  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: Characterizing OCRs in dwarf galaxies
 Exp. Code:  ev026f  


Schedule Version:       2.00
Processed by SCHED version:  11.60  Release 11.6; April 2020

PI:       Dany Vohl

Address:  Anton Pannekoek Institute for Astronomy, University of Amsterdam
          1098 XH Amsterdam
          Amsterdam
          The Netherlands

Phone:    +31 6 1887 9982
EMAIL:    d.vohl@uva.nl
Fax:
Phone during observation: +31 6 1887 9982

Observing mode: vlbi

Notes:    # Please, make sure PHASE CAL is OFF #
 
 
 


COVER LETTER:


This observation is to observe ILT J121407.57+423829.2 first
identified in the LoTSS DR2 data as potential analogue to
persistent radio sources associated to some fast radio bursts.
With the observation, we wish to constrain it s source size,
and evalute if the radio emission is due to star formation
processes or not.

Schedule for HART      (Code Hh )                                   Page   2
               Characterizing OCRs in dwarf 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
----------------------------------------------------------------------------------------

 --- Tue  28 May 2024   Day 149 ---

 ---------- Fringe-finder ----------

 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

14 00 00  J1159+2914   08 17 09  13.2  48.0 -3.7       0.0     0        0   14 00 00
14 02 00  =1156+295    08 19 10  13.5  47.7 -3.7       0.0   120       15   14 00 01

14 02 10  J1159+2914   08 19 20  13.5  47.7 -3.7       0.0   -11       15   14 02 10
14 06 10  =1156+295    08 23 20  14.2  47.1 -3.6       0.0   229       46   14 02 11

 ---------- test pulsar ----------

14 07 10  B1237+25_D   08 24 20  10.0  56.1 -4.3       0.0    13       46   14 07 10
14 10 10  ---          08 27 21  10.5  55.7 -4.2       0.0   180       70   14 07 11

14 34 40  J1214+3309   08 51 55  13.8  42.0 -3.4       0.0  1426       70   14 34 40
14 37 40  =1211+334    08 54 55  14.2  41.6 -3.3       0.0   180       93   14 34 41

14 38 20  J1209+4119   08 55 36   9.1  35.0 -3.3       0.0    -3       93   14 38 20
14 39 40  =1206+416    08 56 56   9.3  34.8 -3.2       0.0    77      103   14 38 21

14 45 20  J1209+4119   09 02 37  10.0  34.0 -3.1       0.0   319      103   14 45 20
14 46 40  =1206+416    09 03 57  10.2  33.8 -3.1       0.0    80      113   14 45 21

14 52 20  J1209+4119   09 09 38  10.9  33.0 -3.0       0.0   319      113   14 52 20
14 53 40  =1206+416    09 10 58  11.1  32.8 -3.0       0.0    80      124   14 52 21

14 53 40  ILTJ1214     09 10 58   9.5  32.6 -3.1       0.0   -29      124   No stop 
14 58 40  ---          09 15 59  10.1  31.9 -3.0       0.0   271      162   14 53 41

14 59 20  J1209+4119   09 16 39  11.7  31.9 -2.9       0.0    11      162   14 59 20
15 00 40  =1206+416    09 17 59  11.9  31.7 -2.9       0.0    80      173   14 59 21

15 00 40  ILTJ1214     09 17 59  10.3  31.6 -3.0       0.0   -29      173   No stop 
15 05 40  ---          09 23 00  10.9  30.9 -2.9       0.0   271      211   15 00 41

15 06 20  J1209+4119   09 23 40  12.6  30.9 -2.8       0.0    11      211   15 06 20
15 07 40  =1206+416    09 25 00  12.7  30.7 -2.8       0.0    80      222   15 06 21

15 07 40  J1214+3309   09 25 00  18.5  36.7 -2.8       0.0   -43      222   No stop 
15 10 40  =1211+334    09 28 01  18.9  36.2 -2.8       0.0   137      245   15 07 41

15 11 20  J1209+4119   09 28 41  13.1  30.1 -2.7       0.0    -3      245   15 11 20
15 12 40  =1206+416    09 30 01  13.3  29.9 -2.7       0.0    77      255   15 11 21
Schedule for HART      (Code Hh )                                   Page   3
               Characterizing OCRs in dwarf 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
----------------------------------------------------------------------------------------

 --- Tue  28 May 2024   Day 149 ---

15 12 40  ILTJ1214     09 30 01  11.7  29.8 -2.8       0.0   -29      255   No stop 
15 17 40  ---          09 35 02  12.3  29.1 -2.7       0.0   271      294   15 12 41

