  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: Is SRGE J170245.3+130104 a blazar?
 Exp. Code:  EA069B  


Schedule Version:       3.00
Processed by SCHED version:  11.60  Release 11.6; April 2020

PI:       Tao An

Address:  Shanghai Astronomical Observatory
          80th Nandan Road, Xuhui District
          Shanghai 200030
          China

Phone:    +86-13261603255
EMAIL:    antao@shao.ac.cn
Fax:
Phone during observation:

Observing mode: Phase-referencing

Notes:    1.4 GHz, dual polarisation, 2048 Mbps
          eVLBI, 6 hours at GST: J1702+1301
          Drafted by Yuanqi Liu
 

Schedule for HART      (Code Hh )                                   Page   2
               Is SRGE J170245.3+130104 a blazar?
  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
----------------------------------------------------------------------------------------

 --- Thu   8 Jun 2023   Day 159 ---

 Next scan frequencies:  1626.49  1626.49  1626.49  1626.49  1690.49  1690.49  1690.49  1690.49
 Next BBC frequencies:    116.49   116.49   116.49   116.49   180.49   180.49   180.49   180.49
 Next scan bandwidths:     32.00    32.00    32.00    32.00    32.00    32.00    32.00    32.00

19 00 00  J1706+1208   13 58 21  30.3  56.3 -3.2       0.0     0        0   19 00 00
19 05 00  =1704+122    14 03 22  31.3  55.4 -3.1       0.0   300       39   19 00 01

19 05 30  J1707+1331   14 03 52  30.2  54.4 -3.1       0.0     1       39   19 05 30
19 07 00  ---          14 05 23  30.5  54.1 -3.1       0.0    90       50   19 05 31

19 07 00  J1702+1301   14 05 23  31.7  53.6 -3.0       0.0   -29       50   No stop 
19 11 00  ---          14 09 23  32.4  52.8 -2.9       0.0   211       81   19 07 01

19 11 30  J1707+1331   14 09 53  31.3  53.2 -3.0       0.0     2       81   19 11 30
19 12 30  ---          14 10 53  31.5  53.0 -3.0       0.0    60       89   19 11 31

19 12 30  J1702+1301   14 10 53  32.7  52.5 -2.9       0.0   -29       89   No stop 
19 16 30  ---          14 14 54  33.4  51.7 -2.8       0.0   211      120   19 12 31

19 16 30  J1707+1331   14 14 54  32.2  52.3 -2.9       0.0   -28      120   No stop 
19 18 00  ---          14 16 24  32.5  52.0 -2.9       0.0    62      131   19 16 31

19 18 00  J1702+1301   14 16 24  33.7  51.4 -2.8       0.0   -29      131   No stop 
19 22 00  ---          14 20 25  34.4  50.6 -2.7       0.0   211      162   19 18 01

19 22 30  J1707+1331   14 20 55  33.3  51.1 -2.8       0.0     2      162   19 22 30
19 23 30  ---          14 21 55  33.4  50.9 -2.8       0.0    60      170   19 22 31

19 23 30  J1702+1301   14 21 55  34.7  50.3 -2.7       0.0   -29      170   No stop 
19 27 30  ---          14 25 56  35.3  49.4 -2.6       0.0   211      201   19 23 31

19 27 30  J1707+1331   14 25 56  34.1  50.0 -2.7       0.0   -28      201   No stop 
19 29 00  ---          14 27 26  34.4  49.7 -2.7       0.0    62      213   19 27 31

19 29 00  J1702+1301   14 27 26  35.6  49.1 -2.6       0.0   -29      213   No stop 
19 33 00  ---          14 31 27  36.3  48.2 -2.5       0.0   211      243   19 29 01

19 33 30  J1707+1331   14 31 57  35.2  48.8 -2.6       0.0     2      243   19 33 30
19 34 30  ---          14 32 57  35.3  48.6 -2.6       0.0    60      251   19 33 31

19 34 30  J1702+1301   14 32 57  36.5  47.9 -2.5       0.0   -29      251   No stop 
19 38 30  ---          14 36 58  37.2  47.0 -2.4       0.0   211      282   19 34 31

19 38 30  J1707+1331   14 36 58  36.0  47.7 -2.5       0.0   -28      282   No stop 
19 40 00  ---          14 38 28  36.3  47.4 -2.5       0.0    62      294   19 38 31
Schedule for HART      (Code Hh )                                   Page   3
               Is SRGE J170245.3+130104 a blazar?
  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
----------------------------------------------------------------------------------------

