  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: Characterizing OCRs in dwarf galaxies
 Exp. Code:  ev026g  


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 ILTJ231715.38+184339.0 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
----------------------------------------------------------------------------------------

 --- Wed  29 May 2024   Day 150 ---

 ---------- 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

02 08 10  J2253+1608   20 27 19  34.6  44.5 -2.5       0.0     0        0   02 08 10
02 12 20  =3C454.3     20 31 30  35.2  43.6 -2.4       0.0   250       32   02 08 11

 ---------- Going to ILTJ2317 ----------

02 13 20  J2320+1829   20 32 30  29.4  47.1 -2.8       0.0    20       32   02 13 20
02 15 20  =2318+182    20 34 30  29.7  46.7 -2.8       0.0   120       48   02 13 21

02 15 20  ILTJ2317     20 34 30  30.1  45.8 -2.7       0.0   -27       48   No stop 
02 20 20  ---          20 39 31  30.9  44.8 -2.6       0.0   273       86   02 15 21

02 20 50  J2320+1829   20 40 01  30.6  45.6 -2.7       0.0     3       86   02 20 50
02 22 10  =2318+182    20 41 21  30.8  45.4 -2.7       0.0    80       97   02 20 51

02 22 10  ILTJ2317     20 41 21  31.2  44.5 -2.6       0.0   -27       97   No stop 
02 27 10  ---          20 46 22  32.0  43.4 -2.5       0.0   273      135   02 22 11

02 27 40  J2320+1829   20 46 52  31.7  44.2 -2.6       0.0     3      135   02 27 40
02 29 00  =2318+182    20 48 12  31.9  43.9 -2.6       0.0    80      146   02 27 41

02 29 00  ILTJ2317     20 48 12  32.3  43.0 -2.5       0.0   -27      146   No stop 
02 34 00  ---          20 53 13  33.0  41.9 -2.4       0.0   273      184   02 29 01

02 34 30  J2320+1829   20 53 43  32.7  42.8 -2.5       0.0     3      184   02 34 30
02 35 50  =2318+182    20 55 03  32.9  42.5 -2.4       0.0    80      195   02 34 31

02 35 50  J2236+2828   20 55 03  30.2  26.1 -1.7       0.0   -50      195   No stop 
02 39 20  =2234+282    20 58 34  30.6  25.3 -1.6       0.0   160      222   02 35 51

02 40 30  J2320+1829   20 59 44  33.6  41.5 -2.4       0.0    21      222   02 40 30
02 41 50  =2318+182    21 01 04  33.8  41.2 -2.3       0.0    80      232   02 40 31

02 41 50  ILTJ2317     21 01 04  34.2  40.2 -2.3       0.0   -27      232   No stop 
02 46 50  ---          21 06 05  34.9  39.0 -2.2       0.0   273      271   02 41 51

02 47 20  J2320+1829   21 06 35  34.7  39.9 -2.3       0.0     3      271   02 47 20
02 48 40  =2318+182    21 07 56  34.8  39.6 -2.2       0.0    80      281   02 47 21

02 48 40  ILTJ2317     21 07 56  35.2  38.6 -2.2       0.0   -27      281   No stop 
02 53 40  ---          21 12 56  35.9  37.4 -2.1       0.0   273      319   02 48 41
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
----------------------------------------------------------------------------------------

 --- Wed  29 May 2024   Day 150 ---

02 54 10  J2320+1829   21 13 26  35.6  38.3 -2.1       0.0     3      319   02 54 10
02 55 30  =2318+182    21 14 47  35.8  38.0 -2.1       0.0    80      330   02 54 11

02 55 30  ILTJ2317     21 14 47  36.1  37.0 -2.1       0.0   -27      330   No stop 
03 00 30  ---          21 19 48  36.8  35.8 -2.0       0.0   273      368   02 55 31

03 01 00  J2320+1829   21 20 18  36.6  36.7 -2.0       0.0     3      368   03 01 00
03 02 20  =2318+182    21 21 38  36.7  36.4 -2.0       0.0    80      379   03 01 01

03 02 20  ILTJ2317     21 21 38  37.0  35.3 -1.9       0.0   -27      379   No stop 
03 07 20  ---          21 26 39  37.7  34.1 -1.9       0.0   273      417   03 02 21

03 07 50  J2320+1829   21 27 09  37.5  35.0 -1.9       0.0     3      417   03 07 50
03 09 10  =2318+182    21 28 29  37.6  34.7 -1.9       0.0    80      428   03 07 51

