  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: 5 GHz observation of RGB J0152+017
 Exp. Code:  EA053A  


Schedule Version:       1.00
Processed by SCHED version:  11.00  Release of Feb. 15, 2013

PI:       Kazunori Akiyama

Address:  National Astronomical Observatory of Japan
          2-21-1, Osawa, Mitaka, Tokyo
          Japan
 

Phone:    +81 422 34 3939
EMAIL:    kazunori.akiyama@nao.ac.jp
Fax:      +81 422 34 3814
Phone during observation: +81 422 34 3939

Observing mode: VLBA/MKIV

Notes:
 
 
 

Schedule for HART      (Code Hh )                                   Page   2
               5 GHz observation of RGB J0152+017
  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
----------------------------------------------------------------------------------------

 --- Tue   4 Mar 2014   Day  63 ---

 Next scan frequencies:  4942.49  4942.49  4942.49  4942.49  4974.49  4974.49  4974.49  4974.49
                         5006.49  5006.49  5006.49  5006.49  5038.49  5038.49  5038.49  5038.49
 Next BBC frequencies:    342.49   342.49   342.49   342.49   374.49   374.49   374.49   374.49
                          406.49   406.49   406.49   406.49   438.49   438.49   438.49   438.49
 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

10 00 00  0150+015     22 39 06  35.5  67.0 -3.2       0.0     0        0   10 00 00
10 05 30  ---          22 44 37  36.6  66.1 -3.1       0.0   330       42   10 00 01

10 06 00  0150+015     22 45 07  36.7  66.0 -3.1       0.0     9       42   10 06 00
10 11 30  ---          22 50 38  37.9  65.0 -3.0       0.0   330       85   10 06 01

10 12 00  0150+015     22 51 08  38.0  64.9 -3.0       0.0     9       85   10 12 00
10 17 30  ---          22 56 39  39.1  63.8 -2.9       0.0   330      127   10 12 01

10 18 00  0150+015     22 57 09  39.2  63.8 -2.9       0.0     9      127   10 18 00
10 23 30  ---          23 02 40  40.3  62.7 -2.8       0.0   330      169   10 18 01

10 24 00  0150+015     23 03 10  40.4  62.6 -2.8       0.0     9      169   10 24 00
10 29 30  ---          23 08 41  41.5  61.5 -2.7       0.0   330      212   10 24 01

10 30 00  0150+015     23 09 11  41.6  61.4 -2.7       0.0     9      212   10 30 00
10 35 30  ---          23 14 42  42.7  60.2 -2.6       0.0   330      254   10 30 01

10 36 00  0150+015     23 15 12  42.8  60.1 -2.6       0.0     9      254   10 36 00
10 41 30  ---          23 20 43  43.9  58.9 -2.5       0.0   330      296   10 36 01

10 42 00  0150+015     23 21 13  43.9  58.8 -2.5       0.0     9      296   10 42 00
10 47 30  ---          23 26 44  45.0  57.6 -2.4       0.0   330      338   10 42 01

10 48 00  0150+015     23 27 14  45.1  57.5 -2.4       0.0     9      338   10 48 00
10 53 30  ---          23 32 45  46.1  56.2 -2.3       0.0   330      381   10 48 01

10 54 30  0158+031     23 33 45  43.8  56.1 -2.5       0.0    29      381   10 54 30
10 59 30  ---          23 38 46  44.7  55.0 -2.4       0.0   300      419   10 54 31

11 00 00  0150+015     23 39 16  47.3  54.6 -2.2       0.0    -1      419   11 00 00
11 05 30  ---          23 44 47  48.3  53.2 -2.1       0.0   329      462   11 00 01

11 06 00  0150+015     23 45 17  48.4  53.0 -2.1       0.0     9      462   11 06 00
11 11 30  ---          23 50 48  49.4  51.5 -2.0       0.0   330      504   11 06 01

11 12 00  0150+015     23 51 18  49.5  51.4 -2.0       0.0     9      504   11 12 00
11 17 30  ---          23 56 49  50.5  49.9 -1.9       0.0   330      546   11 12 01
Schedule for HART      (Code Hh )                                   Page   3
               5 GHz observation of RGB J0152+017
  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
----------------------------------------------------------------------------------------

 --- Tue   4 Mar 2014   Day  63 ---

11 18 00  0150+015     23 57 19  50.5  49.7 -1.9       0.0     9      546   11 18 00
11 23 30  ---          00 02 50  51.5  48.1 -1.8       0.0   330      588   11 18 01

11 24 00  0150+015     00 03 20  51.6  48.0 -1.8       0.0     9      588   11 24 00
11 29 30  ---          00 08 51  52.5  46.3 -1.7       0.0   330      631   11 24 01

11 30 00  0150+015     00 09 21  52.6  46.1 -1.7       0.0     9      631   11 30 00
11 35 30  ---          00 14 52  53.4  44.4 -1.6       0.0   330      673   11 30 01

11 36 00  0150+015     00 15 22  53.5  44.2 -1.6       0.0     9      673   11 36 00
11 41 30  ---          00 20 53  54.4  42.4 -1.5       0.0   330      715   11 36 01