 --- Thu   8 Jun 2023   Day 159 ---

19 40 00  J1702+1301   14 38 28  37.4  46.7 -2.4       0.0   -29      294   No stop 
19 44 00  ---          14 42 29  38.1  45.7 -2.4       0.0   211      325   19 40 01

19 44 30  J1707+1331   14 42 59  37.0  46.4 -2.4       0.0     2      325   19 44 30
19 45 30  ---          14 43 59  37.2  46.1 -2.4       0.0    60      332   19 44 31

19 45 30  J1702+1301   14 43 59  38.3  45.4 -2.3       0.0   -29      332   No stop 
19 49 30  ---          14 48 00  39.0  44.4 -2.3       0.0   211      363   19 45 31

19 49 30  J1707+1331   14 48 00  37.8  45.2 -2.3       0.0   -28      363   No stop 
19 51 00  ---          14 49 30  38.0  44.9 -2.3       0.0    62      375   19 49 31

19 51 00  J1702+1301   14 49 30  39.2  44.1 -2.2       0.0   -29      375   No stop 
19 55 00  ---          14 53 30  39.8  43.1 -2.2       0.0   211      406   19 51 01

19 55 30  J1707+1331   14 54 01  38.7  43.8 -2.2       0.0     2      406   19 55 30
19 56 30  ---          14 55 01  38.9  43.5 -2.2       0.0    60      414   19 55 31

19 56 30  J1702+1301   14 55 01  40.1  42.7 -2.1       0.0   -29      414   No stop 
20 00 30  ---          14 59 01  40.7  41.7 -2.1       0.0   211      444   19 56 31

20 00 30  J1707+1331   14 59 01  39.5  42.6 -2.2       0.0   -28      444   No stop 
20 02 00  ---          15 00 32  39.7  42.2 -2.1       0.0    62      456   20 00 31

20 02 00  J1702+1301   15 00 32  40.9  41.4 -2.1       0.0   -29      456   No stop 
20 06 00  ---          15 04 32  41.5  40.3 -2.0       0.0   211      487   20 02 01

20 06 30  J1707+1331   15 05 02  40.4  41.1 -2.1       0.0     2      487   20 06 30
20 07 30  ---          15 06 03  40.6  40.8 -2.0       0.0    60      495   20 06 31

20 07 30  J1702+1301   15 06 03  41.7  39.9 -2.0       0.0   -29      495   No stop 
20 11 30  ---          15 10 03  42.3  38.9 -1.9       0.0   211      526   20 07 31

20 11 30  J1707+1331   15 10 03  41.2  39.8 -2.0       0.0   -28      526   No stop 
20 13 00  ---          15 11 33  41.4  39.4 -2.0       0.0    62      537   20 11 31

20 13 00  J1702+1301   15 11 33  42.5  38.5 -1.9       0.0   -29      537   No stop 
20 17 00  ---          15 15 34  43.0  37.4 -1.8       0.0   211      568   20 13 01

20 17 30  J1707+1331   15 16 04  42.0  38.2 -1.9       0.0     2      568   20 17 30
20 18 30  ---          15 17 04  42.1  37.9 -1.9       0.0    60      576   20 17 31

20 18 30  J1702+1301   15 17 04  43.2  36.9 -1.8       0.0   -29      576   No stop 
20 22 30  ---          15 21 05  43.8  35.8 -1.7       0.0   211      607   20 18 31
Schedule for HART      (Code Hh )                                   Page   4
               Is SRGE J170245.3+130104 a blazar?
  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
----------------------------------------------------------------------------------------

 --- Thu   8 Jun 2023   Day 159 ---

20 22 30  J1707+1331   15 21 05  42.7  36.8 -1.8       0.0   -28      607   No stop 
20 24 00  ---          15 22 35  42.9  36.4 -1.8       0.0    62      618   20 22 31

20 24 00  J1702+1301   15 22 35  44.0  35.4 -1.7       0.0   -29      618   No stop 
20 28 00  ---          15 26 36  44.5  34.2 -1.6       0.0   211      649   20 24 01

