  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: mas structure of transient radio emission from mid-IR burst galaxies
 Exp. Code:  ES091A  


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

PI:       Shu, Xinwen

Address:  Department of Physics
          Anhui Normal University
          189 South Jiuhua Road
          Wuhu, Anhui, China

Phone:    8617755362162
EMAIL:    xwshu@mail.ahnu.edu.cn
Fax:
Phone during observation: 8617755362162

Observing mode: evn

Notes:    v3 - includes Pi
 
 
 

Schedule for HART      (Code Hh )                                   Page   2
               mas structure of transient radio emission from mid-IR burst galaxies
  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  11 Jun 2020   Day 163 ---

 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

14 31 07  J1241        09 43 26   8.7  30.6 -3.0       0.0     0        0   14 31 07
14 34 37  ---          09 46 56   9.1  30.2 -2.9       0.0   210       27   14 31 08

14 36 32  J1241        09 48 52   9.3  29.9 -2.9       0.0    94       27   14 36 32
14 40 02  ---          09 52 22   9.7  29.4 -2.8       0.0   210       54   14 36 33

14 41 32  J1241        09 53 53   9.9  29.2 -2.8       0.0    69       54   14 41 32
14 45 02  ---          09 57 23  10.3  28.7 -2.8       0.0   210       81   14 41 33

14 46 57  J1241        09 59 18  10.5  28.4 -2.7       0.0    94       81   14 46 57
14 50 27  ---          10 02 49  10.9  27.9 -2.7       0.0   210      108   14 46 58

14 51 57  J1241        10 04 19  11.0  27.6 -2.6       0.0    69      108   14 51 57
14 55 27  ---          10 07 50  11.4  27.1 -2.6       0.0   210      135   14 51 58

14 57 22  J1241        10 09 45  11.6  26.8 -2.5       0.0    94      135   14 57 22
15 00 52  ---          10 13 16  11.9  26.3 -2.5       0.0   210      162   14 57 23

15 02 22  J1241        10 14 46  12.1  26.1 -2.5       0.0    69      162   15 02 22
15 05 52  ---          10 18 17  12.4  25.5 -2.4       0.0   210      189   15 02 23

15 07 47  J1241        10 20 12  12.6  25.2 -2.4       0.0    94      189   15 07 47
15 11 17  ---          10 23 42  12.9  24.7 -2.3       0.0   210      216   15 07 48

15 12 47  J1241        10 25 13  13.1  24.5 -2.3       0.0    69      216   15 12 47
15 16 17  ---          10 28 43  13.4  23.9 -2.2       0.0   210      243   15 12 48

15 18 12  J1241        10 30 39  13.6  23.6 -2.2       0.0    94      243   15 18 12
15 21 42  ---          10 34 09  13.9  23.0 -2.1       0.0   210      271   15 18 13

15 23 12  J1241        10 35 39  14.0  22.8 -2.1       0.0    69      271   15 23 12
15 26 42  ---          10 39 10  14.3  22.2 -2.1       0.0   210      298   15 23 13

15 28 37  J1241        10 41 05  14.5  21.9 -2.0       0.0    94      298   15 28 37
15 32 07  ---          10 44 36  14.8  21.3 -2.0       0.0   210      325   15 28 38

15 33 37  J1241        10 46 06  14.9  21.1 -1.9       0.0    69      325   15 33 37
15 37 07  ---          10 49 37  15.2  20.5 -1.9       0.0   210      352   15 33 38
Schedule for HART      (Code Hh )                                   Page   3
               mas structure of transient radio emission from mid-IR burst galaxies
  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  11 Jun 2020   Day 163 ---

15 39 02  J1241        10 51 32  15.3  20.2 -1.8       0.0    94      352   15 39 02
15 42 32  ---          10 55 03  15.6  19.6 -1.8       0.0   210      379   15 39 03

15 44 02  J1241        10 56 33  15.7  19.4 -1.8       0.0    69      379   15 44 02
15 47 32  ---          11 00 03  16.0  18.8 -1.7       0.0   210      406   15 44 03