03 09 10  J2236+2828   21 28 29  33.0  18.1 -1.2       0.0   -50      428   No stop 
03 12 40  =2234+282    21 32 00  33.3  17.2 -1.1       0.0   160      455   03 09 11

03 13 50  J2320+1829   21 33 10  38.2  33.5 -1.8       0.0    21      455   03 13 50
03 15 10  =2318+182    21 34 30  38.4  33.1 -1.8       0.0    80      465   03 13 51

03 15 10  ILTJ2317     21 34 30  38.6  32.1 -1.7       0.0   -27      465   No stop 
03 20 10  ---          21 39 31  39.2  30.7 -1.6       0.0   273      504   03 15 11

03 20 40  J2320+1829   21 40 01  39.1  31.7 -1.7       0.0     3      504   03 20 40
03 22 00  =2318+182    21 41 21  39.2  31.3 -1.7       0.0    80      514   03 20 41

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

03 23 00  J2253+1608   21 42 21  44.3  24.8 -1.2       0.0    19      514   03 23 00
03 27 00  =3C454.3     21 46 22  44.6  23.5 -1.1       0.0   240      545   03 23 01

 ---------- Going to ILTJ2317 ----------

03 28 00  J2320+1829   21 47 22  39.9  29.7 -1.6       0.0    20      545   03 28 00
03 30 00  =2318+182    21 49 22  40.1  29.2 -1.5       0.0   120      560   03 28 01

03 30 00  ILTJ2317     21 49 22  40.3  28.0 -1.5       0.0   -27      560   No stop 
03 35 00  ---          21 54 23  40.8  26.6 -1.4       0.0   273      599   03 30 01

03 35 30  J2320+1829   21 54 53  40.7  27.6 -1.5       0.0     3      599   03 35 30
03 36 50  =2318+182    21 56 13  40.9  27.3 -1.4       0.0    80      609   03 35 31

03 36 50  ILTJ2317     21 56 13  41.0  26.1 -1.4       0.0   -27      609   No stop 
03 41 50  ---          22 01 14  41.5  24.7 -1.3       0.0   273      648   03 36 51
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
----------------------------------------------------------------------------------------

 --- Wed  29 May 2024   Day 150 ---

03 42 20  J2320+1829   22 01 44  41.4  25.7 -1.3       0.0     3      648   03 42 20
03 43 40  =2318+182    22 03 05  41.5  25.3 -1.3       0.0    80      658   03 42 21

03 43 40  ILTJ2317     22 03 05  41.6  24.1 -1.3       0.0   -27      658   No stop 
03 48 40  ---          22 08 05  42.1  22.7 -1.2       0.0   273      697   03 43 41

03 49 10  J2320+1829   22 08 36  42.0  23.7 -1.2       0.0     3      697   03 49 10
03 50 30  =2318+182    22 09 56  42.2  23.3 -1.2       0.0    80      707   03 49 11

03 50 30  J2236+2828   22 09 56  35.1   7.4 -0.5       0.0   -50      707   No stop 
03 54 00  =2234+282    22 13 26  35.2   6.5 -0.4       0.0   160      734   03 50 31

03 55 10  J2320+1829   22 14 37  42.6  21.9 -1.1       0.0    21      734   03 55 10
03 56 30  =2318+182    22 15 57  42.7  21.5 -1.1       0.0    80      745   03 55 11

03 56 30  ILTJ2317     22 15 57  42.7  20.3 -1.0       0.0   -27      745   No stop 
04 01 30  ---          22 20 58  43.1  18.8 -1.0       0.0   273      783   03 56 31

04 02 00  J2320+1829   22 21 28  43.1  19.8 -1.0       0.0     3      783   04 02 00
04 03 20  =2318+182    22 22 48  43.2  19.4 -1.0       0.0    80      794   04 02 01

04 03 20  ILTJ2317     22 22 48  43.3  18.2 -0.9       0.0   -27      794   No stop 
04 08 20  ---          22 27 49  43.6  16.6 -0.8       0.0   273      832   04 03 21

04 08 50  J2320+1829   22 28 19  43.6  17.7 -0.9       0.0     3      832   04 08 50
04 10 10  =2318+182    22 29 39  43.7  17.3 -0.9       0.0    80      842   04 08 51

04 10 10  ILTJ2317     22 29 39  43.7  16.1 -0.8       0.0   -27      842   No stop 
04 15 10  ---          22 34 40  44.0  14.5 -0.7       0.0   273      881   04 10 11

04 15 40  J2320+1829   22 35 10  44.1  15.5 -0.8       0.0     3      881   04 15 40
04 17 00  =2318+182    22 36 30  44.1  15.1 -0.8       0.0    80      891   04 15 41

