  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: Tracing the Radio Outflows in RQ AGN from Pc- to Kpc-scales
 Exp. Code:  EG131E  


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
----------------------------------------------------------------------------------------

 --- Thu  30 May 2024   Day 151 ---

 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

13 00 00  4C39.25      07 24 53  19.0  25.0 -2.1       0.0     0        0   13 00 00
13 05 00  ---          07 29 53  19.5  24.1 -2.0       0.0   300       39   13 00 01

16 45 00  4C39.25      11 10 30  20.9 339.0  1.7       0.0 13175       39   16 45 00
16 53 00  ---          11 18 31  20.3 337.5  1.8       0.0   480      100   16 45 01

16 55 00  3C286        11 20 31  25.5  31.3 -2.2       0.0   -28      100   16 55 00
16 58 00  ---          11 23 32  25.8  30.7 -2.1       0.0   152      124   16 55 01

 ---------- source change ----------

17 00 00  J1225+1253   11 25 32  48.6  22.8 -1.0       0.0    58      124   17 00 00
17 01 30  =M84         11 27 02  48.8  22.2 -1.0       0.0    90      135   17 00 01

17 01 30  NGC4388      11 27 02  48.9  22.6 -1.0       0.0   -24      135   No stop 
17 05 00  ---          11 30 33  49.2  21.4 -0.9       0.0   186      162   17 01 31

17 05 30  J1225+1253   11 31 03  49.1  20.8 -0.9       0.0     6      162   17 05 30
17 06 30  =M84         11 32 03  49.2  20.5 -0.9       0.0    60      170   17 05 31

17 06 30  NGC4388      11 32 03  49.3  20.8 -0.9       0.0   -24      170   No stop 
17 10 00  ---          11 35 34  49.6  19.6 -0.9       0.0   186      197   17 06 31

17 10 00  J1225+1253   11 35 34  49.4  19.2 -0.8       0.0   -24      197   No stop 
17 11 30  =M84         11 37 04  49.5  18.7 -0.8       0.0    66      209   17 10 01

17 11 30  NGC4388      11 37 04  49.7  19.1 -0.8       0.0   -24      209   No stop 
17 15 00  ---          11 40 34  50.0  17.8 -0.8       0.0   186      236   17 11 31

17 15 30  J1225+1253   11 41 05  49.8  17.2 -0.8       0.0     6      236   17 15 30
17 16 30  =M84         11 42 05  49.9  16.9 -0.7       0.0    60      243   17 15 31

17 16 30  NGC4388      11 42 05  50.1  17.2 -0.7       0.0   -24      243   No stop 
17 20 00  ---          11 45 35  50.3  15.9 -0.7       0.0   186      271   17 16 31

17 20 00  J1225+1253   11 45 35  50.1  15.6 -0.7       0.0   -24      271   No stop 
17 21 30  =M84         11 47 06  50.2  15.0 -0.7       0.0    66      282   17 20 01

17 21 30  NGC4388      11 47 06  50.4  15.4 -0.7       0.0   -24      282   No stop 
17 25 00  ---          11 50 36  50.6  14.1 -0.6       0.0   186      309   17 21 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
----------------------------------------------------------------------------------------

 --- Thu  30 May 2024   Day 151 ---

17 25 30  J1225+1253   11 51 06  50.4  13.5 -0.6       0.0     6      309   17 25 30
17 26 30  =M84         11 52 06  50.5  13.2 -0.6       0.0    60      317   17 25 31

17 26 30  NGC4388      11 52 06  50.7  13.5 -0.6       0.0   -24      317   No stop 
17 30 00  ---          11 55 37  50.8  12.2 -0.5       0.0   186      344   17 26 31

17 30 00  J1225+1253   11 55 37  50.6  11.9 -0.5       0.0   -24      344   No stop 
17 31 30  =M84         11 57 07  50.7  11.3 -0.5       0.0    66      356   17 30 01

