  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: The nuclear structure in nearby AGN
 Exp. Code:  gs032d  


Schedule Version:       1.00
Processed by SCHED version:  11.30  Version 11.3 update 1.  April 14, 2014

PI:       Tuomas Savolainen

Address:  MPIfR Bonn
          Auf dem Huegel 69
          53121 Bonn, Germany
 

Phone:    +49 228 525 473
EMAIL:    tsavolainen@mpifr-bonn.mpg.de
Fax:      +49 228 525 229
Phone during observation: +7 903 661 4865

Observing mode: L-band, dual-pol

Notes:    L-band, Radioastron-compatible frequency setup
          Mark5C stations should record in Mk5B+ format
          P-CAL is ON, Tsys is ON, auto-level (AGC) is ON
          Please send diskpacks to MPIfR Bonn

Schedule for HART      (Code Hh )                                   Page   2
               The nuclear structure in nearby AGN
  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   4 Jun 2014   Day 155 ---

 Next scan frequencies:  1668.00  1668.00  1668.00  1668.00
 Next BBC frequencies:    158.00   158.00   158.00   158.00
 Next scan bandwidths:     16.00    16.00    16.00    16.00

12 48 50  1236+077     07 31 07   8.1  77.7 -5.2       0.0     0        0   12 48 50
12 51 50  ---          07 34 07   8.7  77.3 -5.1       0.0   180        6   12 48 51

12 56 40  1228+126     07 38 58   9.3  71.4 -4.9       0.0   253        6   12 56 40
13 05 40  ---          07 48 00  11.2  70.2 -4.7       0.0   540       23   12 56 41

13 06 10  1228+126     07 48 30  11.3  70.2 -4.7       0.0     9       23   13 06 10
13 15 40  ---          07 58 01  13.3  69.0 -4.6       0.0   570       41   13 06 11

13 16 10  1228+126     07 58 31  13.4  68.9 -4.6       0.0     9       41   13 16 10
13 25 40  ---          08 08 03  15.4  67.7 -4.4       0.0   570       60   13 16 11

13 26 30  1236+077     08 08 53  16.3  73.1 -4.5       0.0    13       60   13 26 30
13 29 00  ---          08 11 23  16.8  72.7 -4.5       0.0   150       64   13 26 31

 ---------- Space segment 03: L-band VLBI scans ----------

13 30 00  1228+126     08 12 24  16.3  67.1 -4.3       0.0    23       64   13 30 00
13 49 30  ---          08 31 57  20.3  64.4 -4.0       0.0  1170      102   13 30 01

13 50 00  1228+126     08 32 27  20.4  64.3 -4.0       0.0     9      102   13 50 00
14 09 30  ---          08 52 00  24.4  61.3 -3.7       0.0  1170      139   13 50 01

 ---------- L-band GRT-only VLBI scans - segment 04L ----------

14 10 30  1236+077     08 53 00  25.6  66.9 -3.8       0.0    23      139   14 10 30
14 13 00  ---          08 55 31  26.1  66.5 -3.7       0.0   150      144   14 10 31

14 14 00  1228+126     08 56 31  25.2  60.6 -3.6       0.0    23      144   14 14 00
14 24 00  ---          09 06 32  27.2  58.9 -3.4       0.0   600      163   14 14 01

 ---------- Allow time for Kalyazin and Evpatoria to change source ----------

14 24 30  1228+126     09 07 02  27.3  58.9 -3.4       0.0     9      163   14 24 30
14 34 30  ---          09 17 04  29.2  57.1 -3.2       0.0   600      183   14 24 31

14 35 30  1236+077     09 18 04  30.7  62.9 -3.4       0.0    23      183   14 35 30
14 38 00  ---          09 20 35  31.2  62.5 -3.3       0.0   150      187   14 35 31

14 39 00  1222+037     09 21 35  36.7  63.6 -3.1       0.0    25      187   14 39 00
14 42 00  ---          09 24 35  37.3  63.0 -3.0       0.0   180      193   14 39 01
Schedule for HART      (Code Hh )                                   Page   3
               The nuclear structure in nearby AGN
  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   4 Jun 2014   Day 155 ---