04 17 00  ILTJ2317     22 36 30  44.1  13.9 -0.7       0.0   -27      891   No stop 
04 22 00  ---          22 41 31  44.4  12.3 -0.6       0.0   273      930   04 17 01

04 22 30  J2320+1829   22 42 01  44.4  13.3 -0.7       0.0     3      930   04 22 30
04 23 50  =2318+182    22 43 21  44.5  12.9 -0.6       0.0    80      940   04 22 31

04 23 50  J2236+2828   22 43 21  35.5 358.4  0.1       0.0   -50      940   No stop 
04 27 20  =2234+282    22 46 52  35.5 357.5  0.2       0.0   160      967   04 23 51

04 28 30  J2320+1829   22 48 02  44.7  11.4 -0.6       0.0    21      967   04 28 30
04 29 50  =2318+182    22 49 22  44.8  10.9 -0.5       0.0    80      978   04 28 31
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
----------------------------------------------------------------------------------------

 --- Wed  29 May 2024   Day 150 ---

04 29 50  ILTJ2317     22 49 22  44.7   9.7 -0.5       0.0   -27      978   No stop 
04 34 50  ---          22 54 23  44.9   8.0 -0.4       0.0   273     1016   04 29 51

04 35 20  J2320+1829   22 54 53  45.0   9.1 -0.5       0.0     3     1016   04 35 20
04 36 40  =2318+182    22 56 13  45.1   8.7 -0.4       0.0    80     1027   04 35 21

04 36 40  ILTJ2317     22 56 13  44.9   7.4 -0.4       0.0   -27     1027   No stop 
04 41 40  ---          23 01 14  45.1   5.8 -0.3       0.0   273     1065   04 36 41

04 42 10  J2320+1829   23 01 44  45.2   6.8 -0.3       0.0     3     1065   04 42 10
04 43 30  =2318+182    23 03 04  45.3   6.4 -0.3       0.0    80     1076   04 42 11

04 43 30  ILTJ2317     23 03 04  45.1   5.2 -0.3       0.0   -27     1076   No stop 
04 48 30  ---          23 08 05  45.2   3.5 -0.2       0.0   273     1114   04 43 31

04 49 00  J2320+1829   23 08 35  45.4   4.5 -0.2       0.0     3     1114   04 49 00
04 50 20  =2318+182    23 09 56  45.4   4.1 -0.2       0.0    80     1125   04 49 01

04 50 20  ILTJ2317     23 09 56  45.2   2.9 -0.1       0.0   -27     1125   No stop 
04 55 20  ---          23 14 56  45.2   1.2 -0.1       0.0   273     1163   04 50 21

04 55 50  J2320+1829   23 15 26  45.5   2.2 -0.1       0.0     3     1163   04 55 50
04 57 10  =2318+182    23 16 47  45.5   1.8 -0.1       0.0    80     1174   04 55 51

04 57 10  J2236+2828   23 16 47  34.7 349.5  0.7       0.0   -50     1174   No stop 
05 00 40  =2234+282    23 20 17  34.5 348.6  0.7       0.0   160     1201   04 57 11

05 01 50  J2320+1829   23 21 27  45.5   0.2 -0.0       0.0    21     1201   05 01 50
05 03 10  =2318+182    23 22 48  45.5 359.7  0.0       0.0    80     1211   05 01 51

05 03 10  ILTJ2317     23 22 48  45.2 358.5  0.1       0.0   -27     1211   No stop 
05 08 10  ---          23 27 49  45.2 356.9  0.2       0.0   273     1250   05 03 11

05 08 40  J2320+1829   23 28 19  45.5 357.9  0.1       0.0     3     1250   05 08 40
05 10 00  =2318+182    23 29 39  45.5 357.4  0.1       0.0    80     1260   05 08 41

05 10 00  ILTJ2317     23 29 39  45.2 356.2  0.2       0.0   -27     1260   No stop 
05 15 00  ---          23 34 40  45.1 354.6  0.3       0.0   273     1298   05 10 01

05 15 30  J2320+1829   23 35 10  45.4 355.6  0.2       0.0     3     1298   05 15 30
05 16 50  =2318+182    23 36 30  45.3 355.1  0.2       0.0    80     1309   05 15 31

05 16 50  ILTJ2317     23 36 30  45.0 354.0  0.3       0.0   -27     1309   No stop 
05 21 50  ---          23 41 31  44.9 352.3  0.4       0.0   273     1347   05 16 51
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
----------------------------------------------------------------------------------------