20 28 30  J1707+1331   15 27 06  43.5  35.1 -1.7       0.0     2      649   20 28 30
20 29 30  ---          15 28 06  43.6  34.9 -1.7       0.0    60      657   20 28 31

20 29 30  J1702+1301   15 28 06  44.7  33.8 -1.6       0.0   -29      657   No stop 
20 33 30  ---          15 32 07  45.2  32.6 -1.5       0.0   211      688   20 29 31

20 33 30  J1707+1331   15 32 07  44.1  33.7 -1.6       0.0   -28      688   No stop 
20 35 00  ---          15 33 37  44.3  33.3 -1.6       0.0    62      699   20 33 31

20 35 00  J1702+1301   15 33 37  45.4  32.1 -1.5       0.0   -29      699   No stop 
20 39 00  ---          15 37 38  45.8  30.9 -1.4       0.0   211      730   20 35 01

20 39 30  J1707+1331   15 38 08  44.9  31.9 -1.5       0.0     2      730   20 39 30
20 40 30  ---          15 39 08  45.0  31.6 -1.5       0.0    60      738   20 39 31

20 40 30  J1702+1301   15 39 08  46.0  30.5 -1.4       0.0   -29      738   No stop 
20 44 30  ---          15 43 09  46.4  29.2 -1.3       0.0   211      769   20 40 31

20 44 30  J1707+1331   15 43 09  45.4  30.4 -1.4       0.0   -28      769   No stop 
20 46 00  ---          15 44 39  45.6  30.0 -1.4       0.0    62      781   20 44 31

20 46 40  J1706+1208   15 45 19  47.1  30.2 -1.4       0.0    11      781   20 46 40
20 50 40  =1704+122    15 49 20  47.5  28.9 -1.3       0.0   240      812   20 46 41

20 51 20  J1707+1331   15 50 00  46.2  28.3 -1.3       0.0    11      812   20 51 20
20 52 20  ---          15 51 00  46.3  28.0 -1.3       0.0    60      819   20 51 21

20 52 20  J1702+1301   15 51 00  47.3  26.7 -1.2       0.0   -29      819   No stop 
20 56 20  ---          15 55 01  47.7  25.4 -1.1       0.0   211      850   20 52 21

20 56 20  J1707+1331   15 55 01  46.7  26.7 -1.2       0.0   -28      850   No stop 
20 57 50  ---          15 56 31  46.9  26.2 -1.2       0.0    62      862   20 56 21

20 57 50  J1702+1301   15 56 31  47.8  24.9 -1.1       0.0   -29      862   No stop 
21 01 50  ---          16 00 31  48.2  23.5 -1.1       0.0   211      893   20 57 51

21 02 20  J1707+1331   16 01 02  47.3  24.7 -1.1       0.0     2      893   21 02 20
21 03 20  ---          16 02 02  47.4  24.4 -1.1       0.0    60      900   21 02 21
Schedule for HART      (Code Hh )                                   Page   5
               Is SRGE J170245.3+130104 a blazar?
  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
----------------------------------------------------------------------------------------

 --- Thu   8 Jun 2023   Day 159 ---

21 03 20  J1702+1301   16 02 02  48.3  23.0 -1.0       0.0   -29      900   No stop 
21 07 20  ---          16 06 02  48.7  21.6 -1.0       0.0   211      931   21 03 21

21 07 20  J1707+1331   16 06 02  47.8  23.0 -1.0       0.0   -28      931   No stop 
21 08 50  ---          16 07 33  47.9  22.5 -1.0       0.0    62      943   21 07 21

21 08 50  J1702+1301   16 07 33  48.8  21.1 -0.9       0.0   -29      943   No stop 
21 12 50  ---          16 11 33  49.1  19.7 -0.9       0.0   211      974   21 08 51

21 13 20  J1707+1331   16 12 03  48.3  21.0 -0.9       0.0     2      974   21 13 20
21 14 20  ---          16 13 04  48.3  20.7 -0.9       0.0    60      982   21 13 21

21 14 20  J1702+1301   16 13 04  49.2  19.1 -0.8       0.0   -29      982   No stop 
21 18 20  ---          16 17 04  49.5  17.7 -0.8       0.0   211     1013   21 14 21

21 18 20  J1707+1331   16 17 04  48.7  19.3 -0.9       0.0   -28     1013   No stop 
21 19 50  ---          16 18 34  48.8  18.7 -0.8       0.0    62     1024   21 18 21