17 31 30  NGC4388      11 57 07  50.9  11.6 -0.5       0.0   -24      356   No stop 
17 35 00  ---          12 00 38  51.0  10.3 -0.4       0.0   186      383   17 31 31

17 35 30  J1225+1253   12 01 08  50.9   9.8 -0.4       0.0     6      383   17 35 30
17 36 30  =M84         12 02 08  50.9   9.4 -0.4       0.0    60      390   17 35 31

17 36 30  NGC4388      12 02 08  51.1   9.7 -0.4       0.0   -24      390   No stop 
17 40 00  ---          12 05 39  51.2   8.4 -0.4       0.0   186      417   17 36 31

17 40 00  J1225+1253   12 05 39  51.0   8.0 -0.3       0.0   -24      417   No stop 
17 41 30  =M84         12 07 09  51.1   7.4 -0.3       0.0    66      429   17 40 01

17 41 30  NGC4388      12 07 09  51.3   7.8 -0.3       0.0   -24      429   No stop 
17 45 00  ---          12 10 39  51.4   6.4 -0.3       0.0   186      456   17 41 31

17 45 30  J1225+1253   12 11 09  51.2   5.9 -0.3       0.0     6      456   17 45 30
17 46 30  =M84         12 12 10  51.2   5.5 -0.2       0.0    60      464   17 45 31

17 46 30  NGC4388      12 12 10  51.4   5.8 -0.2       0.0   -24      464   No stop 
17 50 00  ---          12 15 40  51.5   4.5 -0.2       0.0   186      491   17 46 31

17 50 00  J1225+1253   12 15 40  51.3   4.1 -0.2       0.0   -24      491   No stop 
17 51 30  =M84         12 17 10  51.3   3.6 -0.2       0.0    66      502   17 50 01

17 51 30  NGC4388      12 17 10  51.5   3.9 -0.2       0.0   -24      502   No stop 
17 55 00  ---          12 20 41  51.6   2.5 -0.1       0.0   186      529   17 51 31

17 55 30  J1225+1253   12 21 11  51.3   2.0 -0.1       0.0     6      529   17 55 30
17 56 30  =M84         12 22 11  51.3   1.6 -0.1       0.0    60      537   17 55 31

17 56 30  NGC4388      12 22 11  51.6   1.9 -0.1       0.0   -24      537   No stop 
18 00 00  ---          12 25 42  51.6   0.5 -0.0       0.0   186      564   17 56 31

18 00 00  J1225+1253   12 25 42  51.4   0.2 -0.0       0.0   -24      564   No stop 
18 01 30  =M84         12 27 12  51.4 359.7  0.0       0.0    66      576   18 00 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
----------------------------------------------------------------------------------------

 --- Thu  30 May 2024   Day 151 ---

18 01 30  NGC4388      12 27 12  51.6 359.9  0.0       0.0   -24      576   No stop 
18 05 00  ---          12 30 43  51.6 358.6  0.1       0.0   186      603   18 01 31

18 05 30  J1225+1253   12 31 13  51.3 358.1  0.1       0.0     6      603   18 05 30
18 06 30  =M84         12 32 13  51.3 357.7  0.1       0.0    60      611   18 05 31

18 06 30  NGC4388      12 32 13  51.6 358.0  0.1       0.0   -24      611   No stop 
18 10 00  ---          12 35 43  51.5 356.6  0.1       0.0   186      638   18 06 31

18 10 00  J1225+1253   12 35 43  51.3 356.3  0.2       0.0   -24      638   No stop 
18 11 30  =M84         12 37 14  51.3 355.7  0.2       0.0    66      649   18 10 01

18 11 30  NGC4388      12 37 14  51.5 356.0  0.2       0.0   -24      649   No stop 
18 15 00  ---          12 40 44  51.4 354.6  0.2       0.0   186      676   18 11 31

