  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: AGN Cores
 Exp. Code:  EC070N  


Schedule Version:       5.00
Processed by SCHED version:  11.50  Development version 11.5. Started Apr. 2

PI:       E. Chiaraluce

Address:  INAF-IAPS
          via del Fosso del Cavaliere, 100
          00133 - Rome
          Italy

Phone:    +39 06 4548 8467
EMAIL:    elia.chiaraluce@inaf.it
Fax:      ---
Phone during observation: +39 06 4548 8467

Observing mode: Phase-referencing for sources at 6cm

Notes:    Targets: S52116+81, IGRJ21247+5058, SWIFTJ2127, RXJ2135.9+4728, MR2251-178, MCG-02-58-22
          Phase calibrators: J2133+8239,J2117+5431,J2117+5431, J2123+4614, J2303-1841, J2259-0811
          D-terms calibrator: --;  Fringe finder: 3C454.3, J0237+2848
          v5 incl. out-stations

Schedule for HART      (Code Hh )                                   Page   2
               AGN Cores
  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  17 Jun 2020   Day 169 ---

 Next scan frequencies:  4830.49  4830.49  4830.49  4830.49  4894.49  4894.49  4894.49  4894.49
                         4958.49  4958.49  4958.49  4958.49  5022.49  5022.49  5022.49  5022.49
 Next BBC frequencies:    230.49   230.49   230.49   230.49   294.49   294.49   294.49   294.49
                          358.49   358.49   358.49   358.49   422.49   422.49   422.49   422.49
 Next scan bandwidths:     32.00    32.00    32.00    32.00    32.00    32.00    32.00    32.00
                           32.00    32.00    32.00    32.00    32.00    32.00    32.00    32.00

23 56 53  3C454.3      19 34 24  25.6  54.8 -3.3       0.0     0        0   23 56 53
23 58 53  ---          19 36 24  25.9  54.4 -3.3       0.0   120       31   23 56 54

 --- Thu  18 Jun 2020   Day 170 ---

01 05 15  J2259-0811   20 42 58  52.9  67.5 -2.3       0.0  3907       31   01 05 15
01 06 15  =2256-084    20 43 58  53.1  67.3 -2.3       0.0    60       46   01 05 16

01 07 00 MCG-02-58-22  20 44 43  52.3  69.1 -2.4       0.0    16       46   01 07 00
01 12 00  ---          20 49 44  53.4  68.0 -2.3       0.0   300      124   01 07 01

01 12 45  J2259-0811   20 50 29  54.4  65.8 -2.2       0.0    16      124   01 12 45
01 13 45  =2256-084    20 51 29  54.6  65.5 -2.1       0.0    60      139   01 12 46

01 14 30 MCG-02-58-22  20 52 14  53.9  67.4 -2.2       0.0    16      139   01 14 30
01 19 30  ---          20 57 15  54.9  66.2 -2.1       0.0   300      216   01 14 31

01 20 15  J2259-0811   20 58 00  56.0  63.9 -2.0       0.0    16      216   01 20 15
01 21 15  =2256-084    20 59 00  56.2  63.7 -2.0       0.0    60      232   01 20 16

01 22 00 MCG-02-58-22  20 59 45  55.4  65.6 -2.1       0.0    16      232   01 22 00
01 27 00  ---          21 04 46  56.5  64.4 -2.0       0.0   300      309   01 22 01

01 27 45  J2259-0811   21 05 31  57.5  61.9 -1.9       0.0    16      309   01 27 45
01 28 45  =2256-084    21 06 32  57.7  61.6 -1.9       0.0    60      325   01 27 46

01 29 30 MCG-02-58-22  21 07 17  57.0  63.7 -2.0       0.0    16      325   01 29 30
01 34 30  ---          21 12 18  58.0  62.4 -1.9       0.0   300      402   01 29 31

01 35 15  J2259-0811   21 13 03  58.9  59.8 -1.8       0.0    16      402   01 35 15
01 36 15  =2256-084    21 14 03  59.1  59.5 -1.8       0.0    60      417   01 35 16