15 49 27  J1241        11 01 59  16.1  18.4 -1.7       0.0    94      406   15 49 27
15 52 57  ---          11 05 29  16.3  17.8 -1.6       0.0   210      433   15 49 28

15 54 27  J1241        11 06 59  16.5  17.6 -1.6       0.0    69      433   15 54 27
15 57 57  ---          11 10 30  16.7  17.0 -1.5       0.0   210      460   15 54 28

15 59 52  J1241        11 12 25  16.8  16.6 -1.5       0.0    94      460   15 59 52
16 03 22  ---          11 15 56  17.0  16.0 -1.4       0.0   210      487   15 59 53

16 06 29  3C286        11 19 04  25.3  31.5 -2.2       0.0   133      487   16 06 29
16 09 29  ---          11 22 14  25.7  30.9 -2.2       0.0   180      510   16 06 30

16 11 24  J1522+3144   11 23 59   9.0  48.1 -4.0       0.0    32      510   16 11 24
16 12 54  =1520+319    11 25 39   9.3  47.9 -4.0       0.0    90      522   16 11 25

16 12 54  J1513        11 25 29  11.0  47.2 -3.8       0.0   -31      522   No stop 
16 16 24  ---          11 29 00  11.6  46.7 -3.8       0.0   179      549   16 12 55

16 16 54  J1522+3144   11 29 30   9.9  47.4 -3.9       0.0    -1      549   16 16 54
16 18 19  =1520+319    11 30 55  10.2  47.2 -3.9       0.0    84      560   16 16 55

16 18 19  J1513        11 30 55  11.9  46.4 -3.7       0.0   -31      560   No stop 
16 21 49  ---          11 34 26  12.5  45.9 -3.7       0.0   179      587   16 18 20

16 21 49  J1522+3144   11 34 26  10.7  46.7 -3.8       0.0   -31      587   No stop 
16 23 19  =1520+319    11 35 56  11.0  46.5 -3.8       0.0    59      598   16 21 50

16 23 19  J1513        11 35 56  12.7  45.7 -3.6       0.0   -31      598   No stop 
16 26 49  ---          11 39 27  13.3  45.2 -3.6       0.0   179      625   16 23 20

16 27 19  J1522+3144   11 39 57  11.6  45.9 -3.7       0.0    -1      625   16 27 19
16 28 44  =1520+319    11 41 22  11.9  45.7 -3.7       0.0    84      636   16 27 20

16 28 44  J1513        11 41 22  13.6  44.9 -3.6       0.0   -31      636   No stop 
16 32 14  ---          11 44 52  14.1  44.4 -3.5       0.0   179      663   16 28 45

16 32 14  J1522+3144   11 44 52  12.4  45.2 -3.6       0.0   -31      663   No stop 
16 33 44  =1520+319    11 46 23  12.7  45.0 -3.6       0.0    59      675   16 32 15
Schedule for HART      (Code Hh )                                   Page   4
               mas structure of transient radio emission from mid-IR burst galaxies
  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  11 Jun 2020   Day 163 ---

16 33 44  J1513        11 46 23  14.4  44.2 -3.5       0.0   -31      675   No stop 
16 37 14  ---          11 49 53  14.9  43.6 -3.4       0.0   179      702   16 33 45

16 37 44  J1522+3144   11 50 23  13.3  44.4 -3.5       0.0    -1      702   16 37 44
16 39 09  =1520+319    11 51 49  13.5  44.2 -3.5       0.0    84      713   16 37 45

16 39 09  J1513        11 51 49  15.2  43.4 -3.4       0.0   -31      713   No stop 
16 42 39  ---          11 55 19  15.7  42.8 -3.3       0.0   179      740   16 39 10

16 42 39  J1522+3144   11 55 19  14.1  43.7 -3.5       0.0   -31      740   No stop 
16 44 09  =1520+319    11 56 49  14.3  43.5 -3.4       0.0    59      752   16 42 40

16 44 09  J1513        11 56 49  16.0  42.6 -3.3       0.0   -31      752   No stop 
16 47 39  ---          12 00 20  16.5  42.0 -3.2       0.0   179      779   16 44 10

