  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: Network Monitoring Experiment
 Exp. Code:  N24C1   


Schedule Version:       1.00
Processed by SCHED version:  11.60  Release 11.6; April 2020

PI:       Suma Murthy

Address:  JIVE
          Oude Hoogeveensedijk 4
          7991PD Dwingeloo
          The Netherlands

Phone:    +31 521 596 508
EMAIL:    murthy@jive.eu
Fax:
Phone during observation: +31 521 596 508

Observing mode:

Notes:    6cm NME and ftp fringe test for Session 1 2024
          (4 Gbps, L+R, 2-bit sampling, 32 MHz filters)
          Please DO NOT use the phase cal signal.
          Please send the disk pack by express to JIVE


COVER LETTER:


This is the schedule for the 6cm NME and ftp fringe-test on 25 Feb 2024
involving the following antennas:
Jb1, Wb, Ef, Mc, On85, T6, Ur, Tr, Ys, Hh, Ir, Sr, Cm, Da, De, Pi, Kn

The NME uses a standard setup with 4096 Mbps.

The schedule consists of long integrations on the awesome, iconic 3C84
for ftp-fringe tests. We will use J0316+4119 for phase-referencing check.

The following ftp-fringe tests are scheduled throughout the experiment (UT times):
12:15:00 (scan 2, 2 sec, 3C84)
12:45:00 (scan 4, 2 sec, 3C84)
13:15:00 (scan 8, 2 sec, 3C84)
13:45:00 (scan 12, 2 sec, 3C84)
14:15:00 (scan 16, 2 sec, 3C84)
14:45:00 (scan 20, 2 sec, 3C84)


Good luck with the session!

Suma Murthy
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
----------------------------------------------------------------------------------------

 --- Sun  25 Feb 2024   Day  56 ---

 Next scan frequencies:  4632.00  4632.00  4632.00  4632.00  4696.00  4696.00  4696.00  4696.00
                         4760.00  4760.00  4760.00  4760.00  4824.00  4824.00  4824.00  4824.00
                         4888.00  4888.00  4888.00  4888.00  4952.00  4952.00  4952.00  4952.00
                         5016.00  5016.00  5016.00  5016.00  5080.00  5080.00  5080.00  5080.00
 Next BBC frequencies:     32.00    32.00    32.00    32.00    96.00    96.00    96.00    96.00
                          160.00   160.00   160.00   160.00   224.00   224.00   224.00   224.00
                          288.00   288.00   288.00   288.00   352.00   352.00   352.00   352.00
                          416.00   416.00   416.00   416.00   480.00   480.00   480.00   480.00
 Next scan bandwidths:     32.00    32.00    32.00    32.00    32.00    32.00    32.00    32.00
                           32.00    32.00    32.00    32.00    32.00    32.00    32.00    32.00
                           32.00    32.00    32.00    32.00    32.00    32.00    32.00    32.00
                           32.00    32.00    32.00    32.00    32.00    32.00    32.00    32.00

12 00 00  3C84         00 10 10   9.3  34.2 -3.2       0.0     0        0   12 00 00
12 02 00  ---          00 12 10   9.6  33.9 -3.2       0.0   120       62   12 00 01

12 07 00  3C84         00 17 11  10.2  33.2 -3.1       0.0   279       62   12 07 00
12 17 00  ---          00 27 13  11.4  31.7 -2.9       0.0   600      371   12 07 01

12 22 00  3C84         00 32 14  12.0  31.0 -2.8       0.0   279      371   12 22 00
12 32 00  ---          00 42 15  13.1  29.4 -2.7       0.0   600      680   12 22 01

12 37 00  3C84         00 47 16  13.7  28.6 -2.6       0.0   279      680   12 37 00
12 47 00  ---          00 57 18  14.7  27.0 -2.4       0.0   600      989   12 37 01

12 49 00  3C84         00 59 18  14.9  26.7 -2.4       0.0    99      989   12 49 00
12 53 00  ---          01 03 19  15.3  26.1 -2.3       0.0   240     1113   12 49 01