01 37 00 MCG-02-58-22  21 14 48  58.5  61.7 -1.8       0.0    16      417   01 37 00
01 42 00  ---          21 19 49  59.5  60.2 -1.8       0.0   300      495   01 37 01

01 42 45  J2259-0811   21 20 34  60.4  57.5 -1.7       0.0    16      495   01 42 45
01 43 45  =2256-084    21 21 34  60.6  57.1 -1.6       0.0    60      510   01 42 46
Schedule for HART      (Code Hh )                                   Page   3
               AGN Cores
  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
----------------------------------------------------------------------------------------

 --- Thu  18 Jun 2020   Day 170 ---

01 44 30 MCG-02-58-22  21 22 19  59.9  59.5 -1.7       0.0    16      510   01 44 30
01 49 30  ---          21 27 20  60.9  57.9 -1.6       0.0   300      587   01 44 31

01 50 15  J2259-0811   21 28 05  61.8  54.9 -1.5       0.0    16      587   01 50 15
01 51 15  =2256-084    21 29 05  62.0  54.6 -1.5       0.0    60      603   01 50 16

01 52 00 MCG-02-58-22  21 29 50  61.4  57.1 -1.6       0.0    16      603   01 52 00
01 57 00  ---          21 34 51  62.3  55.4 -1.5       0.0   300      680   01 52 01

01 59 02  3C454.3      21 36 53  43.8  26.4 -1.3       0.0    45      680   01 59 02
02 01 04  ---          21 38 56  44.0  25.8 -1.3       0.0   122      712   01 59 03

02 03 36  J2303-1841   21 41 28  69.6  73.3 -1.4       0.0    55      712   02 03 36
02 04 36  =2300-189    21 42 28  69.8  73.0 -1.4       0.0    60      727   02 03 37

02 05 14  MR2251-178   21 43 06  71.3  66.9 -1.2       0.0     7      727   02 05 14
02 10 03  ---          21 47 56  72.3  65.0 -1.1       0.0   289      802   02 05 15

02 10 48  J2303-1841   21 48 41  71.1  71.1 -1.3       0.0    14      802   02 10 48
02 11 48  =2300-189    21 49 41  71.3  70.8 -1.2       0.0    60      817   02 10 49

02 12 26  MR2251-178   21 50 20  72.8  64.0 -1.1       0.0     7      817   02 12 26
02 17 15  ---          21 55 09  73.7  61.8 -1.0       0.0   289      891   02 12 27

02 18 00  J2303-1841   21 55 54  72.6  68.6 -1.1       0.0    14      891   02 18 00
02 19 00  =2300-189    21 56 55  72.8  68.2 -1.1       0.0    60      907   02 18 01

02 19 38  MR2251-178   21 57 33  74.2  60.7 -1.0       0.0     7      907   02 19 38
02 24 27  ---          22 02 22  75.1  58.1 -0.9       0.0   289      981   02 19 39

02 25 12  J2303-1841   22 03 08  74.1  65.7 -1.0       0.0    14      981   02 25 12
02 26 12  =2300-189    22 04 08  74.3  65.2 -1.0       0.0    60      997   02 25 13

02 26 50  MR2251-178   22 04 46  75.6  56.8 -0.8       0.0     7      997   02 26 50
02 31 39  ---          22 09 36  76.5  53.8 -0.8       0.0   289     1071   02 26 51

02 32 24  J2303-1841   22 10 21  75.6  62.3 -0.9       0.0    14     1071   02 32 24
02 33 24  =2300-189    22 11 21  75.8  61.7 -0.9       0.0    60     1087   02 32 25

02 34 02  MR2251-178   22 11 59  76.9  52.1 -0.7       0.0     7     1087   02 34 02
02 38 51  ---          22 16 49  77.8  48.5 -0.6       0.0   289     1161   02 34 03

02 39 36  J2303-1841   22 17 34  77.0  58.2 -0.8       0.0    14     1161   02 39 36
02 40 36  =2300-189    22 18 34  77.2  57.5 -0.8       0.0    60     1177   02 39 37
Schedule for HART      (Code Hh )                                   Page   4
               AGN Cores
  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
----------------------------------------------------------------------------------------

