  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: UniBoard VDIF cornerturning test
 Exp. Code:  FT018   


Schedule Version:       2.00
Processed by SCHED version:  11.40  Release 11.4.  March 14, 2015

PI:       campbell

Address:  JIVE
 
 
 

Phone:    0521-596-534
EMAIL:    campbell@jive.eu
Fax:
Phone during observation:

Observing mode:

Notes:
 
 
 

Schedule for HART      (Code Hh )                                   Page   2
               UniBoard VDIF cornerturning 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
----------------------------------------------------------------------------------------

 --- Tue  17 Oct 2017   Day 290 ---

 Next scan frequencies:  4966.49  4966.49  4966.49  4966.49  4998.49  4998.49  4998.49  4998.49
 Next BBC frequencies:    366.49   366.49   366.49   366.49   398.49   398.49   398.49   398.49
 Next scan bandwidths:     16.00    16.00    16.00    16.00    16.00    16.00    16.00    16.00

11 00 00  OQ208        14 35 19  35.3 352.6  0.5       0.0     0        0   11 00 00
11 15 00  ---          14 50 21  34.8 348.6  0.7       0.0   900       58   11 00 01

11 45 00  OQ208        15 20 26  33.0 340.9  1.2       0.0  1778       58   11 45 00
12 00 00  ---          15 35 28  31.8 337.3  1.5       0.0   900      116   11 45 01

12 30 00  OQ208        16 05 33  28.8 330.4  2.0       0.0  1778      116   12 30 00
12 45 00  ---          16 20 36  27.1 327.2  2.2       0.0   900      174   12 30 01


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


 ======== Setup file: sess317.C512nme
   Matching groups in /home/guest/rmc/SCHED/sched11.4/catalogs/freq_RDBE.dat:
     hh6cm           Values confirmed by E-mail Jonathan Quick 20140219 (CR)
    ****** Only   64.00 of  128.00 MHz total bandwidth is within the IFs
           in the setup file before any FREQ or DOPPLER shifts.

   Setup group:    2         Station: HART              Total bit rate:   512
   Format: VDIF              Bits per sample: 2         Sample rate: 32.000
   Number of channels:  8    DBE type: DBBC_DDC         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
   Net SB=         L         L         U         U         L         L         U         U
   IF SB =         U         U         U         U         U         U         U         U
   Pol.  =      RCP       LCP       RCP       LCP       RCP       LCP       RCP       LCP 
   BBC   =         1         9         1         9         3        11         3        11
   BBC SB=         L         L         U         U         L         L         U         U
   IF    =        A1        C1        A1        C1        A1        C1        A1        C1

  The following frequency sets based on these setups were used.

   Frequency Set:   4  Setup file default.  Used with PCAL = off
   LO sum=   4966.49  4966.49  4966.49  4966.49  4998.49  4998.49  4998.49  4998.49
   BBC fr=    366.49   366.49   366.49   366.49   398.49   398.49   398.49   398.49
   Bandwd=     16.00    16.00    16.00    16.00    16.00    16.00    16.00    16.00
    Matching frequency sets:   4

   Track assignments are: 
    track1=   1,  2,  3,  4,  5,  6,  7,  8
    barrel=roll_off 

 POSITIONS OF SOURCES USED IN RECORDING SCANS

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

 * OQ208             14 04 45.615156   * 14 07 00.394414     14 07 46.014371       0.24
   J1407+2827        28 41 29.23518    * 28 27 14.69022      28 22 26.73341        0.34
   1404+286          /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc
   J1407+28          GSFC 2015a astro solution, unpublished  67871 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
  OQ208      sess317.C512nme       1 2 3 4                           0.750     7.500


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) 
   OQ208               38.9

  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 

