  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: Network Monitoring Experiment
 Exp. Code:  N18SX1  


Schedule Version:       2.00
Processed by SCHED version:  11.40  Release 11.4.  March 14, 2015

PI:       Jay Blanchard

Address:  JIVE
          Postbus 2
          7990 AA Dwingeloo
          The Netherlands

Phone:    +31-521-596508
EMAIL:    blanchard@jive.eu
Fax:
Phone during observation: +31-521-596508

Observing mode:

Notes:    3.6/13 cm (S/X-band) ftp fringe test for session 2/2018
          (512 Mbps, L+R, 2-bit sampling, 16 x 8 MHz filters)
          This NME tests two modes, dual pol X only and single pol RCP S/X
          Please send the disk pack by express to JIVE, NO PCAL


COVER LETTER:


This is the schedule for the 3.6/13 cm (S/X-band) band test on 01 June 12-15 UT
involving 12 telescopes: Wb Ef Mc Nt O6 Ys Hh Sv Zc Bd Ir Wn
The FTP-NME uses a dual-band S/X RCP only setup.

The schedule consists of long integrations on strong calibrators:

Ftp-fringe tests are scheduled ~ every twenty minutes throughout the experiment:
12:10:00 OJ287
12:30:00 OJ287
12:50:00 OJ287
13:10:00 DA193
13:30:00 DA193
13:50:00 DA193
14:10:00 DA193
14:30:00 DA193
14:50:00 DA193

Clear skies!

Jay
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
----------------------------------------------------------------------------------------

 --- Fri   1 Jun 2018   Day 152 ---

 Next scan frequencies:  8223.99  8223.99  8263.99  8363.99  8543.99  8743.99  8863.99  8883.99
                         8943.99  8943.99  2201.99  2217.99  2249.99  2265.99  2281.99  2297.99
 Next BBC frequencies:    143.99   143.99   183.99   283.99   463.99   663.99   783.99   803.99
                          863.99   863.99   181.99   197.99   229.99   245.99   261.99   277.99
 Next scan bandwidths:      8.00     8.00     8.00     8.00     8.00     8.00     8.00     8.00
                            8.00     8.00     8.00     8.00     8.00     8.00     8.00     8.00

12 00 00  OJ287        06 30 26  32.1  41.1 -2.4       0.0     0        0   12 00 00
12 05 00  ---          06 35 27  32.8  40.0 -2.3       0.0   300       19   12 00 01

12 07 00  OJ287        06 37 28  33.1  39.5 -2.3       0.0    99       19   12 07 00
12 20 00  ---          06 50 30  34.9  36.6 -2.1       0.0   780       70   12 07 01

12 22 00  OJ287        06 52 30  35.2  36.1 -2.1       0.0    99       70   12 22 00
12 25 00  ---          06 55 31  35.6  35.4 -2.0       0.0   180       81   12 22 01

12 27 00  OJ287        06 57 31  35.8  34.9 -2.0       0.0    99       81   12 27 00
12 40 00  ---          07 10 33  37.4  31.6 -1.8       0.0   780      131   12 27 01

12 42 00  OJ287        07 12 33  37.7  31.1 -1.7       0.0    99      131   12 42 00
12 45 00  ---          07 15 34  38.0  30.3 -1.7       0.0   180      143   12 42 01

12 47 00  OJ287        07 17 34  38.2  29.8 -1.6       0.0    99      143   12 47 00
13 00 00  ---          07 30 36  39.6  26.3 -1.4       0.0   780      193   12 47 01

13 02 00  DA193        07 32 37  20.6 340.5  1.6       0.0     3      193   13 02 00
13 05 00  ---          07 35 37  20.4 340.0  1.6       0.0   180      205   13 02 01

13 07 00  DA193        07 37 37  20.2 339.6  1.7       0.0    99      205   13 07 00
13 20 00  ---          07 50 40  19.1 337.2  1.9       0.0   780      255   13 07 01

13 22 00  DA193        07 52 40  19.0 336.8  1.9       0.0    99      255   13 22 00
13 25 00  ---          07 55 40  18.7 336.3  2.0       0.0   180      267   13 22 01

13 27 00  DA193        07 57 41  18.5 335.9  2.0       0.0    99      267   13 27 00
13 40 00  ---          08 10 43  17.3 333.7  2.2       0.0   780      317   13 27 01

13 42 00  DA193        08 12 43  17.1 333.3  2.3       0.0    99      317   13 42 00
13 45 00  ---          08 15 44  16.8 332.8  2.3       0.0   180      328   13 42 01

13 47 00  DA193        08 17 44  16.5 332.5  2.3       0.0    99      328   13 47 00
14 00 00  ---          08 30 46  15.1 330.3  2.6       0.0   780      379   13 47 01