14 43 30  1226+023     09 26 06  37.6  65.0 -3.1       0.0    61      193   14 43 30
14 52 30  ---          09 35 07  39.4  63.3 -2.9       0.0   540      211   14 43 31

 ---------- Allow time for Kalyazin and Evpatoria to change source ----------

14 54 00  1228+126     09 36 37  32.8  53.5 -2.9       0.0    42      211   14 54 00
15 04 00  ---          09 46 39  34.6  51.5 -2.7       0.0   600      230   14 54 01

15 04 30  1228+126     09 47 09  34.7  51.4 -2.7       0.0     9      230   15 04 30
15 14 30  ---          09 57 11  36.4  49.2 -2.6       0.0   600      249   15 04 31

 ---------- Space segment 04: L-band VLBI scans ----------

15 15 00  1228+126     09 57 41  36.5  49.1 -2.6       0.0     9      249   15 15 00
15 34 30  ---          10 17 14  39.7  44.6 -2.2       0.0  1170      287   15 15 01

15 35 00  1228+126     10 17 44  39.8  44.5 -2.2       0.0     9      287   15 35 00
15 54 30  ---          10 37 17  42.8  39.5 -1.9       0.0  1170      324   15 35 01

 ---------- L-band GRT-only VLBI scans - segment 05L ----------

15 55 30  1236+077     10 38 17  45.4  45.8 -2.0       0.0    23      324   15 55 30
15 58 00  ---          10 40 48  45.8  45.1 -2.0       0.0   150      329   15 55 31

15 59 10  1228+126     10 41 58  43.4  38.2 -1.8       0.0    33      329   15 59 10
16 08 00  ---          10 50 49  44.6  35.7 -1.7       0.0   530      346   15 59 11

 ---------- Allow time for Kalyazin and Evpatoria to change source ----------

16 08 30  1228+126     10 51 20  44.7  35.6 -1.7       0.0     9      346   16 08 30
16 18 00  ---          11 00 51  45.9  32.8 -1.5       0.0   570      364   16 08 31

16 19 00  1236+077     11 01 51  49.0  39.0 -1.6       0.0    23      364   16 19 00
16 21 30  ---          11 04 22  49.4  38.2 -1.6       0.0   150      369   16 19 01

16 22 30  1222+037     11 05 22  54.8  36.5 -1.3       0.0    25      369   16 22 30
16 25 30  ---          11 08 22  55.2  35.4 -1.3       0.0   180      375   16 22 31

16 27 00  1228+126     11 09 53  46.9  30.0 -1.4       0.0    45      375   16 27 00
16 35 30  ---          11 18 24  47.9  27.2 -1.2       0.0   510      391   16 27 01

16 36 00  1228+126     11 18 54  47.9  27.0 -1.2       0.0     9      391   16 36 00
16 45 30  ---          11 28 26  48.8  23.8 -1.1       0.0   570      409   16 36 01
Schedule for HART      (Code Hh )                                   Page   4
               The nuclear structure in nearby AGN
  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   4 Jun 2014   Day 155 ---

16 46 40  1236+077     11 29 36  52.5  29.6 -1.2       0.0    33      409   16 46 40
16 49 10  ---          11 32 06  52.8  28.7 -1.1       0.0   150      414   16 46 41

16 50 20  1228+126     11 33 16  49.2  22.1 -1.0       0.0    33      414   16 50 20
16 59 20  ---          11 42 18  50.0  18.9 -0.8       0.0   540      431   16 50 21

 ---------- Space segment 05: L-band VLBI scans ----------

17 00 00  1228+126     11 42 58  50.0  18.7 -0.8       0.0    19      431   17 00 00
17 19 30  ---          12 02 31  51.2  11.4 -0.5       0.0  1170      469   17 00 01

