  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: The parsec scale jet in the enigmatic TeV blazar 0229+200
 Exp. Code:  EG049E  


Schedule Version:       1.00
Processed by SCHED version:  10.10  Release of about Feb. 14, 2012

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
----------------------------------------------------------------------------------------

 --- Tue   5 Jun 2012   Day 157 ---

 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

03 00 00  0229+200     21 46 31   6.5  63.7 -4.8  D    0.0     0        0   03 00 00
03 14 00  ---          22 00 33   9.3  61.9 -4.5       0.0     0      108   03 00 04

03 15 00  0229+200     22 01 34   9.5  61.8 -4.5       0.0    39      108   03 15 00
03 29 00  ---          22 15 36  12.2  60.0 -4.3       0.0   840      217   03 15 04

03 30 00  0239+175     22 16 36  11.9  63.3 -4.4       0.0    28      217   03 30 00
03 33 00  ---          22 19 37  12.5  62.9 -4.4       0.0   180      240   03 30 04

03 34 00  0229+200     22 20 37  13.2  59.3 -4.2       0.0    28      240   03 34 00
03 48 00  ---          22 34 39  15.9  57.3 -4.0       0.0   840      348   03 34 04

03 49 00  0229+200     22 35 39  16.1  57.2 -4.0       0.0    39      348   03 49 00
04 03 00  ---          22 49 42  18.7  55.1 -3.7       0.0   840      457   03 49 04

04 04 00  0234+285     22 50 42  12.6  48.8 -3.8       0.0    16      457   04 04 00
04 11 00  ---          22 57 43  13.8  47.8 -3.7       0.0   420      511   04 04 04

04 12 00  0229+200     22 58 43  20.3  53.7 -3.6       0.0    16      511   04 12 00
04 26 00  ---          23 12 45  22.8  51.4 -3.3       0.0   840      619   04 12 04

04 27 00  0239+175     23 13 45  23.0  55.0 -3.5       0.0    28      619   04 27 00
04 30 00  ---          23 16 46  23.5  54.5 -3.4       0.0   180      643   04 27 04

04 31 00  0229+200     23 17 46  23.7  50.6 -3.3       0.0    28      643   04 31 00
04 45 00  ---          23 31 48  26.1  48.1 -3.0       0.0   840      751   04 31 04

04 46 00  0229+200     23 32 49  26.3  47.9 -3.0       0.0    39      751   04 46 00
05 00 00  ---          23 46 51  28.6  45.2 -2.8       0.0   840      859   04 46 04

05 01 00  0229+200     23 47 51  28.7  45.0 -2.8       0.0    39      859   05 01 00
05 15 00  ---          00 01 53  30.9  42.2 -2.5       0.0   840      968   05 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
----------------------------------------------------------------------------------------

 --- Tue   5 Jun 2012   Day 157 ---

05 16 00  0229+200     00 02 53  31.1  42.0 -2.5       0.0    39      968   05 16 00
05 30 00  ---          00 16 56  33.1  38.9 -2.3       0.0   840     1076   05 16 04

05 31 00  0239+175     00 17 56  33.9  42.8 -2.4       0.0    28     1076   05 31 00
05 34 00  ---          00 20 56  34.3  42.1 -2.4       0.0   180     1099   05 31 04

05 35 00  0229+200     00 21 57  33.8  37.8 -2.2       0.0    28     1099   05 35 00
05 49 00  ---          00 35 59  35.7  34.5 -2.0       0.0   840     1208   05 35 04

05 50 00  0234+285     00 36 59  28.0  30.1 -2.0       0.0    16     1208   05 50 00
05 57 00  ---          00 44 00  28.7  28.6 -1.9       0.0   420     1262   05 50 04

05 58 00  0229+200     00 45 00  36.8  32.3 -1.8       0.0    16     1262   05 58 00
06 12 00  ---          00 59 03  38.4  28.6 -1.6       0.0   840     1370   05 58 04

06 13 00  0229+200     01 00 03  38.5  28.4 -1.6       0.0    39     1370   06 13 00
06 27 00  ---          01 14 05  39.9  24.5 -1.3       0.0   840     1479   06 13 04

06 28 00  0239+175     01 15 05  41.4  28.4 -1.5       0.0    28     1479   06 28 00
06 31 00  ---          01 18 06  41.7  27.5 -1.4       0.0   180     1502   06 28 04

06 32 00  0229+200     01 19 06  40.4  23.1 -1.2       0.0    28     1502   06 32 00
06 46 00  ---          01 33 08  41.5  19.0 -1.0       0.0   840     1610   06 32 04

06 47 00  0229+200     01 34 08  41.6  18.7 -1.0       0.0    39     1610   06 47 00
07 00 00  ---          01 47 11  42.4  14.8 -0.8       0.0   780     1711   06 47 04


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


 ======== Setup file: sess212.C1024
   Matching groups in /irasoft/sched/catalogs/freq.dat:
     hh6cm           Values confirmed by E-mail Jonathan Quick 221105 (CR)

   Setup group:    8         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 30.603380       0.00
                     20 04 06.23334    * 20 17 17.45000      20 20 28.61826        0.00
                     From catalog imbedded in main SCHED input file.
                        3.250 scan and    245.800 baseline hours in setup: sess212.C1024
                     Frequency sets (dups not shown):   1  2  3  4  5  6  7  8  9 12 13

   J0237+2848        02 34 55.589591   * 02 37 52.405678     02 38 36.392534       0.11
 * 0234+285          28 35 11.40769    * 28 48 08.98994      28 51 15.19757        0.10
   J0237+28          /irasoft/sched/catalogs/sources.vlba
                     rfc_2011d Petrov, 2011, unpublished 1059 observations
                        0.233 scan and     18.200 baseline hours in setup: sess212.C1024
                     Frequency sets (dups not shown):   1  2  3  4  5  6  7  8  9 12 13

   J0242+1742        02 39 36.812112   * 02 42 24.268265     02 43 05.870368       0.12
 * 0239+175          17 30 14.07677    * 17 42 58.84905      17 46 03.77563        0.14
                     /irasoft/sched/catalogs/sources.vlba
                     rfc_2011d Petrov, 2011, unpublished 570 observations
                        0.200 scan and     15.600 baseline hours in setup: sess212.C1024
                     Frequency sets (dups not shown):   1  2  3  4  5  6  7  8  9 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            32.8
   0234+285            31.2
   0239+175            31.2

  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 

