757   21 42 21

21 43 20  PSRJ1821+26  16 18 22  29.6  32.0 -2.1       0.0   -29      757   No stop 
21 48 20  ---          16 23 22  30.2  30.9 -2.0       0.0   271      796   21 43 21

21 48 20  J1827+2638   16 23 22  29.5  32.1 -2.1       0.0   -29      796   No stop 
21 49 20  =1825+266    16 24 23  29.6  31.9 -2.1       0.0    31      804   21 48 21

21 49 20  PSRJ1821+26  16 24 23  30.3  30.7 -2.0       0.0   -29      804   No stop 
21 54 20  ---          16 29 23  30.9  29.5 -1.9       0.0   271      842   21 49 21

21 55 00  J1827+2638   16 30 03  30.3  30.6 -2.0       0.0    11      842   21 55 00
21 56 00  =1825+266    16 31 04  30.4  30.4 -2.0       0.0    60      850   21 55 01

21 56 00  PSRJ1821+26  16 31 04  31.0  29.2 -1.9       0.0   -29      850   No stop 
22 01 00  ---          16 36 04  31.6  28.0 -1.8       0.0   271      889   21 56 01

22 01 00  J1827+2638   16 36 04  30.9  29.3 -1.9       0.0   -29      889   No stop 
22 02 00  =1825+266    16 37 05  31.0  29.1 -1.9       0.0    31      897   22 01 01

22 02 00  PSRJ1821+26  16 37 05  31.7  27.8 -1.8       0.0   -29      897   No stop 
22 07 00  ---          16 42 05  32.2  26.6 -1.7       0.0   271      935   22 02 01

22 07 40  J1827+2638   16 42 46  31.6  27.8 -1.8       0.0    11      935   22 07 40
22 08 40  =1825+266    16 43 46  31.8  27.5 -1.7       0.0    60      943   22 07 41

22 08 40  PSRJ1821+26  16 43 46  32.4  26.2 -1.6       0.0   -29      943   No stop 
22 13 40  ---          16 48 47  32.9  25.0 -1.6       0.0   271      982   22 08 41

22 13 40  J1827+2638   16 48 47  32.3  26.4 -1.7       0.0   -29      982   No stop 
22 14 40  =1825+266    16 49 47  32.4  26.1 -1.6       0.0    31      989   22 13 41
Schedule for HART      (Code Hh )                                   Page   5
               Astrometry for three FAST discovered pulsars
  UP:  D => Below limits;  H => Below horizon mask;  W => still slewing at end;  blank => Up.
  Early: Seconds between end of slew and start.   Dwell: On source seconds. 
  Disk: GBytes recorded to this point.
  TPStart:  Recording start time.  Frequencies are LO sum (band edge).
  SYNC: Time correlator is expected to sync up.
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Disk   TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell   GBytes    SYNC
----------------------------------------------------------------------------------------

 --- Sun   2 Jun 2019   Day 153 ---

22 14 40  PSRJ1821+26  16 49 47  33.0  24.8 -1.5       0.0   -29      989   No stop 
22 19 40  ---          16 54 48  33.4  23.6 -1.5       0.0   271     1028   22 14 41

22 20 20  J1827+2638   16 55 28  32.9  24.8 -1.5       0.0    11     1028   22 20 20
22 21 20  =1825+266    16 56 28  33.0  24.5 -1.5       0.0    60     1036   22 20 21

22 21 20  PSRJ1821+26  16 56 28  33.6  23.1 -1.4       0.0   -29     1036   No stop 
22 26 20  ---          17 01 29  34.0  21.9 -1.3       0.0   271     1074   22 21 21

22 26 20  J1827+2638   17 01 29  33.5  23.3 -1.4       0.0   -29     1074   No stop 
22 27 20  =1825+266    17 02 29  33.6  23.0 -1.4       0.0    31     1082   22 26 21

22 27 20  PSRJ1821+26  17 02 29  34.1  21.7 -1.3       0.0   -29     1082   No stop 
22 32 20  ---          17 07 30  34.5  20.4 -1.2       0.0   271     1121   22 27 21