16 48 09  J1522+3144   12 00 50  14.9  42.8 -3.4       0.0    -1      779   16 48 09
16 49 34  =1520+319    12 02 15  15.1  42.6 -3.3       0.0    84      790   16 48 10

16 49 34  J1513        12 02 15  16.8  41.7 -3.2       0.0   -31      790   No stop 
16 53 04  ---          12 05 46  17.3  41.2 -3.1       0.0   179      817   16 49 35

16 53 04  J1522+3144   12 05 46  15.7  42.1 -3.3       0.0   -31      817   No stop 
16 54 34  =1520+319    12 07 16  15.9  41.9 -3.3       0.0    59      828   16 53 05

16 54 34  J1513        12 07 16  17.5  40.9 -3.1       0.0   -31      828   No stop 
16 58 04  ---          12 10 47  18.0  40.3 -3.1       0.0   179      855   16 54 35

16 58 34  J1522+3144   12 11 17  16.5  41.2 -3.2       0.0    -1      855   16 58 34
16 59 59  =1520+319    12 12 42  16.7  41.0 -3.2       0.0    84      866   16 58 35

16 59 59  J1513        12 12 42  18.3  40.0 -3.0       0.0   -31      866   No stop 
17 03 29  ---          12 16 13  18.8  39.4 -3.0       0.0   179      893   17 00 00

17 03 29  J1522+3144   12 16 13  17.2  40.4 -3.1       0.0   -31      893   No stop 
17 04 59  =1520+319    12 17 43  17.4  40.2 -3.1       0.0    59      905   17 03 30

17 06 54  3C286        12 19 38  31.1  18.2 -1.2       0.0    32      905   17 06 54
17 09 54  ---          12 22 49  31.3  17.5 -1.2       0.0   180      928   17 06 55

17 12 49  J1241        12 25 34  19.7   3.2 -0.3       0.0   120      928   17 12 49
17 16 19  ---          12 29 05  19.7   2.6 -0.2       0.0   210      955   17 12 50

17 18 14  J1241        12 31 00  19.7   2.2 -0.2       0.0    94      955   17 18 14
17 21 44  ---          12 34 31  19.7   1.5 -0.1       0.0   210      982   17 18 15
Schedule for HART      (Code Hh )                                   Page   5
               mas structure of transient radio emission from mid-IR burst galaxies
  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  11 Jun 2020   Day 163 ---

17 23 14  J1241        12 36 01  19.8   1.2 -0.1       0.0    69      982   17 23 14
17 26 44  ---          12 39 32  19.8   0.6 -0.1       0.0   210     1009   17 23 15

17 28 39  J1241        12 41 27  19.8   0.2 -0.0       0.0    94     1009   17 28 39
17 32 09  ---          12 44 57  19.8 359.5  0.0       0.0   210     1036   17 28 40

17 33 39  J1241        12 46 28  19.8 359.3  0.1       0.0    69     1036   17 33 39
17 37 09  ---          12 49 58  19.8 358.6  0.1       0.0   210     1063   17 33 40

17 39 04  J1241        12 51 54  19.7 358.2  0.2       0.0    94     1063   17 39 04
17 42 34  ---          12 55 24  19.7 357.6  0.2       0.0   210     1090   17 39 05

17 45 44  3C286        12 58 35  33.1   8.6 -0.6       0.0   136     1090   17 45 44
17 48 44  ---          13 01 46  33.2   7.8 -0.5       0.0   180     1114   17 45 45

17 51 58  J1241        13 04 49  19.6 355.8  0.4       0.0   138     1114   17 51 58
17 55 28  ---          13 08 20  19.5 355.1  0.4       0.0   210     1141   17 51 59

17 57 23  J1241        13 10 15  19.5 354.7  0.5       0.0    94     1141   17 57 23
18 00 53  ---          13 13 46  19.4 354.1  0.5       0.0   210     1168   17 57 24

18 02 23  J1241        13 15 16  19.4 353.8  0.5       0.0    69     1168   18 02 23
18 05 53  ---          13 18 47  19.3 353.1  0.6       0.0   210     1195   18 02 24

