  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: Network Monitoring Experiment
 Exp. Code:  N17K2   


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

PI:       Ross Burns

Address:  JIVE
          Postbus 2
          7990 AA Dwingeloo
          The Netherlands

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

Observing mode:

Notes:    K-Band NME and ftp fringe test for session 3/2017
          (512 Mbps, L+R, 2-bit sampling, 4 and 32 MHz filters)
          Please send the disk pack by express to JIVE
          Please DO NOT use the phase cal signal.


COVER LETTER:


This is the schedule for the K-band NME and ftp fringe-test on 29 October 2017
involving antennas: Ef, Mc, On60, Ys. Hh
The NME uses a standard setup with  512 Mbps.

The schedule consists of:
- long integrations on calibrators 3C345 and J1751+0939 for ftp-fringe tests;
  The latter being included for the sake of high elevations at Hart

The following ftp-fringe tests are scheduled throughout the experiment (512 Mbps):
12:15:00 (scan 2,  2 sec, 3C345)
12:45:00 (scan 6,  2 sec, 3C345)
13:15:00 (scan 10, 2 sec, 3C345)
13:45:00 (scan 14, 2 sec, 3C345)
14:10:00 (scan 17, 2 sec, J1751+0939)
14:30:00 (scan 19, 2 sec, J1751+0939)
14:50:00 (scan 21, 2 sec, J1751+0939)

Good luck with the session!

Ross Burns
Skype account: jive.support.scientist
Slack: evlbi.slack.com

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

 --- Sun  29 Oct 2017   Day 302 ---

 Next scan frequencies:  21661.08  21661.08  21683.07  21683.07
 Next BBC frequencies:     361.08    361.08    383.07    383.07
 Next scan bandwidths:      32.00     32.00     32.00     32.00

12 00 00  3C345        16 22 47  24.1   4.4 -0.3       0.0     0        0   12 00 00
12 10 00  ---          16 32 49  24.3   2.3 -0.2       0.0   600       39   12 00 01

12 12 00  3C345        16 34 49  24.3   1.8 -0.1       0.0    99       39   12 12 00
12 17 00  ---          16 39 50  24.3   0.8 -0.1       0.0   300       58   12 12 01

12 20 00  3C345        16 42 50  24.3   0.1 -0.0       0.0   159       58   12 20 00
12 24 40  ---          16 47 31  24.3 359.2  0.1       0.0   280       76   12 20 01

12 27 40  3C345        16 50 32  24.3 358.5  0.1       0.0   159       76   12 27 40
12 32 20  ---          16 55 12  24.3 357.5  0.2       0.0   280       94   12 27 41

12 35 20  3C345        16 58 13  24.2 356.9  0.2       0.0   159       94   12 35 20
12 40 00  ---          17 02 54  24.2 355.9  0.3       0.0   280      112   12 35 21

12 42 00  3C345        17 04 54  24.1 355.5  0.4       0.0    99      112   12 42 00
12 47 00  ---          17 09 55  24.0 354.5  0.4       0.0   300      131   12 42 01

12 50 00  3C345        17 12 55  24.0 353.8  0.5       0.0   159      131   12 50 00
12 54 40  ---          17 17 36  23.8 352.9  0.6       0.0   280      149   12 50 01

12 57 40  3C345        17 20 37  23.8 352.2  0.6       0.0   159      149   12 57 40
13 02 20  ---          17 25 17  23.6 351.3  0.7       0.0   280      167   12 57 41

13 05 20  3C345        17 28 18  23.5 350.6  0.7       0.0   159      167   13 05 20
13 10 00  ---          17 32 59  23.3 349.7  0.8       0.0   280      185   13 05 21

13 12 00  3C345        17 34 59  23.2 349.3  0.9       0.0    99      185   13 12 00
13 17 00  ---          17 40 00  23.0 348.3  0.9       0.0   300      205   13 12 01

13 20 00  3C345        17 43 00  22.9 347.6  1.0       0.0   159      205   13 20 00
13 24 40  ---          17 47 41  22.6 346.7  1.1       0.0   280      223   13 20 01

13 27 40  3C345        17 50 41  22.5 346.1  1.1       0.0   159      223   13 27 40
13 32 20  ---          17 55 22  22.2 345.2  1.2       0.0   280      241   13 27 41