15 18 20  J1209+4119   09 35 42  13.9  29.0 -2.6       0.0    11      294   15 18 20
15 19 40  =1206+416    09 37 02  14.1  28.8 -2.6       0.0    80      304   15 18 21

 ---------- Fringe-finder ----------

15 21 00  J1159+2914   09 38 23  25.3  34.2 -2.4       0.0    29      304   15 21 00
15 26 00  =1156+295    09 43 23  25.9  33.2 -2.3       0.0   300      343   15 21 01

 ---------- Going to ILTJ1214 ----------

15 27 20  J1209+4119   09 44 44  14.9  27.6 -2.4       0.0    29      343   15 27 20
15 28 50  =1206+416    09 46 14  15.0  27.3 -2.4       0.0    90      354   15 27 21

15 28 50  ILTJ1214     09 46 14  13.5  27.3 -2.5       0.0   -29      354   No stop 
15 33 50  ---          09 51 15  14.0  26.5 -2.4       0.0   271      393   15 28 51

15 34 30  J1209+4119   09 51 55  15.6  26.4 -2.3       0.0    11      393   15 34 30
15 35 50  =1206+416    09 53 15  15.7  26.2 -2.3       0.0    80      403   15 34 31

15 35 50  ILTJ1214     09 53 15  14.2  26.2 -2.4       0.0   -29      403   No stop 
15 40 50  ---          09 58 16  14.7  25.4 -2.3       0.0   271      442   15 35 51

15 41 30  J1209+4119   09 58 56  16.3  25.2 -2.2       0.0    11      442   15 41 30
15 42 50  =1206+416    10 00 16  16.4  25.0 -2.2       0.0    80      452   15 41 31

15 42 50  ILTJ1214     10 00 16  14.8  25.1 -2.3       0.0   -29      452   No stop 
15 47 50  ---          10 05 17  15.3  24.3 -2.2       0.0   271      491   15 42 51

15 48 30  J1209+4119   10 05 57  17.0  24.0 -2.1       0.0    11      491   15 48 30
15 49 50  =1206+416    10 07 17  17.1  23.8 -2.1       0.0    80      501   15 48 31

15 49 50  J1214+3309   10 07 17  23.7  29.0 -2.1       0.0   -43      501   No stop 
15 52 50  =1211+334    10 10 18  24.0  28.4 -2.1       0.0   137      524   15 49 51

15 53 30  J1209+4119   10 10 58  17.4  23.2 -2.0       0.0    -3      524   15 53 30
15 54 50  =1206+416    10 12 18  17.5  22.9 -2.0       0.0    77      535   15 53 31

15 54 50  ILTJ1214     10 12 18  16.0  23.1 -2.1       0.0   -29      535   No stop 
15 59 50  ---          10 17 19  16.4  22.2 -2.0       0.0   271      573   15 54 51

16 00 30  J1209+4119   10 17 59  18.0  21.9 -1.9       0.0    11      573   16 00 30
16 01 50  =1206+416    10 19 19  18.1  21.7 -1.9       0.0    80      584   16 00 31
Schedule for HART      (Code Hh )                                   Page   4
               Characterizing OCRs in dwarf 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
----------------------------------------------------------------------------------------

 --- Tue  28 May 2024   Day 149 ---

16 01 50  ILTJ1214     10 19 19  16.6  21.9 -1.9       0.0   -29      584   No stop 
16 06 50  ---          10 24 20  17.0  21.0 -1.9       0.0   271      622   16 01 51

16 07 30  J1209+4119   10 25 00  18.6  20.7 -1.8       0.0    11      622   16 07 30
16 08 50  =1206+416    10 26 20  18.7  20.4 -1.7       0.0    80      633   16 07 31

16 08 50  ILTJ1214     10 26 20  17.1  20.7 -1.8       0.0   -29      633   No stop 
16 13 50  ---          10 31 21  17.5  19.8 -1.7       0.0   271      671   16 08 51

16 14 30  J1209+4119   10 32 01  19.1  19.4 -1.6       0.0    11      671   16 14 30
16 15 50  =1206+416    10 33 22  19.2  19.2 -1.6       0.0    80      681   16 14 31

16 15 50  ILTJ1214     10 33 22  17.7  19.5 -1.7       0.0   -29      681   No stop 
16 20 50  ---          10 38 22  18.0  18.6 -1.6       0.0   271      720   16 15 51