14 02 00  DA193        08 32 46  14.9 330.0  2.6       0.0    99      379   14 02 00
14 05 00  ---          08 35 47  14.6 329.5  2.7       0.0   180      390   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
----------------------------------------------------------------------------------------

 --- Fri   1 Jun 2018   Day 152 ---

14 07 00  DA193        08 37 47  14.3 329.2  2.7       0.0    99      390   14 07 00
14 20 00  ---          08 50 49  12.8 327.2  2.9       0.0   780      441   14 07 01

14 22 00  DA193        08 52 50  12.6 326.8  2.9       0.0    99      441   14 22 00
14 25 00  ---          08 55 50  12.2 326.4  3.0       0.0   180      452   14 22 01

14 27 00  DA193        08 57 51  11.9 326.1  3.0       0.0    99      452   14 27 00
14 40 00  ---          09 10 53  10.3 324.2  3.2       0.0   780      502   14 27 01

14 42 00  DA193        09 12 53  10.0 323.9  3.3       0.0    99      502   14 42 00
14 45 00  ---          09 15 54   9.6 323.5  3.3       0.0   180      514   14 42 01

14 47 00  DA193        09 17 54   9.3 323.2  3.4       0.0    99      514   14 47 00
15 00 00  ---          09 30 56   7.5 321.4  3.6  D    0.0     0      564   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: sess218.SXgeo512
   Matching groups in /opt/sched/catalogs/freq_RDBE.dat:
     hhsx            Values confirmed by E-mail Jonathan Quick 20140219 (CR)
    ****** Only  120.00 of  128.00 MHz total bandwidth is within the IFs
           in the setup file before any FREQ or DOPPLER shifts.

   Setup group:    1         Station: HART              Total bit rate:   512
   Format: VDIF              Bits per sample: 2         Sample rate: 16.000
   Number of channels: 16    DBE type: DBBC_DDC         Speedup factor:   1.00

   Disk used to record data.

   1st LO=   8080.00   8080.00   8080.00   8080.00   8080.00   8080.00   8080.00   8080.00
             8080.00   8080.00   2020.00   2020.00   2020.00   2020.00   2020.00   2020.00
   Net SB=         L         U         U         U         U         U         U         U
                   L         U         U         U         U         U         U         U
   IF SB =         U         U         U         U         U         U         U         U
                   U         U         U         U         U         U         U         U
   Pol.  =      RCP       RCP       RCP       RCP       RCP       RCP       RCP       RCP 
                RCP       RCP       RCP       RCP       RCP       RCP       RCP       RCP 
   BBC   =         1         1         2         3         4         5         6         7
                   8         8         9        10        11        12        13        14
   BBC SB=         L         U         U         U         U         U         U         U
                   L         U         U         U         U         U         U         U
   IF    =        A1        A1        A1        A1        A1        B2        B2        B2
                  B2        B2        C1        C1        C1        C1        C1        C1

  The following frequency sets based on these setups were used.

   Frequency Set:   6  Setup file default.  Used with PCAL = 1MHz
   LO sum=   8223.99  8223.99  8263.99  8363.99  8543.99  8743.99  8863.99  8883.99
             8943.99  8943.99  2201.99  2217.99  2249.99  2265.99  2281.99  2297.99
   BBC fr=    143.99   143.99   183.99   283.99   463.99   663.99   783.99   803.99
              863.99   863.99   181.99   197.99   229.99   245.99   261.99   277.99
   Bandwd=      8.00     8.00     8.00     8.00     8.00     8.00     8.00     8.00
                8.00     8.00     8.00     8.00     8.00     8.00     8.00     8.00
    Matching frequency sets:   6

   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)

   0552+398          05 52 01.407169   * 05 55 30.805611     05 56 45.093132       0.00
   J0555+3948        39 48 21.94581    * 39 48 49.16496      39 48 50.72283        0.00
 * DA193             /opt/sched/catalogs/sources.gsfc
   J0555+39          GSFC 2015a astro solution, unpublished 394383 observations.

 * OJ287             08 51 57.250615   * 08 54 48.874926     08 55 50.238077       0.00
   J0854+2006        20 17 58.41743    * 20 06 30.64088      20 02 17.98288        0.00
   0851+202          /opt/sched/catalogs/sources.gsfc
   J0854+20          GSFC 2015a astro solution, unpublished 216540 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
  DA193      sess218.SXgeo512      1 2 3 4 5 6 7 10 11 12            1.600    96.995
  OJ287      sess218.SXgeo512      1 2 3 4 5 6 7 10 11 12            0.833    55.000


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) 
   DA193               24.4
   OJ287               59.8

  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 

