  COVER INFORMATION 

 Station:    MC_DBBC   (Code Md ) 
 Experiment: FTP Fringe Test
 Exp. Code:  F14K1   


Schedule Version:       2.00
Processed by SCHED version:  11.00  Release of Feb. 15, 2013

PI:       Ivan Agudo

Address:  JIVE
          Postbus 2
          7990 AA Dwingeloo
          The Netherlands

Phone:    +31-521-596-549
EMAIL:    agudo@jive.nl
Fax:
Phone during observation: +31-521-596-549

Observing mode:

Notes:    1.3cm FTP Fringe Test for session 1/2014
          1024 Mbps, 2-bit sampling, 16 MHz filters
          Participation from Sr (with DBBC), and Sh65 (TIANMA65 or T6) expected
          Additional DBBC testing data from Mc, Tr, and Ys is also expected.


COVER LETTER:


Dear EVN friends,

This is the schedule for the 1.3cm FTP-FT on March 10 2011,
involving 22 stations: Eb Jb2 On20 Mc Nt Tr Sv Zc Bd Ur Sh Hh Ys
Mh Sr Ky, Ku, Kt, as well as Md Td Yd (Mc Tr and Ys with DBBC)
and Sh65. The test uses a standard setup with 1024 Mbps and consists
of two ftp fringe tests, interspersed with a longer set of scans on
0234+285 (~1.5 Jy source at 22 GHz).

The two ftp fringe-test scans, start at:
(1) 12:07:30 UT (scan 2, 2 sec)
(2) 12:56:00 UT (scan 8, 2 sec)

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

Ivan
Support Scientist, JIVE
Skype account: JIVE.Support.Scientist

Schedule for MC_DBBC   (Code Md )                                   Page   2
               FTP Fringe Test
  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  10 Mar 2014   Day  69 ---

 Next scan frequencies:  22187.49  22187.49  22187.49  22187.49  22219.49  22219.49  22219.49  22219.49
                         22251.49  22251.49  22251.49  22251.49  22283.49  22283.49  22283.49  22283.49
 Next BBC frequencies:     223.49    223.49    223.49    223.49    255.49    255.49    255.49    255.49
                           287.49    287.49    287.49    287.49    319.49    319.49    319.49    319.49
 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

12 00 00  0234+285     23 58 56  54.8 462.7 -2.7     -52.6     0        0   12 00 00
12 04 00  ---          00 02 56  55.5 463.6 -2.6     -52.3   240       31   12 00 01

12 04 30  0234+285     00 03 26  55.6 463.7 -2.6     -52.3    27       31   12 04 30
12 08 30  ---          00 07 27  56.3 464.7 -2.5     -51.9   240       62   12 04 31

12 10 30  0234+285     00 09 27  56.6 465.2 -2.5     -51.8   117       62   12 10 30
12 18 30  ---          00 17 29  58.0 467.2 -2.4     -51.0   480      123   12 10 31

12 19 00  0234+285     00 17 59  58.1 467.4 -2.3     -51.0    27      123   12 19 00
12 27 00  ---          00 26 00  59.4 469.5 -2.2     -50.1   480      185   12 19 01

12 27 30  0234+285     00 26 30  59.5 469.6 -2.2     -50.1    27      185   12 27 30
12 35 30  ---          00 34 32  60.9 471.9 -2.1     -49.0   480      246   12 27 31

12 36 00  0234+285     00 35 02  60.9 472.1 -2.1     -49.0    27      246   12 36 00
12 44 00  ---          00 43 03  62.3 474.5 -1.9     -47.8   480      308   12 36 01

12 44 30  0234+285     00 43 33  62.3 474.7 -1.9     -47.7    27      308   12 44 30
12 52 30  ---          00 51 34  63.6 477.3 -1.8     -46.3   480      369   12 44 31

12 53 00  0234+285     00 52 04  63.7 477.5 -1.8     -46.2    27      369   12 53 00
12 57 00  ---          00 56 05  64.3 478.9 -1.7     -45.5   240      400   12 53 01

12 59 00  0234+285     00 58 05  64.6 479.6 -1.7     -45.1   117      400   12 59 00
13 00 00  ---          00 59 06  64.8 480.0 -1.7     -44.8    60      408   12 59 01


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


 ======== Setup file: sess114.K1024
 --- 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:   15         Station: MC_DBBC           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=  21964.00  21964.00  21964.00  21964.00  21964.00  21964.00  21964.00  21964.00
            21964.00  21964.00  21964.00  21964.00  21964.00  21964.00  21964.00  21964.00
   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:  15  Setup file default.
   LO sum=   22187.49  22187.49  22187.49  22187.49  22219.49  22219.49  22219.49  22219.49
             22251.49  22251.49  22251.49  22251.49  22283.49  22283.49  22283.49  22283.49
   BBC fr=     223.49    223.49    223.49    223.49    255.49    255.49    255.49    255.49
               287.49    287.49    287.49    287.49    319.49    319.49    319.49    319.49
   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:  15  19

   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)

   J0237+2848        02 34 55.589591   * 02 37 52.405678     02 38 42.679952       0.11
 * 0234+285          28 35 11.40773    * 28 48 08.98998      28 51 46.49950        0.10
   J0237+28          /usr/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
  0234+285   sess114.K1024         1 2 3 4 5 6 7 10 11 12 13 1 +     0.883   204.050


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) 
   0234+285            57.4

  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 

