  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: 6cm FTP Fringe Test F14C3
 Exp. Code:  F14C3   


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

PI:       Ciriaco GODDI

Address:  JIVE
          Postbus 2
          7990 AA Dwingeloo
          The Netherlands

Phone:    +31-521-596548
EMAIL:    goddi@jive.nl
Fax:
Phone during observation: +31-521-596548

Observing mode:

Notes:    6cm FTP Fringe Test for Session 3/2014
          512 Mbps, L+R, 2-bit sampling, 16 MHz filters
          Please send the disk pack by express to JIVE
 


COVER LETTER:


This is the schedule for the 6cm ftp fringe-test F14C3 on 20 Oct 2014
involving 12 antennas: Eb Wb Jb1 On25 Nt Tr Sv Zc Bd Sh Hh Ys.
The ftp test uses a standard 512 Mbps setup.
The schedule consists of long integrations on VLBI calibrators
J1329+3154 (~1 Jy at 8.6 GHz from the VLBA calibrator Survey)
and J1613+3412 (~2 Jy at 8.6 GHz from the VLBA calibrator Survey).

There are two ftp fringe-test scans
(1) 09:06:00 UT (scan 2, 2 sec, J1329+3154)
(2) 09:50:00 UT (scan 6, 2 sec, J1613+3412)

Please make sure that the autoftp is set up correctly.

See you on Skype group chat
and
Good luck with the session!

Ciriaco Goddi
Support Scientist, JIVE
Skype account: ciriaco.goddi

Schedule for HART      (Code Hh )                                   Page   2
               6cm FTP Fringe Test F14C3
  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  20 Oct 2014   Day 293 ---

 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

09 00 00  J1329+3154   12 45 44  31.3  11.1 -0.7       0.0     0        0   09 00 00
09 02 00  =1327+321    12 47 44  31.4  10.6 -0.7       0.0   120       15   09 00 01

09 04 00  J1329+3154   12 49 44  31.5  10.2 -0.7       0.0    99       15   09 04 00
09 08 00  =1327+321    12 53 45  31.6   9.2 -0.6       0.0   240       46   09 04 01

09 10 00  J1329+3154   12 55 45  31.7   8.7 -0.6       0.0    99       46   09 10 00
09 20 00  =1327+321    13 05 47  32.0   6.2 -0.4       0.0   600      123   09 10 01

09 22 00  J1329+3154   13 07 47  32.0   5.7 -0.4       0.0    99      123   09 22 00
09 32 00  =1327+321    13 17 49  32.2   3.2 -0.2       0.0   600      200   09 22 01

09 38 00  J1613+3412   13 23 50  17.6  36.0 -2.8       0.0   252      200   09 38 00
09 46 00  =1611+343    13 31 51  18.7  34.6 -2.7       0.0   480      262   09 38 01

09 48 00  J1613+3412   13 33 52  18.9  34.3 -2.7       0.0    99      262   09 48 00
09 52 00  =1611+343    13 37 52  19.4  33.6 -2.6       0.0   240      292   09 48 01

09 55 00  J1613+3412   13 40 53  19.8  33.0 -2.6       0.0   159      292   09 55 00
10 00 00  =1611+343    13 45 54  20.4  32.2 -2.5       0.0   300      331   09 55 01


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


 ======== Setup file: sess314.C512
 --- 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:    9         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:  11  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:  11

   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)

 * J1329+3154        13 27 34.876201   * 13 29 52.864906     13 30 32.089544       0.12
   1327+321          32 09 38.80938    * 31 54 11.05448      31 49 43.56075        0.11
   J1329+31          /aps3/sched11.0/catalogs/sources.vlba
                     rfc_2012b Petrov, 2012, unpublished 617 observations

 * J1613+3412        16 11 47.914251   * 16 13 41.064242     16 14 13.294901       0.12
   1611+343          34 20 19.83376    * 34 12 47.90878      34 10 54.20658        0.10
   J1613+34          /aps3/sched11.0/catalogs/sources.vlba
                     rfc_2012b Petrov, 2012, unpublished 151566 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
  J1329+3154 sess314.C512          1 2 3 4 5 6 7 10 11 12            0.433    28.600
  J1613+3412 sess314.C512          1 2 3 4 5 6 7 10 11 12            0.283    18.700


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) 
   J1329+3154          42.3
   J1613+3412          57.7

  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 