22 33 00  J1827+2638   17 08 10  34.0  21.6 -1.3       0.0    11     1121   22 33 00
22 34 00  =1825+266    17 09 10  34.1  21.4 -1.3       0.0    60     1128   22 33 01

22 34 00  PSRJ1821+26  17 09 10  34.6  20.0 -1.2       0.0   -29     1128   No stop 
22 39 00  ---          17 14 11  35.0  18.7 -1.1       0.0   271     1167   22 34 01

22 39 00  J1827+2638   17 14 11  34.5  20.1 -1.2       0.0   -29     1167   No stop 
22 40 00  =1825+266    17 15 11  34.6  19.9 -1.2       0.0    31     1175   22 39 01

22 40 00  PSRJ1821+26  17 15 11  35.1  18.4 -1.1       0.0   -29     1175   No stop 
22 45 00  ---          17 20 12  35.4  17.1 -1.0       0.0   271     1213   22 40 01

22 45 40  J1827+2638   17 20 52  35.0  18.4 -1.1       0.0    11     1213   22 45 40
22 46 40  =1825+266    17 21 52  35.1  18.1 -1.1       0.0    60     1221   22 45 41

22 46 40  PSRJ1821+26  17 21 52  35.5  16.7 -1.0       0.0   -29     1221   No stop 
22 51 40  ---          17 26 53  35.8  15.3 -0.9       0.0   271     1260   22 46 41

22 51 40  J1827+2638   17 26 53  35.4  16.8 -1.0       0.0   -29     1260   No stop 
22 52 40  =1825+266    17 27 53  35.5  16.6 -1.0       0.0    31     1268   22 51 41

22 52 40  PSRJ1821+26  17 27 53  35.9  15.1 -0.9       0.0   -29     1268   No stop 
22 57 40  ---          17 32 54  36.2  13.7 -0.8       0.0   271     1306   22 52 41

22 58 20  J1827+2638   17 33 34  35.8  15.1 -0.9       0.0    11     1306   22 58 20
22 59 20  =1825+266    17 34 34  35.9  14.8 -0.9       0.0    60     1314   22 58 21

22 59 20  PSRJ1821+26  17 34 34  36.3  13.3 -0.8       0.0   -29     1314   No stop 
23 04 20  ---          17 39 35  36.5  11.9 -0.7       0.0   271     1353   22 59 21
Schedule for HART      (Code Hh )                                   Page   6
               Astrometry for three FAST discovered pulsars
  UP:  D => Below limits;  H => Below horizon mask;  W => still slewing at end;  blank => Up.
  Early: Seconds between end of slew and start.   Dwell: On source seconds. 
  Disk: GBytes recorded to this point.
  TPStart:  Recording start time.  Frequencies are LO sum (band edge).
  SYNC: Time correlator is expected to sync up.
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Disk   TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell   GBytes    SYNC
----------------------------------------------------------------------------------------

 --- Sun   2 Jun 2019   Day 153 ---

23 04 20  J1827+2638   17 39 35  36.2  13.5 -0.8       0.0   -29     1353   No stop 
23 05 20  =1825+266    17 40 35  36.2  13.2 -0.8       0.0    31     1360   23 04 21

23 05 20  PSRJ1821+26  17 40 35  36.5  11.7 -0.7       0.0   -29     1360   No stop 
23 10 20  ---          17 45 36  36.8  10.3 -0.6       0.0   271     1399   23 05 21

23 11 00  J1827+2638   17 46 16  36.5  11.7 -0.7       0.0    11     1399   23 11 00
23 12 00  =1825+266    17 47 16  36.5  11.4 -0.7       0.0    60     1407   23 11 01

23 12 00  PSRJ1821+26  17 47 16  36.8   9.8 -0.6       0.0   -29     1407   No stop 
23 17 00  ---          17 52 17  37.0   8.4 -0.5       0.0   271     1445   23 12 01

23 17 00  J1827+2638   17 52 17  36.8  10.0 -0.6       0.0   -29     1445   No stop 
23 18 00  =1825+266    17 53 17  36.8   9.7 -0.6       0.0    31     1453   23 17 01

23 18 00  PSRJ1821+26  17 53 17  37.0   8.2 -0.5       0.0   -29     1453   No stop 
23 23 00  ---          17 58 18  37.2   6.8 -0.4       0.0   271     1492   23 18 01

