  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: M87 monitoring
 Exp. Code:  EG051E  


Schedule Version:       1.00
Processed by SCHED version:   9.40  Release Jan. 13, 2011.

PI:       M. Giroletti

Address:  INAF Istituto di Radioastronomia
          Via Gobetti 101
          40129 Bologna
          Italy

Phone:    +39 051 639 9394
EMAIL:    giroletti@ira.inaf.it
Fax:      +39 051 639 9431
Phone during observation: +39 347 906 6221

Observing mode: EVN, 6cm, 1Gb/s

Notes:
 
 
 

Schedule for HART      (Code Hh )                                   Page   2
               M87 monitoring
  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   2 Jun 2011   Day 153 ---

 Next scan frequencies:  4942.49  4942.49  4942.49  4942.49  4974.49  4974.49
                         4974.49  4974.49  5006.49  5006.49  5006.49  5006.49
                         5038.49  5038.49  5038.49  5038.49
 Next BBC frequencies:    342.49   342.49   342.49   342.49   374.49   374.49
                          374.49   374.49   406.49   406.49   406.49   406.49
                          438.49   438.49   438.49   438.49
 Next scan bandwidths:     16.00    16.00    16.00    16.00    16.00    16.00
                           16.00    16.00    16.00    16.00    16.00    16.00
                           16.00    16.00    16.00    16.00

14 50 00  M87          09 23 39  30.5  55.9 -3.1       0.0     0        0   14 49 55
15 05 00  ---          09 38 41  33.2  53.0 -2.9       0.0   900      117   14 49 59

15 05 40  M87          09 39 21  33.3  52.9 -2.9       0.0    19      117   15 05 35
15 20 00  ---          09 53 44  35.9  49.9 -2.6       0.0   860      228   15 05 39

15 20 40  M87          09 54 24  36.0  49.8 -2.6       0.0    19      228   15 20 35
15 35 00  ---          10 08 46  38.4  46.6 -2.4       0.0   860      340   15 20 39

15 35 40  M87          10 09 26  38.5  46.4 -2.4       0.0    19      340   15 35 35
15 50 00  ---          10 23 49  40.8  43.0 -2.1       0.0   860      452   15 35 39

15 50 40  M87          10 24 29  40.9  42.8 -2.1       0.0    19      452   15 50 35
16 05 00  ---          10 38 51  43.0  39.0 -1.9       0.0   860      563   15 50 39

16 05 40  M87          10 39 31  43.1  38.9 -1.9       0.0    19      563   16 05 35
16 20 00  ---          10 53 54  45.0  34.8 -1.6       0.0   860      675   16 05 39

16 20 40  M87          10 54 34  45.1  34.6 -1.6       0.0    19      675   16 20 35
16 35 00  ---          11 08 56  46.8  30.2 -1.4       0.0   860      786   16 20 39

16 35 40  M87          11 09 36  46.9  30.0 -1.4       0.0    19      786   16 35 35
16 50 00  ---          11 23 59  48.4  25.3 -1.1       0.0   860      898   16 35 39


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


 Setup file: sess211.C1024
   Matching groups in /irasoft/sched/catalogs/freq.dat:
     hh6cm           Values confirmed by E-mail Jonathan Quick 221105 (CR)

   Setup group:    9         Station: HART              Total bit rate: 1024
   Format: MKIV1:2           Bits per sample: 2         Sample rate: 32.000
   Number of channels: 16    DBE type:                  Speedup factor:   0.50

   Disk used to record data.

   1st LO=   4600.00   4600.00   4600.00   4600.00   4600.00   4600.00   4600.00   4600.00
             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
                   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 this setup were used.

   Frequency Set:  13  Setup file default.
   LO sum=    4942.49   4942.49   4942.49   4942.49   4974.49   4974.49   4974.49   4974.49
              5006.49   5006.49   5006.49   5006.49   5038.49   5038.49   5038.49   5038.49
   BBC fr=     342.49    342.49    342.49    342.49    374.49    374.49    374.49    374.49
               406.49    406.49    406.49    406.49    438.49    438.49    438.49    438.49
   Bandwd=     16.000    16.000    16.000    16.000    16.000    16.000    16.000    16.000
               16.000    16.000    16.000    16.000    16.000    16.000    16.000    16.000

   Track assignments are: 
    track1=   2, 10, 18, 26,  3, 11, 19, 27, 66, 74, 82, 90, 67, 75, 83, 91
    barrel=roll_off 
 SOURCES USED IN RECORDING SCANS --                         M87 monitoring
     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)

 * M87               12 28 17.569280   * 12 30 49.423382     12 31 25.629868       0.00
                     12 40 01.74900    * 12 23 28.04382      12 19 36.40487        0.00
                     From catalog imbedded in main SCHED input file.
                        1.922 scan and    149.933 baseline hours in setup: sess211.C1024



  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) 
   M87                109.8

  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 

