  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: RadioAstron AGN polarization imaging
 Exp. Code:  gg083a  


Schedule Version:       1.00
Processed by SCHED version:  11.40  Release 11.4.  March 14, 2015

PI:       Jose L. Gomez

Address:  Instituto de Astrofisica de Andalucia-CSIC
          Glorieta de la Astronomia
          E-18008 Granada, Spain
 

Phone:    +79165452842
EMAIL:    jlgomez@iaa.es, alobanov@mpifr-bonn.mpg.de
Fax:
Phone during observation: +79165452842

Observing mode: K-band,Q-band,U-band dual-pol

Notes:    K-band, Radioastron-compatible frequency setup
          P-CAL is ON
          Tsys is ON
          auto-level (AGC) is ON

Schedule for HART      (Code Hh )                                   Page   2
               RadioAstron AGN polarization imaging
  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   8 Oct 2017   Day 281 ---

 Next scan frequencies:  22236.00  22236.00  22236.00  22236.00  22268.00  22268.00  22268.00  22268.00
 Next BBC frequencies:     236.00    236.00    236.00    236.00    268.00    268.00    268.00    268.00
 Next scan bandwidths:      16.00     16.00     16.00     16.00     16.00     16.00     16.00     16.00

15 40 30  2200+420     18 41 06   7.3  35.1 -3.4  D    0.0     0        0   15 40 19
15 50 00  ---          18 50 37   8.5  33.9 -3.2       0.0     0       37   15 40 20

15 50 15  2200+420     18 50 52   8.6  33.8 -3.2       0.0    -6       37   15 50 04
15 56 15  ---          18 56 53   9.3  33.0 -3.1       0.0   354       61   15 50 05

 ---------- K-band VLBI scans. Ground  segment 01 : full array on 2200+420 ----------

16 12 30  2200+420     19 13 11  11.3  30.6 -2.8       0.0   953       61   16 12 19
16 22 00  ---          19 22 42  12.3  29.2 -2.7       0.0   570       98   16 12 20

 ---------- K-band VLBI scans. Ground  segment 01: 2200+420 with EVN+KVN ----------

16 23 00  2200+420     19 23 43  12.4  29.1 -2.7       0.0    39       98   16 22 49
16 33 00  ---          19 33 44  13.5  27.5 -2.5       0.0   600      137   16 22 50

16 33 30  2200+420     19 34 14  13.6  27.4 -2.5       0.0     9      137   16 33 19
16 43 00  ---          19 43 46  14.5  25.9 -2.3       0.0   570      175   16 33 20

16 43 15  2200+420     19 44 01  14.5  25.9 -2.3       0.0    -6      175   16 43 04
16 52 45  ---          19 53 32  15.5  24.3 -2.2       0.0   564      212   16 43 05

 ---------- K-band VLBI scans. Ground  segment 01: 3C454.3 with EVN+KVN ----------

16 54 45  3C454.3      19 55 33  29.4  51.0 -3.0       0.0    41      212   16 54 34
16 59 45  ---          20 00 34  30.2  50.0 -2.9       0.0   300      232   16 54 35

17 01 00  2200+420     20 01 49  16.2  22.9 -2.0       0.0    -4      232   17 00 49
17 05 40  ---          20 06 30  16.6  22.1 -1.9       0.0   276      251   17 00 50

17 06 40  2200+420     20 07 30  16.7  22.0 -1.9       0.0    39      251   17 06 29
17 16 10  ---          20 17 01  17.5  20.3 -1.8       0.0   570      288   17 06 30

17 16 20  2200+420     20 17 11  17.5  20.3 -1.8       0.0   -11      288   No stop 
17 24 40  ---          20 25 33  18.1  18.8 -1.6       0.0   489      320   17 16 11

 ---------- K-band VLBI scans. Space segment 02: 2200+420 with EVN+KVN ----------

17 25 00  2200+420     20 25 53  18.1  18.7 -1.6       0.0    -1      320   17 24 49
17 35 00  ---          20 35 54  18.8  16.9 -1.5       0.0   599      360   17 24 50
Schedule for HART      (Code Hh )                                   Page   3
               RadioAstron AGN polarization imaging
  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   8 Oct 2017   Day 281 ---

