  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: Tracing the Radio Outflows in RQ AGN from Pc- to Kpc-scales
 Exp. Code:  EG131G  


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

PI:       Salmoli Ghosh

Address:  National Centre for Radio Astrophysics - TIFR
          S.P. Pune Univ. Campus, Ganeshkhind
          Pune
          India : 411007

Phone:    (+91)020-25719000
EMAIL:    salmoli.ghosh@gmail.com
Fax:
Phone during observation: (+91)8240982699/(+91)020-25719230

Observing mode: Phase-referencing continuum

Notes:    PCAL OFF
 
 
 

Schedule for HART      (Code Hh )                                   Page   2
               Tracing the Radio Outflows in RQ AGN from Pc- to Kpc-scales
  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  23 Feb 2025   Day  54 ---

 Next scan frequencies:  1626.49  1626.49  1626.49  1626.49  1690.49  1690.49  1690.49  1690.49
 Next BBC frequencies:    116.49   116.49   116.49   116.49   180.49   180.49   180.49   180.49
 Next scan bandwidths:     32.00    32.00    32.00    32.00    32.00    32.00    32.00    32.00

00 00 00  4C39.25      12 03 18  15.8 329.7  2.6       0.0     0        0   00 00 00
00 07 00  ---          12 10 19  15.0 328.5  2.7       0.0   420       54   00 00 01

00 12 00  J1214+0829   12 15 20  55.8   0.4 -0.0       0.0   190       54   00 12 00
00 17 00  =1212+087    12 20 21  55.7 358.2  0.1       0.0   300       93   00 12 01

00 17 00  NGC4235      12 20 21  57.1 359.1  0.0       0.0   -29       93   No stop 
00 20 30  ---          12 23 51  57.0 357.5  0.1       0.0   181      120   00 17 01

00 21 00  J1214+0829   12 24 21  55.7 356.5  0.1       0.0     1      120   00 21 00
00 22 00  =1212+087    12 25 21  55.7 356.0  0.2       0.0    60      128   00 21 01

00 22 00  NGC4235      12 25 21  57.0 356.9  0.1       0.0   -29      128   No stop 
00 25 30  ---          12 28 52  57.0 355.3  0.2       0.0   181      155   00 22 01

00 25 30  J1214+0829   12 28 52  55.6 354.5  0.2       0.0   -29      155   No stop 
00 27 00  =1212+087    12 30 22  55.6 353.8  0.2       0.0    61      166   00 25 31

00 27 00  NGC4235      12 30 22  56.9 354.6  0.2       0.0   -29      166   No stop 
00 30 30  ---          12 33 53  56.8 353.0  0.3       0.0   181      193   00 27 01

00 31 00  J1214+0829   12 34 23  55.5 352.1  0.3       0.0     1      193   00 31 00
00 32 00  =1212+087    12 35 23  55.5 351.7  0.3       0.0    60      201   00 31 01

00 32 00  NGC4235      12 35 23  56.8 352.3  0.3       0.0   -29      201   No stop 
00 35 30  ---          12 38 54  56.7 350.7  0.3       0.0   181      228   00 32 01

00 35 30  J1214+0829   12 38 54  55.3 350.1  0.4       0.0   -29      228   No stop 
00 37 00  =1212+087    12 40 24  55.3 349.5  0.4       0.0    61      240   00 35 31

00 37 00  NGC4235      12 40 24  56.6 350.1  0.4       0.0   -29      240   No stop 
00 40 30  ---          12 43 54  56.5 348.5  0.4       0.0   181      267   00 37 01

00 41 00  J1214+0829   12 44 25  55.1 347.8  0.5       0.0     1      267   00 41 00
00 42 00  =1212+087    12 45 25  55.0 347.4  0.5       0.0    60      274   00 41 01

00 42 00  NGC4235      12 45 25  56.4 347.9  0.4       0.0   -29      274   No stop 
00 45 30  ---          12 48 55  56.2 346.3  0.5       0.0   181      301   00 42 01

00 45 30  J1214+0829   12 48 55  54.9 345.9  0.5       0.0   -29      301   No stop 
00 47 00  =1212+087    12 50 26  54.8 345.3  0.6       0.0    61      313   00 45 31
Schedule for HART      (Code Hh )                                   Page   3
               Tracing the Radio Outflows in RQ AGN from Pc- to Kpc-scales
  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  23 Feb 2025   Day  54 ---

00 47 00  NGC4235      12 50 26  56.2 345.7  0.5       0.0   -29      313   No stop 
00 50 30  ---          12 53 56  56.0 344.1  0.6       0.0   181      340   00 47 01

00 51 00  J1214+0829   12 54 26  54.5 343.6  0.6       0.0     1      340   00 51 00
00 52 00  =1212+087    12 55 26  54.5 343.2  0.7       0.0    60      348   00 51 01

