  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: EVN observation of 22 GHZ H2O maser line
 Exp. Code:  EK045A  


Schedule Version:       4.00
Processed by SCHED version:  11.50  Development version 11.5. Started Apr. 2

PI:       Dongjin Kim

Address:  Max-Planck-Institut fuer Radioastronomie
          Auf dem Huegel 69
          53121 Bonn
          Germany

Phone:    0049-176457-18197
EMAIL:    dongjin@mpifr-bonn.mpg.de
Fax:      0049-2257-301-106
Phone during observation: 0049-2257-301-155

Observing mode: 5cm 2048 Mbps, 32-16-2

Notes:
 
 
 

Schedule for HART      (Code Hh )                                   Page   2
               EVN observation of 22 GHZ H2O maser line
  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  20 Oct 2019   Day 293 ---

 Next scan frequencies:  22056.00  22056.00  22056.00  22056.00  22120.00  22120.00  22120.00  22120.00
                         22184.00  22184.00  22184.00  22184.00  22248.00  22248.00  22248.00  22248.00
 Next BBC frequencies:      56.00     56.00     56.00     56.00    120.00    120.00    120.00    120.00
                           184.00    184.00    184.00    184.00    248.00    248.00    248.00    248.00
 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

04 00 00  1156+295     07 44 05   7.5  52.4 -4.3  D    0.0     0        0   04 00 00
04 07 00  ---          07 51 06   8.7  51.5 -4.2       0.0     0      108   04 00 01

04 07 40  1156+295     07 51 46   8.9  51.4 -4.1       0.0    19      108   04 07 40
04 16 40  ---          08 00 47  10.4  50.2 -4.0       0.0   540      247   04 07 41

04 17 20  1156+295     08 01 27  10.6  50.1 -4.0       0.0    19      247   04 17 20
04 26 20  ---          08 10 29  12.1  48.9 -3.8       0.0   540      386   04 17 21

04 28 30  NGC4261      08 12 39  22.2  71.5 -4.1       0.0    56      386   04 28 30
04 38 30  ---          08 22 41  24.3  70.1 -4.0       0.0   600      541   04 28 31

04 39 10  NGC4261      08 23 21  24.5  70.0 -4.0       0.0    19      541   04 39 10
04 49 10  ---          08 33 23  26.6  68.5 -3.8       0.0   600      696   04 39 11

04 49 50  NGC4261      08 34 03  26.7  68.4 -3.8       0.0    19      696   04 49 50
04 59 50  ---          08 44 04  28.8  66.8 -3.6       0.0   600      850   04 49 51

05 00 30  NGC4261      08 44 45  28.9  66.7 -3.6       0.0    19      850   05 00 30
05 10 30  ---          08 54 46  31.0  65.1 -3.4       0.0   600     1005   05 00 31

05 18 30  1156+295     09 02 48  20.4  40.7 -3.0       0.0   406     1005   05 18 30
05 21 30  ---          09 05 48  20.8  40.2 -2.9       0.0   180     1051   05 18 31

05 23 45  NGC4261      09 08 03  33.7  62.8 -3.2       0.0    61     1051   05 23 45
05 33 45  ---          09 18 05  35.7  61.0 -3.0       0.0   600     1206   05 23 46

05 34 25  NGC4261      09 18 45  35.8  60.9 -3.0       0.0    19     1206   05 34 25
05 44 25  ---          09 28 47  37.8  58.9 -2.9       0.0   600     1360   05 34 26

05 45 05  NGC4261      09 29 27  37.9  58.8 -2.8       0.0    19     1360   05 45 05
05 55 05  ---          09 39 29  39.8  56.7 -2.7       0.0   600     1515   05 45 06

06 03 05  1156+295     09 47 30  26.4  32.3 -2.2       0.0   406     1515   06 03 05
06 06 05  ---          09 50 30  26.8  31.7 -2.2       0.0   180     1561   06 03 06

06 08 20  NGC4261      09 52 46  42.2  53.8 -2.5       0.0    61     1561   06 08 20
06 18 20  ---          10 02 47  44.0  51.4 -2.3       0.0   600     1716   06 08 21
Schedule for HART      (Code Hh )                                   Page   3
               EVN observation of 22 GHZ H2O maser line
  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  20 Oct 2019   Day 293 ---

06 19 00  NGC4261      10 03 27  44.2  51.3 -2.3       0.0    19     1716   06 19 00
06 29 00  ---          10 13 29  45.9  48.7 -2.1       0.0   600     1870   06 19 01