23 23 40  J1827+2638   17 58 58  37.0   8.2 -0.5       0.0    11     1492   23 23 40
23 24 40  =1825+266    17 59 58  37.0   7.9 -0.5       0.0    60     1499   23 23 41

23 24 40  PSRJ1821+26  17 59 58  37.2   6.3 -0.4       0.0   -29     1499   No stop 
23 29 40  ---          18 04 59  37.3   4.9 -0.3       0.0   271     1538   23 24 41

23 29 40  J1827+2638   18 04 59  37.2   6.5 -0.4       0.0   -29     1538   No stop 
23 30 40  =1825+266    18 05 59  37.2   6.2 -0.4       0.0    31     1546   23 29 41

23 30 40  PSRJ1821+26  18 05 59  37.4   4.6 -0.3       0.0   -29     1546   No stop 
23 35 40  ---          18 11 00  37.4   3.2 -0.2       0.0   271     1584   23 30 41

23 36 20  J1827+2638   18 11 40  37.3   4.6 -0.3       0.0    11     1584   23 36 20
23 37 20  =1825+266    18 12 40  37.3   4.3 -0.3       0.0    60     1592   23 36 21

23 40 20  J1642+3948   18 15 41  20.9 341.2  1.5       0.0   100     1592   23 40 20
23 55 20  =3C345       18 30 43  19.8 338.4  1.8       0.0   900     1708   23 40 21

 --- Start: Sun   2 Jun 2019   Day 153 -- Stop: Mon   3 Jun 2019   Day 154 ---

23 58 20  J2253+1608   18 33 44  13.8  63.9 -4.4       0.0   -31     1708   23 58 20
00 13 20  =3C454.3     18 48 46  16.8  61.9 -4.1       0.0   869     1824   23 58 21

03 52 50  J2253+1608   22 28 52  47.4   9.3 -0.4       0.0 13145     1824   03 52 50
04 07 50  =3C454.3     22 43 55  47.8   3.9 -0.2       0.0   900     1940   03 52 51


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


 ======== Setup file: sess219.L1024
   Matching groups in /home/guest/rmc/SCHED/sched11.5/catalogs/freq.dat:
     hh18cm          Values confirmed by E-mail Jonathan Quick 20140219 (CR)
    ****** Only  122.49 of  256.00 MHz total bandwidth is within the IFs
           in the setup file before any FREQ or DOPPLER shifts.

   Setup group:    8         Station: HART              Total bit rate:  1024
   Format: VDIF              Bits per sample: 2         Sample rate: 32.000
   Number of channels: 16    DBE type: DBBC_DDC         Speedup factor:   1.00

   Disk used to record data.

   1st LO=   1510.00   1510.00   1510.00   1510.00   1510.00   1510.00   1510.00   1510.00
             1510.00   1510.00   1510.00   1510.00   1510.00   1510.00   1510.00   1510.00
   Net SB=         L         L         U         U         L         L         U         U
                   L         L         U         U         L         L         U         U
   IF SB =         U         U         U         U         U         U         U         U
                   U         U         U         U         U         U         U         U
   Pol.  =      RCP       LCP       RCP       LCP       RCP       LCP       RCP       LCP 
                RCP       LCP       RCP       LCP       RCP       LCP       RCP       LCP 
   BBC   =         1         9         1         9         2        10         2        10
                   3        11         3        11         4        12         4        12
   BBC SB=         L         L         U         U         L         L         U         U
                   L         L         U         U         L         L         U         U
   IF    =        A1        C1        A1        C1        A1        C1        A1        C1
                  A1        C1        A1        C1        A1        C1        A1        C1

  The following frequency sets based on these setups were used.