00 52 00  NGC4235      12 55 26  55.9 343.5  0.6       0.0   -29      348   No stop 
00 55 30  ---          12 58 57  55.6 342.0  0.7       0.0   181      375   00 52 01

00 55 30  J1214+0829   12 58 57  54.2 341.8  0.7       0.0   -29      375   No stop 
00 57 00  =1212+087    13 00 27  54.1 341.1  0.7       0.0    61      386   00 55 31

00 57 00  NGC4235      13 00 27  55.5 341.4  0.7       0.0   -29      386   No stop 
01 00 30  ---          13 03 58  55.3 339.9  0.8       0.0   181      414   00 57 01

01 01 00  J1214+0829   13 04 28  53.8 339.5  0.8       0.0     1      414   01 01 00
01 02 00  =1212+087    13 05 28  53.7 339.1  0.8       0.0    60      421   01 01 01

01 02 00  NGC4235      13 05 28  55.1 339.3  0.8       0.0   -29      421   No stop 
01 05 30  ---          13 08 59  54.9 337.9  0.8       0.0   181      448   01 02 01

01 05 30  J1214+0829   13 08 59  53.4 337.8  0.9       0.0   -29      448   No stop 
01 07 00  =1212+087    13 10 29  53.3 337.2  0.9       0.0    61      460   01 05 31

01 07 00  NGC4235      13 10 29  54.7 337.3  0.9       0.0   -29      460   No stop 
01 10 30  ---          13 13 59  54.4 335.9  0.9       0.0   181      487   01 07 01

01 11 00  J1214+0829   13 14 29  53.0 335.6  1.0       0.0     1      487   01 11 00
01 12 00  =1212+087    13 15 30  52.9 335.3  1.0       0.0    60      495   01 11 01

01 12 00  NGC4235      13 15 30  54.3 335.3  1.0       0.0   -29      495   No stop 
01 15 30  ---          13 19 00  53.9 333.9  1.0       0.0   181      522   01 12 01

01 15 30  J1214+0829   13 19 00  52.5 333.9  1.0       0.0   -29      522   No stop 
01 17 00  =1212+087    13 20 30  52.4 333.4  1.1       0.0    61      533   01 15 31

01 17 00  NGC4235      13 20 30  53.8 333.3  1.0       0.0   -29      533   No stop 
01 20 30  ---          13 24 01  53.4 332.0  1.1       0.0   181      560   01 17 01

01 21 00  J1214+0829   13 24 31  52.0 331.9  1.1       0.0     1      560   01 21 00
01 22 00  =1212+087    13 25 31  51.9 331.5  1.2       0.0    60      568   01 21 01

01 22 00  NGC4235      13 25 31  53.3 331.4  1.1       0.0   -29      568   No stop 
01 25 30  ---          13 29 02  52.9 330.1  1.2       0.0   181      595   01 22 01
Schedule for HART      (Code Hh )                                   Page   4
               Tracing the Radio Outflows in RQ AGN from Pc- to Kpc-scales
  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  23 Feb 2025   Day  54 ---

01 25 30  J1214+0829   13 29 02  51.5 330.3  1.2       0.0   -29      595   No stop 
01 27 00  =1212+087    13 30 32  51.3 329.8  1.2       0.0    61      607   01 25 31

01 27 00  NGC4235      13 30 32  52.7 329.6  1.2       0.0   -29      607   No stop 
01 30 30  ---          13 34 03  52.3 328.3  1.3       0.0   181      634   01 27 01

01 31 00  J1214+0829   13 34 33  50.8 328.4  1.3       0.0     1      634   01 31 00
01 32 00  =1212+087    13 35 33  50.7 328.0  1.3       0.0    60      642   01 31 01

01 32 00  NGC4235      13 35 33  52.1 327.8  1.3       0.0   -29      642   No stop 
01 35 30  ---          13 39 04  51.7 326.5  1.3       0.0   181      669   01 32 01

01 35 30  J1214+0829   13 39 04  50.3 326.8  1.4       0.0   -29      669   No stop 
01 37 00  =1212+087    13 40 34  50.1 326.3  1.4       0.0    61      680   01 35 31

01 37 00  NGC4235      13 40 34  51.5 326.0  1.4       0.0   -29      680   No stop 
01 40 30  ---          13 44 04  51.0 324.8  1.4       0.0   181      707   01 37 01

01 41 00  J1214+0829   13 44 34  49.6 325.0  1.5       0.0     1      707   01 41 00
01 42 00  =1212+087    13 45 35  49.5 324.7  1.5       0.0    60      715   01 41 01

01 42 00  NGC4235      13 45 35  50.9 324.3  1.5       0.0   -29      715   No stop 
01 45 30  ---          13 49 05  50.4 323.2  1.5       0.0   181      742   01 42 01