 --- Wed  29 May 2024   Day 150 ---

05 22 20  J2320+1829   23 42 01  45.2 353.3  0.3       0.0     3     1347   05 22 20
05 23 40  =2318+182    23 43 21  45.2 352.8  0.4       0.0    80     1358   05 22 21

05 23 40  ILTJ2317     23 43 21  44.8 351.7  0.4       0.0   -27     1358   No stop 
05 28 40  ---          23 48 22  44.7 350.0  0.5       0.0   273     1396   05 23 41

05 29 10  J2320+1829   23 48 52  45.0 351.0  0.4       0.0     3     1396   05 29 10
05 30 30  =2318+182    23 50 12  45.0 350.5  0.5       0.0    80     1407   05 29 11

05 30 30  J2236+2828   23 50 12  32.8 341.0  1.2       0.0   -50     1407   No stop 
05 34 00  =2234+282    23 53 43  32.5 340.1  1.3       0.0   160     1434   05 30 31

05 35 10  J2320+1829   23 54 53  44.8 349.0  0.5       0.0    21     1434   05 35 10
05 36 30  =2318+182    23 56 13  44.7 348.6  0.6       0.0    80     1444   05 35 11

05 36 30  ILTJ2317     23 56 13  44.3 347.5  0.6       0.0   -27     1444   No stop 
05 41 30  ---          00 01 14  44.1 345.9  0.7       0.0   273     1483   05 36 31

05 42 00  J2320+1829   00 01 44  44.5 346.8  0.7       0.0     3     1483   05 42 00
05 43 20  =2318+182    00 03 04  44.4 346.3  0.7       0.0    80     1493   05 42 01

05 43 20  ILTJ2317     00 03 04  44.0 345.3  0.7       0.0   -27     1493   No stop 
05 48 20  ---          00 08 05  43.7 343.7  0.8       0.0   273     1532   05 43 21

05 48 50  J2320+1829   00 08 35  44.1 344.6  0.8       0.0     3     1532   05 48 50
05 50 10  =2318+182    00 09 55  44.0 344.1  0.8       0.0    80     1542   05 48 51

05 50 10  ILTJ2317     00 09 55  43.5 343.1  0.9       0.0   -27     1542   No stop 
05 55 10  ---          00 14 56  43.2 341.5  0.9       0.0   273     1581   05 50 11

05 55 40  J2320+1829   00 15 26  43.6 342.4  0.9       0.0     3     1581   05 55 40
05 57 00  =2318+182    00 16 47  43.5 342.0  0.9       0.0    80     1591   05 55 41

05 57 00  ILTJ2317     00 16 47  43.1 341.0  1.0       0.0   -27     1591   No stop 
06 02 00  ---          00 21 47  42.7 339.4  1.1       0.0   273     1630   05 57 01

06 02 30  J2320+1829   00 22 17  43.1 340.3  1.0       0.0     3     1630   06 02 30
06 03 50  =2318+182    00 23 38  43.0 339.8  1.0       0.0    80     1640   06 02 31

06 03 50  J2236+2828   00 23 38  29.8 333.1  1.8       0.0   -50     1640   No stop 
06 07 20  =2234+282    00 27 08  29.5 332.3  1.8       0.0   160     1667   06 03 51

06 08 30  J2320+1829   00 28 18  42.7 338.4  1.1       0.0    21     1667   06 08 30
06 09 50  =2318+182    00 29 39  42.6 338.0  1.1       0.0    80     1677   06 08 31
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
----------------------------------------------------------------------------------------

 --- Wed  29 May 2024   Day 150 ---

06 09 50  ILTJ2317     00 29 39  42.0 337.1  1.2       0.0   -27     1677   No stop 
06 14 50  ---          00 34 39  41.6 335.6  1.3       0.0   273     1716   06 09 51

06 15 20  J2320+1829   00 35 10  42.1 336.4  1.2       0.0     3     1716   06 15 20
06 16 40  =2318+182    00 36 30  41.9 336.0  1.2       0.0    80     1726   06 15 21

06 16 40  ILTJ2317     00 36 30  41.4 335.1  1.3       0.0   -27     1726   No stop 
06 21 40  ---          00 41 31  40.9 333.6  1.4       0.0   273     1765   06 16 41

06 22 10  J2320+1829   00 42 01  41.4 334.4  1.3       0.0     3     1765   06 22 10
06 23 30  =2318+182    00 43 21  41.3 334.0  1.4       0.0    80     1775   06 22 11

06 23 30  ILTJ2317     00 43 21  40.7 333.1  1.4       0.0   -27     1775   No stop 
06 28 30  ---          00 48 22  40.2 331.7  1.5       0.0   273     1814   06 23 31