12 53 00  J0316+4119   01 03 19  15.8  25.7 -2.2       0.0   -27     1113   No stop 
12 56 00  ---          01 06 19  16.1  25.2 -2.2       0.0   153     1206   12 53 01

12 58 00  3C84         01 08 19  15.8  25.2 -2.2       0.0    93     1206   12 58 00
13 02 00  ---          01 12 20  16.2  24.6 -2.2       0.0   240     1329   12 58 01

13 07 00  3C84         01 17 21  16.7  23.7 -2.1       0.0   279     1329   13 07 00
13 17 00  ---          01 27 23  17.5  22.0 -1.9       0.0   600     1639   13 07 01

13 22 00  3C84         01 32 23  17.9  21.1 -1.8       0.0   279     1639   13 22 00
13 24 00  ---          01 34 24  18.1  20.7 -1.8       0.0   120     1700   13 22 01

13 24 00  J0316+4119   01 34 24  18.5  20.3 -1.7       0.0   -27     1700   No stop 
13 26 00  ---          01 36 24  18.7  19.9 -1.7       0.0    93     1762   13 24 01

13 28 00  3C84         01 38 24  18.4  20.0 -1.7       0.0    93     1762   13 28 00
13 32 00  ---          01 42 25  18.7  19.3 -1.6       0.0   240     1886   13 28 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  25 Feb 2024   Day  56 ---

13 37 00  3C84         01 47 26  19.1  18.4 -1.6       0.0   279     1886   13 37 00
13 47 00  ---          01 57 28  19.8  16.5 -1.4       0.0   600     2195   13 37 01

13 49 00  3C84         01 59 28  19.9  16.2 -1.4       0.0    99     2195   13 49 00
13 53 00  ---          02 03 29  20.1  15.4 -1.3       0.0   240     2319   13 49 01

13 53 00  J0316+4119   02 03 29  20.5  14.9 -1.2       0.0   -27     2319   No stop 
13 56 00  ---          02 06 29  20.7  14.3 -1.2       0.0   153     2411   13 53 01

13 58 00  3C84         02 08 29  20.4  14.5 -1.2       0.0    93     2411   13 58 00
14 02 00  ---          02 12 30  20.7  13.7 -1.1       0.0   240     2535   13 58 01

14 07 00  3C84         02 17 31  20.9  12.7 -1.1       0.0   279     2535   14 07 00
14 17 00  ---          02 27 32  21.4  10.8 -0.9       0.0   600     2844   14 07 01

14 19 00  3C84         02 29 33  21.4  10.4 -0.9       0.0    99     2844   14 19 00
14 23 00  ---          02 33 33  21.6   9.6 -0.8       0.0   240     2968   14 19 01

14 23 00  J0316+4119   02 33 33  21.9   9.0 -0.7       0.0   -27     2968   No stop 
14 26 00  ---          02 36 34  22.0   8.4 -0.7       0.0   153     3061   14 23 01

14 28 00  3C84         02 38 34  21.8   8.6 -0.7       0.0    93     3061   14 28 00
14 32 00  ---          02 42 35  21.9   7.8 -0.6       0.0   240     3184   14 28 01

14 37 00  3C84         02 47 36  22.1   6.8 -0.6       0.0   279     3184   14 37 00
14 47 00  ---          02 57 37  22.3   4.8 -0.4       0.0   600     3494   14 37 01

14 49 00  3C84         02 59 38  22.3   4.4 -0.4       0.0    99     3494   14 49 00
14 52 00  ---          03 02 38  22.4   3.8 -0.3       0.0   180     3586   14 49 01

14 52 00  J0316+4119   03 02 38  22.6   3.2 -0.3       0.0   -27     3586   No stop 
14 55 00  ---          03 05 39  22.6   2.6 -0.2       0.0   153     3679   14 52 01

14 57 00  3C84         03 07 39  22.4   2.8 -0.2       0.0    93     3679   14 57 00
15 00 00  ---          03 10 40  22.5   2.2 -0.2       0.0   180     3772   14 57 01


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


 ======== Setup file: sess124.C4096
   Matching groups in /home/guest/rmc/SCHED/sched11.6/catalogs/freq_RDBE.dat:
     hh6cm_S2        Values confirmed by E-mail Jonathan Quick 20140219 (CR)
    ****** Only  462.00 of 1024.00 MHz total bandwidth is within the IFs
           in the setup file before any FREQ or DOPPLER shifts.

