  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: Accurate Localization of FAST FRB 190520 and its Host
 Exp. Code:  RZ001C  


Schedule Version:       1.00
Processed by SCHED version:  11.50  Development version 11.5. Started Apr. 2

PI:       Chenhui Niu

Address:  National Astronomical Observatories, CAS
          20A Datun Road, Chaoyang District
          100012, Beijing
          China

Phone:    86 010 64888708
EMAIL:    peterniu@@nao.cas.cn
Fax:
Phone during observation:

Observing mode:

Notes:    SCHED key file contact person: Bo Zhang
          Email: zb@shao.ac.cn
          PLEASE TURN OFF CONTINUOUS-CAL AND AUTOMATIC GAIN CONTROL SYSTEMS
          AS WELL AS PHASE-CAL TONES

Schedule for HART      (Code Hh )                                   Page   2
               Accurate Localization of FAST FRB 190520 and its Host
  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
----------------------------------------------------------------------------------------

 --- Mon   6 Jul 2020   Day 188 ---

 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

18 30 00  1600+335     15 21 32  29.9  10.0 -0.7       0.0     0        0   18 30 00
18 32 00  ---          15 23 32  30.0   9.5 -0.7       0.0   120       15   18 30 01

18 35 25  J1605-1139   15 26 58  73.0  35.1 -0.7       0.0    88       15   18 35 25
18 36 45  ---          15 28 18  73.2  34.1 -0.6       0.0    80       26   18 35 26

18 36 45  FRB190520    15 28 18  73.3  31.1 -0.6       0.0   -27       26   No stop 
18 41 45  ---          15 33 19  73.8  27.2 -0.5       0.0   273       64   18 36 46

18 41 45  J1605-1139   15 33 19  73.8  30.4 -0.6       0.0   -27       64   No stop 
18 43 15  ---          15 34 49  74.0  29.2 -0.5       0.0    63       76   18 41 46

18 43 55  FRB190520    15 35 29  74.1  25.5 -0.5       0.0    13       76   18 43 55
18 48 55  ---          15 40 30  74.5  21.2 -0.4       0.0   300      115   18 43 56

18 48 55  J1605-1139   15 40 30  74.6  24.5 -0.4       0.0   -27      115   No stop 
18 50 25  ---          15 42 00  74.7  23.2 -0.4       0.0    63      126   18 48 56

18 51 05  FRB190520    15 42 40  74.7  19.3 -0.3       0.0    13      126   18 51 05
18 56 05  ---          15 47 41  75.0  14.8 -0.3       0.0   300      165   18 51 06

18 56 05  J1605-1139   15 47 41  75.1  18.2 -0.3       0.0   -27      165   No stop 
18 57 35  ---          15 49 11  75.3  16.8 -0.3       0.0    63      176   18 56 06

18 58 15  FRB190520    15 49 52  75.1  12.8 -0.2       0.0    13      176   18 58 15
19 03 15  ---          15 54 52  75.3   8.0 -0.1       0.0   300      215   18 58 16

19 03 15  J1605-1139   15 54 52  75.6  11.4 -0.2       0.0   -27      215   No stop 
19 04 45  ---          15 56 23  75.6  10.0 -0.2       0.0    63      227   19 03 16

19 05 25  FRB190520    15 57 03  75.4   5.9 -0.1       0.0    13      227   19 05 25
19 10 25  ---          16 02 04  75.5   1.1 -0.0       0.0   300      265   19 05 26

19 10 25  J1605-1139   16 02 04  75.8   4.4 -0.1       0.0   -27      265   No stop 
19 11 55  ---          16 03 34  75.8   2.9 -0.0       0.0    63      277   19 10 26

19 12 35  FRB190520    16 04 14  75.5 359.0  0.0       0.0    13      277   19 12 35
19 17 35  ---          16 09 15  75.4 354.1  0.1       0.0   300      316   19 12 36
Schedule for HART      (Code Hh )                                   Page   3
               Accurate Localization of FAST FRB 190520 and its Host
  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
----------------------------------------------------------------------------------------