18 07 48  J1241        13 20 42  19.2 352.8  0.6       0.0    94     1195   18 07 48
18 11 18  ---          13 24 13  19.1 352.1  0.7       0.0   210     1222   18 07 49

18 12 48  J1241        13 25 43  19.1 351.9  0.7       0.0    69     1222   18 12 48
18 16 18  ---          13 29 13  19.0 351.2  0.8       0.0   210     1249   18 12 49

18 18 13  J1241        13 31 09  18.9 350.8  0.8       0.0    94     1249   18 18 13
18 21 43  ---          13 34 39  18.8 350.2  0.9       0.0   210     1276   18 18 14

18 25 57  J1522+3144   13 38 54  27.3  24.9 -1.7       0.0   147     1276   18 25 57
18 27 27  =1520+319    13 40 34  27.5  24.5 -1.7       0.0    90     1288   18 25 58

18 27 27  J1513        13 40 24  28.7  23.0 -1.6       0.0   -31     1288   No stop 
18 30 57  ---          13 43 55  29.0  22.2 -1.5       0.0   179     1315   18 27 28

18 31 27  J1522+3144   13 44 25  27.8  23.7 -1.6       0.0    -1     1315   18 31 27
18 32 52  =1520+319    13 45 50  27.9  23.4 -1.6       0.0    84     1326   18 31 28

18 32 52  J1513        13 45 50  29.2  21.7 -1.5       0.0   -31     1326   No stop 
18 36 22  ---          13 49 21  29.5  20.9 -1.4       0.0   179     1353   18 32 53
Schedule for HART      (Code Hh )                                   Page   6
               mas structure of transient radio emission from mid-IR burst galaxies
  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  11 Jun 2020   Day 163 ---

18 36 22  J1522+3144   13 49 21  28.3  22.6 -1.6       0.0   -31     1353   No stop 
18 37 52  =1520+319    13 50 51  28.4  22.2 -1.5       0.0    59     1364   18 36 23

18 37 52  J1513        13 50 51  29.6  20.6 -1.4       0.0   -31     1364   No stop 
18 41 22  ---          13 54 21  29.9  19.8 -1.3       0.0   179     1391   18 37 53

18 41 52  J1522+3144   13 54 52  28.7  21.4 -1.5       0.0    -1     1391   18 41 52
18 43 17  =1520+319    13 56 17  28.8  21.0 -1.4       0.0    84     1402   18 41 53

18 43 17  J1513        13 56 17  30.0  19.3 -1.3       0.0   -31     1402   No stop 
18 46 47  ---          13 59 47  30.3  18.5 -1.2       0.0   179     1429   18 43 18

18 46 47  J1522+3144   13 59 47  29.1  20.2 -1.4       0.0   -31     1429   No stop 
18 48 17  =1520+319    14 01 18  29.2  19.9 -1.4       0.0    59     1441   18 46 48

18 48 17  J1513        14 01 18  30.4  18.2 -1.2       0.0   -31     1441   No stop 
18 51 47  ---          14 04 48  30.6  17.4 -1.2       0.0   179     1468   18 48 18

18 52 17  J1522+3144   14 05 18  29.5  19.0 -1.3       0.0    -1     1468   18 52 17
18 53 42  =1520+319    14 06 43  29.6  18.7 -1.3       0.0    84     1479   18 52 18

18 53 42  J1513        14 06 43  30.7  16.9 -1.1       0.0   -31     1479   No stop 
18 57 12  ---          14 10 14  31.0  16.1 -1.1       0.0   179     1506   18 53 43

18 57 12  J1522+3144   14 10 14  29.9  17.8 -1.2       0.0   -31     1506   No stop 
18 58 42  =1520+319    14 11 44  30.0  17.5 -1.2       0.0    59     1517   18 57 13

18 58 42  J1513        14 11 44  31.0  15.7 -1.0       0.0   -31     1517   No stop 
19 02 12  ---          14 15 15  31.3  14.9 -1.0       0.0   179     1545   18 58 43