13 35 20  3C345        17 58 23  22.1 344.6  1.2       0.0   159      241   13 35 20
13 40 00  ---          18 03 03  21.8 343.7  1.3       0.0   280      259   13 35 21

13 42 00  3C345        18 05 04  21.6 343.3  1.4       0.0    99      259   13 42 00
13 47 00  ---          18 10 05  21.3 342.3  1.4       0.0   300      278   13 42 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
----------------------------------------------------------------------------------------

 --- Sun  29 Oct 2017   Day 302 ---

13 52 00  J1751+0939   18 15 05  54.0 350.4  0.4       0.0   213      278   13 52 00
13 56 00  =1749+096    18 19 06  53.9 348.8  0.4       0.0   240      294   13 52 01

14 01 00  J1751+0939   18 24 07  53.6 346.7  0.5       0.0   279      294   14 01 00
14 05 00  =1749+096    18 28 08  53.4 345.1  0.6       0.0   240      309   14 01 01

14 07 00  J1751+0939   18 30 08  53.3 344.3  0.6       0.0    99      309   14 07 00
14 12 00  =1749+096    18 35 09  53.0 342.3  0.7       0.0   300      328   14 07 01

14 19 00  J1751+0939   18 42 10  52.5 339.6  0.8       0.0   398      328   14 19 00
14 25 00  =1749+096    18 48 11  52.0 337.3  0.9       0.0   360      352   14 19 01

14 27 00  J1751+0939   18 50 11  51.8 336.6  1.0       0.0    99      352   14 27 00
14 32 00  =1749+096    18 55 12  51.3 334.7  1.0       0.0   300      371   14 27 01

14 39 00  J1751+0939   19 02 13  50.6 332.2  1.2       0.0   398      371   14 39 00
14 45 00  =1749+096    19 08 14  50.0 330.1  1.3       0.0   360      394   14 39 01

14 47 00  J1751+0939   19 10 14  49.7 329.4  1.3       0.0    99      394   14 47 00
14 52 00  =1749+096    19 15 15  49.1 327.8  1.4       0.0   300      414   14 47 01

14 56 00  J1751+0939   19 19 16  48.7 326.5  1.4       0.0   219      414   14 56 00
15 00 00  =1749+096    19 23 17  48.1 325.2  1.5       0.0   240      429   14 56 01


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


 ======== Setup file: sess317.K512nme
 --- 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:    3         Station: HART              Total bit rate:   512
   Format: VDIF              Bits per sample: 2         Sample rate: 64.000
   Number of channels:  4    DBE type: DBBC_DDC         Speedup factor:   1.00

   Disk used to record data.

   1st LO=  21300.00  21300.00  21300.00  21300.00
   Net SB=         U         U         U         U
   IF SB =         U         U         U         U
   Pol.  =      RCP       LCP       RCP       LCP 
   BBC   =         1         9         3        11
   BBC SB=         U         U         U         U
   IF    =        A1        C1        A1        C1

  The following frequency sets based on these setups were used.

   Frequency Set:   5  Setup file default.  Used with PCAL = off
   LO sum=   21661.08  21661.08  21683.07  21683.07
   BBC fr=     361.08    361.08    383.07    383.07
   Bandwd=      32.00     32.00     32.00     32.00
    Matching frequency sets:   5

   Track assignments are: 
    track1=   1,  2,  3,  4
    barrel=roll_off 

 POSITIONS OF SOURCES USED IN RECORDING SCANS

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

 * 3C345             16 41 17.606228   * 16 42 58.809966     16 43 32.804552       0.76
   J1642+3948        39 54 10.81496    * 39 48 36.99402      39 46 59.34387        0.52
   1641+399          /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc
   J1642+39          GSFC 2015a astro solution, unpublished  53430 observations.

   1749+096          17 49 10.387931   * 17 51 32.818574     17 52 21.996835       0.00
 * J1751+0939        09 39 42.82591    * 09 39 00.72847      09 39 04.21184        0.00
   J1751+09          /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc
                     GSFC 2015a astro solution, unpublished 144578 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
  3C345      sess317.K512nme       1 2 4 5                           1.200    12.000
  J1751+0939 sess317.K512nme       1 2 4 5                           0.650     6.500


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) 
   3C345               63.5
   J1751+0939          58.5

  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 