   Frequency Set:   9  Setup file default.  Used with PCAL = off
   LO sum=   1610.49  1610.49  1610.49  1610.49  1642.49  1642.49  1642.49  1642.49
             1674.49  1674.49  1674.49  1674.49  1706.49  1706.49  1706.49  1706.49
   BBC fr=    100.49   100.49   100.49   100.49   132.49   132.49   132.49   132.49
              164.49   164.49   164.49   164.49   196.49   196.49   196.49   196.49
   Bandwd=     16.00    16.00    16.00    16.00    16.00    16.00    16.00    16.00
               16.00    16.00    16.00    16.00    16.00    16.00    16.00    16.00
    Matching frequency sets:   9

   Track assignments are: 
    track1=   1,  2,  3,  4,  5,  6,  7,  8,  9, 10, 11, 12, 13, 14, 15, 16
    barrel=roll_off 

 POSITIONS OF SOURCES USED IN RECORDING SCANS

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

 * PSRJ1821+26       18 19 37.203357   * 18 21 37.700000     18 22 25.036569       0.00
                     26 34 10.29717    * 26 35 40.40000      26 36 14.82137        0.00
                     From catalog imbedded in main SCHED input file.

 * PSRJ2053+47       20 51 31.283991   * 20 53 12.100000     20 53 51.693054       0.00
                     47 15 43.10320    * 47 27 07.60000      47 31 18.11550        0.00
                     From catalog imbedded in main SCHED input file.

 * PSRJ2336+48       23 34 22.400030   * 23 36 48.200000     23 37 43.857634       0.00
                     48 10 28.77202    * 48 27 05.00000      48 33 09.31410        0.00
                     From catalog imbedded in main SCHED input file.

   3C345             16 41 17.606229   * 16 42 58.809967     16 43 39.082666       0.79
 * J1642+3948        39 54 10.81492    * 39 48 36.99399      39 46 33.26029        0.59
   1641+399          /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc
   J1642+39          GSFC 2016a X/S astro solution,  53724 observations.

   1825+266          18 25 19.613641   * 18 27 20.134570     18 28 07.468435       0.27
 * J1827+2638        26 36 29.22901    * 26 38 24.15140      26 39 07.81597        0.50
                     /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution,     58 observations.

   2100+468          21 00 33.500167   * 21 02 17.056074     21 02 57.629572       0.38
 * J2102+4702        46 50 23.37641    * 47 02 16.25338      47 06 37.27722        0.39
   J2102+47          /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution,     41 observations.

   3C454.3           22 51 29.519739   * 22 53 57.747939     22 54 54.353563       0.65
 * J2253+1608        15 52 54.34808    * 16 08 53.56091      16 14 53.21443        0.73
   2251+158          /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc
   J2253+16          GSFC 2016a X/S astro solution,  41272 observations.

   2323+478          23 23 22.550407   * 23 25 44.912246     23 26 39.333943       0.26
 * J2325+4806        47 49 55.33098    * 48 06 25.28761      48 12 27.44042        0.25
                     /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution,     75 observations.



SOURCE SCAN SUMMARY FOR SOURCES LISTED ABOVE

     Scan hours are for recording scans only. 
     Baseline hours are only counted for scans above horizon at both ends.
  Source       Setup file             Frequency sets                  Observing hours
                                   (duplicates not shown)              Scan  Baseline
  PSRJ1821+26sess219.L1024         1 2 3 4 5 6 7 8 9 10 13 14        2.833   240.031
  PSRJ2053+47sess219.L1024         1 2 3 4 5 6 7 8 10 13 14          2.833   187.775
  PSRJ2336+48sess219.L1024         1 2 3 4 5 6 7 8 10 13 14          3.000   194.095
  J1642+3948 sess219.L1024         1 2 3 4 5 6 7 9 10 13             0.250    16.500
  J1827+2638 sess219.L1024         1 2 3 4 5 6 7 8 9 10 13 14        0.600    45.900
  J2102+4702 sess219.L1024         1 2 3 4 5 6 7 8 10 13 14          0.600    34.094
  J2253+1608 sess219.L1024         1 2 3 4 5 6 7 8 9 10 13 14        0.500    39.645
  J2325+4806 sess219.L1024         1 2 3 4 5 6 7 8 10 13 14          0.636    32.325


EFFECT OF SOLAR CORONA

  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) 
   PSRJ1821+26        125.5
   PSRJ2053+47         90.4
   PSRJ2336+48         64.6
   J1642+3948         118.0
   J1827+2638         124.9
   J2102+4702          89.4
   J2253+1608          81.3
   J2325+4806          66.5

  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 

