  COVER INFORMATION 

 Station:    MC_DBBC   (Code Md ) 
 Experiment: FTP Fringe Test
 Exp. Code:  F13L4   


Schedule Version:       2.00
Processed by SCHED version:  10.20  Release of about July 12, 2012

PI:       Ivan Agudo

Address:  JIVE
          Postbus 2
          7990 AA Dwingeloo
          The Netherlands

Phone:    +31-521-596549
EMAIL:    agudo@jive.nl
Fax:
Phone during observation: +31-521-596549

Observing mode:

Notes:    18cm FTP Fringe Test for session 3/2013
          512 Mbps, 2-bit sampling, 8 MHz filters
          Send the disk pack by express to JIVE
          Additional DBBC testing data from Mc and Tr is expected.


COVER LETTER:


Dear EVN friends,

This is the schedule for the 18cm FTP-FT on October 24 2013,
involving 14 stations: Eb Wb Jb1 On25 Mc Nt Tr Sv Zc Bd Ur Sh Hh Ir
The test uses a standard setup with 512 Mbps and consists of two
ftp fringe tests, interspersed with a longer set of scans on
2005+403 (~2.5 Jy source at 1.4 GHz).

The two ftp fringe-test scans, start at:
(1) 13:04:30 UT (scan 2, 2 sec)
(2) 13:53:00 UT (scan 8, 2 sec)

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

Ivan
Skype account: ivan-agudo

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
----------------------------------------------------------------------------------------

 --- Thu  24 Oct 2013   Day 297 ---

 Next scan frequencies:  1634.49  1634.49  1634.49  1634.49  1650.49  1650.49  1650.49  1650.49
                         1666.49  1666.49  1666.49  1666.49  1682.49  1682.49  1682.49  1682.49
 Next BBC frequencies:    339.49   339.49   339.49   339.49   355.49   355.49   355.49   355.49
                          371.49   371.49   371.49   371.49   387.49   387.49   387.49   387.49
 Next scan bandwidths:      8.00     8.00     8.00     8.00     8.00     8.00     8.00     8.00
                            8.00     8.00     8.00     8.00     8.00     8.00     8.00     8.00

14 00 00  2005+403     16 59 07  55.4 439.6 -3.2     -67.4     0        0   14 00 00
14 04 00  ---          17 03 08  56.1 440.2 -3.1     -67.6   240       15   14 00 01

14 04 30  2005+403     17 03 38  56.2 440.2 -3.1     -67.6    27       15   14 04 30
14 08 30  ---          17 07 39  56.9 440.8 -3.0     -67.8   240       31   14 04 31

14 10 30  2005+403     17 09 39  57.3 441.0 -3.0     -67.9   117       31   14 10 30
14 18 30  ---          17 17 40  58.7 442.1 -2.8     -68.3   480       62   14 10 31

14 19 00  2005+403     17 18 10  58.8 442.2 -2.8     -68.4    27       62   14 19 00
14 27 00  ---          17 26 12  60.2 443.3 -2.7     -68.7   480       93   14 19 01

14 27 30  2005+403     17 26 42  60.3 443.3 -2.7     -68.7    27       93   14 27 30
14 35 30  ---          17 34 43  61.7 444.5 -2.6     -69.0   480      124   14 27 31

14 36 00  2005+403     17 35 13  61.8 444.5 -2.6     -69.1    27      124   14 36 00
14 44 00  ---          17 43 15  63.2 445.7 -2.4     -69.3   480      155   14 36 01

14 44 30  2005+403     17 43 45  63.3 445.8 -2.4     -69.3    27      155   14 44 30
14 52 30  ---          17 51 46  64.7 447.0 -2.3     -69.6   480      186   14 44 31

14 53 00  2005+403     17 52 16  64.8 447.1 -2.3     -69.6    27      186   14 53 00
14 57 00  ---          17 56 17  65.5 447.7 -2.2     -69.6   240      201   14 53 01

14 59 00  2005+403     17 58 17  65.9 448.0 -2.2     -69.7   117      201   14 59 00
15 00 00  ---          17 59 17  66.1 448.2 -2.1     -69.7    60      205   14 59 01


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


 ======== Setup file: sess313.L512
 --- 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:   14         Station: MC_DBBC           Total bit rate:  512
   Format: MARK5B            Bits per sample: 2         Sample rate: 16.000
   Number of channels: 16    DBE type:                  Speedup factor:   1.00

   Disk used to record data.

   1st LO=   1295.00   1295.00   1295.00   1295.00   1295.00   1295.00   1295.00   1295.00
             1295.00   1295.00   1295.00   1295.00   1295.00   1295.00   1295.00   1295.00
   Net SB=         L         L         U         U         L         L         U         U
                   L         L         U         U         L         L         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=   1634.49  1634.49  1634.49  1634.49  1650.49  1650.49  1650.49  1650.49
             1666.49  1666.49  1666.49  1666.49  1682.49  1682.49  1682.49  1682.49
   BBC fr=    339.49   339.49   339.49   339.49   355.49   355.49   355.49   355.49
              371.49   371.49   371.49   371.49   387.49   387.49   387.49   387.49
   Bandwd=      8.00     8.00     8.00     8.00     8.00     8.00     8.00     8.00
                8.00     8.00     8.00     8.00     8.00     8.00     8.00     8.00
    Matching frequency sets:  15

   Track assignments are: 
    track1=   2,  4,  6,  8, 10, 12, 14, 16, 18, 20, 22, 24, 26, 28, 30, 32
    barrel=roll_off 
 SOURCES USED IN RECORDING SCANS --                         FTP Fringe Test
     Catalog positions marked with *. 
     Precession of date coordinates is based on stop time of first scan.
     Names used in schedule marked with *. 
     Short names used in VLA and SNAP files marked with +. 
     Observation date used in B1950/J2000 coordinate conversion (PRECDATE):  1979.900
     No adjustments are made for rates (DRA, DDEC).
     Scan hours are for recording scans only. 
     Baseline hours are only counted for scans above horizon at both ends.

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

   J2007+4029        20 05 59.558893   * 20 07 44.944844     20 08 14.585970       0.30
 * 2005+403          40 21 01.80221    * 40 29 48.60406      40 32 41.18056        0.23
   J2007+40          /aps3/sched10.2/catalogs/sources.vlba
                     rfc_2012b Petrov, 2012, unpublished 169 observations
                        0.883 scan and     94.750 baseline hours in setup: sess313.L512
                     Frequency sets (dups not shown):   1  2  3  4  5  6  7  8 11 12 13 14 15 16



  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) 
   2005+403            99.9

  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 