 --- Thu  18 Jun 2020   Day 170 ---

02 41 14  MR2251-178   22 19 12  78.1  46.5 -0.6       0.0     7     1177   02 41 14
02 46 03  ---          22 24 02  78.9  42.2 -0.5       0.0   289     1251   02 41 15

02 46 48  J2303-1841   22 24 47  78.3  53.2 -0.7       0.0    14     1251   02 46 48
02 47 48  =2300-189    22 25 47  78.5  52.4 -0.6       0.0    60     1267   02 46 49

02 48 26  MR2251-178   22 26 25  79.3  39.8 -0.5       0.0     7     1267   02 48 26
02 53 15  ---          22 31 15  79.9  34.6 -0.4       0.0   289     1341   02 48 27

02 53 53  J2303-1841   22 31 53  79.6  47.2 -0.5       0.0     7     1341   02 53 53
02 54 53  =2300-189    22 32 53  79.7  46.2 -0.5       0.0    60     1356   02 53 54

02 55 31  MR2251-178   22 33 32  80.2  31.9 -0.4       0.0     7     1356   02 55 31
03 00 31  ---          22 38 32  80.7  25.5 -0.3       0.0   300     1434   02 55 32

03 58 00  J0237+2848   23 36 11  19.8  41.8 -3.0       0.0  3311     1434   03 58 00
04 00 00  =0234+285    23 38 11  20.1  41.4 -3.0       0.0   120     1465   03 58 01


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


 ======== Setup file: sess220.C2048
   Matching groups in /home/guest/rmc/SCHED/sched11.5/catalogs/freq_RDBE.dat:
     hh6cm           Values confirmed by E-mail Jonathan Quick 20140219 (CR)
    ****** Only  256.00 of  512.00 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:  2048
   Format: VDIF              Bits per sample: 2         Sample rate: 64.000
   Number of channels: 16    DBE type: DBBC_DDC         Speedup factor:   1.00

   Disk used to record data.

   1st LO=   4600.00   4600.00   4600.00   4600.00   4600.00   4600.00   4600.00   4600.00
             4600.00   4600.00   4600.00   4600.00   4600.00   4600.00   4600.00   4600.00
   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:  20  Setup file default.  Used with PCAL = off
   LO sum=   4830.49  4830.49  4830.49  4830.49  4894.49  4894.49  4894.49  4894.49
             4958.49  4958.49  4958.49  4958.49  5022.49  5022.49  5022.49  5022.49
   BBC fr=    230.49   230.49   230.49   230.49   294.49   294.49   294.49   294.49
              358.49   358.49   358.49   358.49   422.49   422.49   422.49   422.49
   Bandwd=     32.00    32.00    32.00    32.00    32.00    32.00    32.00    32.00
               32.00    32.00    32.00    32.00    32.00    32.00    32.00    32.00
    Matching frequency sets:  20

   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)

 * S52116+81         21 16 39.225408   * 21 14 01.180000     21 13 00.315720       0.00
                     81 52 14.09043    * 82 04 48.35000      82 09 34.24081        0.00
                     From catalog imbedded in main SCHED input file.

 * IGRJ21247+50      21 22 57.303310   * 21 24 39.370000     21 25 21.702323       0.00
                     50 45 27.75135    * 50 58 25.87000      51 03 27.44800        0.00
                     From catalog imbedded in main SCHED input file.

 * SWIFTJ2127        21 26 14.904661   * 21 27 45.416000     21 28 23.251310       0.00
                     56 43 26.61870    * 56 56 33.45000      57 01 37.27429        0.00
                     From catalog imbedded in main SCHED input file.

 * RXJ2135.9+47      21 34 03.266457   * 21 35 54.150000     21 36 39.877989       0.00
                     47 14 52.38037    * 47 28 20.34000      47 33 34.14777        0.00
                     From catalog imbedded in main SCHED input file.

 * MR2251-178        22 51 26.032144   * 22 54 05.980000     22 55 10.527258       0.00
                    -17 50 54.73690    *-17 34 55.30000     -17 28 22.93861        0.00
                     From catalog imbedded in main SCHED input file.

