  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: C-band FTP fringe-test
 Exp. Code:  F22C1   


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

PI:       Benito Marcote

Address:  JIVE
          Oude Hoogeveensedijk 4
          7991PD Dwingeloo
          The Netherlands

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

Observing mode:

Notes:    6cm ftp fringe test for Session 2 2022
          4096 Mbps, L+R, 2-bit sampling, 32 MHz filters
          Please send the disk pack by express to JIVE
 


COVER LETTER:


This is the schedule for the 6cm ftp fringe-test on 9th June 2022
involving the following antennas:
Jb2 Wb1 Ef Mc Nt On85 T6 Ur Tr Ys Hh Ib Km Cm Da De Pi Kn

The NME uses a standard setup with 4096 Mbps.

The schedule consists of long integrations on calibrator J0854+2006 for ftp-fringe tests.

The following ftp-fringe tests are scheduled throughout the experiment (UT times):
12:05:00 (scan 1, 2 sec, J0854+2006)
12:18:00 (scan 3, 2 sec, J0854+2006)
12:38:00 (scan 5, 2 sec, J0854+2006)
12:58:00 (scan 7, 2 sec, J0854+2006)

Good luck with the C-session!

Benito Marcote
Mattermost: coms.evlbi.org

Schedule for HART      (Code Hh )                                   Page   2
               C-band 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
----------------------------------------------------------------------------------------

 --- Thu   9 Jun 2022   Day 160 ---

 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  J0854+2006   07 02 06  36.4  33.8 -1.9       0.0     0        0   12 00 00
12 07 00  =OJ287       07 09 07  37.3  32.1 -1.8       0.0   420      216   12 00 01

12 10 00  J0854+2006   07 12 08  37.6  31.3 -1.7       0.0   159      216   12 10 00
12 12 00  =OJ287       07 14 08  37.8  30.8 -1.7       0.0   120      278   12 10 01

12 15 00  J0854+2006   07 17 09  38.2  30.0 -1.6       0.0   159      278   12 15 00
12 20 00  =OJ287       07 22 10  38.7  28.7 -1.6       0.0   300      433   12 15 01

12 23 00  J0854+2006   07 25 10  39.1  27.9 -1.5       0.0   159      433   12 23 00
12 25 00  =OJ287       07 27 10  39.3  27.3 -1.5       0.0   120      495   12 23 01

12 30 00  J0854+2006   07 32 11  39.8  25.9 -1.4       0.0   279      495   12 30 00
12 40 00  =OJ287       07 42 13  40.7  23.1 -1.2       0.0   600      804   12 30 01

12 42 00  J0854+2006   07 44 13  40.9  22.5 -1.2       0.0    99      804   12 42 00
12 46 00  =OJ287       07 48 14  41.2  21.4 -1.1       0.0   240      927   12 42 01

12 51 00  J0854+2006   07 53 15  41.6  19.9 -1.0       0.0   279      927   12 51 00
13 00 00  =OJ287       08 02 16  42.3  17.2 -0.9       0.0   540     1206   12 51 01


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


 ======== Setup file: sess222.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:  11  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:  11

   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 04.088484       0.00
 * J0854+2006        20 17 58.41740    * 20 06 30.64085      20 01 30.83571        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 sess222.C4096         1 2 3 4 5 6 7 8 9 11 12 13  +     0.650    99.450


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          52.2

  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 