   Setup group:    4         Station: HART              Total bit rate:  4096
   Format: VDIF              Bits per sample: 2         Sample rate: 64.000
   Number of channels: 32    DBE type: DBBC_DDC         Speedup factor:   1.00

   Disk used to record data.

   1st LO=   4600.00   4600.00   4600.00   4600.00   4600.00   4600.00   4600.00   4600.00
             4600.00   4600.00   4600.00   4600.00   4600.00   4600.00   4600.00   4600.00
             4600.00   4600.00   4600.00   4600.00   4600.00   4600.00   4600.00   4600.00
             4600.00   4600.00   4600.00   4600.00   4600.00   4600.00   4600.00   4600.00
   Net SB=         L         L         U         U         L         L         U         U
                   L         L         U         U         L         L         U         U
                   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
                   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 
                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
                   5        13         5        13         6        14         6        14
                   7        15         7        15         8        16         8        16
   BBC SB=         L         L         U         U         L         L         U         U
                   L         L         U         U         L         L         U         U
                   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
                  B2        C1        B2        C1        B2        C1        B2        C1
                  B2        C1        B2        C1        B2        C1        B2        C1

  The following frequency sets based on these setups were used.

   Frequency Set:  10  Setup file default.  Used with PCAL = off
   LO sum=   4632.00  4632.00  4632.00  4632.00  4696.00  4696.00  4696.00  4696.00
             4760.00  4760.00  4760.00  4760.00  4824.00  4824.00  4824.00  4824.00
             4888.00  4888.00  4888.00  4888.00  4952.00  4952.00  4952.00  4952.00
             5016.00  5016.00  5016.00  5016.00  5080.00  5080.00  5080.00  5080.00
   BBC fr=     32.00    32.00    32.00    32.00    96.00    96.00    96.00    96.00
              160.00   160.00   160.00   160.00   224.00   224.00   224.00   224.00
              288.00   288.00   288.00   288.00   352.00   352.00   352.00   352.00
              416.00   416.00   416.00   416.00   480.00   480.00   480.00   480.00
   Bandwd=     32.00    32.00    32.00    32.00    32.00    32.00    32.00    32.00
               32.00    32.00    32.00    32.00    32.00    32.00    32.00    32.00
               32.00    32.00    32.00    32.00    32.00    32.00    32.00    32.00
               32.00    32.00    32.00    32.00    32.00    32.00    32.00    32.00
    Matching frequency sets:  10

   Track assignments are: 
    track1=   1,  2,  3,  4,  5,  6,  7,  8,  9, 10, 11, 12, 13, 14, 15, 16, 17, 18, 19, 20, 21, 22, 23, 24, 25, 26, 27, 28, 29, 30, 31, 32
    barrel=roll_off 

 POSITIONS OF SOURCES USED IN RECORDING SCANS

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

 * J0316+4119        03 13 25.195715   * 03 16 42.978200     03 18 17.723756       0.00
                     41 08 29.24380    * 41 19 29.61600      41 24 57.41827        0.00
                     From catalog imbedded in main SCHED input file.

 * 3C84              03 16 29.567265   * 03 19 48.160096     03 21 23.319735       1.50
   J0319+4130        41 19 51.91692    * 41 30 42.10404      41 36 05.12391        2.86
   0316+413          /home/guest/rmc/SCHED/sched11.6/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
  J0316+4119 sess124.C4096         1 2 3 4 5 6 7 8 10 12 13          0.233    28.206
  3C84       sess124.C4096         1 2 3 4 5 6 7 8 10 12 13          1.800   244.800


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) 
   J0316+4119          82.5
   3C84                83.1

  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 