 * MCG-02-58-22      23 02 07.169293   * 23 04 43.478000     23 05 46.533406       0.00
                    -08 57 20.44512    *-08 41 08.62000     -08 34 34.39147        0.00
                     From catalog imbedded in main SCHED input file.

   0234+285          02 34 55.589590   * 02 37 52.405677     02 39 02.655320       0.00
 * J0237+2848        28 35 11.40773    * 28 48 08.98999      28 53 11.70180        0.00
   J0237+28          /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution,  58420 observations.

   2116+543          21 16 23.596185   * 21 17 56.484554     21 18 35.268168       0.18
 * J2117+5431        54 18 52.99626    * 54 31 32.50199      54 36 26.22676        0.11
                     /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution,     95 observations.

   2121+460          21 21 42.102489   * 21 23 31.828455     21 24 17.140268       0.14
 * J2123+4614        46 01 28.11490    * 46 14 22.96066      46 19 24.23025        0.12
                     /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution,    312 observations.

   2136+824          21 36 02.221764   * 21 33 34.079661     21 32 36.596352       2.73
 * J2133+8239        82 25 38.57599    * 82 39 06.05333      82 44 12.63864        0.38
                     /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution,     78 observations.

 * 3C454.3           22 51 29.519739   * 22 53 57.747939     22 54 57.718181       0.65
   J2253+1608        15 52 54.34808    * 16 08 53.56091      16 15 14.45236        0.73
   2251+158          /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc
   J2253+16          GSFC 2016a X/S astro solution,  41272 observations.

   2256-084          22 56 24.290681   * 22 59 00.688855     23 00 03.813193       0.14
 * J2259-0811       -08 27 08.46119    *-08 11 03.04608     -08 04 31.49342        0.33
                     /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution,    134 observations.

   2300-189          23 00 23.470432   * 23 03 02.975979     23 04 07.290988       0.06
 * J2303-1841       -18 57 35.85334    *-18 41 25.82275     -18 34 48.92710        0.14
                     /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution,    165 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
  S52116+81  sess220.C2048         1 2 3 4 5 6 7 8 9 10 11 15        0.500    85.500
  IGRJ21247+5sess220.C2048         1 2 3 4 5 6 7 8 9 10 11 15        0.500    83.988
  SWIFTJ2127 sess220.C2048         1 2 3 4 5 6 7 8 9 10 11 15        0.667   114.000
  RXJ2135.9+4sess220.C2048         1 2 3 4 5 6 7 8 9 10 11 15        0.667   102.083
  MR2251-178 sess220.C2048         1 2 3 4 5 6 8 9 10 11 15 20       0.645    98.728
  MCG-02-58-2sess220.C2048         1 2 3 4 5 6 7 8 9 10 11 15  +     0.583   107.667
  J0237+2848 sess220.C2048         1 2 3 4 5 6 7 8 9 10 11 15  +     0.033     6.333
  J2117+5431 sess220.C2048         1 2 3 4 5 6 7 8 9 10 11 15        0.233    39.900
  J2123+4614 sess220.C2048         1 2 3 4 5 6 7 8 9 10 11 15        0.133    20.117
  J2133+8239 sess220.C2048         1 2 3 4 5 6 7 8 9 10 11 15        0.100    17.100
  3C454.3    sess220.C2048         1 2 3 4 5 6 7 8 9 10 11 15  +     0.067    12.772
  J2259-0811 sess220.C2048         1 2 3 4 5 6 7 8 9 10 11 15  +     0.117    21.850
  J2303-1841 sess220.C2048         1 2 3 4 5 6 8 9 10 11 15 20       0.133    19.283


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) 
   S52116+81           71.6
   IGRJ21247+50        91.6
   SWIFTJ2127          87.3
   RXJ2135.9+47        92.5
   MR2251-178         108.6
   MCG-02-58-22       103.1
   J0237+2848          42.5
   J2117+5431          89.9
   J2123+4614          94.9
   J2133+8239          70.8
   3C454.3             95.2
   J2259-0811         104.2
   J2303-1841         107.0

  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 