16 21 30  J1209+4119   10 39 03  19.6  18.1 -1.5       0.0    11      720   16 21 30
16 22 50  =1206+416    10 40 23  19.7  17.9 -1.5       0.0    80      730   16 21 31

16 22 50  J1214+3309   10 40 23  26.9  22.2 -1.6       0.0   -43      730   No stop 
16 25 50  =1211+334    10 43 23  27.2  21.6 -1.5       0.0   137      754   16 22 51

16 26 30  J1209+4119   10 44 03  20.0  17.2 -1.4       0.0    -3      754   16 26 30
16 27 50  =1206+416    10 45 24  20.1  16.9 -1.4       0.0    77      764   16 26 31

16 27 50  ILTJ1214     10 45 24  18.5  17.3 -1.5       0.0   -29      764   No stop 
16 32 50  ---          10 50 24  18.9  16.4 -1.4       0.0   271      803   16 27 51

16 33 30  J1209+4119   10 51 05  20.4  15.9 -1.3       0.0    11      803   16 33 30
16 34 50  =1206+416    10 52 25  20.5  15.6 -1.3       0.0    80      813   16 33 31

16 34 50  ILTJ1214     10 52 25  19.0  16.0 -1.4       0.0   -29      813   No stop 
16 39 50  ---          10 57 26  19.3  15.1 -1.3       0.0   271      851   16 34 51

16 40 30  J1209+4119   10 58 06  20.8  14.5 -1.2       0.0    11      851   16 40 30
16 41 50  =1206+416    10 59 26  20.9  14.3 -1.2       0.0    80      862   16 40 31

16 41 50  ILTJ1214     10 59 26  19.4  14.7 -1.3       0.0   -29      862   No stop 
16 46 50  ---          11 04 27  19.7  13.8 -1.2       0.0   271      900   16 41 51

16 47 30  J1209+4119   11 05 07  21.2  13.2 -1.1       0.0    11      900   16 47 30
16 48 50  =1206+416    11 06 27  21.3  12.9 -1.1       0.0    80      911   16 47 31

16 48 50  ILTJ1214     11 06 27  19.8  13.4 -1.1       0.0   -29      911   No stop 
16 53 50  ---          11 11 28  20.0  12.5 -1.1       0.0   271      949   16 48 51
Schedule for HART      (Code Hh )                                   Page   5
               Characterizing OCRs in dwarf 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
----------------------------------------------------------------------------------------

 --- Tue  28 May 2024   Day 149 ---

16 54 30  J1209+4119   11 12 08  21.6  11.8 -1.0       0.0    11      949   16 54 30
16 55 50  =1206+416    11 13 28  21.6  11.5 -1.0       0.0    80      960   16 54 31

16 55 50  J1214+3309   11 13 28  29.3  14.8 -1.0       0.0   -43      960   No stop 
16 58 50  =1211+334    11 16 29  29.4  14.1 -1.0       0.0   137      983   16 55 51

16 59 30  J1209+4119   11 17 09  21.8  10.8 -0.9       0.0    -3      983   16 59 30
17 00 50  =1206+416    11 18 29  21.8  10.5 -0.9       0.0    77      993   16 59 31

17 00 50  ILTJ1214     11 18 29  20.4  11.1 -0.9       0.0   -29      993   No stop 
17 05 50  ---          11 23 30  20.6  10.2 -0.9       0.0   271     1032   17 00 51

17 06 30  J1209+4119   11 24 10  22.1   9.4 -0.8       0.0    11     1032   17 06 30
17 07 50  =1206+416    11 25 30  22.1   9.1 -0.8       0.0    80     1042   17 06 31

17 07 50  ILTJ1214     11 25 30  20.6   9.8 -0.8       0.0   -29     1042   No stop 
17 12 50  ---          11 30 31  20.8   8.8 -0.7       0.0   271     1081   17 07 51

17 13 30  J1209+4119   11 31 11  22.3   8.0 -0.7       0.0    11     1081   17 13 30
17 14 50  =1206+416    11 32 31  22.3   7.7 -0.6       0.0    80     1091   17 13 31

17 14 50  ILTJ1214     11 32 31  20.9   8.4 -0.7       0.0   -29     1091   No stop 
17 19 50  ---          11 37 32  21.0   7.5 -0.6       0.0   271     1130   17 14 51

17 20 30  J1209+4119   11 38 12  22.5   6.6 -0.5       0.0    11     1130   17 20 30
17 21 50  =1206+416    11 39 32  22.5   6.3 -0.5       0.0    80     1140   17 20 31

