  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: EVN observations of CSOs at 1.3cm (Session 2)
 Exp. Code:  EY045B  


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

PI:       Xi Yan

Address:  Calaxy and Cosmology Group
          Xinjiang Astronomical Observatory (XAO), CAS
          150 Science 1-Street, Urumqi
          830011, China

Phone:    +86 17335173376
EMAIL:    yanxi@xao.ac.cn
Fax:
Phone during observation: +86 17335173376

Observing mode: vlbi

Notes:
          Target 1: J1148+5924(NGC3894), 0.4 Jy at KVN22GHz; 0.3 Jy at VLBA15GHz. Calibrator: J1128+5925/NGC3998)
          Target 2: J1347+1217 (1 Jy at 22GHz and 43GHz)
          Exclude the third target due to the absence of suitable PRing-source. Fringe Finder: J1058+8114 (0.9Jy at 24GHz, compact)

Schedule for HART      (Code Hh )                                   Page   2
               EVN observations of CSOs at 1.3cm (Session 2)
  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  26 Feb 2025   Day  57 ---

 Next scan frequencies:  22139.49  22139.49  22139.49  22139.49  22203.49  22203.49  22203.49  22203.49
                         22267.49  22267.49  22267.49  22267.49  22331.49  22331.49  22331.49  22331.49
 Next BBC frequencies:     659.49    659.49    659.49    659.49    723.49    723.49    723.49    723.49
                           787.49    787.49    787.49    787.49    851.49    851.49    851.49    851.49
 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

21 00 00  1156+295     09 18 34  22.6  38.0 -2.7       0.0     0        0   21 00 00
21 03 30  ---          09 22 05  23.1  37.4 -2.6       0.0   210       54   21 00 01

22 46 30  J1347+1217   11 05 22  35.0  51.3 -2.7       0.0  6099       54   22 46 30
22 48 30  =1345+125    11 07 22  35.3  50.9 -2.7       0.0   120       85   22 46 31

22 48 30  J1347+1217   11 07 22  35.3  50.9 -2.7       0.0   -20       85   No stop 
22 52 30  =1345+125    11 11 23  36.0  50.0 -2.6       0.0   220      147   22 48 31

22 52 30  J1347+1217   11 11 23  36.0  50.0 -2.6       0.0   -20      147   No stop 
22 56 30  =1345+125    11 15 24  36.7  49.2 -2.6       0.0   220      209   22 52 31

22 56 30  J1347+1217   11 15 24  36.7  49.2 -2.6       0.0   -20      209   No stop 
23 00 30  =1345+125    11 19 24  37.4  48.3 -2.5       0.0   220      271   22 56 31

23 01 00  J1347+1217   11 19 54  37.5  48.2 -2.5       0.0     9      271   23 01 00
23 05 00  =1345+125    11 23 55  38.1  47.3 -2.4       0.0   240      332   23 01 01

23 05 00  J1347+1217   11 23 55  38.1  47.3 -2.4       0.0   -20      332   No stop 
23 09 00  =1345+125    11 27 56  38.8  46.3 -2.3       0.0   220      394   23 05 01

23 09 30  J1347+1217   11 28 26  38.9  46.2 -2.3       0.0     9      394   23 09 30
23 13 30  =1345+125    11 32 26  39.5  45.3 -2.3       0.0   240      456   23 09 31

23 13 30  J1347+1217   11 32 26  39.5  45.3 -2.3       0.0   -20      456   No stop 
23 18 00  =1345+125    11 36 57  40.2  44.2 -2.2       0.0   250      526   23 13 31

23 18 00  J1347+1217   11 36 57  40.2  44.2 -2.2       0.0   -20      526   No stop 
23 22 30  =1345+125    11 41 28  40.9  43.0 -2.1       0.0   250      595   23 18 01

23 23 00  J1347+1217   11 41 58  41.0  42.9 -2.1       0.0     9      595   23 23 00
23 27 00  =1345+125    11 45 59  41.6  41.9 -2.0       0.0   240      657   23 23 01

23 27 00  J1347+1217   11 45 59  41.6  41.9 -2.0       0.0   -20      657   No stop 
23 31 30  =1345+125    11 50 29  42.3  40.7 -2.0       0.0   250      727   23 27 01

