  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: 2Gbps test in session: 2Gbps stations
 Exp. Code:  F13C1B  


Schedule Version:       1.00
Processed by SCHED version:  10.20  Release of about July 12, 2012

PI:       JOPS

Address:  JIVE
 
 
 

Phone:    0521-596-534
EMAIL:    jops@jive.nl
Fax:
Phone during observation:

Observing mode:

Notes:
 
 
 

Schedule for HART      (Code Hh )                                   Page   2
               2Gbps test in session: 2Gbps stations
  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  21 Feb 2013   Day  52 ---

 Next scan frequencies:  4948.00  4948.00  4916.00  4916.00  4884.00  4884.00  4852.00  4852.00
                         4820.00  4820.00  4788.00  4788.00  4756.00  4756.00  4724.00  4724.00
 Next BBC frequencies:    336.00   336.00   304.00   304.00   272.00   272.00   240.00   240.00
                          208.00   208.00   176.00   176.00   144.00   144.00   112.00   112.00
 Next scan bandwidths:     32.00    32.00    32.00    32.00    32.00    32.00    32.00    32.00
                           32.00    32.00    32.00    32.00    32.00    32.00    32.00    32.00

10 00 00  3C454.3      21 56 41  45.6  20.1 -1.0       0.0     0        0   10 00 00
10 08 00  ---          22 04 42  46.2  17.4 -0.8       0.0   480      124   10 00 01

10 09 00  3C454.3      22 05 43  46.2  17.1 -0.8       0.0    39      124   10 09 00
10 17 00  ---          22 13 44  46.7  14.4 -0.7       0.0   480      248   10 09 01

10 18 00  3C454.3      22 14 44  46.8  14.0 -0.7       0.0    39      248   10 18 00
10 26 00  ---          22 22 45  47.2  11.3 -0.5       0.0   480      372   10 18 01

10 30 00  0234+285     22 26 46   8.5  52.1 -4.2       0.0   102      372   10 30 00
10 38 00  ---          22 34 47   9.9  51.0 -4.1       0.0   480      495   10 30 01

10 39 00  0234+285     22 35 48  10.1  50.9 -4.0       0.0    39      495   10 39 00
10 47 00  ---          22 43 49  11.4  49.8 -3.9       0.0   480      619   10 39 01

10 48 00  0234+285     22 44 49  11.6  49.6 -3.9       0.0    39      619   10 48 00
10 56 00  ---          22 52 50  13.0  48.5 -3.8       0.0   480      743   10 48 01

11 00 00  0234+285     22 56 51  13.7  47.9 -3.7       0.0   219      743   11 00 00
11 08 00  ---          23 04 52  15.0  46.7 -3.6       0.0   480      867   11 00 01

11 09 00  0234+285     23 05 52  15.1  46.6 -3.5       0.0    39      867   11 09 00
11 17 00  ---          23 13 54  16.4  45.4 -3.4       0.0   480      991   11 09 01

11 18 00  0234+285     23 14 54  16.6  45.2 -3.4       0.0    39      991   11 18 00
11 26 00  ---          23 22 55  17.9  43.9 -3.3       0.0   480     1115   11 18 01

11 30 00  0234+285     23 26 56  18.5  43.3 -3.2       0.0   219     1115   11 30 00
11 38 00  ---          23 34 57  19.7  41.9 -3.1       0.0   480     1239   11 30 01

11 39 00  0234+285     23 35 57  19.9  41.8 -3.0       0.0    39     1239   11 39 00
11 47 00  ---          23 43 59  21.0  40.4 -2.9       0.0   480     1362   11 39 01

11 48 00  0234+285     23 44 59  21.2  40.2 -2.9       0.0    39     1362   11 48 00
11 56 00  ---          23 53 00  22.3  38.8 -2.8       0.0   480     1486   11 48 01


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


 ======== Setup file: sess113.pfb
 --- 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:    5         Station: HART              Total bit rate: 2048
   Format: MARK5B            Bits per sample: 2         Sample rate: 64.000
   Number of channels: 16    DBE type:                  Speedup factor:   1.00

   Disk used to record data.

   1st LO=   4612.00   4612.00   4612.00   4612.00   4612.00   4612.00   4612.00   4612.00
             4612.00   4612.00   4612.00   4612.00   4612.00   4612.00   4612.00   4612.00
   Net 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   =        15        16        13        14        11        12         9        10
                   7         8         5         6         3         4         1         2
   BBC SB=         U         U         U         U         U         U         U         U
                   U         U         U         U         U         U         U         U
   IF    =        A         C         A         C         A         C         A         C 
                  A         C         A         C         A         C         A         C 

  The following frequency sets based on these setups were used.

   Frequency Set:   3  Setup file default.
   LO sum=   4948.00  4948.00  4916.00  4916.00  4884.00  4884.00  4852.00  4852.00
             4820.00  4820.00  4788.00  4788.00  4756.00  4756.00  4724.00  4724.00
   BBC fr=    336.00   336.00   304.00   304.00   272.00   272.00   240.00   240.00
              208.00   208.00   176.00   176.00   144.00   144.00   112.00   112.00
   Bandwd=     32.00    32.00    32.00    32.00    32.00    32.00    32.00    32.00
               32.00    32.00    32.00    32.00    32.00    32.00    32.00    32.00
    Matching frequency sets:   3   5

   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 --                         2Gbps test in session: 2Gbps stations
     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)

   J0237+2848        02 34 55.589591   * 02 37 52.405678     02 38 39.659177       0.11
 * 0234+285          28 35 11.40773    * 28 48 08.98998      28 51 35.44005        0.10
   J0237+28          /aps3/sched10.2/catalogs/sources.vlba
                     rfc_2012b Petrov, 2012, unpublished 56811 observations
                        1.200 scan and     54.000 baseline hours in setup: sess113.pfb
                     Frequency sets (dups not shown):   1  3  6  9

   J2253+1608        22 51 29.519738   * 22 53 57.747937     22 54 36.387911       0.68
 * 3C454.3           15 52 54.34810    * 16 08 53.56093      16 13 07.69286        0.72
   2251+158          /aps3/sched10.2/catalogs/sources.vlba
   J2253+16          GSFC 2011A astro solution     39747 Observations
                        0.400 scan and     18.000 baseline hours in setup: sess113.pfb
                     Frequency sets (dups not shown):   1  3  6  9



  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            73.7
   3C454.3             28.0

  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 