06 29 00  J2320+1829   00 48 52  40.7 332.4  1.4       0.0     3     1814   06 29 00
06 30 20  =2318+182    00 50 12  40.6 332.1  1.5       0.0    80     1824   06 29 01

06 30 20  ILTJ2317     00 50 12  40.0 331.2  1.5       0.0   -27     1824   No stop 
06 35 20  ---          00 55 13  39.5 329.9  1.6       0.0   273     1863   06 30 21

06 35 50  J2320+1829   00 55 43  40.0 330.5  1.6       0.0     3     1863   06 35 50
06 37 10  =2318+182    00 57 03  39.9 330.2  1.6       0.0    80     1873   06 35 51

06 37 10  J2236+2828   00 57 03  26.0 326.0  2.3       0.0   -50     1873   No stop 
06 40 40  =2234+282    01 00 34  25.6 325.3  2.4       0.0   160     1900   06 37 11

06 41 50  J2320+1829   01 01 44  39.3 328.9  1.7       0.0    21     1900   06 41 50
06 43 10  =2318+182    01 03 04  39.2 328.6  1.7       0.0    80     1910   06 41 51

06 43 10  ILTJ2317     01 03 04  38.5 327.8  1.7       0.0   -27     1910   No stop 
06 48 10  ---          01 08 05  37.9 326.5  1.8       0.0   273     1949   06 43 11

06 48 40  J2320+1829   01 08 35  38.5 327.1  1.8       0.0     3     1949   06 48 40
06 50 00  =2318+182    01 09 55  38.3 326.8  1.8       0.0    80     1959   06 48 41

06 50 00  ILTJ2317     01 09 55  37.7 326.0  1.9       0.0   -27     1959   No stop 
06 53 20  ---          01 13 16  37.3 325.2  1.9       0.0   173     1985   06 50 01

06 54 00  J2320+1829   01 13 56  37.8 325.7  1.9       0.0    13     1985   06 54 00
06 55 00  =2318+182    01 14 56  37.7 325.5  1.9       0.0    60     1993   06 54 01
Schedule for HART      (Code Hh )                                   Page   8
               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
----------------------------------------------------------------------------------------

 --- Wed  29 May 2024   Day 150 ---

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

06 56 00  J2253+1608   01 15 56  35.7 317.1  2.3       0.0    19     1993   06 56 00
07 00 00  =3C454.3     01 19 57  35.1 316.2  2.4       0.0   240     2024   06 56 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:  13  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:  13

   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)

 * ILTJ2317          23 14 45.892345   * 23 17 15.380000     23 18 27.698821       0.00
                     18 27 15.44487    * 18 43 39.10000      18 51 27.48916        0.00
                     From catalog imbedded in main SCHED input file.

 * B2319+60_D        23 19 41.329180   * 23 21 55.200000     23 22 59.103077       0.00
                     60 08 03.45038    * 60 24 30.70000      60 32 11.63925        0.00
                     From catalog imbedded in main SCHED input file.

   2234+282          22 34 01.728802   * 22 36 22.470847     22 37 30.696616       0.34
 * J2236+2828        28 13 23.21045    * 28 28 57.41317      28 36 17.90081        0.31
   J2236+28          /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution,  91001 observations.

   3C454.3           22 51 29.519739   * 22 53 57.747939     22 55 09.602203       0.65
 * J2253+1608        15 52 54.34808    * 16 08 53.56091      16 16 30.32517        0.73
   2251+158          /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc
   J2253+16          GSFC 2016a X/S astro solution,  41272 observations.

   2318+182          23 18 16.895310   * 23 20 46.775967     23 21 59.268461       0.13
 * J2320+1829        18 12 59.29947    * 18 29 25.77527      18 37 15.69772        0.18
                     /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution,    136 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
  ILTJ2317   sess224.L1024         1 2 3 4 5 6 7 8 13 14             2.722   230.361
  B2319+60_D sess224.L1024         1 2 3 4 5 6 7 8                   0.075     4.831
  J2236+2828 sess224.L1024         1 2 3 4 5 6 7 8 13                0.467    24.791
  J2253+1608 sess224.L1024         1 2 3 4 5 6 7 8 13 14             0.203    18.433
  J2320+1829 sess224.L1024         1 2 3 4 5 6 7 8 13 14             0.972    82.780


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) 
   ILTJ2317            71.5
   B2319+60_D          64.3
   J2236+2828          77.5
   J2253+1608          77.5
   J2320+1829          70.7

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