17 35 30  2200+420     20 36 24  18.8  16.8 -1.5       0.0     9      360   17 35 19
17 45 00  ---          20 45 56  19.4  15.1 -1.3       0.0   570      397   17 35 20

17 45 30  2200+420     20 46 26  19.5  15.0 -1.3       0.0     9      397   17 45 19
17 55 00  ---          20 55 58  20.0  13.2 -1.1       0.0   570      434   17 45 20

17 55 30  2200+420     20 56 28  20.0  13.1 -1.1       0.0     9      434   17 55 19
18 05 00  ---          21 05 59  20.5  11.3 -1.0       0.0   570      471   17 55 20

 ---------- K-band VLBI scans. Space segment 02: 2200+420 with EVN+KVN+VLBA ----------

18 05 30  2200+420     21 06 29  20.5  11.2 -0.9       0.0     9      471   18 05 19
18 15 00  ---          21 16 01  20.9   9.4 -0.8       0.0   570      509   18 05 20

18 15 30  2200+420     21 16 31  20.9   9.3 -0.8       0.0     9      509   18 15 19
18 25 00  ---          21 26 03  21.2   7.4 -0.6       0.0   570      546   18 15 20

18 25 30  2200+420     21 26 33  21.2   7.3 -0.6       0.0     9      546   18 25 19
18 35 00  ---          21 36 04  21.4   5.4 -0.5       0.0   570      583   18 25 20

18 35 30  2200+420     21 36 34  21.5   5.3 -0.4       0.0     9      583   18 35 19
18 45 00  ---          21 46 06  21.6   3.5 -0.3       0.0   570      620   18 35 20

18 45 30  2200+420     21 46 36  21.6   3.4 -0.3       0.0     9      620   18 45 19
18 55 00  ---          21 56 08  21.7   1.5 -0.1       0.0   570      658   18 45 20

 ---------- K-band VLBI scans. Ground  segment 02 : 3C454.3 with EVN+KVN ----------

18 57 30  3C454.3      21 58 38  45.7  19.5 -0.9       0.0    71      658   18 57 19
19 02 30  ---          22 03 39  46.1  17.9 -0.9       0.0   300      677   18 57 20

 ---------- K-band VLBI scans. Ground  segment 01: 2200+420 with EVN+KVN ----------

19 04 45  2200+420     22 05 54  21.7 359.5  0.0       0.0    56      677   19 04 34
19 10 45  ---          22 11 55  21.7 358.3  0.1       0.0   360      701   19 04 35

 ---------- K-band VLBI scans. Ground  segment 02 : full array on 2200+420 ----------

19 11 15  2200+420     22 12 25  21.7 358.2  0.1       0.0     9      701   19 11 04
19 20 45  ---          22 21 57  21.6 356.3  0.3       0.0   570      739   19 11 05

19 21 15  2200+420     22 22 27  21.6 356.2  0.3       0.0     9      739   19 21 04
19 30 45  ---          22 31 58  21.4 354.4  0.5       0.0   570      776   19 21 05
Schedule for HART      (Code Hh )                                   Page   4
               RadioAstron AGN polarization imaging
  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   8 Oct 2017   Day 281 ---

19 31 00  2200+420     22 32 13  21.4 354.3  0.5       0.0    -6      776   19 30 49
19 40 45  ---          22 42 00  21.2 352.4  0.6       0.0   579      814   19 30 50

19 41 15  2200+420     22 42 30  21.2 352.3  0.7       0.0     9      814   19 41 04
19 50 45  ---          22 52 02  20.8 350.4  0.8       0.0   570      851   19 41 05

19 51 15  2200+420     22 52 32  20.8 350.3  0.8       0.0     9      851   19 51 04
20 00 45  ---          23 02 03  20.4 348.5  1.0       0.0   570      888   19 51 05

 ---------- K-band VLBI scans. Ground  segment 01: 2200+420 with EVN+KVN ----------

