  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: The parsec scale jet in the enigmatic TeV blazar 0229+200
 Exp. Code:  EG049C  


Schedule Version:       1.00
Processed by SCHED version:  10.00  Release Sept. 15, 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
               The parsec scale jet in the enigmatic TeV blazar 0229+200
  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  20 Oct 2011   Day 293 ---

 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

18 00 00  0229+200     21 46 08   6.4  63.7 -4.8  D    0.0     0        0   18 00 00
18 14 00  ---          22 00 10   9.2  62.0 -4.6       0.0     0      108   18 00 04

18 15 00  0229+200     22 01 10   9.4  61.8 -4.5       0.0    39      108   18 15 00
18 29 00  ---          22 15 13  12.1  60.0 -4.3       0.0   840      217   18 15 04

18 30 00  0239+175     22 16 13  11.8  63.4 -4.4       0.0    28      217   18 30 00
18 33 00  ---          22 19 13  12.5  63.0 -4.4       0.0   180      240   18 30 04

18 34 00  0229+200     22 20 13  13.1  59.3 -4.2       0.0    28      240   18 34 00
18 48 00  ---          22 34 16  15.8  57.4 -4.0       0.0   840      348   18 34 04

18 49 00  0229+200     22 35 16  16.0  57.2 -4.0       0.0    39      348   18 49 00
19 03 00  ---          22 49 18  18.6  55.2 -3.7       0.0   840      457   18 49 04

19 04 00  0234+285     22 50 18  12.6  48.9 -3.8       0.0    16      457   19 04 00
19 11 00  ---          22 57 19  13.7  47.9 -3.7       0.0   420      511   19 04 04

19 12 00  0229+200     22 58 20  20.3  53.8 -3.6       0.0    16      511   19 12 00
19 26 00  ---          23 12 22  22.8  51.5 -3.4       0.0   840      619   19 12 04

19 27 00  0239+175     23 13 22  22.9  55.0 -3.5       0.0    28      619   19 27 00
19 30 00  ---          23 16 23  23.4  54.5 -3.4       0.0   180      643   19 27 04

19 31 00  0229+200     23 17 23  23.7  50.6 -3.3       0.0    28      643   19 31 00
19 45 00  ---          23 31 25  26.1  48.1 -3.0       0.0   840      751   19 31 04

19 46 00  0229+200     23 32 25  26.2  48.0 -3.0       0.0    39      751   19 46 00
20 00 00  ---          23 46 28  28.5  45.3 -2.8       0.0   840      859   19 46 04

20 01 00  0229+200     23 47 28  28.7  45.1 -2.8       0.0    39      859   20 01 00
20 15 00  ---          00 01 30  30.9  42.3 -2.5       0.0   840      968   20 01 04
Schedule for HART      (Code Hh )                                   Page   3
               The parsec scale jet in the enigmatic TeV blazar 0229+200
  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  20 Oct 2011   Day 293 ---

20 16 00  0229+200     00 02 30  31.0  42.1 -2.5       0.0    39      968   20 16 00
20 30 00  ---          00 16 32  33.1  39.0 -2.3       0.0   840     1076   20 16 04

20 31 00  0239+175     00 17 33  33.8  42.8 -2.4       0.0    28     1076   20 31 00
20 34 00  ---          00 20 33  34.3  42.2 -2.4       0.0   180     1099   20 31 04

20 35 00  0229+200     00 21 33  33.8  37.9 -2.2       0.0    28     1099   20 35 00
20 49 00  ---          00 35 36  35.6  34.6 -2.0       0.0   840     1208   20 35 04

20 50 00  0234+285     00 36 36  27.9  30.2 -2.0       0.0    16     1208   20 50 00
20 57 00  ---          00 43 37  28.7  28.7 -1.9       0.0   420     1262   20 50 04

20 58 00  0229+200     00 44 37  36.7  32.4 -1.8       0.0    16     1262   20 58 00
21 12 00  ---          00 58 39  38.4  28.7 -1.6       0.0   840     1370   20 58 04

21 13 00  0229+200     00 59 40  38.5  28.5 -1.6       0.0    39     1370   21 13 00
21 27 00  ---          01 13 42  39.9  24.6 -1.3       0.0   840     1479   21 13 04

21 28 00  0239+175     01 14 42  41.3  28.5 -1.5       0.0    28     1479   21 28 00
21 31 00  ---          01 17 42  41.7  27.6 -1.4       0.0   180     1502   21 28 04

21 32 00  0229+200     01 18 43  40.3  23.2 -1.2       0.0    28     1502   21 32 00
21 46 00  ---          01 32 45  41.5  19.1 -1.0       0.0   840     1610   21 32 04

21 47 00  0229+200     01 33 45  41.5  18.8 -1.0       0.0    39     1610   21 47 00
22 00 00  ---          01 46 47  42.4  14.9 -0.8       0.0   780     1711   21 47 04


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


 Setup file: sess311.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: MARK5B            Bits per sample: 2         Sample rate: 32.000
   Number of channels: 16    DBE type:                  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
             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 these setups 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
    Matching frequency sets:  13

   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 --                         The parsec scale jet in the enigmatic TeV blazar 0229+200
     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)

 * 0229+200          02 29 59.796088   * 02 32 48.616000     02 33 30.969355       0.00
                     20 04 06.23334    * 20 17 17.45000      20 20 32.78143        0.00
                     From catalog imbedded in main SCHED input file.
                        3.250 scan and    245.800 baseline hours in setup: sess311.C1024
                     Frequency sets (dups not shown):   1  2  3  4  5  6  7  8  9 10 11 12 13

   J0237+2848        02 34 55.589590   * 02 37 52.405677     02 38 36.825359       0.01
 * 0234+285          28 35 11.40778    * 28 48 08.99003      28 51 19.88160        0.01
   J0237+28          /irasoft/sched/catalogs/sources.vlba
                     GSFC 2010a astro solution     53368 Observations
                        0.233 scan and     18.200 baseline hours in setup: sess311.C1024
                     Frequency sets (dups not shown):   1  2  3  4  5  6  7  8  9 10 11 12 13

   J0242+1742        02 39 36.812122   * 02 42 24.268275     02 43 06.249244       0.09
 * 0239+175          17 30 14.07693    * 17 42 58.84921      17 46 07.64833        0.14
                     /irasoft/sched/catalogs/sources.vlba
                     GSFC 2010a astro solution       252 Observations
                        0.200 scan and     15.600 baseline hours in setup: sess311.C1024
                     Frequency sets (dups not shown):   1  2  3  4  5  6  7  8  9 10 11 12 13



  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) 
   0229+200           163.9
   0234+285           157.1
   0239+175           163.2

  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 

