  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: X band FTP-FT Experiment F12X1
 Exp. Code:  F12X1   


Schedule Version:       1.00
Processed by SCHED version:  10.00  Release Sept. 15, 2011

PI:       Jun YANG

Address:  JIVE, The Netherlands
 
 
 

Phone:    +31 521 596 507
EMAIL:    yang@jive.nl
Fax:
Phone during observation:

Observing mode: 512-16-2

Notes:    512 Mbps, 16 x 8 MHz, 2 bit sampling
          Check antenna pointing, Please
          Three FTP-FT scans scheduled.
 

Schedule for HART      (Code Hh )                                   Page   2
               X band FTP-FT Experiment F12X1
  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
----------------------------------------------------------------------------------------

 --- Fri  24 Feb 2012   Day  55 ---

 Next scan frequencies:  8391.49  8391.49  8391.49  8391.49  8407.49  8407.49
                         8407.49  8407.49  8423.49  8423.49  8423.49  8423.49
                         8439.49  8439.49  8439.49  8439.49
 Next BBC frequencies:    311.49   311.49   311.49   311.49   327.49   327.49
                          327.49   327.49   343.49   343.49   343.49   343.49
                          359.49   359.49   359.49   359.49
 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  0528+134     02 06 11  26.3  57.9 -3.4       0.0     0        0   14 00 00
14 08 00  ---          02 14 12  27.9  56.6 -3.3       0.0   480       31   14 00 04

14 12 00  0528+134     02 18 13  28.6  55.9 -3.2       0.0   219       31   14 12 00
14 20 00  ---          02 26 14  30.1  54.4 -3.1       0.0   480       62   14 12 04

14 22 00  0528+134     02 28 15  30.5  54.0 -3.1       0.0    99       62   14 22 00
14 30 00  ---          02 36 16  31.9  52.5 -2.9       0.0   480       93   14 22 04

14 32 00  0528+134     02 38 16  32.3  52.1 -2.9       0.0    99       93   14 32 00
14 40 00  ---          02 46 17  33.7  50.5 -2.8       0.0   480      124   14 32 04

14 42 00  0528+134     02 48 18  34.0  50.1 -2.7       0.0    99      124   14 42 00
14 50 00  ---          02 56 19  35.4  48.4 -2.6       0.0   480      155   14 42 04

14 52 00  0528+134     02 58 19  35.7  48.0 -2.6       0.0    99      155   14 52 00
15 00 00  ---          03 06 21  37.0  46.2 -2.4       0.0   480      186   14 52 04


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


 Setup file: sess112.X512
   Matching groups in /aps3/sched10.0/catalogs/freq.dat:
     hh4cm           Values confirmed by E-mail Jonathan Quick 291100 (CR)

   Setup group:    7         Station: HART              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=   8080.00   8080.00   8080.00   8080.00   8080.00   8080.00   8080.00   8080.00
             8080.00   8080.00   8080.00   8080.00   8080.00   8080.00   8080.00   8080.00
   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   =         2         1         2         1         4         3         4         3
                   6         5         6         5         8         7         8         7
   BBC SB=         L         L         U         U         L         L         U         U
                   L         L         U         U         L         L         U         U
   IF    =        2N        1N        2N        1N        2N        1N        2N        1N
                  2N        1N        2N        1N        2N        1N        2N        1N

  The following frequency sets based on these setups were used.

   Frequency Set:  11  Setup file default.
   LO sum=    8391.49   8391.49   8391.49   8391.49   8407.49   8407.49   8407.49   8407.49
              8423.49   8423.49   8423.49   8423.49   8439.49   8439.49   8439.49   8439.49
   BBC fr=     311.49    311.49    311.49    311.49    327.49    327.49    327.49    327.49
               343.49    343.49    343.49    343.49    359.49    359.49    359.49    359.49
   Bandwd=      8.000     8.000     8.000     8.000     8.000     8.000     8.000     8.000
                8.000     8.000     8.000     8.000     8.000     8.000     8.000     8.000
    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 
 SOURCES USED IN RECORDING SCANS --                         X band FTP-FT Experiment F12X1
     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)

   J0530+1331        05 28 06.759216   * 05 30 56.416747     05 31 39.288347       0.21
 * 0528+134          13 29 42.28887    * 13 31 55.14954      13 32 20.85266        0.23
   J0530+13          /aps3/sched10.0/catalogs/sources.vlba
                     GSFC 2010a astro solution    133158 Observations
                        0.800 scan and     44.000 baseline hours in setup: sess112.X512
                     Frequency sets (dups not shown):   1  2  3  4  5  6  7 10 11



  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) 
   0528+134           107.4

  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 