23 31 30  J1347+1217   11 50 29  42.3  40.7 -2.0       0.0   -20      727   No stop 
23 36 00  =1345+125    11 55 00  42.9  39.5 -1.9       0.0   250      796   23 31 31
Schedule for HART      (Code Hh )                                   Page   3
               EVN observations of CSOs at 1.3cm (Session 2)
  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  26 Feb 2025   Day  57 ---

23 36 30  J1347+1217   11 55 30  43.0  39.4 -1.9       0.0     9      796   23 36 30
23 40 30  =1345+125    11 59 31  43.6  38.3 -1.8       0.0   240      858   23 36 31

23 40 30  J1347+1217   11 59 31  43.6  38.3 -1.8       0.0   -20      858   No stop 
23 45 00  =1345+125    12 04 02  44.2  37.0 -1.7       0.0   250      927   23 40 31

23 45 00  J1347+1217   12 04 02  44.2  37.0 -1.7       0.0   -20      927   No stop 
23 49 30  =1345+125    12 08 32  44.8  35.7 -1.7       0.0   250      997   23 45 01

23 50 00  J1347+1217   12 09 02  44.9  35.6 -1.7       0.0     9      997   23 50 00
23 54 00  =1345+125    12 13 03  45.4  34.4 -1.6       0.0   240     1059   23 50 01

23 54 00  J1347+1217   12 13 03  45.4  34.4 -1.6       0.0   -20     1059   No stop 
23 58 30  =1345+125    12 17 34  45.9  33.0 -1.5       0.0   250     1128   23 54 01

 --- Start: Wed  26 Feb 2025   Day  57 -- Stop: Thu  27 Feb 2025   Day  58 ---

23 58 30  J1347+1217   12 17 34  45.9  33.0 -1.5       0.0   -20     1128   No stop 
00 03 00  =1345+125    12 22 05  46.5  31.6 -1.4       0.0   250     1198   23 58 31

00 03 30  J1347+1217   12 22 35  46.5  31.5 -1.4       0.0     9     1198   00 03 30
00 07 30  =1345+125    12 26 35  47.0  30.2 -1.4       0.0   240     1260   00 03 31

00 07 30  J1347+1217   12 26 35  47.0  30.2 -1.4       0.0   -20     1260   No stop 
00 12 00  =1345+125    12 31 06  47.5  28.8 -1.3       0.0   250     1329   00 07 31

00 12 00  J1347+1217   12 31 06  47.5  28.8 -1.3       0.0   -20     1329   No stop 
00 16 30  =1345+125    12 35 37  48.0  27.3 -1.2       0.0   250     1399   00 12 01

00 17 00  J1347+1217   12 36 07  48.0  27.1 -1.2       0.0     9     1399   00 17 00
00 21 00  =1345+125    12 40 07  48.4  25.8 -1.1       0.0   240     1461   00 17 01

00 21 00  J1347+1217   12 40 07  48.4  25.8 -1.1       0.0   -20     1461   No stop 
00 25 30  =1345+125    12 44 38  48.9  24.2 -1.1       0.0   250     1530   00 21 01

00 25 30  J1347+1217   12 44 38  48.9  24.2 -1.1       0.0   -20     1530   No stop 
00 30 00  =1345+125    12 49 09  49.3  22.7 -1.0       0.0   250     1600   00 25 31

00 30 30  J1347+1217   12 49 39  49.3  22.5 -1.0       0.0     9     1600   00 30 30
00 34 30  =1345+125    12 53 40  49.7  21.1 -0.9       0.0   240     1662   00 30 31

00 34 30  J1347+1217   12 53 40  49.7  21.1 -0.9       0.0   -20     1662   No stop 
00 39 00  =1345+125    12 58 10  50.0  19.5 -0.8       0.0   250     1731   00 34 31
Schedule for HART      (Code Hh )                                   Page   4
               EVN observations of CSOs at 1.3cm (Session 2)
  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  27 Feb 2025   Day  58 ---

