  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: Network Monitoring Experiment
 Exp. Code:  N17C3   


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

PI:       Benito Marcote

Address:  JIVE
          Postbus 2
          7990 AA Dwingeloo
          The Netherlands

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

Observing mode:

Notes:    6cm NME and ftp fringe test for session 3/2017 with 2 modes
          (512 and 2048 Mbps, L+R, 2-bit sampling, 8 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 6cm NME and ftp fringe-test on 25 October 2017
involving antennas: Jb2, Wb, Ef, Mc, Nt, On85, T6, Ur, Tr, Ys, Sv, Zc, Bd, Hh, Ir, Nk, and MERLIN outstations.
The NME uses a standard setup with  512 Mbps during the first 2 hr.
The NME uses a standard setup with 2048 Mbps during the last hr (Jb 2Gb).

The schedule consists of:
- long integrations on calibrator J1848+3219 for ftp-fringe tests;
  Strong fringes were found in N16C3 on this source.

The following ftp-fringe tests are scheduled throughout the experiment (512 Mbps):
12:15:00 (scan 2,  2 sec, J1848+3219)
12:45:00 (scan 6,  2 sec, J1848+3219)
13:15:00 (scan 10, 2 sec, J1848+3219)
13:45:00 (scan 14, 2 sec, J1848+3219)
Change to 2048 Mbps setup.
14:10:00 (scan 17, 2 sec, J1848+3219)
14:30:00 (scan 19, 2 sec, J1848+3219)
14:50:00 (scan 21, 2 sec, J1848+3219)

Good luck with the session!

Benito Marcote
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
----------------------------------------------------------------------------------------

 --- Wed  25 Oct 2017   Day 298 ---

 Next scan frequencies:  4966.49  4966.49  4966.49  4966.49  4982.49  4982.49  4982.49  4982.49
                         4998.49  4998.49  4998.49  4998.49  5014.49  5014.49  5014.49  5014.49
 Next BBC frequencies:    366.49   366.49   366.49   366.49   382.49   382.49   382.49   382.49
                          398.49   398.49   398.49   398.49   414.49   414.49   414.49   414.49
 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  J1848+3219   16 07 01  20.1  35.8 -2.7       0.0     0        0   12 00 00
12 10 00  =1846+322    16 17 02  21.4  34.0 -2.5       0.0   600       39   12 00 01

12 12 00  J1848+3219   16 19 03  21.7  33.6 -2.5       0.0    99       39   12 12 00
12 17 00  =1846+322    16 24 04  22.3  32.7 -2.4       0.0   300       58   12 12 01

12 20 00  J1848+3219   16 27 04  22.7  32.1 -2.4       0.0   159       58   12 20 00
12 24 40  =1846+322    16 31 45  23.2  31.2 -2.3       0.0   280       76   12 20 01

12 27 40  J1848+3219   16 34 45  23.6  30.6 -2.2       0.0   159       76   12 27 40
12 32 20  =1846+322    16 39 26  24.1  29.7 -2.2       0.0   280       94   12 27 41

12 35 20  J1848+3219   16 42 27  24.4  29.1 -2.1       0.0   159       94   12 35 20
12 40 00  =1846+322    16 47 07  24.9  28.2 -2.0       0.0   280      112   12 35 21

12 42 00  J1848+3219   16 49 08  25.1  27.8 -2.0       0.0    99      112   12 42 00
12 47 00  =1846+322    16 54 09  25.7  26.8 -1.9       0.0   300      131   12 42 01

12 50 00  J1848+3219   16 57 09  26.0  26.1 -1.9       0.0   159      131   12 50 00
12 54 40  =1846+322    17 01 50  26.4  25.2 -1.8       0.0   280      149   12 50 01

12 57 40  J1848+3219   17 04 50  26.7  24.5 -1.7       0.0   159      149   12 57 40
13 02 20  =1846+322    17 09 31  27.1  23.5 -1.7       0.0   280      167   12 57 41

13 05 20  J1848+3219   17 12 32  27.4  22.9 -1.6       0.0   159      167   13 05 20
13 10 00  =1846+322    17 17 12  27.8  21.9 -1.5       0.0   280      185   13 05 21

13 12 00  J1848+3219   17 19 13  28.0  21.4 -1.5       0.0    99      185   13 12 00
13 17 00  =1846+322    17 24 13  28.4  20.3 -1.4       0.0   300      205   13 12 01

13 20 00  J1848+3219   17 27 14  28.6  19.6 -1.4       0.0   159      205   13 20 00
13 24 40  =1846+322    17 31 55  28.9  18.6 -1.3       0.0   280      223   13 20 01

13 27 40  J1848+3219   17 34 55  29.1  17.9 -1.2       0.0   159      223   13 27 40
13 32 20  =1846+322    17 39 36  29.5  16.8 -1.2       0.0   280      241   13 27 41

13 35 20  J1848+3219   17 42 36  29.7  16.1 -1.1       0.0   159      241   13 35 20
13 40 00  =1846+322    17 47 17  29.9  15.0 -1.0       0.0   280      259   13 35 21
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
----------------------------------------------------------------------------------------