06 29 40  NGC4261      10 14 09  46.0  48.5 -2.1       0.0    19     1870   06 29 40
06 39 40  ---          10 24 11  47.7  45.8 -1.9       0.0   600     2025   06 29 41

06 47 40  3C273        10 32 12  50.2  50.1 -2.0       0.0   445     2025   06 47 40
06 50 40  ---          10 35 13  50.7  49.3 -1.9       0.0   180     2071   06 47 41

06 51 50  NGC4261      10 36 23  49.6  42.2 -1.7       0.0    35     2071   06 51 50
07 01 50  ---          10 46 24  51.0  39.1 -1.6       0.0   600     2226   06 51 51

07 02 30  NGC4261      10 47 05  51.1  38.9 -1.6       0.0    19     2226   07 02 30
07 12 30  ---          10 57 06  52.5  35.5 -1.4       0.0   600     2381   07 02 31

07 13 10  NGC4261      10 57 46  52.6  35.3 -1.4       0.0    19     2381   07 13 10
07 23 10  ---          11 07 48  53.8  31.7 -1.2       0.0   600     2535   07 13 11

07 31 10  3C273        11 15 49  56.9  35.6 -1.2       0.0   445     2535   07 31 10
07 34 10  ---          11 18 50  57.3  34.4 -1.2       0.0   180     2582   07 31 11

07 35 20  NGC4261      11 20 00  55.2  27.0 -1.0       0.0    35     2582   07 35 20
07 45 20  ---          11 30 02  56.1  22.9 -0.8       0.0   600     2736   07 35 21

07 46 00  NGC4261      11 30 42  56.2  22.6 -0.8       0.0    19     2736   07 46 00
07 56 00  ---          11 40 43  57.0  18.3 -0.7       0.0   600     2891   07 46 01

07 56 40  NGC4261      11 41 23  57.0  18.0 -0.6       0.0    19     2891   07 56 40
08 06 40  ---          11 51 25  57.6  13.5 -0.5       0.0   600     3045   07 56 41

08 14 40  3C273        11 59 26  61.2  16.1 -0.5       0.0   445     3045   08 14 40
08 17 40  ---          12 02 27  61.4  14.5 -0.5       0.0   180     3092   08 14 41

08 18 50  NGC4261      12 03 37  58.1   7.9 -0.3       0.0    35     3092   08 18 50
08 28 50  ---          12 13 39  58.3   3.2 -0.1       0.0   600     3246   08 18 51

08 29 30  NGC4261      12 14 19  58.4   2.9 -0.1       0.0    19     3246   08 29 30
08 39 30  ---          12 24 21  58.4 358.1  0.1       0.0   600     3401   08 29 31

08 40 10  NGC4261      12 25 01  58.4 357.8  0.1       0.0    19     3401   08 40 10
08 50 10  ---          12 35 02  58.2 353.1  0.2       0.0   600     3555   08 40 11

08 58 10  3C273        12 43 04  62.0 353.1  0.2       0.0   445     3555   08 58 10
09 01 10  ---          12 46 04  61.9 351.5  0.3       0.0   180     3602   08 58 11
Schedule for HART      (Code Hh )                                   Page   4
               EVN observation of 22 GHZ H2O maser line
  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  20 Oct 2019   Day 293 ---

09 02 20  NGC4261      12 47 14  57.7 347.4  0.4       0.0    35     3602   09 02 20
09 12 20  ---          12 57 16  57.1 342.9  0.6       0.0   600     3756   09 02 21

09 13 00  NGC4261      12 57 56  57.1 342.6  0.6       0.0    19     3756   09 13 00
09 23 00  ---          13 07 58  56.3 338.3  0.8       0.0   600     3911   09 13 01

09 23 40  NGC4261      13 08 38  56.3 338.0  0.8       0.0    19     3911   09 23 40
09 33 40  ---          13 18 39  55.4 333.9  1.0       0.0   600     4066   09 23 41

09 40 40  3C273        13 25 41  59.1 332.1  0.9       0.0   385     4066   09 40 40
09 43 40  ---          13 28 41  58.8 330.8  1.0       0.0   180     4112   09 40 41

09 44 50  NGC4261      13 29 51  54.2 329.5  1.2       0.0    35     4112   09 44 50
09 54 50  ---          13 39 53  53.0 325.8  1.3       0.0   600     4266   09 44 51

09 55 30  NGC4261      13 40 33  52.9 325.6  1.3       0.0    19     4266   09 55 30
10 05 30  ---          13 50 35  51.6 322.1  1.5       0.0   600     4421   09 55 31

