  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: Accurate Localization of FAST FRB 190520 and its Host
 Exp. Code:  RZ001A  


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
          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
----------------------------------------------------------------------------------------

 --- Sun  14 Jun 2020   Day 166 ---

 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

20 00 00  1600+335     15 25 02  30.0   9.1 -0.6       0.0     0        0   20 00 00
20 02 00  ---          15 27 03  30.1   8.7 -0.6       0.0   120       15   20 00 01

20 05 25  J1605-1139   15 30 28  73.5  32.5 -0.6       0.0    88       15   20 05 25
20 06 45  ---          15 31 49  73.6  31.5 -0.6       0.0    80       26   20 05 26

20 06 45  FRB190520    15 31 49  73.7  28.4 -0.5       0.0   -27       26   No stop 
20 11 45  ---          15 36 49  74.2  24.4 -0.4       0.0   273       64   20 06 46

20 11 45  J1605-1139   15 36 49  74.2  27.6 -0.5       0.0   -27       64   No stop 
20 13 15  ---          15 38 20  74.3  26.4 -0.5       0.0    63       76   20 11 46

20 13 55  FRB190520    15 39 00  74.4  22.5 -0.4       0.0    13       76   20 13 55
20 18 55  ---          15 44 01  74.8  18.1 -0.3       0.0   300      115   20 13 56

20 18 55  J1605-1139   15 44 01  74.9  21.5 -0.4       0.0   -27      115   No stop 
20 20 25  ---          15 45 31  75.0  20.1 -0.3       0.0    63      126   20 18 56

20 21 05  FRB190520    15 46 11  74.9  16.2 -0.3       0.0    13      126   20 21 05
20 26 05  ---          15 51 12  75.2  11.5 -0.2       0.0   300      165   20 21 06

20 26 05  J1605-1139   15 51 12  75.4  14.9 -0.3       0.0   -27      165   No stop 
20 27 35  ---          15 52 42  75.5  13.5 -0.2       0.0    63      176   20 26 06

20 28 15  FRB190520    15 53 22  75.3   9.5 -0.2       0.0    13      176   20 28 15
20 33 15  ---          15 58 23  75.4   4.7 -0.1       0.0   300      215   20 28 16

20 33 15  J1605-1139   15 58 23  75.7   8.0 -0.1       0.0   -27      215   No stop 
20 34 45  ---          15 59 53  75.7   6.5 -0.1       0.0    63      227   20 33 16

20 35 25  FRB190520    16 00 33  75.4   2.5 -0.0       0.0    13      227   20 35 25
20 40 25  ---          16 05 34  75.4 357.6  0.0       0.0   300      265   20 35 26

20 40 25  J1605-1139   16 05 34  75.8   0.9 -0.0       0.0   -27      265   No stop 
20 41 55  ---          16 07 04  75.8 359.4  0.0       0.0    63      277   20 40 26

20 42 35  FRB190520    16 07 44  75.4 355.5  0.1       0.0    13      277   20 42 35
20 47 35  ---          16 12 45  75.3 350.7  0.2       0.0   300      316   20 42 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
----------------------------------------------------------------------------------------

 --- Sun  14 Jun 2020   Day 166 ---

20 47 35  J1605-1139   16 12 45  75.7 353.7  0.1       0.0   -27      316   No stop 
20 49 05  ---          16 14 16  75.7 352.2  0.1       0.0    63      327   20 47 36

20 49 45  FRB190520    16 14 56  75.2 348.6  0.2       0.0    13      327   20 49 45
20 54 45  ---          16 19 56  74.9 344.0  0.3       0.0   300      366   20 49 46

20 54 45  J1605-1139   16 19 56  75.5 346.7  0.2       0.0   -27      366   No stop 
20 56 15  ---          16 21 27  75.4 345.3  0.3       0.0    63      377   20 54 46

20 56 55  FRB190520    16 22 07  74.8 342.0  0.3       0.0    13      377   20 56 55
21 01 55  ---          16 27 08  74.4 337.6  0.4       0.0   300      416   20 56 56

21 01 55  J1605-1139   16 27 08  75.0 340.0  0.3       0.0   -27      416   No stop 
21 03 25  ---          16 28 38  74.9 338.7  0.4       0.0    63      428   21 01 56

21 04 05  FRB190520    16 29 18  74.2 335.8  0.4       0.0    13      428   21 04 05
21 09 05  ---          16 34 19  73.7 331.7  0.5       0.0   300      466   21 04 06

21 09 05  J1605-1139   16 34 19  74.4 333.8  0.5       0.0   -27      466   No stop 
21 10 35  ---          16 35 49  74.2 332.6  0.5       0.0    63      478   21 09 06

21 14 10  1611+343     16 39 25  29.7 354.1  0.4       0.0    96      478   21 14 10
21 16 10  ---          16 41 35  29.6 353.6  0.5       0.0   120      493   21 14 11

21 19 45  J1605-1139   16 45 01  73.2 325.5  0.6       0.0    96      493   21 19 45
21 21 05  ---          16 46 21  73.0 324.6  0.7       0.0    80      504   21 19 46

21 21 05  FRB190520    16 46 21  72.2 323.0  0.7       0.0   -27      504   No stop 
21 26 05  ---          16 51 22  71.5 319.7  0.8       0.0   273      542   21 21 06

21 26 05  J1605-1139   16 51 22  72.3 321.1  0.7       0.0   -27      542   No stop 
21 27 35  ---          16 52 52  72.1 320.2  0.8       0.0    63      554   21 26 06