20 15 00  2200+420     23 16 21  19.7 345.8  1.2       0.0   833      888   20 15 00
20 21 00  ---          23 22 22  19.4 344.7  1.3       0.0   360      912   20 15 01

 ---------- K-band VLBI scans. Ground  segment 02 : full array on 2200+420 ----------

20 21 30  2200+420     23 22 52  19.3 344.6  1.3       0.0     9      912   20 21 19
20 31 00  ---          23 32 23  18.7 342.8  1.5       0.0   570      949   20 21 20

20 31 30  2200+420     23 32 53  18.7 342.7  1.5       0.0     9      949   20 31 19
20 41 00  ---          23 42 25  18.0 341.0  1.6       0.0   570      986   20 31 20

20 41 30  2200+420     23 42 55  18.0 340.9  1.7       0.0     9      986   20 41 19
20 51 00  ---          23 52 27  17.3 339.3  1.8       0.0   570     1023   20 41 20

20 51 15  2200+420     23 52 42  17.2 339.2  1.8       0.0    -6     1023   20 51 04
21 01 00  ---          00 02 28  16.4 337.5  2.0       0.0   579     1061   20 51 05

21 01 30  2200+420     00 02 58  16.4 337.4  2.0       0.0     9     1061   21 01 19
21 11 00  ---          00 12 30  15.5 335.8  2.2       0.0   570     1099   21 01 20

21 11 15  2200+420     00 12 45  15.5 335.8  2.2       0.0    -6     1099   21 11 04
21 14 15  ---          00 15 45  15.2 335.3  2.2       0.0   174     1111   21 11 05

 ---------- K-band VLBI scans. Space segment 03: 2200+420 with EVN+KVN+VLBA+VLA ----------

21 15 00  2200+420     00 16 31  15.2 335.2  2.2       0.0    24     1111   21 14 49
21 16 00  ---          00 17 31  15.1 335.0  2.2       0.0    60     1116   21 14 50

21 16 10  2200+420     00 17 41  15.1 335.0  2.2       0.0   -11     1116   No stop 
21 19 55  ---          00 21 26  14.7 334.4  2.3       0.0   214     1131   21 16 01

21 20 05  2200+420     00 21 36  14.7 334.3  2.3       0.0   -11     1131   No stop 
21 21 05  ---          00 22 37  14.6 334.2  2.3       0.0    49     1135   21 19 56
Schedule for HART      (Code Hh )                                   Page   5
               RadioAstron AGN polarization imaging
  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   8 Oct 2017   Day 281 ---

21 21 15  2200+420     00 22 47  14.6 334.2  2.3       0.0   -11     1135   No stop 
21 25 00  ---          00 26 32  14.2 333.6  2.4       0.0   214     1150   21 21 06

21 25 30  2200+420     00 27 02  14.1 333.5  2.4       0.0     9     1150   21 25 19
21 26 30  ---          00 28 02  14.0 333.3  2.4       0.0    60     1155   21 25 20

21 26 40  2200+420     00 28 12  14.0 333.3  2.4       0.0   -11     1155   No stop 
21 30 10  ---          00 31 43  13.7 332.7  2.5       0.0   199     1169   21 26 31

21 30 20  2200+420     00 31 53  13.6 332.7  2.5       0.0   -11     1169   No stop 
21 31 20  ---          00 32 53  13.5 332.5  2.5       0.0    49     1173   21 30 11

21 31 30  2200+420     00 33 03  13.5 332.5  2.5       0.0   -11     1173   No stop 
21 35 00  ---          00 36 34  13.2 332.0  2.6       0.0   199     1187   21 31 21

21 35 30  2200+420     00 37 04  13.1 331.9  2.6       0.0     9     1187   21 35 19
21 36 30  ---          00 38 04  13.0 331.7  2.6       0.0    60     1192   21 35 20

21 36 40  2200+420     00 38 14  13.0 331.7  2.6       0.0   -11     1192   No stop 
21 40 10  ---          00 41 45  12.6 331.2  2.6       0.0   199     1206   21 36 31

21 40 20  2200+420     00 41 55  12.6 331.1  2.6       0.0   -11     1206   No stop 
21 41 20  ---          00 42 55  12.5 331.0  2.7       0.0    49     1211   21 40 11

