  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: 5cm test experiment
 Exp. Code:  f04m1   


Schedule Version:       1.00                                              
Processed by SCHED version: Release of 18 Sept. 2003                      

PI:       Zsolt Paragi                                                    

Address:  JIVE                                                            
                                                                          
                                                                          
                                                                          

Phone:    +31-521-596536                                                  
EMAIL:    paragi@jive.nl                                                  
Fax:                                                                      
Phone during observation: +31-521-596536                                  

Observing mode:                                                           

Notes:    5cm band test (256 Mbps, dualpol, 2 bit sampling)               
          Please send the tape or disk pack to JIVE                       
                                                                          
                                                                          

Schedule for HART      (Code Hh )                                   Page   2
               5cm test experiment
  UP:  D => Below limits;  H => Below horizon mask.  blank => Up.
  Early: Seconds between end of slew and start.   Dwell: On source seconds. 
  Tapes: Drive, Index, Start footage / Direction, Head Group, End footage.
  TPStart:  Tape motion start time.  Frequencies are LO sum (band edge).
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)
----------------------------------------------------------------------------------------

 --- Tue  24 Feb 2004   Day  55 ---

 Next scan frequencies:  6028.49  6028.49  6028.49  6028.49  6044.49  6044.49
                         6044.49  6044.49
 Next BBC frequencies:    148.49   148.49   148.49   148.49   164.49   164.49
                          164.49   164.49
 Next scan bandwidths:      8.00     8.00     8.00     8.00     8.00     8.00
                            8.00     8.00

10 00 00  3C454.3      22 05 17  46.3  17.1 -0.8       0.0     0   1  1      0  10 00 00
10 11 00  ---          22 16 19  46.9  13.4 -0.6       0.0   660   F  1   8800

10 12 00  3C454.3      22 17 19  47.0  13.0 -0.6       0.0    36   1  1   8800  10 12 00
10 23 00  ---          22 28 20  47.5   9.2 -0.4       0.0   660   F  1  17600

10 24 00  3C454.3      22 29 21  47.5   8.8 -0.4       0.0    36   1  2  17600  10 24 00
10 35 00  ---          22 40 22  47.8   4.9 -0.2       0.0   660   R  1   8800

 Next scan frequencies:  6658.49  6658.49  6658.49  6658.49  6674.49  6674.49
                         6674.49  6674.49
 Next BBC frequencies:    148.49   148.49   148.49   148.49   164.49   164.49
                          164.49   164.49

10 37 00  3C454.3      22 42 23  47.8   4.2 -0.2       0.0    95   1  2   8800  10 37 00
10 48 00  ---          22 53 25  47.9   0.3  0.0       0.0   660   R  1      0

10 49 00  3C454.3      22 54 25  47.9 359.9  0.0       0.0    36   1  3      0  10 49 00
11 00 00  ---          23 05 27  47.9 356.0  0.2       0.0   660   F  1   8800


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


 Setup file: 256MBPS.5CMOH
   Matches group hh5cm_S2 in ./freq.dat
    Values confirmed by E-mail Jonathan Quick 291100 (CR)
    ****** Only   63.02 of   64.00 MHz total bandwidth is within the IFs
           in the setup file before any FREQ or DOPPLER shifts.

   Setup group:    5         Station: HART              Total bit rate:  256
   Format: MKIV1:2           Bits per sample: 2         Sample rate: 16.000
   Number of channels:  8    Passes/head pos:   1       Speedup factor:   1.00

   Tape speeds: Low density - 270.000 ips,  High density - 160.00 ips
   Time per pass for  17600 ft, High density tapes is: 00:22:00

   1st LO=   5880.00   5880.00   5880.00   5880.00   5880.00   5880.00   5880.00   5880.00
   Net SB=         L         L         U         U         L         L         U         U
   Pol.  =      RCP       LCP       RCP       LCP       RCP       LCP       RCP       LCP 
   BBC   =         2         1         2         1         4         3         4         3
   BBC SB=         L         L         U         U         L         L         U         U
   IF    =        2N        1N        2N        1N        2N        1N        2N        1N

  The following frequency sets based on this setup were used.

   Frequency Set:   5  Setup file default.  No pcal detection.
   LO sum=    6028.49   6028.49   6028.49   6028.49   6044.49   6044.49   6044.49   6044.49
   BBC fr=     148.49    148.49    148.49    148.49    164.49    164.49    164.49    164.49
   Bandwd=      8.000     8.000     8.000     8.000     8.000     8.000     8.000     8.000

   Track assignments are: 
    track1=   2, 10, 18, 26,  3, 11, 19, 27
    barrel=roll_off 


 Setup file: 256MBPS.5CM
   Matches group hh4.5cm_S2 in ./freq.dat
    Values confirmed by E-mail Jonathan Quick 291100 (CR)
    ****** Only   63.02 of   64.00 MHz total bandwidth is within the IFs
           in the setup file before any FREQ or DOPPLER shifts.

   Setup group:   10         Station: HART              Total bit rate:  256
   Format: MKIV1:2           Bits per sample: 2         Sample rate: 16.000
   Number of channels:  8    Passes/head pos:   1       Speedup factor:   1.00

   Tape speeds: Low density - 270.000 ips,  High density - 160.00 ips
   Time per pass for  17600 ft, High density tapes is: 00:22:00

   1st LO=   6510.00   6510.00   6510.00   6510.00   6510.00   6510.00   6510.00   6510.00
   Net SB=         L         L         U         U         L         L         U         U
   Pol.  =      RCP       LCP       RCP       LCP       RCP       LCP       RCP       LCP 
   BBC   =         2         1         2         1         4         3         4         3
   BBC SB=         L         L         U         U         L         L         U         U
   IF    =        2N        1N        2N        1N        2N        1N        2N        1N

  The following frequency sets based on this setup were used.

   Frequency Set:  10  Setup file default.  No pcal detection.
   LO sum=    6658.49   6658.49   6658.49   6658.49   6674.49   6674.49   6674.49   6674.49
   BBC fr=     148.49    148.49    148.49    148.49    164.49    164.49    164.49    164.49
   Bandwd=      8.000     8.000     8.000     8.000     8.000     8.000     8.000     8.000

   Track assignments are: 
    track1=   2, 10, 18, 26,  3, 11, 19, 27
    barrel=roll_off 
 SOURCE LIST -- 5cm test experiment
     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).

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

   J2253+1608        22 51 29.519733   * 22 53 57.747932     22 54 07.958015 
   2251+158          15 52 54.34806    * 16 08 53.56089      16 10 01.05549 
 * 3C454.3           /aps3/sched/catalogs/sources.vlba
   J2253+16          ICRF - Ext.1 Source - 1998 IERS Annual Report



  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) 
   3C454.3             26.6

  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 

