  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: Accurate Localization of FAST FRB 190520 and its Host
 Exp. Code:  RZ001B  


Schedule Version:       2.00
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, zb@shao.ac.cn
          PLEASE TURN OFF CONTINUOUS-CAL AND AUTOMATIC GAIN CONTROL SYSTEMS
          AS WELL AS PHASE-CAL TONES
          v2 with out-stations

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  22 Jun 2020   Day 174 ---

 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

19 30 00  1600+335     15 26 30  30.1   8.8 -0.6       0.0     0        0   19 30 00
19 32 00  ---          15 28 30  30.2   8.3 -0.6       0.0   120       15   19 30 01

19 35 25  J1605-1139   15 31 56  73.7  31.4 -0.6       0.0    88       15   19 35 25
19 36 45  ---          15 33 16  73.8  30.4 -0.6       0.0    80       26   19 35 26

19 36 45  FRB190520    15 33 16  73.8  27.3 -0.5       0.0   -27       26   No stop 
19 41 45  ---          15 38 17  74.3  23.1 -0.4       0.0   273       64   19 36 46

19 41 45  J1605-1139   15 38 17  74.3  26.4 -0.5       0.0   -27       64   No stop 
19 43 15  ---          15 39 47  74.5  25.1 -0.4       0.0    63       76   19 41 46

19 43 55  FRB190520    15 40 27  74.5  21.3 -0.4       0.0    13       76   19 43 55
19 48 55  ---          15 45 28  74.9  16.8 -0.3       0.0   300      115   19 43 56

19 48 55  J1605-1139   15 45 28  75.0  20.2 -0.3       0.0   -27      115   No stop 
19 50 25  ---          15 46 58  75.1  18.8 -0.3       0.0    63      126   19 48 56

19 51 05  FRB190520    15 47 38  75.0  14.9 -0.3       0.0    13      126   19 51 05
19 56 05  ---          15 52 39  75.2  10.2 -0.2       0.0   300      165   19 51 06

19 56 05  J1605-1139   15 52 39  75.5  13.5 -0.2       0.0   -27      165   No stop 
19 57 35  ---          15 54 10  75.5  12.1 -0.2       0.0    63      176   19 56 06

19 58 15  FRB190520    15 54 50  75.3   8.1 -0.1       0.0    13      176   19 58 15
20 03 15  ---          15 59 50  75.4   3.2 -0.1       0.0   300      215   19 58 16

20 03 15  J1605-1139   15 59 50  75.7   6.6 -0.1       0.0   -27      215   No stop 
20 04 45  ---          16 01 21  75.8   5.1 -0.1       0.0    63      227   20 03 16

20 05 25  FRB190520    16 02 01  75.5   1.1 -0.0       0.0    13      227   20 05 25
20 10 25  ---          16 07 02  75.4 356.2  0.1       0.0   300      265   20 05 26

20 10 25  J1605-1139   16 07 02  75.8 359.4  0.0       0.0   -27      265   No stop 
20 11 55  ---          16 08 32  75.8 357.9  0.0       0.0    63      277   20 10 26

20 12 35  FRB190520    16 09 12  75.4 354.1  0.1       0.0    13      277   20 12 35
20 17 35  ---          16 14 13  75.2 349.3  0.2       0.0   300      316   20 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  22 Jun 2020   Day 174 ---

20 17 35  J1605-1139   16 14 13  75.7 352.3  0.1       0.0   -27      316   No stop 
20 19 05  ---          16 15 43  75.7 350.8  0.2       0.0    63      327   20 17 36

20 19 45  FRB190520    16 16 23  75.1 347.3  0.2       0.0    13      327   20 19 45
20 24 45  ---          16 21 24  74.8 342.7  0.3       0.0   300      366   20 19 46

20 24 45  J1605-1139   16 21 24  75.4 345.3  0.2       0.0   -27      366   No stop 
20 26 15  ---          16 22 54  75.3 343.9  0.3       0.0    63      377   20 24 46

20 26 55  FRB190520    16 23 34  74.7 340.7  0.3       0.0    13      377   20 26 55
20 31 55  ---          16 28 35  74.3 336.4  0.4       0.0   300      416   20 26 56

20 31 55  J1605-1139   16 28 35  74.9 338.7  0.4       0.0   -27      416   No stop 
20 33 25  ---          16 30 05  74.8 337.4  0.4       0.0    63      428   20 31 56

20 34 05  FRB190520    16 30 46  74.1 334.6  0.5       0.0    13      428   20 34 05
20 39 05  ---          16 35 46  73.5 330.6  0.5       0.0   300      466   20 34 06

20 39 05  J1605-1139   16 35 46  74.2 332.6  0.5       0.0   -27      466   No stop 
20 40 35  ---          16 37 17  74.1 331.4  0.5       0.0    63      478   20 39 06

20 44 10  1611+343     16 40 53  29.6 353.7  0.4       0.0    97      478   20 44 10
20 46 10  ---          16 43 03  29.6 353.2  0.5       0.0   120      493   20 44 11

20 49 45  J1605-1139   16 46 28  73.0 324.5  0.7       0.0    96      493   20 49 45
20 51 05  ---          16 47 49  72.8 323.5  0.7       0.0    80      504   20 49 46

20 51 05  FRB190520    16 47 49  72.0 322.0  0.7       0.0   -27      504   No stop 
20 56 05  ---          16 52 50  71.3 318.8  0.8       0.0   273      542   20 51 06