18 15 30  J1225+1253   12 41 14  51.2 354.2  0.2       0.0     6      676   18 15 30
18 16 30  =M84         12 42 15  51.2 353.8  0.3       0.0    60      684   18 15 31

18 16 30  NGC4388      12 42 15  51.4 354.0  0.3       0.0   -24      684   No stop 
18 20 00  ---          12 45 45  51.3 352.7  0.3       0.0   186      711   18 16 31

18 20 00  J1225+1253   12 45 45  51.1 352.4  0.3       0.0   -24      711   No stop 
18 21 30  =M84         12 47 15  51.0 351.9  0.3       0.0    66      723   18 20 01

18 21 30  NGC4388      12 47 15  51.3 352.1  0.3       0.0   -24      723   No stop 
18 25 00  ---          12 50 46  51.2 350.7  0.4       0.0   186      750   18 21 31

18 25 30  J1225+1253   12 51 16  50.9 350.3  0.4       0.0     6      750   18 25 30
18 26 30  =M84         12 52 16  50.8 349.9  0.4       0.0    60      757   18 25 31

18 26 30  NGC4388      12 52 16  51.1 350.2  0.4       0.0   -24      757   No stop 
18 30 00  ---          12 55 47  51.0 348.8  0.5       0.0   186      785   18 26 31

18 30 00  J1225+1253   12 55 47  50.7 348.6  0.5       0.0   -24      785   No stop 
18 31 30  =M84         12 57 17  50.6 348.0  0.5       0.0    66      796   18 30 01

18 31 30  NGC4388      12 57 17  50.9 348.2  0.5       0.0   -24      796   No stop 
18 35 00  ---          13 00 48  50.7 346.9  0.6       0.0   186      823   18 31 31

18 35 30  J1225+1253   13 01 18  50.4 346.5  0.6       0.0     6      823   18 35 30
18 36 30  =M84         13 02 18  50.4 346.2  0.6       0.0    60      831   18 35 31

18 36 30  NGC4388      13 02 18  50.6 346.4  0.6       0.0   -24      831   No stop 
18 40 00  ---          13 05 48  50.4 345.0  0.6       0.0   186      858   18 36 31
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
----------------------------------------------------------------------------------------

 --- Thu  30 May 2024   Day 151 ---

18 40 00  J1225+1253   13 05 48  50.2 344.9  0.7       0.0   -24      858   No stop 
18 41 30  =M84         13 07 19  50.1 344.3  0.7       0.0    66      870   18 40 01

18 41 30  NGC4388      13 07 19  50.4 344.5  0.7       0.0   -24      870   No stop 
18 45 00  ---          13 10 49  50.1 343.2  0.7       0.0   186      897   18 41 31

18 45 30  J1225+1253   13 11 19  49.8 342.8  0.8       0.0     6      897   18 45 30
18 46 30  =M84         13 12 19  49.8 342.5  0.8       0.0    60      904   18 45 31

18 46 30  NGC4388      13 12 19  50.0 342.6  0.8       0.0   -24      904   No stop 
18 50 00  ---          13 15 50  49.8 341.4  0.8       0.0   186      931   18 46 31

18 50 00  J1225+1253   13 15 50  49.5 341.2  0.8       0.0   -24      931   No stop 
18 51 30  =M84         13 17 20  49.4 340.7  0.9       0.0    66      943   18 50 01

18 51 30  NGC4388      13 17 20  49.7 340.8  0.8       0.0   -24      943   No stop 
18 55 00  ---          13 20 51  49.4 339.6  0.9       0.0   186      970   18 51 31

18 55 30  J1225+1253   13 21 21  49.1 339.2  0.9       0.0     6      970   18 55 30
18 56 30  =M84         13 22 21  49.0 338.9  0.9       0.0    60      978   18 55 31

18 56 30  NGC4388      13 22 21  49.3 339.0  0.9       0.0   -24      978   No stop 
19 00 00  ---          13 25 52  49.0 337.8  1.0       0.0   186     1005   18 56 31