11 42 00  0150+015     00 21 23  54.4  42.2 -1.5       0.0     9      715   11 42 00
11 47 30  ---          00 26 54  55.3  40.3 -1.4       0.0   330      758   11 42 01

11 48 00  0150+015     00 27 24  55.3  40.1 -1.4       0.0     9      758   11 48 00
11 53 30  ---          00 32 55  56.1  38.1 -1.3       0.0   330      800   11 48 01

11 54 30  0158+031     00 33 55  53.8  39.0 -1.5       0.0    29      800   11 54 30
11 59 30  ---          00 38 56  54.5  37.3 -1.4       0.0   300      838   11 54 31

12 02 00  0234+285     00 41 26  28.4  29.2 -2.0       0.0    72      838   12 02 00
12 12 00  ---          00 51 28  29.5  27.0 -1.8       0.0   600      915   12 02 01

12 14 30  0150+015     00 53 58  58.8  29.6 -1.0       0.0    69      915   12 14 30
12 24 00  ---          01 03 30  59.7  25.4 -0.8       0.0   570      988   12 14 31

12 24 30  0150+015     01 04 00  59.8  25.1 -0.8       0.0     9      988   12 24 30
12 30 00  ---          01 09 31  60.3  22.6 -0.7       0.0   330     1031   12 24 31

12 30 30  0150+015     01 10 01  60.3  22.3 -0.7       0.0     9     1031   12 30 30
12 36 00  ---          01 15 32  60.8  19.7 -0.6       0.0   330     1073   12 30 31

12 36 30  0150+015     01 16 02  60.8  19.4 -0.6       0.0     9     1073   12 36 30
12 42 00  ---          01 21 33  61.2  16.7 -0.5       0.0   330     1115   12 36 31

12 42 30  0150+015     01 22 03  61.2  16.5 -0.5       0.0     9     1115   12 42 30
12 48 00  ---          01 27 34  61.6  13.7 -0.4       0.0   330     1158   12 42 31

12 48 30  0150+015     01 28 04  61.6  13.4 -0.4       0.0     9     1158   12 48 30
12 54 00  ---          01 33 35  61.8  10.5 -0.3       0.0   330     1200   12 48 31

12 55 00  0158+031     01 34 35  60.0  13.5 -0.4       0.0    29     1200   12 55 00
13 00 00  ---          01 39 35  60.2  11.0 -0.4       0.0   300     1238   12 55 01


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


 ======== Setup file: sess114.C1024
 --- WARNING ---  This group does not match an entry in the frequency catalog.
                  This might be ok because the catalog is not complete.
                  But be very careful to be sure that the setup is correct.

   Setup group:   12         Station: HART              Total bit rate:  1024
   Format: MARK5B            Bits per sample: 2         Sample rate: 32.000
   Number of channels: 16    DBE type:                  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         5         1         5         2         6         2         6
                   3         7         3         7         4         8         4         8
   BBC SB=         L         L         U         U         L         L         U         U
                   L         L         U         U         L         L         U         U
   IF    =        A1        B1        A1        B1        A1        B1        A1        B1
                  A1        B1        A1        B1        A1        B1        A1        B1

  The following frequency sets based on these setups were used.

   Frequency Set:  14  Setup file default.
   LO sum=   4942.49  4942.49  4942.49  4942.49  4974.49  4974.49  4974.49  4974.49
             5006.49  5006.49  5006.49  5006.49  5038.49  5038.49  5038.49  5038.49
   BBC fr=    342.49   342.49   342.49   342.49   374.49   374.49   374.49   374.49
              406.49   406.49   406.49   406.49   438.49   438.49   438.49   438.49
   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:  14

   Track assignments are: 
    track1=   2,  4,  6,  8, 10, 12, 14, 16, 18, 20, 22, 24, 26, 28, 30, 32
    barrel=roll_off 

 POSITIONS OF SOURCES USED IN RECORDING SCANS

   Source                         Source position (RA/Dec)                        Error
                        (B1950)             (J2000)             (Date)            (mas)

 * 0150+015          01 50 04.944956   * 01 52 39.610900     01 53 23.219076       0.00
                     01 32 31.24587    * 01 47 17.38300      01 51 20.07749        0.00
                     From catalog imbedded in main SCHED input file.

 * 0158+031          01 58 05.164743   * 02 00 40.816500     02 01 24.756169       0.38
                     03 08 20.27885    * 03 22 49.50700      03 26 47.47354        0.38
                     From catalog imbedded in main SCHED input file.

   J0237+2848        02 34 55.589591   * 02 37 52.405678     02 38 42.756132       0.11
 * 0234+285          28 35 11.40773    * 28 48 08.98998      28 51 47.15343        0.10
   J0237+28          /usr2/local/sched/catalogs/sources.vlba
                     rfc_2012b Petrov, 2012, unpublished 56811 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
  0150+015   sess114.C1024         1 2 3 4 5 6 7 8 9 10 11 14        2.267   202.678
  0158+031   sess114.C1024         1 2 3 4 5 6 7 8 9 10 11 14        0.250    21.667
  0234+285   sess114.C1024         1 2 3 4 5 6 7 8 9 10 11 14        0.167    15.167


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) 
   0150+015            44.0
   0158+031            46.2
   0234+285            63.2

  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 