 --- Mon   6 Jul 2020   Day 188 ---

19 17 35  J1605-1139   16 09 15  75.8 357.2  0.0       0.0   -27      316   No stop 
19 19 05  ---          16 10 45  75.8 355.7  0.1       0.0    63      327   19 17 36

19 19 45  FRB190520    16 11 25  75.3 352.0  0.1       0.0    13      327   19 19 45
19 24 45  ---          16 16 26  75.1 347.2  0.2       0.0   300      366   19 19 46

19 24 45  J1605-1139   16 16 26  75.6 350.1  0.2       0.0   -27      366   No stop 
19 26 15  ---          16 17 56  75.6 348.6  0.2       0.0    63      377   19 24 46

19 26 55  FRB190520    16 18 36  75.0 345.2  0.3       0.0    13      377   19 26 55
19 31 55  ---          16 23 37  74.7 340.7  0.3       0.0   300      416   19 26 56

19 31 55  J1605-1139   16 23 37  75.3 343.2  0.3       0.0   -27      416   No stop 
19 33 25  ---          16 25 07  75.2 341.9  0.3       0.0    63      428   19 31 56

19 34 05  FRB190520    16 25 47  74.5 338.8  0.4       0.0    13      428   19 34 05
19 39 05  ---          16 30 48  74.1 334.6  0.5       0.0   300      466   19 34 06

19 39 05  J1605-1139   16 30 48  74.7 336.8  0.4       0.0   -27      466   No stop 
19 40 35  ---          16 32 19  74.6 335.5  0.4       0.0    63      478   19 39 06

19 44 09  1611+343     16 35 53  29.7 354.9  0.4       0.0    95      478   19 44 09
19 46 09  ---          16 38 04  29.7 354.4  0.4       0.0   120      493   19 44 10

19 49 44  J1605-1139   16 41 29  73.6 328.1  0.6       0.0    96      493   19 49 44
19 51 04  ---          16 42 49  73.4 327.1  0.6       0.0    80      504   19 49 45

19 51 04  FRB190520    16 42 49  72.7 325.4  0.7       0.0   -27      504   No stop 
19 56 04  ---          16 47 50  72.0 322.0  0.7       0.0   273      542   19 51 05

19 56 04  J1605-1139   16 47 50  72.8 323.5  0.7       0.0   -27      542   No stop 
19 57 34  ---          16 49 21  72.6 322.5  0.7       0.0    63      554   19 56 05

19 58 14  FRB190520    16 50 01  71.7 320.6  0.8       0.0    13      554   19 58 14
20 03 14  ---          16 55 01  71.0 317.5  0.9       0.0   300      593   19 58 15

20 03 14  J1605-1139   16 55 01  71.8 318.8  0.8       0.0   -27      593   No stop 
20 04 37  ---          16 56 25  71.6 317.9  0.8       0.0    56      603   20 03 15

20 05 17  FRB190520    16 57 05  70.7 316.3  0.9       0.0    13      603   20 05 17
20 10 17  ---          17 02 06  69.9 313.5  1.0       0.0   300      642   20 05 18

20 10 17  J1605-1139   17 02 06  70.7 314.6  0.9       0.0   -27      642   No stop 
20 11 40  ---          17 03 29  70.5 313.9  1.0       0.0    56      653   20 10 18
Schedule for HART      (Code Hh )                                   Page   4
               Accurate Localization of FAST FRB 190520 and its Host
  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
----------------------------------------------------------------------------------------

 --- Mon   6 Jul 2020   Day 188 ---

20 12 20  FRB190520    17 04 09  69.5 312.5  1.0       0.0    13      653   20 12 20
20 17 20  ---          17 09 10  68.7 310.0  1.1       0.0   300      691   20 12 21

20 17 20  J1605-1139   17 09 10  69.5 310.9  1.0       0.0   -27      691   No stop 
20 18 43  ---          17 10 33  69.3 310.2  1.1       0.0    56      702   20 17 21

20 19 23  FRB190520    17 11 13  68.3 309.0  1.1       0.0    13      702   20 19 23
20 24 23  ---          17 16 14  67.4 306.8  1.2       0.0   300      741   20 19 24