17 20 00  1228+126     12 03 01  51.2  11.2 -0.5       0.0     9      469   17 20 00
17 39 30  ---          12 22 34  51.7   3.5 -0.1       0.0  1170      506   17 20 01

 ---------- L-band GRT-only VLBI scans - segment 06L ----------

17 40 40  1236+077     12 23 45  56.4   7.4 -0.3       0.0    33      506   17 40 40
17 43 10  ---          12 26 15  56.5   6.3 -0.2       0.0   150      511   17 40 41

17 44 20  1228+126     12 27 25  51.8   1.6 -0.1       0.0    33      511   17 44 20
17 53 10  ---          12 36 17  51.8 358.1  0.1       0.0   530      528   17 44 21

 ---------- Allow time for Kalyazin and Evpatoria to change source ----------

17 53 40  1228+126     12 36 47  51.8 357.9  0.1       0.0     9      528   17 53 40
18 03 10  ---          12 46 18  51.6 354.2  0.2       0.0   570      546   17 53 41

18 04 20  1236+077     12 47 29  56.6 356.7  0.1       0.0    33      546   18 04 20
18 06 50  ---          12 49 59  56.6 355.6  0.2       0.0   150      551   18 04 21

18 07 50  1222+037     12 50 59  60.0 347.2  0.4       0.0    25      551   18 07 50
18 10 50  ---          12 54 00  59.9 345.8  0.5       0.0   180      557   18 07 51

18 11 40  1226+023     12 54 50  61.5 346.8  0.4       0.0    21      557   18 11 40
18 20 00  ---          13 03 11  61.0 342.6  0.6       0.0   500      573   18 11 41

18 21 40  1228+126     13 04 51  50.9 347.0  0.6       0.0    52      573   18 21 40
18 30 10  ---          13 13 23  50.5 343.8  0.7       0.0   510      589   18 21 41

18 30 40  1228+126     13 13 53  50.4 343.6  0.7       0.0     9      589   18 30 40
18 40 10  ---          13 23 24  49.8 340.2  0.9       0.0   570      608   18 30 41

18 41 20  1236+077     13 24 35  55.0 340.6  0.7       0.0    33      608   18 41 20
18 43 50  ---          13 27 05  54.8 339.5  0.8       0.0   150      612   18 41 21
Schedule for HART      (Code Hh )                                   Page   5
               The nuclear structure in nearby AGN
  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   4 Jun 2014   Day 155 ---

 ---------- Space segment 06: L-band VLBI scans ----------

18 45 00  1228+126     13 28 15  49.4 338.4  0.9       0.0    33      612   18 45 00
19 04 30  ---          13 47 48  47.5 331.8  1.3       0.0  1170      650   18 45 01

19 05 00  1228+126     13 48 19  47.5 331.6  1.3       0.0     9      650   19 05 00
19 24 30  ---          14 07 52  45.2 325.6  1.6       0.0  1170      687   19 05 01

 ---------- L-band GRT-only VLBI scans - segment 07L ----------

19 25 30  1236+077     14 08 52  50.3 324.1  1.5       0.0    23      687   19 25 30
19 28 00  ---          14 11 22  50.0 323.3  1.5       0.0   150      692   19 25 31

19 29 00  1228+126     14 12 22  44.6 324.2  1.7       0.0    23      692   19 29 00
19 38 00  ---          14 21 24  43.4 321.7  1.8       0.0   540      710   19 29 01

 ---------- Allow time for Kalyazin and Evpatoria to change source ----------

19 38 30  1228+126     14 21 54  43.3 321.6  1.8       0.0     9      710   19 38 30
19 48 00  ---          14 31 26  41.9 319.0  2.0       0.0   570      728   19 38 31

19 49 00  1236+077     14 32 26  46.9 316.9  1.9       0.0    23      728   19 49 00
19 51 30  ---          14 34 56  46.6 316.2  1.9       0.0   150      733   19 49 01

19 52 30  1222+037     14 35 56  46.9 308.1  2.2       0.0    25      733   19 52 30
19 55 30  ---          14 38 57  46.4 307.3  2.2       0.0   180      738   19 52 31