21 19 50  J1702+1301   16 18 34  49.6  17.2 -0.8       0.0   -29     1024   No stop 
21 23 50  ---          16 22 35  49.9  15.7 -0.7       0.0   211     1055   21 19 51

21 24 20  J1707+1331   16 23 05  49.1  17.1 -0.8       0.0     2     1055   21 24 20
21 25 20  ---          16 24 05  49.1  16.8 -0.7       0.0    60     1063   21 24 21

21 25 20  J1702+1301   16 24 05  49.9  15.2 -0.7       0.0   -29     1063   No stop 
21 29 20  ---          16 28 06  50.2  13.7 -0.6       0.0   211     1094   21 25 21

21 29 20  J1707+1331   16 28 06  49.4  15.3 -0.7       0.0   -28     1094   No stop 
21 30 50  ---          16 29 36  49.5  14.8 -0.7       0.0    62     1105   21 29 21

21 30 50  J1702+1301   16 29 36  50.2  13.1 -0.6       0.0   -29     1105   No stop 
21 34 50  ---          16 33 37  50.4  11.6 -0.5       0.0   211     1136   21 30 51

21 35 20  J1707+1331   16 34 07  49.7  13.1 -0.6       0.0     2     1136   21 35 20
21 36 20  ---          16 35 07  49.8  12.8 -0.6       0.0    60     1144   21 35 21

21 36 20  J1702+1301   16 35 07  50.5  11.0 -0.5       0.0   -29     1144   No stop 
21 40 20  ---          16 39 08  50.7   9.5 -0.4       0.0   211     1175   21 36 21

21 40 20  J1707+1331   16 39 08  50.0  11.3 -0.5       0.0   -28     1175   No stop 
21 41 50  ---          16 40 38  50.0  10.7 -0.5       0.0    62     1186   21 40 21

21 41 50  J1702+1301   16 40 38  50.7   9.0 -0.4       0.0   -29     1186   No stop 
21 45 50  ---          16 44 39  50.8   7.4 -0.3       0.0   211     1217   21 41 51
Schedule for HART      (Code Hh )                                   Page   6
               Is SRGE J170245.3+130104 a blazar?
  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
----------------------------------------------------------------------------------------

 --- Thu   8 Jun 2023   Day 159 ---

21 46 20  J1707+1331   16 45 09  50.2   9.0 -0.4       0.0     2     1217   21 46 20
21 47 20  ---          16 46 09  50.2   8.6 -0.4       0.0    60     1225   21 46 21

21 47 20  J1702+1301   16 46 09  50.9   6.8 -0.3       0.0   -29     1225   No stop 
21 51 20  ---          16 50 10  51.0   5.3 -0.2       0.0   211     1256   21 47 21

21 51 20  J1707+1331   16 50 10  50.4   7.1 -0.3       0.0   -28     1256   No stop 
21 52 50  ---          16 51 40  50.4   6.6 -0.3       0.0    62     1268   21 51 21

21 52 50  J1702+1301   16 51 40  51.0   4.7 -0.2       0.0   -29     1268   No stop 
21 56 50  ---          16 55 40  51.1   3.2 -0.1       0.0   211     1298   21 52 51

21 57 20  J1707+1331   16 56 11  50.5   4.8 -0.2       0.0     2     1298   21 57 20
21 58 20  ---          16 57 11  50.5   4.5 -0.2       0.0    60     1306   21 57 21

21 58 20  J1702+1301   16 57 11  51.1   2.6 -0.1       0.0   -29     1306   No stop 
22 02 20  ---          17 01 11  51.1   1.0 -0.0       0.0   211     1337   21 58 21

22 02 20  J1707+1331   17 01 11  50.6   2.9 -0.1       0.0   -28     1337   No stop 
22 03 50  ---          17 02 42  50.6   2.4 -0.1       0.0    62     1349   22 02 21

22 03 50  J1702+1301   17 02 42  51.1   0.5 -0.0       0.0   -29     1349   No stop 
22 07 50  ---          17 06 42  51.1 358.9  0.0       0.0   211     1380   22 03 51

22 08 20  J1707+1331   17 07 12  50.6   0.6 -0.0       0.0     2     1380   22 08 20
22 09 20  ---          17 08 13  50.6   0.2 -0.0       0.0    60     1387   22 08 21