10 06 10  NGC4261      13 51 15  51.5 321.9  1.5       0.0    19     4421   10 06 10
10 16 10  ---          14 01 16  50.0 318.7  1.7       0.0   600     4576   10 06 11

10 23 10  3C273        14 08 18  53.4 315.8  1.6       0.0   385     4576   10 23 10
10 26 10  ---          14 11 18  52.9 314.9  1.7       0.0   180     4622   10 23 11

10 27 20  NGC4261      14 12 28  48.3 315.3  1.9       0.0    35     4622   10 27 20
10 37 20  ---          14 22 30  46.7 312.5  2.0       0.0   600     4777   10 27 21

10 38 00  NGC4261      14 23 10  46.6 312.4  2.0       0.0    19     4777   10 38 00
10 48 00  ---          14 33 12  44.9 309.7  2.2       0.0   600     4931   10 38 01

10 48 40  NGC4261      14 33 52  44.8 309.6  2.2       0.0    19     4931   10 48 40
10 58 40  ---          14 43 53  43.0 307.1  2.4       0.0   600     5086   10 48 41

11 05 40  3C273        14 50 55  46.0 303.9  2.3       0.0   385     5086   11 05 40
11 08 40  ---          14 53 55  45.5 303.2  2.4       0.0   180     5132   11 05 41

11 09 50  NGC4261      14 55 05  40.9 304.6  2.6       0.0    35     5132   11 09 50
11 19 50  ---          15 05 07  39.1 302.4  2.7       0.0   600     5287   11 09 51

11 20 30  NGC4261      15 05 47  38.9 302.3  2.8       0.0    19     5287   11 20 30
11 30 30  ---          15 15 49  37.0 300.3  2.9       0.0   600     5441   11 20 31

11 31 10  NGC4261      15 16 29  36.9 300.2  2.9       0.0    19     5441   11 31 10
11 41 10  ---          15 26 30  34.9 298.3  3.1       0.0   600     5596   11 31 11
Schedule for HART      (Code Hh )                                   Page   5
               EVN observation of 22 GHZ H2O maser line
  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  20 Oct 2019   Day 293 ---

11 41 50  NGC4261      15 27 10  34.8 298.2  3.1       0.0    19     5596   11 41 50
11 55 50  ---          15 41 13  32.0 295.7  3.3       0.0   840     5812   11 41 51

11 57 00  3C273        15 42 23  35.9 293.4  3.2       0.0    35     5812   11 57 00
12 00 00  ---          15 45 23  35.2 292.9  3.3       0.0   180     5859   11 57 01


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


 ======== Setup file: sess319.K2048line
 --- 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:    7         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=  22000.00  22000.00  22000.00  22000.00  22000.00  22000.00  22000.00  22000.00
            22000.00  22000.00  22000.00  22000.00  22000.00  22000.00  22000.00  22000.00
   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:  10  Setup file default.  Used with PCAL = off
   LO sum=   22056.00  22056.00  22056.00  22056.00  22120.00  22120.00  22120.00  22120.00
             22184.00  22184.00  22184.00  22184.00  22248.00  22248.00  22248.00  22248.00
   BBC fr=      56.00     56.00     56.00     56.00    120.00    120.00    120.00    120.00
               184.00    184.00    184.00    184.00    248.00    248.00    248.00    248.00
   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
    Matching frequency sets:  10

   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)

 * NGC4261           12 16 50.004473   * 12 19 23.216071     12 20 21.570488       0.00
                     06 06 08.63926    * 05 49 29.70008      05 43 08.20006        0.00
                     From catalog imbedded in main SCHED input file.

 * 3C273             12 26 33.245835   * 12 29 06.699731     12 30 05.155415       0.00
                     02 19 43.30577    * 02 03 08.59827      01 56 49.52867        0.00
                     From catalog imbedded in main SCHED input file.

 * 1156+295          11 56 57.786210   * 11 59 31.833911     12 00 30.259088       0.00
                     29 31 25.73872    * 29 14 43.82682      29 08 16.03268        0.00
                     From catalog imbedded in main SCHED input file.



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
  NGC4261    sess319.K2048line     1 2 3 4 5 6 7 8 9 10 11 14  +     5.400   749.000
  3C273      sess319.K2048line     1 2 3 4 5 6 7 8 9 10 11 14  +     0.400    56.300
  1156+295   sess319.K2048line     1 2 3 4 5 6 7 8 9 10 11 14  +     1.200   136.917


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) 
   NGC4261             25.3
   3C273               21.0
   1156+295            46.0

  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 