17 21 50  ILTJ1214     11 39 32  21.1   7.1 -0.6       0.0   -29     1140   No stop 
17 26 50  ---          11 44 33  21.2   6.1 -0.5       0.0   271     1179   17 21 51

17 27 30  J1209+4119   11 45 13  22.7   5.2 -0.4       0.0    11     1179   17 27 30
17 28 50  =1206+416    11 46 34  22.7   4.9 -0.4       0.0    80     1189   17 27 31

17 28 50  J1214+3309   11 46 34  30.7   7.0 -0.5       0.0   -43     1189   No stop 
17 31 50  =1211+334    11 49 34  30.8   6.3 -0.4       0.0   137     1212   17 28 51

17 32 30  J1209+4119   11 50 14  22.7   4.2 -0.3       0.0    -3     1212   17 32 30
17 33 50  =1206+416    11 51 34  22.8   3.9 -0.3       0.0    77     1222   17 32 31

17 33 50  ILTJ1214     11 51 34  21.4   4.7 -0.4       0.0   -29     1222   No stop 
17 38 50  ---          11 56 35  21.5   3.7 -0.3       0.0   271     1261   17 33 51

17 39 30  J1209+4119   11 57 15  22.8   2.7 -0.2       0.0    11     1261   17 39 30
17 40 50  =1206+416    11 58 36  22.9   2.5 -0.2       0.0    80     1271   17 39 31
Schedule for HART      (Code Hh )                                   Page   6
               Characterizing OCRs in dwarf 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
----------------------------------------------------------------------------------------

 --- Tue  28 May 2024   Day 149 ---

17 40 50  ILTJ1214     11 58 36  21.5   3.3 -0.3       0.0   -29     1271   No stop 
17 45 50  ---          12 03 36  21.5   2.3 -0.2       0.0   271     1310   17 40 51

17 46 30  J1209+4119   12 04 17  22.9   1.3 -0.1       0.0    11     1310   17 46 30
17 47 50  =1206+416    12 05 37  22.9   1.0 -0.1       0.0    80     1320   17 46 31

17 47 50  ILTJ1214     12 05 37  21.6   1.9 -0.2       0.0   -29     1320   No stop 
17 52 50  ---          12 10 38  21.6   0.9 -0.1       0.0   271     1359   17 47 51

17 53 30  J1209+4119   12 11 18  22.9 359.9  0.0       0.0    11     1359   17 53 30
17 54 50  =1206+416    12 12 38  22.9 359.6  0.0       0.0    80     1369   17 53 31

17 54 50  ILTJ1214     12 12 38  21.6   0.5 -0.0       0.0   -29     1369   No stop 
17 59 50  ---          12 17 39  21.6 359.5  0.0       0.0   271     1408   17 54 51

18 00 30  J1209+4119   12 18 19  22.9 358.4  0.1       0.0    11     1408   18 00 30
18 01 50  =1206+416    12 19 39  22.9 358.2  0.2       0.0    80     1418   18 00 31

18 01 50  J1214+3309   12 19 39  31.1 358.9  0.1       0.0   -43     1418   No stop 
18 04 50  =1211+334    12 22 40  31.1 358.2  0.1       0.0   137     1441   18 01 51

18 05 30  J1209+4119   12 23 20  22.9 357.4  0.2       0.0    -3     1441   18 05 30
18 06 50  =1206+416    12 24 40  22.8 357.1  0.2       0.0    77     1452   18 05 31

18 06 50  ILTJ1214     12 24 40  21.6 358.2  0.2       0.0   -29     1452   No stop 
18 11 50  ---          12 29 41  21.5 357.2  0.2       0.0   271     1490   18 06 51

18 12 30  J1209+4119   12 30 21  22.8 356.0  0.3       0.0    11     1490   18 12 30
18 13 50  =1206+416    12 31 41  22.7 355.7  0.4       0.0    80     1501   18 12 31

18 13 50  ILTJ1214     12 31 41  21.5 356.8  0.3       0.0   -29     1501   No stop 
18 18 50  ---          12 36 42  21.4 355.8  0.4       0.0   271     1539   18 13 51

18 19 30  J1209+4119   12 37 22  22.6 354.6  0.4       0.0    11     1539   18 19 30
18 20 50  =1206+416    12 38 42  22.6 354.3  0.5       0.0    80     1550   18 19 31

18 20 50  ILTJ1214     12 38 42  21.4 355.4  0.4       0.0   -29     1550   No stop 
18 25 50  ---          12 43 43  21.3 354.4  0.5       0.0   271     1588   18 20 51