20 24 23  J1605-1139   17 16 14  68.3 307.5  1.2       0.0   -27      741   No stop 
20 25 46  ---          17 17 37  68.0 306.9  1.2       0.0    56      751   20 24 24

20 26 26  FRB190520    17 18 17  67.1 305.9  1.3       0.0    13      751   20 26 26
20 31 26  ---          17 23 18  66.1 303.8  1.3       0.0   300      790   20 26 27

20 31 26  J1605-1139   17 23 18  67.0 304.4  1.3       0.0   -27      790   No stop 
20 32 49  ---          17 24 41  66.7 303.9  1.3       0.0    56      801   20 31 27

20 33 29  FRB190520    17 25 21  65.8 303.0  1.4       0.0    13      801   20 33 29
20 38 29  ---          17 30 22  64.8 301.2  1.5       0.0   300      839   20 33 30

20 38 29  J1605-1139   17 30 22  65.7 301.7  1.4       0.0   -27      839   No stop 
20 39 52  ---          17 31 45  65.4 301.2  1.4       0.0    56      850   20 38 30

20 40 32  FRB190520    17 32 26  64.4 300.5  1.5       0.0    13      850   20 40 32
20 45 32  ---          17 37 26  63.4 298.8  1.6       0.0   300      889   20 40 33

20 45 32  J1605-1139   17 37 26  64.3 299.2  1.5       0.0   -27      889   No stop 
20 46 55  ---          17 38 50  64.0 298.7  1.5       0.0    56      899   20 45 33

20 47 35  FRB190520    17 39 30  63.0 298.1  1.6       0.0    13      899   20 47 35
20 52 35  ---          17 44 31  62.0 296.6  1.7       0.0   300      938   20 47 36

20 52 35  J1605-1139   17 44 31  62.9 296.9  1.6       0.0   -27      938   No stop 
20 53 58  ---          17 45 54  62.6 296.5  1.7       0.0    56      949   20 52 36

20 58 03  1641+399     17 49 59  22.5 346.3  1.1       0.0   115      949   20 58 03
21 00 03  ---          17 52 09  22.4 345.8  1.1       0.0   120      964   20 58 04


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:    5         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:   6  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:   6

   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)

 * 1600+335          16 00 11.909370   * 16 02 07.263500     16 02 54.990892       0.00
                     33 35 09.59231    * 33 26 53.07200      33 23 44.07618        0.00
                     From catalog imbedded in main SCHED input file.

 * 1611+343          16 11 47.914209   * 16 13 41.064200     16 14 27.967672       0.00
                     34 20 19.83398    * 34 12 47.90900      34 09 56.65579        0.00
                     From catalog imbedded in main SCHED input file.

 * 1641+399          16 41 17.606263   * 16 42 58.810000     16 43 41.119332       0.00
                     39 54 10.81494    * 39 48 36.99400      39 46 32.90244        0.00
                     From catalog imbedded in main SCHED input file.

 * J1605-1139        16 02 31.767616   * 16 05 17.531700     16 06 25.518843       0.00
                    -11 31 20.63016    *-11 39 26.83100     -11 42 40.64765        0.00
                     From catalog imbedded in main SCHED input file.

 * FRB190520         15 59 16.359238   * 16 02 01.640000     16 03 09.417979       0.00
                    -11 09 09.88153    *-11 17 28.50000     -11 20 47.31866        0.00
                     From catalog imbedded in main SCHED input file.



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
  1600+335   sess220.L1024         1 2 3 4 5 6 7 8                   0.033     2.200
  1611+343   sess220.L1024         1 2 3 4 5 6 7 8                   0.033     2.200
  1641+399   sess220.L1024         1 2 3 4 5 6 7 8                   0.033     2.200
  J1605-1139 sess220.L1024         1 2 3 4 5 6 7 8                   0.479    23.721
  FRB190520  sess220.L1024         1 2 3 4 5 6 7 8                   1.500    90.956


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) 
   1600+335           109.1
   1611+343           110.1
   1641+399           109.4
   J1605-1139         135.9
   FRB190520          135.1

  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 

