  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: Network Monitoring Experiment
 Exp. Code:  N20M1   


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:    5cm (m-band) NME and ftp fringe test for session 1/2020
          (256 Mbps, L+R, 2-bit sampling, 4 MHz filters)
          Please send the disk pack by express to JIVE
          last bit = 4Gbps test via 64MHz filters


COVER LETTER:


This is the schedule for the 5cm NME and ftp fringe-test on 5th March 2020 12-15UT.
involving 15 telescopes: Jb2 Wb Ef On85 T6 Tr Ys Hh Ir Sr Cm Da De Kn Pi
The NME uses a standard setup with 256 Mbps.

The schedule consists of long integrations on strong calibrators:

Ftp-fringe tests are scheduled ~ every twenty minutes throughout the experiment:
12:15:00 J0238+1636
12:35:00 J0238+1636
12:55:00 J0238+1636
13:15:00 3C84
13:35:00 3C84
13:55:00 3C84
14:15:00 3C84
14:35:00 3C84
14:55:00 3C84

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

 --- Thu   5 Mar 2020   Day  65 ---

 Next scan frequencies:  6655.49  6655.49  6655.49  6655.49  6663.49  6663.49  6663.49  6663.49
                         6671.49  6671.49  6671.49  6671.49  6679.49  6679.49  6679.49  6679.49
 Next BBC frequencies:    145.49   145.49   145.49   145.49   153.49   153.49   153.49   153.49
                          161.49   161.49   161.49   161.49   169.49   169.49   169.49   169.49
 Next scan bandwidths:      4.00     4.00     4.00     4.00     4.00     4.00     4.00     4.00
                            4.00     4.00     4.00     4.00     4.00     4.00     4.00     4.00

12 00 00  J0238+1636   00 45 32  39.2  36.2 -1.9       0.0     0        0   12 00 00
12 05 00  =0235+164    00 50 32  39.8  34.9 -1.8       0.0   300       10   12 00 01

12 07 00  J0238+1636   00 52 33  40.1  34.4 -1.8       0.0    99       10   12 07 00
12 20 00  =0235+164    01 05 35  41.6  30.8 -1.6       0.0   780       35   12 07 01

12 22 00  J0238+1636   01 07 35  41.9  30.2 -1.5       0.0    99       35   12 22 00
12 25 00  =0235+164    01 10 36  42.2  29.4 -1.5       0.0   180       41   12 22 01

12 27 00  J0238+1636   01 12 36  42.4  28.8 -1.5       0.0    99       41   12 27 00
12 40 00  =0235+164    01 25 38  43.8  24.9 -1.2       0.0   780       66   12 27 01

12 42 00  J0238+1636   01 27 38  43.9  24.3 -1.2       0.0    99       66   12 42 00
12 45 00  =0235+164    01 30 39  44.2  23.4 -1.2       0.0   180       71   12 42 01

12 47 00  J0238+1636   01 32 39  44.4  22.8 -1.1       0.0    99       71   12 47 00
13 00 00  =0235+164    01 45 41  45.4  18.6 -0.9       0.0   780       97   12 47 01

13 02 00  J0238+1636   01 47 42  45.6  17.9 -0.9       0.0    99       97   13 02 00
13 05 00  =0235+164    01 50 42  45.8  17.0 -0.8       0.0   180      102   13 02 01

13 08 00  3C84         01 53 43  19.6  17.2 -1.5       0.0   103      102   13 08 00
13 20 00  ---          02 05 45  20.3  14.9 -1.3       0.0   720      126   13 08 01

13 22 00  3C84         02 07 45  20.4  14.5 -1.2       0.0    99      126   13 22 00
13 25 00  ---          02 10 46  20.6  14.0 -1.2       0.0   180      131   13 22 01

13 27 00  3C84         02 12 46  20.7  13.6 -1.1       0.0    99      131   13 27 00
13 40 00  ---          02 25 48  21.3  11.1 -0.9       0.0   780      157   13 27 01

13 42 00  3C84         02 27 48  21.4  10.7 -0.9       0.0    99      157   13 42 00
13 45 00  ---          02 30 49  21.5  10.1 -0.8       0.0   180      162   13 42 01

13 47 00  3C84         02 32 49  21.6   9.7 -0.8       0.0    99      162   13 47 00
14 00 00  ---          02 45 51  22.0   7.1 -0.6       0.0   780      187   13 47 01

14 02 00  3C84         02 47 52  22.1   6.7 -0.6       0.0    99      187   14 02 00
14 05 00  ---          02 50 52  22.2   6.1 -0.5       0.0   180      193   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
----------------------------------------------------------------------------------------

 --- Thu   5 Mar 2020   Day  65 ---

14 07 00  3C84         02 52 52  22.2   5.7 -0.5       0.0    99      193   14 07 00
14 20 00  ---          03 05 55  22.4   3.1 -0.3       0.0   780      218   14 07 01