20 56 05  J1605-1139   16 52 50  72.1 320.2  0.8       0.0   -27      542   No stop 
20 57 35  ---          16 54 20  71.9 319.2  0.8       0.0    63      554   20 56 06

20 58 15  FRB190520    16 55 00  71.0 317.5  0.9       0.0    13      554   20 58 15
21 03 15  ---          17 00 01  70.2 314.7  0.9       0.0   300      593   20 58 16

21 03 15  J1605-1139   17 00 01  71.0 315.8  0.9       0.0   -27      593   No stop 
21 04 38  ---          17 01 24  70.8 315.0  0.9       0.0    56      603   21 03 16

21 05 18  FRB190520    17 02 04  69.9 313.6  1.0       0.0    13      603   21 05 18
21 10 18  ---          17 07 05  69.0 311.0  1.1       0.0   300      642   21 05 19

21 10 18  J1605-1139   17 07 05  69.9 311.9  1.0       0.0   -27      642   No stop 
21 11 41  ---          17 08 28  69.6 311.2  1.0       0.0    56      653   21 10 19
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  22 Jun 2020   Day 174 ---

21 12 21  FRB190520    17 09 08  68.7 310.0  1.1       0.0    13      653   21 12 21
21 17 21  ---          17 14 09  67.8 307.7  1.2       0.0   300      691   21 12 22

21 17 21  J1605-1139   17 14 09  68.6 308.4  1.1       0.0   -27      691   No stop 
21 18 44  ---          17 15 32  68.4 307.8  1.2       0.0    56      702   21 17 22

21 19 24  FRB190520    17 16 12  67.4 306.8  1.2       0.0    13      702   21 19 24
21 24 24  ---          17 21 13  66.5 304.7  1.3       0.0   300      741   21 19 25

21 24 24  J1605-1139   17 21 13  67.4 305.3  1.2       0.0   -27      741   No stop 
21 25 47  ---          17 22 36  67.1 304.7  1.3       0.0    56      751   21 24 25

21 26 27  FRB190520    17 23 17  66.2 303.8  1.3       0.0    13      751   21 26 27
21 31 27  ---          17 28 17  65.2 301.9  1.4       0.0   300      790   21 26 28

21 31 27  J1605-1139   17 28 17  66.1 302.5  1.4       0.0   -27      790   No stop 
21 32 50  ---          17 29 41  65.8 302.0  1.4       0.0    56      801   21 31 28

21 33 30  FRB190520    17 30 21  64.8 301.2  1.5       0.0    13      801   21 33 30
21 38 30  ---          17 35 21  63.8 299.5  1.5       0.0   300      839   21 33 31

21 38 30  J1605-1139   17 35 21  64.7 299.9  1.5       0.0   -27      839   No stop 
21 39 53  ---          17 36 45  64.4 299.4  1.5       0.0    56      850   21 38 31

21 40 33  FRB190520    17 37 25  63.4 298.8  1.6       0.0    13      850   21 40 33
21 45 33  ---          17 42 26  62.4 297.2  1.7       0.0   300      889   21 40 34

21 45 33  J1605-1139   17 42 26  63.3 297.6  1.6       0.0   -27      889   No stop 
21 46 56  ---          17 43 49  63.0 297.1  1.6       0.0    56      899   21 45 34

21 47 36  FRB190520    17 44 29  62.0 296.6  1.7       0.0    13      899   21 47 36
21 52 36  ---          17 49 30  61.0 295.1  1.8       0.0   300      938   21 47 37

21 52 36  J1605-1139   17 49 30  61.9 295.4  1.7       0.0   -27      938   No stop 
21 53 59  ---          17 50 53  61.6 295.0  1.7       0.0    56      949   21 52 37

21 58 05  1641+399     17 54 59  22.3 345.3  1.2       0.0   116      949   21 58 05
22 00 05  ---          17 57 10  22.1 344.8  1.2       0.0   120      964   21 58 06


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 55.082054       0.00
                     33 35 09.59231    * 33 26 53.07200      33 23 41.36848        0.00
                     From catalog imbedded in main SCHED input file.

 * 1611+343          16 11 47.914209   * 16 13 41.064200     16 14 28.049355       0.00
                     34 20 19.83398    * 34 12 47.90900      34 09 53.80790        0.00
                     From catalog imbedded in main SCHED input file.

 * 1641+399          16 41 17.606263   * 16 42 58.810000     16 43 41.188996       0.00
                     39 54 10.81494    * 39 48 36.99400      39 46 29.58639        0.00
                     From catalog imbedded in main SCHED input file.

 * J1605-1139        16 02 31.767616   * 16 05 17.531700     16 06 25.527812       0.00
                    -11 31 20.63016    *-11 39 26.83100     -11 42 41.06438        0.00
                     From catalog imbedded in main SCHED input file.

 * FRB190520         15 59 16.359238   * 16 02 01.640000     16 03 09.430530       0.00
                    -11 09 09.88153    *-11 17 28.50000     -11 20 47.75530        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    23.505
  FRB190520  sess220.L1024         1 2 3 4 5 6 7 8                   1.500    90.093


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           115.8
   1611+343           116.4
   1641+399           113.8
   J1605-1139         148.8
   FRB190520          147.9

  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 

