  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: Network Monitoring Experiment
 Exp. Code:  N16L1   


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

PI:       Minnie Mao

Address:  JIVE
          Postbus 2
          7990 AA Dwingeloo
          The Netherlands

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

Observing mode:

Notes:    18cm NME and 4 ftp fringe tests for session 1/2016
          512 Mbps, L+R, 2-bit sampling, 8 MHz filters
          Please send the disk pack by express to JIVE
 


COVER LETTER:


This is the schedule for the 18cm NME and ftp fringe-test on 03 March
2016 involving 14 antennas: Ef Wb1 Jb1 O8 Mc Sh T6 Ur Tr Sv Zc Bd Hh
Sr.  The NME uses a standard 512 Mbps setup.

The schedule consists of long integrations on strong calibrators
(0234+285 & 3C84) for ftp-fringe tests. At 18cm, 0234+285 is ~1.3
Jy/beam and 3C84 is ~10.4Jy/beam)

Four ftp-fringe tests are scheduled throughout the experiment:
12:09:00 (scan 2, 2 sec, 0234+285, all ants)
12:54:00 (scan 8, 2 sec, 3C84, Hh ~20deg)
13:39:00 (scan 14, 2 sec, 0234+285, Sh & T6 ~15deg)
14:24:00 (scan 20, 2 sec, 3C84, no Zc; Sh, T6, Hh ~20deg)

All antennas will participate in at least two FTP fringe tests.

Please make sure that the autoftp is set up correctly. Thanks!

Good luck with the session and see you on Skype!

Minnie
Skype account: mini_mintaka

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

 --- Thu   3 Mar 2016   Day  63 ---

 Next scan frequencies:  1634.49  1634.49  1634.49  1634.49  1650.49  1650.49  1650.49  1650.49
                         1666.49  1666.49  1666.49  1666.49  1682.49  1682.49  1682.49  1682.49
 Next BBC frequencies:    124.49   124.49   124.49   124.49   140.49   140.49   140.49   140.49
                          156.49   156.49   156.49   156.49   172.49   172.49   172.49   172.49
 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  0234+285     00 37 31  28.0  30.0 -2.0       0.0     0        0   12 00 00
12 04 00  ---          00 41 32  28.4  29.2 -2.0       0.0   240       15   12 00 01

12 06 00  0234+285     00 43 32  28.6  28.8 -1.9       0.0    99       15   12 06 00
12 10 00  ---          00 47 33  29.1  27.9 -1.9       0.0   240       31   12 06 01

12 12 00  0234+285     00 49 33  29.3  27.4 -1.8       0.0    99       31   12 12 00
12 15 00  ---          00 52 34  29.6  26.8 -1.8       0.0   180       42   12 12 01

12 16 00  0234+285     00 53 34  29.7  26.5 -1.8       0.0    39       42   12 16 00
12 24 00  ---          01 01 35  30.5  24.7 -1.6       0.0   480       73   12 16 01

12 25 00  0234+285     01 02 35  30.6  24.5 -1.6       0.0    39       73   12 25 00
12 33 00  ---          01 10 36  31.3  22.6 -1.5       0.0   480      104   12 25 01

12 34 00  0234+285     01 11 37  31.4  22.4 -1.5       0.0    39      104   12 34 00
12 42 00  ---          01 19 38  32.0  20.5 -1.3       0.0   480      135   12 34 01

12 45 00  3C84         01 22 38  17.2  22.7 -2.0       0.0   128      135   12 45 00
12 49 00  ---          01 26 39  17.5  22.0 -1.9       0.0   240      150   12 45 01

12 51 00  3C84         01 28 39  17.7  21.7 -1.9       0.0    99      150   12 51 00
12 55 00  ---          01 32 40  18.0  21.0 -1.8       0.0   240      165   12 51 01

12 57 00  3C84         01 34 40  18.2  20.6 -1.8       0.0    99      165   12 57 00
13 00 00  ---          01 37 41  18.4  20.1 -1.7       0.0   180      177   12 57 01

13 01 00  3C84         01 38 41  18.5  19.9 -1.7       0.0    39      177   13 01 00
13 09 00  ---          01 46 42  19.1  18.4 -1.6       0.0   480      208   13 01 01

13 10 00  3C84         01 47 43  19.2  18.3 -1.6       0.0    39      208   13 10 00
13 18 00  ---          01 55 44  19.7  16.8 -1.4       0.0   480      238   13 10 01

13 19 00  3C84         01 56 44  19.8  16.6 -1.4       0.0    39      238   13 19 00
13 27 00  ---          02 04 45  20.3  15.1 -1.3       0.0   480      269   13 19 01