18 26 30  J1209+4119   12 44 23  22.5 353.1  0.6       0.0    11     1588   18 26 30
18 27 50  =1206+416    12 45 43  22.4 352.9  0.6       0.0    80     1599   18 26 31

18 27 50  ILTJ1214     12 45 43  21.2 354.0  0.5       0.0   -29     1599   No stop 
18 32 50  ---          12 50 44  21.1 353.0  0.6       0.0   271     1637   18 27 51
Schedule for HART      (Code Hh )                                   Page   7
               Characterizing OCRs in dwarf 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
----------------------------------------------------------------------------------------

 --- Tue  28 May 2024   Day 149 ---

18 33 30  J1209+4119   12 51 24  22.3 351.7  0.7       0.0    11     1637   18 33 30
18 34 50  =1206+416    12 52 44  22.2 351.5  0.7       0.0    80     1648   18 33 31

18 34 50  J1214+3309   12 52 44  30.4 350.9  0.6       0.0   -43     1648   No stop 
18 37 50  =1211+334    12 55 45  30.3 350.2  0.7       0.0   137     1671   18 34 51

18 38 30  J1209+4119   12 56 25  22.1 350.7  0.8       0.0    -3     1671   18 38 30
18 39 50  =1206+416    12 57 45  22.0 350.5  0.8       0.0    77     1681   18 38 31

18 39 50  ILTJ1214     12 57 45  20.9 351.7  0.7       0.0   -29     1681   No stop 
18 44 50  ---          13 02 46  20.7 350.7  0.8       0.0   271     1720   18 39 51

18 45 30  J1209+4119   13 03 26  21.8 349.3  0.9       0.0    11     1720   18 45 30
18 46 50  =1206+416    13 04 46  21.7 349.1  0.9       0.0    80     1730   18 45 31

18 46 50  ILTJ1214     13 04 46  20.7 350.3  0.8       0.0   -29     1730   No stop 
18 51 50  ---          13 09 47  20.5 349.3  0.9       0.0   271     1769   18 46 51

18 52 30  J1209+4119   13 10 27  21.5 348.0  1.0       0.0    11     1769   18 52 30
18 53 50  =1206+416    13 11 48  21.4 347.7  1.0       0.0    80     1779   18 52 31

 ---------- Fringe-finder ----------

18 55 00  J1159+2914   13 12 58  32.3 341.3  1.2       0.0    19     1779   18 55 00
19 00 00  =1156+295    13 17 59  32.0 340.1  1.3       0.0   300     1818   18 55 01


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


 ======== Setup file: sess224.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:    5         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)

 * ILTJ1214          12 11 37.280056   * 12 14 07.570000     12 15 21.707455       0.00
                     42 55 09.49919    * 42 38 29.20000      42 30 32.22412        0.00
                     From catalog imbedded in main SCHED input file.

 * B1237+25_D        12 37 11.843793   * 12 39 40.400000     12 40 53.567676       0.00
                     25 10 17.10031    * 24 53 49.20000      24 45 52.16493        0.00
                     From catalog imbedded in main SCHED input file.

   1156+295          11 56 57.786211   * 11 59 31.833912     12 00 47.466951       0.00
 * J1159+2914        29 31 25.73880    * 29 14 43.82690      29 06 42.77135        0.00
   J1159+29          /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution,  78215 observations.

   1206+416          12 06 51.117947   * 12 09 22.788006     12 10 37.529148       0.17
 * J1209+4119        41 36 22.62761    * 41 19 41.37011      41 11 43.78026        0.16
                     /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution,    150 observations.

   1211+334          12 11 32.805725   * 12 14 04.115761     12 15 18.573025       0.10
 * J1214+3309        33 26 25.95140    * 33 09 45.59508      33 01 45.93285        0.13
                     /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution,    144 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
  ILTJ1214   sess224.L1024         1 2 3 4 5 6 7 8 9 10              2.750   220.837
  B1237+25_D sess224.L1024         1 3 4 5 6 7 8 9 10                0.050     3.877
  J1159+2914 sess224.L1024         1 2 3 4 5 6 7 8 9 10              0.267    23.537
  J1209+4119 sess224.L1024         1 2 3 4 5 6 7 8 9 10              0.961    77.882
  J1214+3309 sess224.L1024         1 2 3 4 5 6 7 8 9 10              0.400    24.710


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) 
   ILTJ1214            94.0
   B1237+25_D         108.7
   J1159+2914          98.8
   J1209+4119          94.1
   J1214+3309          99.3

  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 

