  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: Network Monitoring Experiment
 Exp. Code:  N19K1   


Schedule Version:       1.00
Processed by SCHED version:  11.50  Development version 11.5. Started Apr. 2

PI:       Katharina Immer

Address:  JIVE
          Postbus 2
          7990 AA Dwingeloo
          The Netherlands

Phone:    +31-521-596507
EMAIL:    immer@jive.eu
Fax:
Phone during observation: +31-521-596507

Observing mode:

Notes:    1.3 cm (K-band) ftp fringe test for session 1/2019
          (1024 Mbps, L+R, 2-bit sampling, 8 x 16 MHz filters)
          Please send the disk pack by express to JIVE, NO PCAL
          Please DO NOT use the phase cal signal.


COVER LETTER:


This is the schedule for the 1.3 cm K-band fringe test on March 12 2019
involving 18 telescopes: Jb2 Ef Mc Nt On60 T6 Ur Tr Ys Hh Sv Zc Bd Sr Mh Kt Ky Ku
The FTP-NME uses a standard setup at 1024 Mbps:

The schedule consists of long integrations on strong calibrators:

Ftp-fringe tests are scheduled every 20 min throughout the experiment:
12:10:00 0234+285
12:30:00 0234+285
12:50:00 0234+285
13:10:00 0528+134
13:30:00 0528+134
13:50:00 0528+134
14:10:00 0528+134
14:30:00 0528+134
14:50:00 0528+134

Clear skies!

Katharina
Mattermost: coms.evlbi.org
Schedule for HART      (Code Hh )                                   Page   2
               Network Monitoring Experiment
  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  12 Mar 2019   Day  71 ---

 Next scan frequencies:  22187.49  22187.49  22187.49  22187.49  22219.49  22219.49  22219.49  22219.49
                         22251.49  22251.49  22251.49  22251.49  22283.49  22283.49  22283.49  22283.49
 Next BBC frequencies:     187.49    187.49    187.49    187.49    219.49    219.49    219.49    219.49
                           251.49    251.49    251.49    251.49    283.49    283.49    283.49    283.49
 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

12 00 00  0234+285     01 10 08  31.2  22.8 -1.5       0.0     0        0   12 00 00
12 05 00  ---          01 15 09  31.6  21.6 -1.4       0.0   300       39   12 00 01

12 07 00  0234+285     01 17 09  31.8  21.1 -1.4       0.0    99       39   12 07 00
12 20 00  ---          01 30 11  32.8  17.9 -1.1       0.0   780      139   12 07 01

12 22 00  0234+285     01 32 12  32.9  17.4 -1.1       0.0    99      139   12 22 00
12 25 00  ---          01 35 12  33.1  16.7 -1.1       0.0   180      162   12 22 01

12 27 00  0234+285     01 37 13  33.3  16.2 -1.0       0.0    99      162   12 27 00
12 40 00  ---          01 50 15  34.0  12.9 -0.8       0.0   780      263   12 27 01

12 42 00  0234+285     01 52 15  34.1  12.4 -0.8       0.0    99      263   12 42 00
12 45 00  ---          01 55 16  34.2  11.6 -0.7       0.0   180      286   12 42 01

12 47 00  0234+285     01 57 16  34.3  11.1 -0.7       0.0    99      286   12 47 00
13 00 00  ---          02 10 18  34.8   7.6 -0.5       0.0   780      386   12 47 01

13 04 00  0528+134     02 14 19  27.8  56.6 -3.3       0.0   127      386   13 04 00
13 05 00  ---          02 15 19  28.0  56.4 -3.3       0.0    60      394   13 04 01

13 07 00  0528+134     02 17 19  28.4  56.1 -3.2       0.0    99      394   13 07 00
13 20 00  ---          02 30 21  30.8  53.7 -3.0       0.0   780      495   13 07 01

13 22 00  0528+134     02 32 22  31.1  53.3 -3.0       0.0    99      495   13 22 00
13 25 00  ---          02 35 22  31.7  52.7 -2.9       0.0   180      518   13 22 01