13 30 00  0234+285     02 07 46  34.7   8.3 -0.5       0.0   128      269   13 30 00
13 34 00  ---          02 11 46  34.9   7.2 -0.5       0.0   240      285   13 30 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
----------------------------------------------------------------------------------------

 --- Thu   3 Mar 2016   Day  63 ---

13 36 00  0234+285     02 13 47  34.9   6.7 -0.4       0.0    99      285   13 36 00
13 40 00  ---          02 17 47  35.0   5.6 -0.4       0.0   240      300   13 36 01

13 42 00  0234+285     02 19 48  35.0   5.1 -0.3       0.0    99      300   13 42 00
13 45 00  ---          02 22 48  35.1   4.3 -0.3       0.0   180      312   13 42 01

13 46 00  0234+285     02 23 48  35.1   4.0 -0.3       0.0    39      312   13 46 00
13 54 00  ---          02 31 50  35.2   1.9 -0.1       0.0   480      342   13 46 01

13 55 00  0234+285     02 32 50  35.2   1.6 -0.1       0.0    39      342   13 55 00
14 03 00  ---          02 40 51  35.2 359.5  0.0       0.0   480      373   13 55 01

14 04 00  0234+285     02 41 51  35.2 359.2  0.1       0.0    39      373   14 04 00
14 12 00  ---          02 49 53  35.2 357.0  0.2       0.0   480      404   14 04 01

14 15 00  3C84         02 52 53  22.2   5.6 -0.5       0.0   128      404   14 15 00
14 19 00  ---          02 56 54  22.3   4.8 -0.4       0.0   240      419   14 15 01

14 21 00  3C84         02 58 54  22.3   4.4 -0.4       0.0    99      419   14 21 00
14 25 00  ---          03 02 55  22.4   3.6 -0.3       0.0   240      435   14 21 01

14 27 00  3C84         03 04 55  22.4   3.2 -0.3       0.0    99      435   14 27 00
14 30 00  ---          03 07 56  22.5   2.6 -0.2       0.0   180      446   14 27 01

14 32 00  3C84         03 09 56  22.5   2.2 -0.2       0.0    99      446   14 32 00
14 40 00  ---          03 17 57  22.5   0.6 -0.0       0.0   480      477   14 32 01

14 42 00  3C84         03 19 58  22.5   0.2 -0.0       0.0    99      477   14 42 00
14 50 00  ---          03 27 59  22.5 358.6  0.1       0.0   480      508   14 42 01

14 52 00  3C84         03 29 59  22.5 358.2  0.2       0.0    99      508   14 52 00
15 00 00  ---          03 38 01  22.4 356.5  0.3       0.0   480      538   14 52 01


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


 ======== Setup file: sess116.L5nme
   Matching groups in /home/guest/rmc/SCHED/sched11.4/catalogs/freq_RDBE.dat:
     hh18cm          Values confirmed by E-mail Jonathan Quick 20140219 (CR)
    ****** Only   64.00 of  128.00 MHz total bandwidth is within the IFs
           in the setup file before any FREQ or DOPPLER shifts.

   Setup group:   10         Station: HART              Total bit rate:   512
   Format: MARK5B            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=   1510.00   1510.00   1510.00   1510.00   1510.00   1510.00   1510.00   1510.00
             1510.00   1510.00   1510.00   1510.00   1510.00   1510.00   1510.00   1510.00
   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:  11  Setup file default.  Used with PCAL = off
   LO sum=   1634.49  1634.49  1634.49  1634.49  1650.49  1650.49  1650.49  1650.49
             1666.49  1666.49  1666.49  1666.49  1682.49  1682.49  1682.49  1682.49
   BBC fr=    124.49   124.49   124.49   124.49   140.49   140.49   140.49   140.49
              156.49   156.49   156.49   156.49   172.49   172.49   172.49   172.49
   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:  11

   Track assignments are: 
    track1=  18, 26,  2, 10, 20, 28,  4, 12, 22, 30,  6, 14, 24, 32,  8, 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 49.086810       0.00
   J0237+2848        28 35 11.40776    * 28 48 08.99001      28 52 13.64079        0.00
   J0237+28          /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc
                     GSFC 2015a astro solution, unpublished  54650 observations.

 * 3C84              03 16 29.567263   * 03 19 48.160094     03 20 52.163420       1.30
   J0319+4130        41 19 51.91701    * 41 30 42.10413      41 34 08.86432        2.69
   0316+413          /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc
   J0319+41          GSFC 2015a astro solution, unpublished  10208 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   sess116.L5nme         1 2 3 4 5 6 7 8 11 12 13 14 +     1.167   122.500
  3C84       sess116.L5nme         1 2 3 4 5 6 7 8 11 12 13 14 +     1.167   110.833


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            63.6
   3C84                76.5

  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 