 --- Wed  25 Oct 2017   Day 298 ---

13 42 00  J1848+3219   17 49 18  30.1  14.6 -1.0       0.0    99      259   13 42 00
13 47 00  =1846+322    17 54 18  30.3  13.4 -0.9       0.0   300      278   13 42 01

 Next scan frequencies:  4830.49  4830.49  4830.49  4830.49  4894.49  4894.49  4894.49  4894.49
                         4958.49  4958.49  4958.49  4958.49  5022.49  5022.49  5022.49  5022.49
 Next BBC frequencies:    230.49   230.49   230.49   230.49   294.49   294.49   294.49   294.49
                          358.49   358.49   358.49   358.49   422.49   422.49   422.49   422.49
 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

13 52 00  J1848+3219   17 59 19  30.6  12.2 -0.8       0.0   279      278   13 52 00
13 56 00  =1846+322    18 03 20  30.8  11.2 -0.8       0.0   240      340   13 52 25

14 01 00  J1848+3219   18 08 21  31.0  10.0 -0.7       0.0   279      340   14 01 00
14 05 00  =1846+322    18 12 21  31.1   9.0 -0.6       0.0   240      402   14 01 01

14 07 00  J1848+3219   18 14 22  31.2   8.6 -0.6       0.0    99      402   14 07 00
14 12 00  =1846+322    18 19 23  31.3   7.3 -0.5       0.0   300      479   14 07 01

14 19 00  J1848+3219   18 26 24  31.5   5.6 -0.4       0.0   398      479   14 19 00
14 25 00  =1846+322    18 32 25  31.6   4.1 -0.3       0.0   360      572   14 19 01

14 27 00  J1848+3219   18 34 25  31.7   3.6 -0.2       0.0    99      572   14 27 00
14 32 00  =1846+322    18 39 26  31.7   2.4 -0.2       0.0   300      649   14 27 01

14 39 00  J1848+3219   18 46 27  31.8   0.6 -0.0       0.0   398      649   14 39 00
14 45 00  =1846+322    18 52 28  31.8 359.1  0.1       0.0   360      742   14 39 01

14 47 00  J1848+3219   18 54 28  31.8 358.6  0.1       0.0    99      742   14 47 00
14 52 00  =1846+322    18 59 29  31.7 357.4  0.2       0.0   300      819   14 47 01

14 56 00  J1848+3219   19 03 30  31.7 356.4  0.2       0.0   219      819   14 56 00
15 00 00  =1846+322    19 07 30  31.6 355.4  0.3       0.0   240      881   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.C512nme
   Matching groups in /home/guest/rmc/SCHED/sched11.4/catalogs/freq_RDBE.dat:
     hh6cm           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:    7         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=   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
   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         3        11         3        11
                   5        13         5        13         7        15         7        15
   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
                  B2        C1        B2        C1        B2        C1        B2        C1

  The following frequency sets based on these setups were used.

   Frequency Set:  14  Setup file default.  Used with PCAL = off
   LO sum=   4966.49  4966.49  4966.49  4966.49  4982.49  4982.49  4982.49  4982.49
             4998.49  4998.49  4998.49  4998.49  5014.49  5014.49  5014.49  5014.49
   BBC fr=    366.49   366.49   366.49   366.49   382.49   382.49   382.49   382.49
              398.49   398.49   398.49   398.49   414.49   414.49   414.49   414.49
   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:  14

   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: sess317.C2048nme
   Matching groups in /home/guest/rmc/SCHED/sched11.4/catalogs/freq_RDBE.dat:
     hh6cm           Values confirmed by E-mail Jonathan Quick 20140219 (CR)
    ****** Only  256.00 of  512.00 MHz total bandwidth is within the IFs
           in the setup file before any FREQ or DOPPLER shifts.

   Setup group:   27         Station: HART              Total bit rate:  2048
   Format: VDIF              Bits per sample: 2         Sample rate: 64.000
   Number of channels: 16    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
   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         3        11         3        11
                   5        13         5        13         7        15         7        15
   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
                  B2        C1        B2        C1        B2        C1        B2        C1

  The following frequency sets based on these setups were used.

   Frequency Set:  31  Setup file default.  Used with PCAL = off
   LO sum=   4830.49  4830.49  4830.49  4830.49  4894.49  4894.49  4894.49  4894.49
             4958.49  4958.49  4958.49  4958.49  5022.49  5022.49  5022.49  5022.49
   BBC fr=    230.49   230.49   230.49   230.49   294.49   294.49   294.49   294.49
              358.49   358.49   358.49   358.49   422.49   422.49   422.49   422.49
   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
    Matching frequency sets:  31

   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)

   1846+322          18 46 29.612032   * 18 48 22.088575     18 49 01.039387       0.00
 * J1848+3219        32 15 36.66046    * 32 19 02.60386      32 20 39.00936        0.00
                     /home/guest/rmc/SCHED/sched11.4/catalogs/sources.gsfc
                     GSFC 2015a astro solution, unpublished  29306 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
  J1848+3219 sess317.C512nme       1 2 3 4 5 6 7 8 9 10 11 14  +     1.200   228.000
             sess317.C2048nme      21 22 23 24 25 26 27 28 31  +     0.650    68.250


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) 
   J1848+3219          82.0

  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 