19 57 00  1228+126     14 40 27  40.6 316.7  2.1       0.0    45      738   19 57 00
20 05 30  ---          14 48 58  39.2 314.6  2.3       0.0   510      755   19 57 01

20 06 00  1228+126     14 49 29  39.2 314.5  2.3       0.0     9      755   20 06 00
20 15 30  ---          14 59 00  37.6 312.3  2.5       0.0   570      773   20 06 01

20 16 30  1236+077     15 00 00  42.4 309.7  2.3       0.0    23      773   20 16 30
20 19 00  ---          15 02 31  42.0 309.1  2.4       0.0   150      778   20 16 31

20 20 00  1228+126     15 03 31  36.8 311.3  2.5       0.0    23      778   20 20 00
20 29 20  ---          15 12 52  35.2 309.3  2.7       0.0   560      796   20 20 01

 ---------- Space segment 07: L-band VLBI scans ----------

20 30 00  1228+126     15 13 33  35.1 309.1  2.7       0.0    19      796   20 30 00
20 49 30  ---          15 33 06  31.6 305.2  3.0       0.0  1170      833   20 30 01
Schedule for HART      (Code Hh )                                   Page   6
               The nuclear structure in nearby AGN
  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   4 Jun 2014   Day 155 ---

20 50 00  1228+126     15 33 36  31.5 305.2  3.0       0.0     9      833   20 50 00
21 09 30  ---          15 53 09  27.9 301.6  3.4       0.0  1170      871   20 50 01

 ---------- L-band GRT-only VLBI scans - segment 08L ----------

21 10 30  1236+077     15 54 09  32.3 298.5  3.2       0.0    23      871   21 10 30
21 13 00  ---          15 56 40  31.8 298.1  3.3       0.0   150      876   21 10 31

21 14 00  1228+126     15 57 40  27.0 300.9  3.4       0.0    23      876   21 14 00
21 24 00  ---          16 07 41  25.0 299.2  3.6       0.0   600      895   21 14 01

 ---------- Allow time for Kalyazin and Evpatoria to change source ----------

21 24 30  1228+126     16 08 11  24.9 299.1  3.6       0.0     9      895   21 24 30
21 34 00  ---          16 17 43  23.1 297.7  3.8       0.0   570      913   21 24 31

21 35 00  1236+077     16 18 43  27.4 294.4  3.6       0.0    23      913   21 35 00
21 37 30  ---          16 21 14  26.9 294.0  3.7       0.0   150      918   21 35 01

21 38 30  1222+037     16 22 14  25.7 287.9  3.9       0.0    25      918   21 38 30
21 41 30  ---          16 25 14  25.1 287.5  4.0       0.0   180      924   21 38 31

21 43 00  1228+126     16 26 44  21.2 296.3  3.9       0.0    45      924   21 43 00
21 51 30  ---          16 35 16  19.5 295.1  4.1       0.0   510      940   21 43 01

21 52 00  1228+126     16 35 46  19.4 295.0  4.1       0.0     9      940   21 52 00
22 01 30  ---          16 45 18  17.5 293.6  4.2       0.0   570      958   21 52 01

22 02 30  1236+077     16 46 18  21.6 290.3  4.1       0.0    23      958   22 02 30
22 05 00  ---          16 48 48  21.1 290.0  4.1       0.0   150      963   22 02 31

22 06 00  1228+126     16 49 48  16.5 293.0  4.3       0.0    23      963   22 06 00
22 14 30  ---          16 58 20  14.8 291.9  4.4       0.0   510      979   22 06 01

22 15 00  1228+126     16 58 50  14.7 291.8  4.5       0.0     9      979   22 15 00
22 20 30  ---          17 04 21  13.5 291.1  4.5       0.0   330      990   22 15 01

22 21 30  1236+077     17 05 21  17.6 287.7  4.4       0.0    23      990   22 21 30
22 24 00  ---          17 07 51  17.1 287.4  4.5       0.0   150      995   22 21 31

