  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: Probing blazar dynamics in an extreme case of jet realignment
 Exp. Code:  RSB02B  


Schedule Version:       2.00
Processed by SCHED version:  11.50  Development version 11.5. Started Apr. 2

PI:       Gabriele Bruni

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

Phone:    +39 06 4548 8456
EMAIL:    gabriele.bruni@inaf.it
Fax:      ---
Phone during observation: +39 06 4548 8456

Observing mode: Phase-referencing of a source at 3.6cm

Notes:
 
 
 

Schedule for HART      (Code Hh )                                   Page   2
               Probing blazar dynamics in an extreme case of jet realignment
  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  23 Oct 2019   Day 296 ---

 Next scan frequencies:  8319.49  8319.49  8319.49  8319.49  8383.49  8383.49  8383.49  8383.49
                         8447.49  8447.49  8447.49  8447.49  8511.49  8511.49  8511.49  8511.49
 Next BBC frequencies:    239.49   239.49   239.49   239.49   303.49   303.49   303.49   303.49
                          367.49   367.49   367.49   367.49   431.49   431.49   431.49   431.49
 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

20 30 00  PBC2333      00 28 37  77.6 277.7  0.9       0.0     0        0   20 30 00
20 35 00  ---          00 33 38  76.5 276.5  1.0       0.0   300       77   20 30 01

20 35 00  PBC2333      00 33 38  76.5 276.5  1.0       0.0   -20       77   No stop 
20 40 00  ---          00 38 39  75.4 275.5  1.1       0.0   280      155   20 35 01

20 40 30  PBC2333      00 39 09  75.3 275.4  1.1       0.0     9      155   20 40 30
20 45 30  ---          00 44 09  74.1 274.5  1.2       0.0   300      232   20 40 31

20 45 30  PBC2333      00 44 09  74.1 274.5  1.2       0.0   -20      232   No stop 
20 50 30  ---          00 49 10  73.0 273.7  1.2       0.0   280      309   20 45 31

20 50 30  PBC2333      00 49 10  73.0 273.7  1.2       0.0   -20      309   No stop 
20 55 30  ---          00 54 11  71.9 272.9  1.3       0.0   280      386   20 50 31

20 56 00  PBC2333      00 54 41  71.8 272.9  1.3       0.0     9      386   20 56 00
21 01 00  ---          00 59 42  70.6 272.2  1.4       0.0   300      464   20 56 01

21 01 00  PBC2333      00 59 42  70.6 272.2  1.4       0.0   -20      464   No stop 
21 06 00  ---          01 04 43  69.5 271.5  1.5       0.0   280      541   21 01 01

21 06 00  PBC2333      01 04 43  69.5 271.5  1.5       0.0   -20      541   No stop 
21 11 00  ---          01 09 44  68.4 270.9  1.6       0.0   280      618   21 06 01

21 11 30  PBC2333      01 10 14  68.3 270.9  1.6       0.0     9      618   21 11 30
21 16 30  ---          01 15 15  67.2 270.3  1.7       0.0   300      696   21 11 31

21 16 30  PBC2333      01 15 15  67.2 270.3  1.7       0.0   -20      696   No stop 
21 21 30  ---          01 20 15  66.0 269.7  1.8       0.0   280      773   21 16 31

21 21 30  PBC2333      01 20 15  66.0 269.7  1.8       0.0   -20      773   No stop 
21 26 30  ---          01 25 16  64.9 269.2  1.8       0.0   280      850   21 21 31

21 27 00  PBC2333      01 25 46  64.8 269.2  1.8       0.0     9      850   21 27 00
21 32 00  ---          01 30 47  63.7 268.7  1.9       0.0   300      927   21 27 01

21 32 00  PBC2333      01 30 47  63.7 268.7  1.9       0.0   -20      927   No stop 
21 37 00  ---          01 35 48  62.5 268.2  2.0       0.0   280     1005   21 32 01
Schedule for HART      (Code Hh )                                   Page   3
               Probing blazar dynamics in an extreme case of jet realignment
  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  23 Oct 2019   Day 296 ---

21 37 00  PBC2333      01 35 48  62.5 268.2  2.0       0.0   -20     1005   No stop 
21 42 00  ---          01 40 49  61.4 267.7  2.1       0.0   280     1082   21 37 01

21 42 30  PBC2333      01 41 19  61.3 267.7  2.1       0.0     9     1082   21 42 30
21 47 30  ---          01 46 20  60.2 267.2  2.2       0.0   300     1159   21 42 31

21 47 30  PBC2333      01 46 20  60.2 267.2  2.2       0.0   -20     1159   No stop 
21 54 07  ---          01 52 58  58.7 266.6  2.3       0.0   377     1262   21 47 31

21 57 00  3C454.3      01 55 51  29.1 308.8  3.0       0.0    66     1262   21 57 00
22 00 00  ---          01 58 51  28.6 308.2  3.1       0.0   180     1308   21 57 01


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


 ======== Setup file: sess319.X2048
   Matching groups in /home/guest/rmc/SCHED/sched11.5/catalogs/freq.dat:
     hhsx            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:    4         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=   8080.00   8080.00   8080.00   8080.00   8080.00   8080.00   8080.00   8080.00
             8080.00   8080.00   8080.00   8080.00   8080.00   8080.00   8080.00   8080.00
   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:   7  Setup file default.  Used with PCAL = off
   LO sum=   8319.49  8319.49  8319.49  8319.49  8383.49  8383.49  8383.49  8383.49
             8447.49  8447.49  8447.49  8447.49  8511.49  8511.49  8511.49  8511.49
   BBC fr=    239.49   239.49   239.49   239.49   303.49   303.49   303.49   303.49
              367.49   367.49   367.49   367.49   431.49   431.49   431.49   431.49
   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:   7

   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)

 * PBC2333           23 31 17.940448   * 23 33 55.237800     23 34 57.355889       0.00
                    -24 00 15.79862    *-23 43 40.65802     -23 37 11.62125        0.00
                     From catalog imbedded in main SCHED input file.

 * 3C454.3           22 51 29.519739   * 22 53 57.747939     22 54 56.325043       0.65
   J2253+1608        15 52 54.34808    * 16 08 53.56091      16 15 18.81592        0.73
   2251+158          /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc
   J2253+16          GSFC 2016a X/S astro solution,  41272 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
  PBC2333    sess319.X2048         1 2 3 4 5 6 7 8                   1.360    46.844
  3C454.3    sess319.X2048         1 2 3 4 5 6 7 8                   0.050     1.800


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) 
   PBC2333            131.4
   3C454.3            136.8

  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 