21 41 30  2200+420     00 43 05  12.5 331.0  2.7       0.0   -11     1211   No stop 
21 45 00  ---          00 46 35  12.1 330.4  2.7       0.0   199     1225   21 41 21

21 45 30  2200+420     00 47 06  12.0 330.4  2.7       0.0     9     1225   21 45 19
21 46 30  ---          00 48 06  11.9 330.2  2.7       0.0    60     1229   21 45 20

21 46 40  2200+420     00 48 16  11.9 330.2  2.7       0.0   -11     1229   No stop 
21 50 10  ---          00 51 46  11.5 329.7  2.8       0.0   199     1243   21 46 31

21 50 20  2200+420     00 51 56  11.5 329.6  2.8       0.0   -11     1243   No stop 
21 51 20  ---          00 52 57  11.4 329.5  2.8       0.0    49     1248   21 50 11

21 51 30  2200+420     00 53 07  11.3 329.5  2.8       0.0   -11     1248   No stop 
21 55 00  ---          00 56 37  10.9 328.9  2.9       0.0   199     1262   21 51 21

21 55 30  2200+420     00 57 07  10.9 328.9  2.9       0.0     9     1262   21 55 19
21 56 30  ---          00 58 07  10.8 328.7  2.9       0.0    60     1266   21 55 20

21 56 40  2200+420     00 58 17  10.7 328.7  2.9       0.0   -11     1266   No stop 
22 00 10  ---          01 01 48  10.3 328.2  3.0       0.0   199     1281   21 56 31
Schedule for HART      (Code Hh )                                   Page   6
               RadioAstron AGN polarization imaging
  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   8 Oct 2017   Day 281 ---

22 00 20  2200+420     01 01 58  10.3 328.2  3.0       0.0   -11     1281   No stop 
22 01 20  ---          01 02 58  10.2 328.0  3.0       0.0    49     1285   22 00 11

22 01 30  2200+420     01 03 08  10.2 328.0  3.0       0.0   -11     1285   No stop 
22 05 00  ---          01 06 39   9.7 327.5  3.1       0.0   199     1299   22 01 21

22 05 30  2200+420     01 07 09   9.7 327.4  3.1       0.0     9     1299   22 05 19
22 06 30  ---          01 08 09   9.6 327.3  3.1       0.0    60     1304   22 05 20

22 06 40  2200+420     01 08 19   9.5 327.3  3.1       0.0   -11     1304   No stop 
22 10 10  ---          01 11 50   9.1 326.8  3.1       0.0   199     1318   22 06 31

22 10 20  2200+420     01 12 00   9.1 326.7  3.1       0.0   -11     1318   No stop 
22 11 20  ---          01 13 00   9.0 326.6  3.2  H    0.0     0     1322   22 10 11

22 11 30  2200+420     01 13 10   8.9 326.6  3.2  H    0.0   -11     1322   No stop 
22 15 00  ---          01 16 40   8.5 326.1  3.2  H    0.0     0     1336   22 11 21

22 15 30  2200+420     01 17 10   8.4 326.0  3.2  H    0.0     9     1336   22 15 19
22 16 30  ---          01 18 11   8.3 325.9  3.2  H    0.0     0     1341   22 15 20

22 16 40  2200+420     01 18 21   8.3 325.9  3.2  H    0.0   -11     1341   No stop 
22 20 10  ---          01 21 51   7.9 325.4  3.3  D    0.0     0     1355   22 16 31


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


 ======== Setup file: ra1cm2.set
 --- 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:   17         Station: HART              Total bit rate:   512
   Format: MARK5B            Bits per sample: 2         Sample rate: 32.000
   Number of channels:  8    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
   Net SB=         U         U         L         L         U         U         L         L
   IF SB =         U         U         U         U         U         U         U         U
   Pol.  =      RCP       LCP       RCP       LCP       RCP       LCP       RCP       LCP 
   BBC   =         1         9         1         9         3        11         3        11
   BBC SB=         U         U         L         L         U         U         L         L
   IF    =        A1        C1        A1        C1        A1        C1        A1        C1

  The following frequency sets based on these setups were used.