19 02 42  J1522+3144   14 15 45  30.2  16.6 -1.1       0.0    -1     1545   19 02 42
19 04 07  =1520+319    14 17 10  30.3  16.2 -1.1       0.0    84     1555   19 02 43

19 04 07  J1513        14 17 10  31.4  14.4 -1.0       0.0   -31     1555   No stop 
19 07 37  ---          14 20 41  31.6  13.5 -0.9       0.0   179     1583   19 04 08

19 07 37  J1522+3144   14 20 41  30.6  15.4 -1.0       0.0   -31     1583   No stop 
19 09 07  =1520+319    14 22 11  30.6  15.0 -1.0       0.0    59     1594   19 07 38

19 14 43  J1241        14 27 48  15.8 340.8  1.8       0.0   228     1594   19 14 43
19 18 13  ---          14 31 19  15.5 340.2  1.8       0.0   210     1621   19 14 44

19 20 08  J1241        14 33 14  15.3 339.8  1.8       0.0    94     1621   19 20 08
19 23 38  ---          14 36 45  15.1 339.3  1.9       0.0   210     1648   19 20 09
Schedule for HART      (Code Hh )                                   Page   7
               mas structure of transient radio emission from mid-IR burst galaxies
  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  11 Jun 2020   Day 163 ---

19 25 08  J1241        14 38 15  15.0 339.0  1.9       0.0    69     1648   19 25 08
19 28 38  ---          14 41 46  14.7 338.4  2.0       0.0   210     1675   19 25 09

19 30 33  J1241        14 43 41  14.5 338.1  2.0       0.0    94     1675   19 30 33
19 34 03  ---          14 47 11  14.2 337.6  2.1       0.0   210     1702   19 30 34

19 35 33  J1241        14 48 42  14.1 337.3  2.1       0.0    69     1702   19 35 33
19 39 03  ---          14 52 12  13.8 336.7  2.2       0.0   210     1729   19 35 34

19 40 58  J1241        14 54 08  13.6 336.4  2.2       0.0    94     1729   19 40 58
19 44 28  ---          14 57 38  13.3 335.9  2.3       0.0   210     1756   19 40 59

19 49 56  J1522+3144   15 03 07  32.2   5.0 -0.3       0.0   221     1756   19 49 56
19 51 26  =1520+319    15 04 47  32.3   4.6 -0.3       0.0    90     1768   19 49 57

19 51 26  J1513        15 04 37  32.9   2.5 -0.2       0.0   -31     1768   No stop 
19 54 56  ---          15 08 08  33.0   1.7 -0.1       0.0   179     1795   19 51 27

19 55 26  J1522+3144   15 08 38  32.3   3.6 -0.2       0.0    -1     1795   19 55 26
19 56 51  =1520+319    15 10 03  32.4   3.3 -0.2       0.0    84     1806   19 55 27

19 56 51  J1513        15 10 03  33.0   1.2 -0.1       0.0   -31     1806   No stop 
20 00 21  ---          15 13 34  33.0   0.3 -0.0       0.0   179     1833   19 56 52

20 00 21  J1522+3144   15 13 34  32.4   2.4 -0.2       0.0   -31     1833   No stop 
20 01 51  =1520+319    15 15 04  32.4   2.0 -0.1       0.0    59     1845   20 00 22

20 01 51  J1513        15 15 04  33.0 359.9  0.0       0.0   -31     1845   No stop 
20 05 21  ---          15 18 34  33.0 359.0  0.1       0.0   179     1872   20 01 52

20 05 51  J1522+3144   15 19 04  32.4   1.0 -0.1       0.0    -1     1872   20 05 51
20 07 16  =1520+319    15 20 30  32.4   0.6 -0.0       0.0    84     1883   20 05 52

20 07 16  J1513        15 20 30  33.0 358.5  0.1       0.0   -31     1883   No stop 
20 10 46  ---          15 24 00  32.9 357.6  0.2       0.0   179     1910   20 07 17

20 10 46  J1522+3144   15 24 00  32.4 359.7  0.0       0.0   -31     1910   No stop 
20 12 16  =1520+319    15 25 30  32.4 359.4  0.0       0.0    59     1921   20 10 47