 ---------- Space segment 08: L-band VLBI scans ----------

22 25 00  1228+126     17 08 51  12.5 290.5  4.6       0.0    23      995   22 25 00
22 44 30  ---          17 28 25   8.4 288.1  4.9       0.0  1170     1032   22 25 01


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


 ======== Setup file: ra18cm2.set
   Matching groups in ./gs032d_freq.dat:
     hh18cm          Values confirmed by E-mail Jonathan Quick 20140219 (CR)

   Setup group:   24         Station: HART              Total bit rate:   256
   Format: MARK5B            Bits per sample: 2         Sample rate: 32.000
   Number of channels:  4    DBE type: DBBC_DDC         Speedup factor:   1.00

   Disk used to record data.

   1st LO=   1510.00   1510.00   1510.00   1510.00
   Net SB=         U         U         L         L
   IF SB =         U         U         U         U
   Pol.  =      RCP       LCP       RCP       LCP 
   BBC   =         1         5         1         5
   BBC SB=         U         U         L         L
   IF    =        A1        B1        A1        B1

  The following frequency sets based on these setups were used.

   Frequency Set:  15  Setup file default.  Used with PCAL = 1MHz
   LO sum=   1668.00  1668.00  1668.00  1668.00
   BBC fr=    158.00   158.00   158.00   158.00
   Bandwd=     16.00    16.00    16.00    16.00
    Matching frequency sets:  15

   Track assignments are: 
    track1=   2,  4,  6,  8
    barrel=roll_off 

 POSITIONS OF SOURCES USED IN RECORDING SCANS

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

 * FAKERA            11 57 21.769299   * 12 00 00.000000     12 00 41.923521       0.00
                     85 16 41.77889    * 85 00 00.00000      84 55 27.17430        0.00
                     From catalog imbedded in main SCHED input file.
                     fake circumpolar target for a TS to look at

   J1239+0730        12 36 52.308755   * 12 39 24.588327     12 40 09.440650       0.10
 * 1236+077          07 46 45.39997    * 07 30 17.18902      07 25 31.24531        0.11
   J1239+07          From catalog imbedded in main SCHED input file.
                     rfc_2012b Petrov, 2012, unpublished 1855 observations

   J1224+0330        12 22 19.097169   * 12 24 52.421935     12 25 37.543272       0.11
 * 1222+037          03 47 27.06583    * 03 30 50.29268      03 25 59.94064        0.13
   J1224+03          From catalog imbedded in main SCHED input file.
                     rfc_2012b Petrov, 2012, unpublished 688 observations

 * 1226+023          12 26 33.245835   * 12 29 06.699731     12 29 51.900411       0.00
   J1229+0203        02 19 43.30547    * 02 03 08.59797      01 58 18.56773        0.00
   3C273B            ./gs032d_sources.radioastron
   3C273             AGN, rfc_2013d Petrov, 2013, unpublished 32011 observations

 * 1228+126          12 28 17.569280   * 12 30 49.423382     12 31 34.048480       0.00
   J1230+1223        12 40 01.74883    * 12 23 28.04365      12 18 41.71051        0.00
   3C274             ./gs032d_sources.radioastron
   M87               AGN, rfc_2013d Petrov, 2013, unpublished 55201 observations
   VIR-A



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
  FAKERA     ra18cm2.set           8                                 5.525     0.000
  1236+077   ra18cm2.set           1 2 3 4 6 7 8 13 14 15 16 1 +     1.192    78.475
  1222+037   ra18cm2.set           1 2 3 4 6 7 13 14 15 16 17  +     0.483    28.442
  1226+023   ra18cm2.set           1 2 3 4 6 7 8 13 14 15 16 1 +     0.589    40.489
  1228+126   ra18cm2.set           1 2 3 4 6 7 8 13 14 15 16 1 +    12.719  1103.989


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) 
   FAKERA              69.1
   1236+077           111.8
   1222+037           110.4
   1226+023           112.0
   1228+126           107.7

  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 