22 09 20  J1702+1301   17 08 13  51.1 358.3  0.1       0.0   -29     1387   No stop 
22 13 20  ---          17 12 13  51.1 356.8  0.1       0.0   211     1418   22 09 21

22 13 20  J1707+1331   17 12 13  50.6 358.7  0.1       0.0   -28     1418   No stop 
22 14 50  ---          17 13 43  50.6 358.1  0.1       0.0    62     1430   22 13 21

22 14 50  J1702+1301   17 13 43  51.1 356.2  0.2       0.0   -29     1430   No stop 
22 18 50  ---          17 17 44  51.0 354.6  0.2       0.0   211     1461   22 14 51

22 19 20  J1707+1331   17 18 14  50.6 356.4  0.2       0.0     2     1461   22 19 20
22 20 20  ---          17 19 14  50.5 356.0  0.2       0.0    60     1469   22 19 21

22 20 20  J1702+1301   17 19 14  50.9 354.0  0.3       0.0   -29     1469   No stop 
22 24 20  ---          17 23 15  50.8 352.5  0.3       0.0   211     1499   22 20 21

22 24 20  J1707+1331   17 23 15  50.5 354.5  0.2       0.0   -28     1499   No stop 
22 25 50  ---          17 24 45  50.4 353.9  0.3       0.0    62     1511   22 24 21
Schedule for HART      (Code Hh )                                   Page   7
               Is SRGE J170245.3+130104 a blazar?
  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
----------------------------------------------------------------------------------------

 --- Thu   8 Jun 2023   Day 159 ---

22 26 30  J1706+1208   17 25 25  51.7 352.9  0.3       0.0    11     1511   22 26 30
22 30 00  =1704+122    17 28 56  51.6 351.5  0.4       0.0   210     1538   22 26 31


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


 ======== Setup file: sess223.L1024
   Matching groups in /home/guest/rmc/SCHED/sched11.6/catalogs/freq_RDBE.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:    4         Station: HART              Total bit rate:  1024
   Format: VDIF              Bits per sample: 2         Sample rate: 64.000
   Number of channels:  8    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
   Net SB=         L         L         U         U         L         L         U         U
   IF SB =         U         U         U         U         U         U         U         U
   Pol.  =      RCP       LCP       RCP       LCP       RCP       LCP       RCP       LCP 
   BBC   =         1         9         1         9         2        10         2        10
   BBC SB=         L         L         U         U         L         L         U         U
   IF    =        A1        C1        A1        C1        A1        C1        A1        C1

  The following frequency sets based on these setups were used.

   Frequency Set:   8  Setup file default.  Used with PCAL = off
   LO sum=   1626.49  1626.49  1626.49  1626.49  1690.49  1690.49  1690.49  1690.49
   BBC fr=    116.49   116.49   116.49   116.49   180.49   180.49   180.49   180.49
   Bandwd=     32.00    32.00    32.00    32.00    32.00    32.00    32.00    32.00
    Matching frequency sets:   8

   Track assignments are: 
    track1=   1,  2,  3,  4,  5,  6,  7,  8
    barrel=roll_off 

 POSITIONS OF SOURCES USED IN RECORDING SCANS

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

 * J1702+1301        17 00 26.513935   * 17 02 45.312000     17 03 51.262267       0.00
                     13 05 14.77344    * 13 01 02.22220      12 58 59.49161        0.00
                     From catalog imbedded in main SCHED input file.

 * J1707+1331        17 05 27.517191   * 17 07 45.637300     17 08 51.273097       0.00
                     13 34 56.52195    * 13 31 05.23300      13 29 12.26316        0.00
                     From catalog imbedded in main SCHED input file.

   1704+122          17 04 00.724110   * 17 06 20.497447     17 07 26.893637       0.12
 * J1706+1208        12 12 57.17741    * 12 08 59.79450      12 07 04.04481        0.20
                     /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution,    127 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
  J1702+1301 sess223.L1024         1 2 3 4 5 6 7 8                   2.333    55.567
  J1707+1331 sess223.L1024         1 2 3 4 5 6 7 8                   0.775    17.539
  J1706+1208 sess223.L1024         1 2 3 4 5 6 7 8                   0.208     5.425


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) 
   J1702+1301         144.1
   J1707+1331         143.6
   J1706+1208         145.0

  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 