00 39 00  J1347+1217   12 58 10  50.0  19.5 -0.8       0.0   -20     1731   No stop 
00 43 30  =1345+125    13 02 41  50.3  17.8 -0.8       0.0   250     1801   00 39 01

00 44 30  J1347+1217   13 03 41  50.4  17.5 -0.8       0.0    39     1801   00 44 30
00 49 00  =1345+125    13 08 12  50.7  15.8 -0.7       0.0   270     1870   00 44 31

00 49 00  J1347+1217   13 08 12  50.7  15.8 -0.7       0.0   -20     1870   No stop 
00 53 00  =1345+125    13 12 13  50.9  14.3 -0.6       0.0   220     1932   00 49 01


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


 ======== Setup file: sess125.K2048
 --- 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:    4         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=  21480.00  21480.00  21480.00  21480.00  21480.00  21480.00  21480.00  21480.00
            21480.00  21480.00  21480.00  21480.00  21480.00  21480.00  21480.00  21480.00
   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=   22139.49  22139.49  22139.49  22139.49  22203.49  22203.49  22203.49  22203.49
             22267.49  22267.49  22267.49  22267.49  22331.49  22331.49  22331.49  22331.49
   BBC fr=     659.49    659.49    659.49    659.49    723.49    723.49    723.49    723.49
               787.49    787.49    787.49    787.49    851.49    851.49    851.49    851.49
   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:   8   9

   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)

 * NGC3998           11 55 20.947530   * 11 57 56.133331     11 59 16.874136       0.00
                     55 43 54.65353    * 55 27 12.92205      55 18 37.42249        0.00
                     From catalog imbedded in main SCHED input file.

   1053+815          10 53 36.229432   * 10 58 11.535369     11 00 37.853651       0.03
 * J1058+8114        81 30 35.56783    * 81 14 32.67518      81 06 23.71190        0.00
   J1058+81          /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution,  35777 observations.

   1125+596          11 25 23.181651   * 11 28 13.340676     11 29 41.945018       0.11
 * J1128+5925        59 41 46.14385    * 59 25 14.79854      59 16 47.30813        0.06
   J1128+59          /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution,    477 observations.

 * NGC3894           11 46 10.410918   * 11 48 50.358256     11 50 13.820333       0.36
   J1148+5924        59 41 36.72438    * 59 24 56.38192      59 16 22.53506        0.19
   1146+596          /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution,    120 observations.

 * 1156+295          11 56 57.786211   * 11 59 31.833912     12 00 50.969786       0.00
   J1159+2914        29 31 25.73880    * 29 14 43.82690      29 06 08.48410        0.00
   J1159+29          /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution,  78215 observations.

 * 3C286             13 28 49.657769   * 13 31 08.288061     13 32 19.394240       0.17
   J1331+3030        30 45 58.64066    * 30 30 32.95930      30 22 30.58841        0.16
   1328+307          /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc
   J1331+30          GSFC 2016a X/S astro solution,    269 observations.

   1345+125          13 45 06.171234   * 13 47 33.361612     13 48 48.446212       0.10
 * J1347+1217        12 32 20.33883    * 12 17 24.24015      12 09 39.64632        0.21
   J1347+12          /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution,    201 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
  NGC3998    sess125.K2048         1 2 3 6 7 8 10 11 12 13 14  +     0.867    71.210
  J1058+8114 sess125.K2048         1 2 3 6 7 8 10 11 12 13 14  +     0.050     5.247
  J1128+5925 sess125.K2048         1 2 3 6 7 8 10 11 12 13 14  +     0.150    18.843
  NGC3894    sess125.K2048         1 2 3 6 7 8 10 11 12 13 14  +     2.200   260.287
  1156+295   sess125.K2048         1 2 3 6 7 8 10 11 12 13 14  +     0.058     8.925
  3C286      sess125.K2048         2 14                              0.050     0.500
  J1347+1217 sess125.K2048         1 2 3 6 7 8 10 11 12 13 14  +     2.025   277.350


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) 
   NGC3998            130.5
   J1058+8114         107.2
   J1128+5925         128.2
   NGC3894            127.4
   1156+295           152.0
   3C286              134.4
   J1347+1217         133.7

  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 

