  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: e-EVN: EG096B, EL058C, ED042
 Exp. Code:  eg096bUB


Schedule Version:       1.00
Processed by SCHED version:  11.40  Release 11.4.  March 14, 2015

PI:       Gawronsky, Lobanov, Davelaar

Address:  JIVE
          Oude Hoogeveensedijk 4
          Dwingeloo
          Netherlands

Phone:    +31 521 596 536
EMAIL:    marcote@jive.eu
Fax:      +31 521 596 539
Phone during observation: +31 521 596 508

Observing mode: realtime e-vlbi

Notes:    UniBoard test version:  16MHz subbands
 
 
 

Schedule for HART      (Code Hh )                                   Page   2
               e-EVN: EG096B, EL058C, ED042
  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  20 Jun 2017   Day 171 ---

 ---------- clock-search ----------

 Next scan frequencies:  4830.49  4830.49  4830.49  4830.49  4894.49  4894.49  4894.49  4894.49
                         4958.49  4958.49  4958.49  4958.49  5022.49  5022.49  5022.49  5022.49
 Next BBC frequencies:    230.49   230.49   230.49   230.49   294.49   294.49   294.49   294.49
                          358.49   358.49   358.49   358.49   422.49   422.49   422.49   422.49
 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

09 00 00  J0854+2006   04 45 49  13.9  59.1 -4.2       0.0     0        0   09 00 00
09 10 00  =0851+202    04 55 50  15.9  57.7 -4.0       0.0   600       77   09 00 01

09 11 00  J0854+2006   04 56 51  16.0  57.6 -4.0       0.0    39       77   09 11 00
09 25 00  =0851+202    05 10 53  18.7  55.5 -3.7       0.0   840      185   09 11 01

09 26 00  J0854+2006   05 11 53  18.9  55.4 -3.7       0.0    39      185   09 26 00
09 40 00  =0851+202    05 25 55  21.4  53.2 -3.5       0.0   840      294   09 26 01

09 41 00  J0854+2006   05 26 55  21.6  53.0 -3.5       0.0    39      294   09 41 00
09 55 00  =0851+202    05 40 58  24.1  50.6 -3.2       0.0   840      402   09 41 01

09 56 00  J0854+2006   05 41 58  24.3  50.5 -3.2       0.0    39      402   09 56 00
10 10 00  =0851+202    05 56 00  26.7  47.9 -3.0       0.0   840      510   09 56 01

10 11 00  J0854+2006   05 57 00  26.8  47.8 -3.0       0.0    39      510   10 11 00
10 25 00  =0851+202    06 11 03  29.1  45.1 -2.7       0.0   840      618   10 11 01

10 26 00  J0854+2006   06 12 03  29.3  44.9 -2.7       0.0    39      618   10 26 00
10 40 00  =0851+202    06 26 05  31.4  42.0 -2.5       0.0   840      727   10 26 01

10 42 00  J0854+2006   06 28 05  31.7  41.6 -2.5       0.0    99      727   10 42 00
10 55 00  =0851+202    06 41 08  33.6  38.7 -2.2       0.0   780      827   10 42 01

10 56 00  J0854+2006   06 42 08  33.8  38.5 -2.2       0.0    39      827   10 56 00
11 10 00  =0851+202    06 56 10  35.7  35.2 -2.0       0.0   840      935   10 56 01

11 11 00  J0854+2006   06 57 10  35.8  35.0 -2.0       0.0    39      935   11 11 00
11 25 00  =0851+202    07 11 13  37.5  31.5 -1.7       0.0   840     1043   11 11 01

11 26 00  J0854+2006   07 12 13  37.6  31.2 -1.7       0.0    39     1043   11 26 00
11 40 00  =0851+202    07 26 15  39.2  27.5 -1.5       0.0   840     1152   11 26 01

11 41 00  J0854+2006   07 27 15  39.3  27.2 -1.5       0.0    39     1152   11 41 00
11 55 00  =0851+202    07 41 17  40.6  23.3 -1.2       0.0   840     1260   11 41 01


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


 ======== Setup file: sess117.C2048e
   Matching groups in /home/guest/rmc/SCHED/sched11.4/catalogs/freq.dat:
     hh6cm           Values confirmed by E-mail Jonathan Quick 20140219 (CR)
    ****** Only  128.00 of  256.00 MHz total bandwidth is within the IFs
           in the setup file before any FREQ or DOPPLER shifts.

   Setup group:    3         Station: HART              Total bit rate:  1024
   Format: VDIF              Bits per sample: 2         Sample rate: 32.000
   Number of channels: 16    DBE type: DBBC_DDC         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
   IF SB =         U         U         U         U         U         U         U         U
                   U         U         U         U         U         U         U         U
   Pol.  =      RCP       LCP       RCP       LCP       RCP       LCP       RCP       LCP 
                RCP       LCP       RCP       LCP       RCP       LCP       RCP       LCP 
   BBC   =         1         9         1         9         3        11         3        11
                   5        13         5        13         7        15         7        15
   BBC SB=         L         L         U         U         L         L         U         U
                   L         L         U         U         L         L         U         U
   IF    =        A1        C1        A1        C1        A1        C1        A1        C1
                  B2        C1        B2        C1        B2        C1        B2        C1

  The following frequency sets based on these setups were used.

   Frequency Set:  10  Setup file default.  Used with PCAL = off
   LO sum=   4830.49  4830.49  4830.49  4830.49  4894.49  4894.49  4894.49  4894.49
             4958.49  4958.49  4958.49  4958.49  5022.49  5022.49  5022.49  5022.49
   BBC fr=    230.49   230.49   230.49   230.49   294.49   294.49   294.49   294.49
              358.49   358.49   358.49   358.49   422.49   422.49   422.49   422.49
   Bandwd=     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
    Matching frequency sets:  10

   Track assignments are: 
    track1=   1,  2,  3,  4,  5,  6,  7,  8,  9, 10, 11, 12, 13, 14, 15, 16
    barrel=roll_off 

 POSITIONS OF SOURCES USED IN RECORDING SCANS

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

   0851+202          08 51 57.250617   * 08 54 48.874929     08 55 46.916720       0.11
 * J0854+2006        20 17 58.41738    * 20 06 30.64083      20 02 29.67103        0.10
                     /home/guest/rmc/SCHED/sched11.4/catalogs/sources.rfc
                     rfc_2015a Petrov, 2015, unpublished.  232903 observations



SOURCE SCAN SUMMARY FOR SOURCES LISTED ABOVE

     Scan hours are for recording scans only. 
     Baseline hours are only counted for scans above horizon at both ends.
  Source       Setup file             Frequency sets                  Observing hours
                                   (duplicates not shown)              Scan  Baseline
  J0854+2006 sess117.C2048e        1 2 3 4 5 6 7 8 9 10              2.717   149.417


EFFECT OF SOLAR CORONA

  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) 
   J0854+2006          41.5

  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 