19 00 00  J1225+1253   13 25 52  48.7 337.7  1.0       0.0   -24     1005   No stop 
19 01 30  =M84         13 27 22  48.6 337.2  1.0       0.0    66     1016   19 00 01

19 01 30  NGC4388      13 27 22  48.9 337.3  1.0       0.0   -24     1016   No stop 
19 05 00  ---          13 30 53  48.6 336.1  1.1       0.0   186     1043   19 01 31

19 05 30  J1225+1253   13 31 23  48.2 335.8  1.1       0.0     6     1043   19 05 30
19 06 30  =M84         13 32 23  48.1 335.4  1.1       0.0    60     1051   19 05 31

19 06 30  NGC4388      13 32 23  48.4 335.6  1.1       0.0   -24     1051   No stop 
19 10 00  ---          13 35 53  48.1 334.4  1.1       0.0   186     1078   19 06 31

19 10 00  J1225+1253   13 35 53  47.8 334.3  1.2       0.0   -24     1078   No stop 
19 11 30  =M84         13 37 24  47.7 333.8  1.2       0.0    66     1090   19 10 01

19 11 30  NGC4388      13 37 24  47.9 333.9  1.2       0.0   -24     1090   No stop 
19 15 00  ---          13 40 54  47.6 332.7  1.2       0.0   186     1117   19 11 31

19 15 30  J1225+1253   13 41 24  47.3 332.5  1.3       0.0     6     1117   19 15 30
19 16 30  =M84         13 42 24  47.1 332.1  1.3       0.0    60     1125   19 15 31
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
----------------------------------------------------------------------------------------

 --- Thu  30 May 2024   Day 151 ---

19 16 30  NGC4388      13 42 24  47.4 332.2  1.3       0.0   -24     1125   No stop 
19 20 00  ---          13 45 55  47.1 331.1  1.3       0.0   186     1152   19 16 31

19 20 00  J1225+1253   13 45 55  46.8 331.0  1.3       0.0   -24     1152   No stop 
19 21 30  =M84         13 47 25  46.6 330.5  1.4       0.0    66     1163   19 20 01

19 21 30  NGC4388      13 47 25  46.9 330.6  1.3       0.0   -24     1163   No stop 
19 25 00  ---          13 50 56  46.5 329.5  1.4       0.0   186     1190   19 21 31

19 25 30  J1225+1253   13 51 26  46.2 329.3  1.4       0.0     6     1190   19 25 30
19 26 30  =M84         13 52 26  46.0 329.0  1.4       0.0    60     1198   19 25 31

19 26 30  NGC4388      13 52 26  46.3 329.0  1.4       0.0   -24     1198   No stop 
19 30 00  ---          13 55 57  45.9 327.9  1.5       0.0   186     1225   19 26 31

19 30 00  J1225+1253   13 55 57  45.6 327.9  1.5       0.0   -24     1225   No stop 
19 31 30  =M84         13 57 27  45.4 327.4  1.5       0.0    66     1237   19 30 01

19 31 30  NGC4388      13 57 27  45.7 327.5  1.5       0.0   -24     1237   No stop 
19 35 00  ---          14 00 57  45.3 326.4  1.6       0.0   186     1264   19 31 31

19 35 30  J1225+1253   14 01 28  45.0 326.2  1.6       0.0     6     1264   19 35 30
19 36 30  =M84         14 02 28  44.8 325.9  1.6       0.0    60     1271   19 35 31

19 36 30  NGC4388      14 02 28  45.1 326.0  1.6       0.0   -24     1271   No stop 
19 40 00  ---          14 05 58  44.7 324.9  1.6       0.0   186     1298   19 36 31

19 40 00  J1225+1253   14 05 58  44.4 324.9  1.7       0.0   -24     1298   No stop 
19 41 30  =M84         14 07 29  44.2 324.5  1.7       0.0    66     1310   19 40 01

23 52 00  3C345        18 18 40  20.7 340.7  1.6       0.0 14875     1310   23 52 00
23 59 59  ---          18 26 41  20.1 339.2  1.7       0.0   479     1372   23 52 01


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


 ======== Setup file: sess224.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)

 * MRK9              07 32 42.186828   * 07 36 57.020000     07 38 59.084199       0.00
                     58 52 56.23686    * 58 46 13.40000      58 43 09.45480        0.00
                     From catalog imbedded in main SCHED input file.