01 45 30  J1214+0829   13 49 05  49.0 323.6  1.5       0.0   -29      742   No stop 
01 47 00  =1212+087    13 50 35  48.8 323.1  1.6       0.0    61      754   01 45 31

01 47 00  NGC4235      13 50 35  50.2 322.7  1.5       0.0   -29      754   No stop 
01 50 30  ---          13 54 06  49.7 321.6  1.6       0.0   181      781   01 47 01

01 51 00  J1214+0829   13 54 36  48.3 321.8  1.6       0.0     1      781   01 51 00
01 52 00  =1212+087    13 55 36  48.1 321.5  1.7       0.0    60      788   01 51 01

01 52 00  NGC4235      13 55 36  49.5 321.1  1.6       0.0   -29      788   No stop 
01 55 30  ---          13 59 07  49.0 320.0  1.7       0.0   181      815   01 52 01

01 55 30  J1214+0829   13 59 07  47.6 320.5  1.7       0.0   -29      815   No stop 
01 57 00  =1212+087    14 00 37  47.4 320.0  1.7       0.0    61      827   01 55 31

01 57 00  NGC4235      14 00 37  48.8 319.5  1.7       0.0   -29      827   No stop 
02 00 30  ---          14 04 08  48.2 318.5  1.8       0.0   181      854   01 57 01

02 01 00  J1214+0829   14 04 38  46.8 318.8  1.8       0.0     1      854   02 01 00
02 02 00  =1212+087    14 05 38  46.7 318.6  1.8       0.0    60      862   02 01 01
Schedule for HART      (Code Hh )                                   Page   5
               Tracing the Radio Outflows in RQ AGN from Pc- to Kpc-scales
  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  23 Feb 2025   Day  54 ---

02 02 00  NGC4235      14 05 38  48.0 318.0  1.8       0.0   -29      862   No stop 
02 05 30  ---          14 09 08  47.5 317.0  1.8       0.0   181      889   02 02 01

02 05 30  J1214+0829   14 09 08  46.1 317.6  1.9       0.0   -29      889   No stop 
02 07 00  =1212+087    14 10 39  45.9 317.1  1.9       0.0    61      900   02 05 31

02 07 00  NGC4235      14 10 39  47.3 316.6  1.9       0.0   -29      900   No stop 
02 10 30  ---          14 14 09  46.7 315.6  1.9       0.0   181      927   02 07 01

02 11 00  J1214+0829   14 14 39  45.3 316.0  2.0       0.0     1      927   02 11 00
02 12 00  =1212+087    14 15 40  45.1 315.7  2.0       0.0    60      935   02 11 01

02 12 00  NGC4235      14 15 40  46.5 315.2  2.0       0.0   -29      935   No stop 
02 15 30  ---          14 19 10  45.9 314.2  2.0       0.0   181      962   02 12 01

02 15 30  J1214+0829   14 19 10  44.6 314.8  2.0       0.0   -29      962   No stop 
02 17 00  =1212+087    14 20 40  44.3 314.4  2.1       0.0    61      974   02 15 31

02 17 00  NGC4235      14 20 40  45.7 313.8  2.0       0.0   -29      974   No stop 
02 20 30  ---          14 24 11  45.1 312.9  2.1       0.0   181     1001   02 17 01

02 21 00  J1214+0829   14 24 41  43.7 313.4  2.1       0.0     1     1001   02 21 00
02 22 00  =1212+087    14 25 41  43.5 313.1  2.2       0.0    60     1009   02 21 01

02 22 00  NGC4235      14 25 41  44.8 312.5  2.1       0.0   -29     1009   No stop 
02 25 30  ---          14 29 12  44.3 311.6  2.2       0.0   181     1036   02 22 01

02 25 30  J1214+0829   14 29 12  42.9 312.2  2.2       0.0   -29     1036   No stop 
02 27 00  =1212+087    14 30 42  42.7 311.9  2.2       0.0    61     1047   02 25 31

02 27 00  NGC4235      14 30 42  44.0 311.2  2.2       0.0   -29     1047   No stop 
02 30 30  ---          14 34 13  43.4 310.3  2.3       0.0   181     1074   02 27 01

02 31 00  J1214+0829   14 34 43  42.0 310.9  2.3       0.0     1     1074   02 31 00
02 32 00  =1212+087    14 35 43  41.8 310.6  2.3       0.0    60     1082   02 31 01

02 32 00  NGC4235      14 35 43  43.1 309.9  2.3       0.0   -29     1082   No stop 
02 35 30  ---          14 39 13  42.5 309.1  2.3       0.0   181     1109   02 32 01