 Next scan frequencies:  6476.49  6476.49  6476.49  6476.49  6604.49  6604.49  6604.49  6604.49
                         6732.49  6732.49  6732.49  6732.49  6860.49  6860.49  6860.49  6860.49
 Next BBC frequencies:     76.49    76.49    76.49    76.49   204.49   204.49   204.49   204.49
                          332.49   332.49   332.49   332.49   460.49   460.49   460.49   460.49
 Next scan bandwidths:     64.00    64.00    64.00    64.00    64.00    64.00    64.00    64.00
                           64.00    64.00    64.00    64.00    64.00    64.00    64.00    64.00

14 25 00  3C84         03 10 55  22.5   2.1 -0.2       0.0   279      218   14 25 00
14 28 00  ---          03 13 56  22.5   1.5 -0.1       0.0   180      311   14 25 25

14 30 00  3C84         03 15 56  22.5   1.0 -0.1       0.0    99      311   14 30 00
14 37 00  ---          03 22 57  22.5 359.6  0.0       0.0   420      528   14 30 01

14 43 00  3C84         03 28 58  22.5 358.4  0.1       0.0   339      528   14 43 00
14 46 00  ---          03 31 59  22.5 357.8  0.2       0.0   180      620   14 43 01

14 48 00  3C84         03 33 59  22.5 357.4  0.2       0.0    99      620   14 48 00
14 55 00  ---          03 41 00  22.4 356.0  0.3       0.0   420      837   14 48 01


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


 ======== Setup file: sess120.M256nme
   Matching groups in /home/guest/rmc/SCHED/sched11.5/catalogs/freq_RDBE.dat:
     hh5cm           Values confirmed by E-mail Jonathan Quick 20170808 (CR)
    ****** Only   30.51 of   64.00 MHz total bandwidth is within the IFs
           in the setup file before any FREQ or DOPPLER shifts.

   Setup group:    5         Station: HART              Total bit rate:   256
   Format: VDIF              Bits per sample: 2         Sample rate:  8.000
   Number of channels: 16    DBE type: DBBC_DDC         Speedup factor:   1.00

   Disk used to record data.

   1st LO=   6510.00   6510.00   6510.00   6510.00   6510.00   6510.00   6510.00   6510.00
             6510.00   6510.00   6510.00   6510.00   6510.00   6510.00   6510.00   6510.00
   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:   8  Setup file default.  Used with PCAL = off
   LO sum=   6655.49  6655.49  6655.49  6655.49  6663.49  6663.49  6663.49  6663.49
             6671.49  6671.49  6671.49  6671.49  6679.49  6679.49  6679.49  6679.49
   BBC fr=    145.49   145.49   145.49   145.49   153.49   153.49   153.49   153.49
              161.49   161.49   161.49   161.49   169.49   169.49   169.49   169.49
   Bandwd=      4.00     4.00     4.00     4.00     4.00     4.00     4.00     4.00
                4.00     4.00     4.00     4.00     4.00     4.00     4.00     4.00
    Matching frequency sets:   8

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


 ======== Setup file: sess120.M4096_64
 --- 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:   19         Station: HART              Total bit rate:  4096
   Format: VDIF              Bits per sample: 2         Sample rate:128.000
   Number of channels: 16    DBE type: DBBC_DDC         Speedup factor:   1.00

   Disk used to record data.

   1st LO=   6400.00   6400.00   6400.00   6400.00   6400.00   6400.00   6400.00   6400.00
             6400.00   6400.00   6400.00   6400.00   6400.00   6400.00   6400.00   6400.00
   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:  22  Setup file default.  Used with PCAL = off
   LO sum=   6476.49  6476.49  6476.49  6476.49  6604.49  6604.49  6604.49  6604.49
             6732.49  6732.49  6732.49  6732.49  6860.49  6860.49  6860.49  6860.49
   BBC fr=     76.49    76.49    76.49    76.49   204.49   204.49   204.49   204.49
              332.49   332.49   332.49   332.49   460.49   460.49   460.49   460.49
   Bandwd=     64.00    64.00    64.00    64.00    64.00    64.00    64.00    64.00
               64.00    64.00    64.00    64.00    64.00    64.00    64.00    64.00
    Matching frequency sets:  22  24

   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)

   0235+164          02 35 52.630214   * 02 38 38.930106     02 39 44.319071       0.12
 * J0238+1636        16 24 04.01612    * 16 36 59.27454      16 42 01.71522        0.16
   J0238+16          /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution,  64441 observations.

 * 3C84              03 16 29.567265   * 03 19 48.160096     03 21 06.575438       1.50
   J0319+4130        41 19 51.91692    * 41 30 42.10404      41 35 02.71165        2.86
   0316+413          /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc
   J0319+41          GSFC 2016a X/S astro solution,  10291 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
  J0238+1636 sess120.M256nme       1 2 3 4 5 6 7 8 9 10 11           0.883    92.750
  3C84       sess120.M256nme       1 2 3 4 5 6 7 8 9 10 11           1.000   105.000
             sess120.M4096_64      16 17 18 19 20 21 22 23           0.333    12.000


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) 
   J0238+1636          57.3
   3C84                74.7

  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 