   Frequency Set:  17  Setup file default.  Used with PCAL = 1MHz
   LO sum=   22236.00  22236.00  22236.00  22236.00  22268.00  22268.00  22268.00  22268.00
   BBC fr=     236.00    236.00    236.00    236.00    268.00    268.00    268.00    268.00
   Bandwd=      16.00     16.00     16.00     16.00     16.00     16.00     16.00     16.00
    Matching frequency sets:  17

   Track assignments are: 
    track1=   2,  6, 10, 14,  4,  8, 12, 16
    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 34.789477       0.00
                     85 16 41.77889    * 85 00 00.00000      84 54 03.68850        0.00
                     From catalog imbedded in main SCHED input file.
                     fake circumpolar target for a TS to look at

   1328+307          13 28 49.657778   * 13 31 08.288070     13 31 55.127711       0.00
   J1331+3030        30 45 58.64060    * 30 30 32.95924      30 25 19.56062        0.00
 * 3C286             ./gg083a_sources.radioastron
                     WSRT calibrator, not for 92cm, rfc_2013d Petrov, 2013, unpublished 542 observati

   0316+413          03 16 29.567283   * 03 19 48.160114     03 20 59.660736       0.00
   J0319+4130        41 19 51.91847    * 41 30 42.10559      41 34 21.39346        0.00
 * 3C84              ./gg083a_sources.radioastron
                     AGN, rfc_2013d Petrov, 2013, unpublished 15448 observations, RA-AO3-04, RA-AO2-1

   0355+508          03 55 45.261370   * 03 59 29.747271     04 00 50.453528       0.00
   J0359+5057        50 49 20.28584    * 50 57 50.16179      51 00 34.74763        0.00
 * NRAO150           ./gg083a_sources.radioastron
                     AGN, rfc_2013d Petrov, 2013, unpublished 19270 observations, RA-AO3-04, RA-AO2-1

 * 2200+420          22 00 39.362504   * 22 02 43.291371     22 03 28.303492       0.00
   J2202+4216        42 02 08.59073    * 42 16 39.97987      42 22 04.96074        0.00
   BLLAC             ./gg083a_sources.radioastron
                     AGN, rfc_2013d Petrov, 2013, unpublished 59417 observations, RA-AO3-04, RA-AO2-1

   2251+158          22 51 29.519741   * 22 53 57.747940     22 54 50.943009       0.00
   J2253+1608        15 52 54.34791    * 16 08 53.56074      16 14 42.95221        0.00
 * 3C454.3           ./gg083a_sources.radioastron
                     AGN, rfc_2013d Petrov, 2013, unpublished 40570 observations, RA-AO3-04, RA-AO2-1



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     ra1cm2.set            16                                6.383     0.000
  3C286      ra1cm2.set            33                                0.322     0.000
             ra2cm2.set            34                                0.317     0.000
             ra7mm2.set            32                                0.322     0.000
  3C84       ra1cm2.set            1 2 3 4 7 9 11 23 33              0.322    47.150
             ra2cm2.set            34 38 39                          0.197    13.016
             ra7mm2.set            21 22 32 49                       0.242    16.917
  NRAO150    ra1cm2.set            1 2 3 4 5 6 7 8 9 11 12 23  +     0.589    81.892
             ra2cm2.set            34 39                             0.200    10.000
             ra7mm2.set            18 21 22 32 49                    0.333    13.083
  2200+420   ra1cm2.set            1 2 3 4 5 6 7 8 9 11 12 17  +    17.874  2530.536
             ra2cm2.set            34 38 39                          0.928    56.510
             ra7mm2.set            18 21 22 32 49                    1.081    82.250
  3C454.3    ra1cm2.set            1 2 3 4 5 6 7 8 9 11 12 17  +     0.267    23.448
             ra2cm2.set            34 39                             0.161     8.250
             ra7mm2.set            18 21 22 32 49                    0.250     6.250


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              91.3
   3C286               37.5
   3C84               132.6
   NRAO150            121.5
   2200+420           127.1
   3C454.3            148.1

  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 