21 28 15  FRB190520    16 53 32  71.2 318.4  0.8       0.0    13      554   21 28 15
21 33 15  ---          16 58 33  70.4 315.5  0.9       0.0   300      593   21 28 16

21 33 15  J1605-1139   16 58 33  71.2 316.7  0.9       0.0   -27      593   No stop 
21 34 45  ---          17 00 03  71.0 315.8  0.9       0.0    63      604   21 33 16

21 35 25  FRB190520    17 00 43  70.1 314.3  1.0       0.0    13      604   21 35 25
21 40 25  ---          17 05 44  69.3 311.7  1.0       0.0   300      643   21 35 26

21 40 25  J1605-1139   17 05 44  70.1 312.6  1.0       0.0   -27      643   No stop 
21 41 55  ---          17 07 14  69.8 311.8  1.0       0.0    63      654   21 40 26
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
----------------------------------------------------------------------------------------

 --- Sun  14 Jun 2020   Day 166 ---

21 42 35  FRB190520    17 07 54  68.9 310.6  1.1       0.0    13      654   21 42 35
21 47 35  ---          17 12 55  68.0 308.2  1.2       0.0   300      693   21 42 36

21 47 35  J1605-1139   17 12 55  68.9 309.0  1.1       0.0   -27      693   No stop 
21 49 05  ---          17 14 25  68.6 308.3  1.1       0.0    63      705   21 47 36

21 49 45  FRB190520    17 15 06  67.6 307.3  1.2       0.0    13      705   21 49 45
21 54 45  ---          17 20 06  66.7 305.1  1.3       0.0   300      743   21 49 46

21 54 45  J1605-1139   17 20 06  67.6 305.8  1.2       0.0   -27      743   No stop 
21 56 15  ---          17 21 37  67.3 305.1  1.3       0.0    63      755   21 54 46

21 56 55  FRB190520    17 22 17  66.3 304.2  1.3       0.0    13      755   21 56 55
22 01 55  ---          17 27 18  65.4 302.3  1.4       0.0   300      794   21 56 56

22 01 55  J1605-1139   17 27 18  66.2 302.9  1.3       0.0   -27      794   No stop 
22 03 25  ---          17 28 48  66.0 302.3  1.4       0.0    63      805   22 01 56

22 04 05  FRB190520    17 29 28  65.0 301.5  1.4       0.0    13      805   22 04 05
22 09 05  ---          17 34 29  64.0 299.8  1.5       0.0   300      844   22 04 06

22 09 05  J1605-1139   17 34 29  64.9 300.2  1.5       0.0   -27      844   No stop 
22 10 35  ---          17 35 59  64.6 299.7  1.5       0.0    63      855   22 09 06

22 11 15  FRB190520    17 36 39  63.6 299.0  1.6       0.0    13      855   22 11 15
22 16 15  ---          17 41 40  62.6 297.4  1.6       0.0   300      894   22 11 16

22 16 15  J1605-1139   17 41 40  63.5 297.8  1.6       0.0   -27      894   No stop 
22 17 45  ---          17 43 10  63.2 297.3  1.6       0.0    63      906   22 16 16

22 18 25  FRB190520    17 43 50  62.2 296.8  1.7       0.0    13      906   22 18 25
22 23 25  ---          17 48 51  61.1 295.3  1.8       0.0   300      944   22 18 26

22 23 25  J1605-1139   17 48 51  62.0 295.6  1.7       0.0   -27      944   No stop 
22 24 55  ---          17 50 21  61.7 295.2  1.7       0.0    63      956   22 23 26

22 29 01  1641+399     17 54 28  22.3 345.4  1.2       0.0   116      956   22 29 01
22 31 01  ---          17 56 38  22.2 344.9  1.2       0.0   120      971   22 29 02


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:    7         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 55.105237       0.00
                     33 35 09.59231    * 33 26 53.07200      33 23 39.41806        0.00
                     From catalog imbedded in main SCHED input file.

 * 1611+343          16 11 47.914209   * 16 13 41.064200     16 14 28.065333       0.00
                     34 20 19.83398    * 34 12 47.90900      34 09 51.77979        0.00
                     From catalog imbedded in main SCHED input file.

 * 1641+399          16 41 17.606263   * 16 42 58.810000     16 43 41.192334       0.00
                     39 54 10.81494    * 39 48 36.99400      39 46 27.29361        0.00
                     From catalog imbedded in main SCHED input file.

 * J1605-1139        16 02 31.767616   * 16 05 17.531700     16 06 25.500829       0.00
                    -11 31 20.63016    *-11 39 26.83100     -11 42 41.49265        0.00
                     From catalog imbedded in main SCHED input file.

 * FRB190520         15 59 16.359238   * 16 02 01.640000     16 03 09.405926       0.00
                    -11 09 09.88153    *-11 17 28.50000     -11 20 48.19364        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 9 10                0.033     1.500
  1611+343   sess220.L1024         1 2 3 4 5 6 7 9 10                0.033     1.500
  1641+399   sess220.L1024         1 2 3 4 5 6 7 9 10                0.033     1.500
  J1605-1139 sess220.L1024         1 2 3 4 5 6 7 9 10                0.494    16.408
  FRB190520  sess220.L1024         1 2 3 4 5 6 7 9 10                1.500    61.006


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           119.2
   1611+343           119.4
   1641+399           115.8
   J1605-1139         156.0
   FRB190520          155.1

  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 