13 27 00  0528+134     02 37 22  32.0  52.4 -2.9       0.0    99      518   13 27 00
13 40 00  ---          02 50 25  34.3  49.7 -2.7       0.0   780      618   13 27 01

13 42 00  0528+134     02 52 25  34.7  49.3 -2.7       0.0    99      618   13 42 00
13 45 00  ---          02 55 25  35.2  48.7 -2.6       0.0   180      642   13 42 01

13 47 00  0528+134     02 57 26  35.5  48.2 -2.6       0.0    99      642   13 47 00
14 00 00  ---          03 10 28  37.6  45.3 -2.4       0.0   780      742   13 47 01

14 02 00  0528+134     03 12 28  38.0  44.9 -2.3       0.0    99      742   14 02 00
14 05 00  ---          03 15 29  38.4  44.1 -2.3       0.0   180      765   14 02 01
Schedule for HART      (Code Hh )                                   Page   3
               Network Monitoring Experiment
  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  12 Mar 2019   Day  71 ---

14 07 00  0528+134     03 17 29  38.8  43.7 -2.2       0.0    99      765   14 07 00
14 20 00  ---          03 30 31  40.7  40.4 -2.0       0.0   780      866   14 07 01

14 22 00  0528+134     03 32 32  41.0  39.9 -2.0       0.0    99      866   14 22 00
14 25 00  ---          03 35 32  41.4  39.1 -1.9       0.0   180      889   14 22 01

14 27 00  0528+134     03 37 32  41.7  38.6 -1.9       0.0    99      889   14 27 00
14 40 00  ---          03 50 34  43.5  35.0 -1.7       0.0   780      989   14 27 01

14 42 00  0528+134     03 52 35  43.7  34.4 -1.7       0.0    99      989   14 42 00
14 45 00  ---          03 55 35  44.1  33.6 -1.6       0.0   180     1013   14 42 01

14 47 00  0528+134     03 57 36  44.4  33.0 -1.6       0.0    99     1013   14 47 00
15 00 00  ---          04 10 38  45.9  29.0 -1.4       0.0   780     1113   14 47 01


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


 ======== Setup file: sess119.K1024
 --- WARNING ---  This group does not match an entry in the frequency catalog.
                  This might be ok because the catalog is not complete.
                  But be very careful to be sure that the setup is correct.

   Setup group:    7         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=  22000.00  22000.00  22000.00  22000.00  22000.00  22000.00  22000.00  22000.00
            22000.00  22000.00  22000.00  22000.00  22000.00  22000.00  22000.00  22000.00
   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         2        10         2        10
                   3        11         3        11         4        12         4        12
   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
                  A1        C1        A1        C1        A1        C1        A1        C1

  The following frequency sets based on these setups were used.

   Frequency Set:  10  Setup file default.  Used with PCAL = off
   LO sum=   22187.49  22187.49  22187.49  22187.49  22219.49  22219.49  22219.49  22219.49
             22251.49  22251.49  22251.49  22251.49  22283.49  22283.49  22283.49  22283.49
   BBC fr=     187.49    187.49    187.49    187.49    219.49    219.49    219.49    219.49
               251.49    251.49    251.49    251.49    283.49    283.49    283.49    283.49
   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)

 * 0234+285          02 34 55.589590   * 02 37 52.405677     02 38 58.475754       0.00
   J0237+2848        28 35 11.40773    * 28 48 08.98999      28 52 58.42250        0.00
   J0237+28          /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution,  58420 observations.

 * 0528+134          05 28 06.759216   * 05 30 56.416746     05 32 00.575865       0.21
   J0530+1331        13 29 42.28882    * 13 31 55.14948      13 32 35.57474        0.24
   J0530+13          /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution, 138236 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
  0234+285   sess119.K1024         1 2 3 4 5 6 7 8 9 10 11 15  +     0.833   192.500
  0528+134   sess119.K1024         1 2 3 4 5 6 7 8 9 10 11 15  +     1.567   361.550


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) 
   0234+285            55.7
   0528+134            91.4

  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 