20 12 16  J1513        15 25 30  32.9 357.2  0.2       0.0   -31     1921   No stop 
20 15 46  ---          15 29 01  32.9 356.3  0.2       0.0   179     1948   20 12 17

20 16 16  J1522+3144   15 29 31  32.4 358.4  0.1       0.0    -1     1948   20 16 16
20 17 41  =1520+319    15 30 56  32.4 358.0  0.1       0.0    84     1959   20 16 17
Schedule for HART      (Code Hh )                                   Page   8
               mas structure of transient radio emission from mid-IR burst galaxies
  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  11 Jun 2020   Day 163 ---

20 17 41  J1513        15 30 56  32.9 355.8  0.3       0.0   -31     1959   No stop 
20 21 11  ---          15 34 27  32.8 354.9  0.3       0.0   179     1986   20 17 42

20 21 11  J1522+3144   15 34 27  32.4 357.1  0.2       0.0   -31     1986   No stop 
20 22 41  =1520+319    15 35 57  32.4 356.7  0.2       0.0    59     1998   20 21 12

20 22 41  J1513        15 35 57  32.8 354.6  0.4       0.0   -31     1998   No stop 
20 26 11  ---          15 39 28  32.7 353.7  0.4       0.0   179     2025   20 22 42

20 26 41  J1522+3144   15 39 58  32.3 355.7  0.3       0.0    -1     2025   20 26 41
20 28 06  =1520+319    15 41 23  32.3 355.4  0.3       0.0    84     2036   20 26 42

20 28 06  J1513        15 41 23  32.6 353.2  0.4       0.0   -31     2036   No stop 
20 31 36  ---          15 44 54  32.5 352.3  0.5       0.0   179     2063   20 28 07

20 31 36  J1522+3144   15 44 54  32.2 354.5  0.4       0.0   -31     2063   No stop 
20 33 06  =1520+319    15 46 24  32.2 354.1  0.4       0.0    59     2075   20 31 37

21 46 50  J1522+3144   17 00 20  27.9 336.6  1.6       0.0  4401     2075   21 46 50
21 48 20  =1520+319    17 02 01  27.8 336.2  1.7       0.0    90     2086   21 46 51

21 48 20  J1513        17 01 51  27.5 334.2  1.8       0.0   -31     2086   No stop 
21 51 50  ---          17 05 21  27.2 333.4  1.8       0.0   179     2113   21 48 21

21 52 20  J1522+3144   17 05 51  27.4 335.4  1.7       0.0    -1     2113   21 52 20
21 53 45  =1520+319    17 07 17  27.3 335.1  1.7       0.0    84     2124   21 52 21

21 53 45  J1513        17 07 17  27.0 333.0  1.9       0.0   -31     2124   No stop 
21 57 15  ---          17 10 47  26.6 332.3  1.9       0.0   179     2151   21 53 46

21 57 15  J1522+3144   17 10 47  27.0 334.4  1.8       0.0   -31     2151   No stop 
21 58 45  =1520+319    17 12 17  26.8 334.0  1.8       0.0    59     2163   21 57 16

21 58 45  J1513        17 12 17  26.4 332.0  2.0       0.0   -31     2163   No stop 
22 02 15  ---          17 15 48  26.1 331.3  2.0       0.0   179     2190   21 58 46

22 02 45  J1522+3144   17 16 18  26.4 333.2  1.9       0.0    -1     2190   22 02 45
22 04 10  =1520+319    17 17 43  26.3 332.9  1.9       0.0    84     2201   22 02 46

22 04 10  J1513        17 17 43  25.9 330.9  2.1       0.0   -31     2201   No stop 
22 07 40  ---          17 21 14  25.5 330.2  2.1       0.0   179     2228   22 04 11

22 07 40  J1522+3144   17 21 14  25.9 332.2  2.0       0.0   -31     2228   No stop 
22 09 10  =1520+319    17 22 44  25.7 331.9  2.0       0.0    59     2240   22 07 41
Schedule for HART      (Code Hh )                                   Page   9
               mas structure of transient radio emission from mid-IR burst galaxies
  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  11 Jun 2020   Day 163 ---

