  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: FTP Fringe Test
 Exp. Code:  F24X1   


Schedule Version:       2.00
Processed by SCHED version:  11.60  Release 11.6; April 2020

PI:       Gabor Orosz

Address:  JIVE
          Oude Hoogeveensedijk 4
          Dwingeloo
          Netherlands

Phone:    +31 521 596 530
EMAIL:    orosz@jive.eu
Fax:
Phone during observation: +31 521 596 530

Observing mode: vlbi

Notes:    X-band (3.6cm) ftp fringe test for Session 1, 2024.
          4Gbps/16IF/32MHz/dual/2bit, evn4cm-4Gbps-32MHz.set
          v2: shifts to 4Gbps for Kunming testing
 


COVER LETTER:

This is the schedule for the 3.6cm FTP-FT on March 4, 2024
involving the following 12 antennas:
Wb1, Ef, Mc, Nt, On60, T6, Ur, Tr, Ys, Hh, Ir, Km.

The FTP-FT uses a standard 2 Gbps setup (16BBC/32MHz/dual),
exc. Wb1 (1 Gbps w/ 8 BBCs).

The FTP-FT lasts for 1 hour (04/03,18-19UT) with scans on calibrator:
J0854+2006 (OJ287) -- https://obs.vlba.nrao.edu/cst/calibsource/6716

with ftp grabs every other scan at the following times (in UT):
18:05:00 (scan  2, 2 sec, J1613+3412)
18:20:00 (scan  4, 2 sec, J1613+3412)
18:40:00 (scan  6, 2 sec, J1613+3412)
18:59:00 (scan  8, 2 sec, J1613+3412)

--
Gabor Orosz
Mattermost: coms.evlbi.org
Schedule for HART      (Code Hh )                                   Page   2
               FTP Fringe Test
  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
----------------------------------------------------------------------------------------

 --- Mon   4 Mar 2024   Day  64 ---

 Next scan frequencies:  8112.00  8112.00  8112.00  8112.00  8176.00  8176.00  8176.00  8176.00
                         8240.00  8240.00  8240.00  8240.00  8304.00  8304.00  8304.00  8304.00
                         8368.00  8368.00  8368.00  8368.00  8432.00  8432.00  8432.00  8432.00
                         8496.00  8496.00  8496.00  8496.00  8560.00  8560.00  8560.00  8560.00
 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

18 00 00  J0854+2006   06 42 42  33.8  38.5 -2.2       0.0     0        0   18 00 00
18 02 00  =OJ287       06 44 42  34.1  38.0 -2.2       0.0   120       62   18 00 01

18 03 00  J0854+2006   06 45 42  34.2  37.8 -2.2       0.0    39       62   18 03 00
18 06 00  =OJ287       06 48 43  34.6  37.1 -2.1       0.0   180      155   18 03 01

18 07 00  J0854+2006   06 49 43  34.8  36.9 -2.1       0.0    39      155   18 07 00
18 11 00  =OJ287       06 53 43  35.3  35.9 -2.0       0.0   240      278   18 07 01

18 13 00  J0854+2006   06 55 44  35.6  35.4 -2.0       0.0    99      278   18 13 00
18 21 00  =OJ287       07 03 45  36.6  33.5 -1.9       0.0   480      526   18 13 01

18 23 00  J0854+2006   07 05 45  36.8  33.0 -1.8       0.0    99      526   18 23 00
18 31 00  =OJ287       07 13 47  37.8  30.9 -1.7       0.0   480      773   18 23 01

18 33 00  J0854+2006   07 15 47  38.0  30.4 -1.7       0.0    99      773   18 33 00
18 41 00  =OJ287       07 23 48  38.9  28.3 -1.5       0.0   480     1020   18 33 01

18 43 00  J0854+2006   07 25 49  39.1  27.7 -1.5       0.0    99     1020   18 43 00
18 50 00  =OJ287       07 32 50  39.8  25.8 -1.4       0.0   420     1237   18 43 01

18 52 00  J0854+2006   07 34 50  40.0  25.3 -1.4       0.0    99     1237   18 52 00
19 00 00  =OJ287       07 42 51  40.8  23.0 -1.2       0.0   480     1484   18 52 01


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


 ======== Setup file: sess124.X4096
   Matching groups in /home/guest/rmc/SCHED/sched11.6/catalogs/freq_RDBE.dat:
     hhsx            Values confirmed by E-mail Jonathan Quick 20140219 (CR)
    ****** Only  412.00 of 1024.00 MHz total bandwidth is within the IFs
           in the setup file before any FREQ or DOPPLER shifts.

   Setup group:    3         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=   8080.00   8080.00   8080.00   8080.00   8080.00   8080.00   8080.00   8080.00
             8080.00   8080.00   8080.00   8080.00   8080.00   8080.00   8080.00   8080.00
             8080.00   8080.00   8080.00   8080.00   8080.00   8080.00   8080.00   8080.00
             8080.00   8080.00   8080.00   8080.00   8080.00   8080.00   8080.00   8080.00
   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=   8112.00  8112.00  8112.00  8112.00  8176.00  8176.00  8176.00  8176.00
             8240.00  8240.00  8240.00  8240.00  8304.00  8304.00  8304.00  8304.00
             8368.00  8368.00  8368.00  8368.00  8432.00  8432.00  8432.00  8432.00
             8496.00  8496.00  8496.00  8496.00  8560.00  8560.00  8560.00  8560.00
   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)

   OJ287             08 51 57.250615   * 08 54 48.874927     08 56 12.754839       0.00
 * J0854+2006        20 17 58.41740    * 20 06 30.64085      20 00 58.29198        0.00
   0851+202          /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc
   J0854+20          GSFC 2016a X/S astro solution, 270807 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
  J0854+2006 sess124.X4096         1 2 3 4 5 6 7 8 9 10 12           0.800    52.800


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) 
   J0854+2006         146.1

  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 