 * NGC4388           12 23 14.667279   * 12 25 46.810000     12 27 01.498572       0.00
                     12 56 19.70042    * 12 39 43.40000      12 31 39.24087        0.00
                     From catalog imbedded in main SCHED input file.

 * NGC3516           11 03 22.809672   * 11 06 47.460000     11 08 27.869385       0.00
                     72 50 20.39872    * 72 34 07.20000      72 26 32.40388        0.00
                     From catalog imbedded in main SCHED input file.

   UG03927           07 33 11.618492   * 07 37 30.086987     07 39 33.864594       0.42
 * J0737+5941        59 47 48.11460    * 59 41 03.19422      59 37 58.33032        0.54
   0733+597          /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution,     51 observations.

 * 4C39.25           09 23 55.319216   * 09 27 03.013937     09 28 33.839979       0.31
   J0927+3902        39 15 23.56644    * 39 02 20.85185      38 56 11.89601        0.16
   0923+392          /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc
   J0927+39          GSFC 2016a X/S astro solution, 250526 observations.

   1104+728          11 04 17.979109   * 11 07 41.722541     11 09 21.716986       0.11
 * J1107+7232        72 48 50.14178    * 72 32 36.00502      72 25 00.73332        0.03
                     /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution,   1253 observations.

   M84               12 22 31.582018   * 12 25 03.743334     12 26 18.438568       0.04
 * J1225+1253        13 09 49.76866    * 12 53 13.13927      12 45 08.91099        0.11
   1222+131          /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc
                     GSFC 2016a X/S astro solution,    667 observations.

 * 3C286             13 28 49.657769   * 13 31 08.288061     13 32 16.993584       0.17
   J1331+3030        30 45 58.64066    * 30 30 32.95930      30 23 05.63249        0.16
   1328+307          /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc
   J1331+30          GSFC 2016a X/S astro solution,    269 observations.

 * 3C345             16 41 17.606229   * 16 42 58.809967     16 43 49.928936       0.79
   J1642+3948        39 54 10.81492    * 39 48 36.99399      39 45 46.70940        0.59
   1641+399          /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc
   J1642+39          GSFC 2016a X/S astro solution,  53724 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
  MRK9       sess224.L1024         1 2 3 4 5 6 7 9 10                2.450   157.043
  NGC4388    sess224.L1024         1 2 3 4 5 6 7 8 9 10              1.867   158.603
  NGC3516    sess224.L1024         1 2 3 4 5 6 7 9 10                2.417   179.474
  J0737+5941 sess224.L1024         1 2 3 4 5 6 7 9 10                0.925    49.872
  4C39.25    sess224.L1024         1 2 3 4 5 6 7 8 9 10              0.400    23.533
  J1107+7232 sess224.L1024         1 2 3 4 5 6 7 9 10                1.042    66.712
  J1225+1253 sess224.L1024         1 2 3 4 5 6 7 8 9 10              0.692    52.706
  3C286      sess224.L1024         1 2 3 4 5 6 7 8 9 10              0.050     1.295
  3C345      sess224.L1024         2 3 4 5 6 7 8 9 10                0.133     6.687


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) 
   MRK9                49.4
   NGC4388            110.6
   NGC3516             71.8
   J0737+5941          49.9
   4C39.25             64.3
   J1107+7232          71.9
   J1225+1253         110.4
   3C286              112.1
   3C345              118.3

  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 