22 09 10  J1513        17 22 44  25.3 329.9  2.1       0.0   -31     2240   No stop 
22 12 40  ---          17 26 15  24.9 329.2  2.2       0.0   179     2267   22 09 11

22 13 10  J1522+3144   17 26 45  25.3 331.1  2.1       0.0    -1     2267   22 13 10
22 14 35  =1520+319    17 28 10  25.2 330.8  2.1       0.0    84     2278   22 13 11

22 14 35  J1513        17 28 10  24.7 328.8  2.2       0.0   -31     2278   No stop 
22 18 05  ---          17 31 41  24.3 328.1  2.3       0.0   179     2305   22 14 36

22 18 05  J1522+3144   17 31 41  24.8 330.1  2.1       0.0   -31     2305   No stop 
22 19 35  =1520+319    17 33 11  24.6 329.8  2.2       0.0    59     2316   22 18 06

22 19 35  J1513        17 33 11  24.1 327.8  2.3       0.0   -31     2316   No stop 
22 23 05  ---          17 36 41  23.7 327.1  2.4       0.0   179     2343   22 19 36

22 23 35  J1522+3144   17 37 11  24.1 329.0  2.2       0.0    -1     2343   22 23 35
22 25 00  =1520+319    17 38 37  24.0 328.7  2.3       0.0    84     2354   22 23 36

22 25 00  J1513        17 38 37  23.4 326.7  2.4       0.0   -31     2354   No stop 
22 28 30  ---          17 42 07  23.0 326.1  2.5       0.0   179     2381   22 25 01

22 28 30  J1522+3144   17 42 07  23.6 328.0  2.3       0.0   -31     2381   No stop 
22 30 00  =1520+319    17 43 38  23.4 327.7  2.3       0.0    59     2393   22 28 31


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


 ======== Setup file: sess220.L1024
   Matching groups in /home/guest/rmc/SCHED/sched11.5/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:    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:  16  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:  16

   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)

 * J1513             15 11 42.234794   * 15 13 45.762470     15 14 36.707870       0.00
                     31 22 33.09499    * 31 11 25.09053      31 07 03.20182        0.00
                     From catalog imbedded in main SCHED input file.

 * J1241             12 39 12.040924   * 12 41 34.263460     12 42 31.865153       0.00
                     44 43 05.52128    * 44 26 39.16972      44 20 15.52751        0.00
                     From catalog imbedded in main SCHED input file.

   1252+458          12 52 10.870115   * 12 54 28.828713     12 55 24.839449       0.27
 * J1254+4536        45 52 19.18369    * 45 36 04.32738      45 29 45.46916        0.27
                     /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution,    118 observations.

 * 3C286             13 28 49.657769   * 13 31 08.288061     13 32 04.748742       0.17
   J1331+3030        30 45 58.64066    * 30 30 32.95930      30 24 29.58706        0.16
   1328+307          /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc
   J1331+30          GSFC 2016a X/S astro solution,    269 observations.

   1520+319          15 20 08.107588   * 15 22 09.991731     15 23 00.316817       0.01
 * J1522+3144        31 54 54.51271    * 31 44 14.38197      31 40 03.50858        0.01
   J1522+31          /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution,   7763 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
  J1513      sess220.L1024         1 2 3 4 5 6 7 8 9 10 13 14  +     1.983   203.173
  J1241      sess220.L1024         1 2 3 4 5 6 7 8 9 10 13 14  +     2.800   260.014
  J1254+4536 sess220.L1024         1 2 3 4 5 6 7 8 9 10 13 14  +     1.285   103.006
  3C286      sess220.L1024         1 2 3 4 5 6 7 8 9 10 13 14  +     0.150    17.962
  J1522+3144 sess220.L1024         1 2 3 4 5 6 7 8 9 10 13 14  +     0.926    92.184


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) 
   J1513              117.7
   J1241               87.2
   J1254+4536          88.6
   3C286              103.1
   J1522+3144         118.2

  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 