02 35 30  J1214+0829   14 39 13  41.2 309.8  2.4       0.0   -29     1109   No stop 
02 37 00  =1212+087    14 40 44  41.0 309.4  2.4       0.0    61     1121   02 35 31

02 37 00  NGC4235      14 40 44  42.3 308.7  2.4       0.0   -29     1121   No stop 
02 40 30  ---          14 44 14  41.7 307.9  2.4       0.0   181     1148   02 37 01
Schedule for HART      (Code Hh )                                   Page   6
               Tracing the Radio Outflows in RQ AGN from Pc- to Kpc-scales
  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  23 Feb 2025   Day  54 ---

02 41 00  J1214+0829   14 44 44  40.3 308.5  2.5       0.0     1     1148   02 41 00
02 42 00  =1212+087    14 45 44  40.1 308.3  2.5       0.0    60     1156   02 41 01

02 42 00  NGC4235      14 45 44  41.4 307.6  2.5       0.0   -29     1156   No stop 
02 45 30  ---          14 49 15  40.8 306.8  2.5       0.0   181     1183   02 42 01

02 45 30  J1214+0829   14 49 15  39.5 307.5  2.5       0.0   -29     1183   No stop 
02 47 00  =1212+087    14 50 45  39.2 307.2  2.6       0.0    61     1194   02 45 31

02 54 00  3C286        14 57 46  30.1 338.7  1.4       0.0   349     1194   02 54 00
03 00 00  ---          15 03 47  29.6 337.3  1.5       0.0   360     1241   02 54 01


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


 ======== Setup file: sess125.L1024
   Matching groups in /home/guest/rmc/SCHED/sched11.6/catalogs/freq_RDBE.dat:
     hh18cm          Values confirmed by E-mail Jonathan Quick 20140219 (CR)
    ****** Only  122.49 of  256.00 MHz total bandwidth is within the IFs
           in the setup file before any FREQ or DOPPLER shifts.

   Setup group:    5         Station: HART              Total bit rate:  1024
   Format: VDIF              Bits per sample: 2         Sample rate: 64.000
   Number of channels:  8    DBE type: DBBC_DDC         Speedup factor:   1.00

   Disk used to record data.

   1st LO=   1510.00   1510.00   1510.00   1510.00   1510.00   1510.00   1510.00   1510.00
   Net SB=         L         L         U         U         L         L         U         U
   IF SB =         U         U         U         U         U         U         U         U
   Pol.  =      RCP       LCP       RCP       LCP       RCP       LCP       RCP       LCP 
   BBC   =         1         9         1         9         2        10         2        10
   BBC SB=         L         L         U         U         L         L         U         U
   IF    =        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=   1626.49  1626.49  1626.49  1626.49  1690.49  1690.49  1690.49  1690.49
   BBC fr=    116.49   116.49   116.49   116.49   180.49   180.49   180.49   180.49
   Bandwd=     32.00    32.00    32.00    32.00    32.00    32.00    32.00    32.00
    Matching frequency sets:   8

   Track assignments are: 
    track1=   1,  2,  3,  4,  5,  6,  7,  8
    barrel=roll_off 

 POSITIONS OF SOURCES USED IN RECORDING SCANS

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

 * NGC4235           12 14 36.713052   * 12 17 09.880000     12 18 28.134699       0.00
                     07 28 09.25124    * 07 11 29.60000      07 02 57.23478        0.00
                     From catalog imbedded in main SCHED input file.

 * 4C39.25           09 23 55.319216   * 09 27 03.013937     09 28 39.230622       0.31
   J0927+3902        39 15 23.56644    * 39 02 20.85185      38 55 45.55204        0.16
   0923+392          /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc
   J0927+39          GSFC 2016a X/S astro solution, 250526 observations.

   1212+087          12 12 26.757767   * 12 14 59.913189     12 16 18.178938       0.96
 * J1214+0829        08 46 02.77335    * 08 29 22.51814      08 20 49.70342        1.14
                     /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution,     46 observations.

 * 3C286             13 28 49.657769   * 13 31 08.288061     13 32 19.270192       0.17
   J1331+3030        30 45 58.64066    * 30 30 32.95930      30 22 30.64299        0.16
   1328+307          /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc
   J1331+30          GSFC 2016a X/S astro solution,    269 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
  NGC4235    sess125.L1024         1 2 3 4 5 6 7 8 9                 1.750   114.877
  4C39.25    sess125.L1024         1 2 3 4 5 6 7 8 9                 0.167    10.153
  J1214+0829 sess125.L1024         1 2 3 4 5 6 7 8 9                 0.708    41.911
  3C286      sess125.L1024         1 2 3 4 5 6 7 8 9                 0.100     3.688


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) 
   NGC4235            152.1
   4C39.25            148.2
   J1214+0829         152.8
   3C286              132.1

  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 

