  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: Fine-scale imaging of M87
 Exp. Code:  gs042   


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

PI:       Tuomas Savolainen

Address:  Aalto University Metsahovi Radio Observatory
          Metsahovintie 114, 02540 Kylmala, Finland
 
 

Phone:    +358505819717
EMAIL:    tuomas.k.savolainen@aalto.fi
Fax:
Phone during observation: +358505819717

Observing mode: K-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
               Fine-scale imaging of M87
  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
----------------------------------------------------------------------------------------

 --- Mon  14 May 2018   Day 134 ---

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

14 21 00  1228+126     07 40 52   9.7  71.2 -4.8       0.0     0        0   14 21 00
14 27 20  ---          07 47 13  11.0  70.4 -4.7       0.0   380       12   14 21 01

14 27 50  1236+077     07 47 43  11.7  75.7 -4.9       0.0    -7       12   14 27 50
14 29 10  ---          07 49 03  12.0  75.6 -4.9       0.0    73       15   14 27 51

 ---------- K-band VLBI scans. Space segment 02: 1228+126 ----------

14 30 00  1228+126     07 49 53  11.6  70.1 -4.7       0.0    13       15   14 30 00
14 50 00  ---          08 09 56  15.8  67.5 -4.4       0.0  1200       53   14 30 01

14 50 30  1228+126     08 10 26  15.9  67.4 -4.4       0.0     9       53   14 50 30
14 51 30  ---          08 11 27  16.1  67.3 -4.3       0.0    60       55   14 50 31

14 52 10  1228+126     08 12 07  16.2  67.2 -4.3       0.0    19       55   14 52 10
15 10 00  ---          08 30 00  19.9  64.7 -4.0       0.0  1070       90   14 52 11

 ---------- K-band VLBI scans. Ground segment 03: ----------

15 10 20  1236+077     08 30 20  20.8  70.2 -4.2       0.0   -17       90   15 10 20
15 11 50  ---          08 31 50  21.1  70.0 -4.1       0.0    73       93   15 10 21

15 12 40  1228+126     08 32 40  20.5  64.3 -4.0       0.0    13       93   15 12 40
15 22 10  ---          08 42 12  22.4  62.9 -3.8       0.0   570      111   15 12 41

15 23 10  1226+023     08 43 12  28.6  72.1 -3.8       0.0    12      111   15 23 10
15 28 10  ---          08 48 13  29.7  71.3 -3.7       0.0   300      121   15 23 11

15 28 40  1236+077     08 48 43  24.7  67.6 -3.9       0.0    -8      121   15 28 40
15 30 10  ---          08 50 13  25.0  67.4 -3.8       0.0    82      124   15 28 41

15 31 00  1228+126     08 51 03  24.1  61.5 -3.7       0.0    13      124   15 31 00
15 40 30  ---          09 00 35  26.0  60.0 -3.5       0.0   570      142   15 31 01

15 42 10  1253-055     09 02 15  30.6  81.1 -3.9       0.0    37      142   15 42 10
15 46 10  ---          09 06 16  31.5  80.6 -3.8       0.0   240      150   15 42 11

15 47 50  1228+126     09 07 56  27.4  58.8 -3.4       0.0    37      150   15 47 50
15 56 50  ---          09 16 57  29.2  57.2 -3.2       0.0   540      167   15 47 51

15 57 30  1228+126     09 17 37  29.3  57.1 -3.2       0.0    19      167   15 57 30
16 06 50  ---          09 26 59  31.0  55.4 -3.1       0.0   560      185   15 57 31
Schedule for HART      (Code Hh )                                   Page   3
               Fine-scale imaging of M87
  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
----------------------------------------------------------------------------------------

 --- Mon  14 May 2018   Day 134 ---

16 08 30  1156+295     09 28 39  24.0  36.0 -2.5       0.0    39      185   16 08 30
16 12 30  ---          09 32 40  24.5  35.2 -2.5       0.0   240      193   16 08 31

16 14 00  1228+126     09 34 10  32.4  54.0 -3.0       0.0    29      193   16 14 00
16 22 30  ---          09 42 42  33.9  52.3 -2.8       0.0   510      209   16 14 01

16 23 10  1228+126     09 43 22  34.0  52.2 -2.8       0.0    19      209   16 23 10
16 32 30  ---          09 52 43  35.6  50.3 -2.7       0.0   560      227   16 23 11

16 33 30  1226+023     09 53 43  43.1  59.6 -2.6       0.0    12      227   16 33 30
16 37 30  ---          09 57 44  43.9  58.7 -2.5       0.0   240      235   16 33 31

16 38 30  1228+126     09 58 44  36.7  49.0 -2.6       0.0    12      235   16 38 30
16 47 30  ---          10 07 46  38.2  46.9 -2.4       0.0   540      252   16 38 31

16 48 10  1228+126     10 08 26  38.3  46.8 -2.4       0.0    19      252   16 48 10
16 57 30  ---          10 17 47  39.8  44.6 -2.2       0.0   560      271   16 48 11

16 59 10  1253-055     10 19 28  47.4  68.9 -2.6       0.0    37      271   16 59 10
17 03 10  ---          10 23 28  48.2  68.1 -2.6       0.0   240      278   16 59 11

17 04 50  1228+126     10 25 09  40.9  42.7 -2.1       0.0    37      278   17 04 50
17 14 10  ---          10 34 30  42.3  40.3 -2.0       0.0   560      296   17 04 51

17 14 50  1228+126     10 35 10  42.4  40.1 -1.9       0.0    19      296   17 14 50
17 25 00  ---          10 45 22  43.9  37.4 -1.8       0.0   610      316   17 14 51

17 25 50  1228+126     10 46 12  44.0  37.1 -1.8       0.0    29      316   17 25 50
17 34 20  ---          10 54 43  45.1  34.7 -1.6       0.0   510      332   17 25 51

17 36 00  1156+295     10 56 24  32.9  16.7 -1.1       0.0    39      332   17 36 00
17 39 20  ---          10 59 44  33.1  15.8 -1.0       0.0   200      339   17 36 01

17 41 00  1228+126     11 01 24  45.9  32.7 -1.5       0.0    39      339   17 41 00
17 49 20  ---          11 09 46  46.9  30.1 -1.4       0.0   500      355   17 41 01

17 50 20  1226+023     11 10 46  56.2  37.5 -1.3       0.0    12      355   17 50 20
17 54 20  ---          11 14 47  56.7  36.0 -1.3       0.0   240      363   17 50 21

17 55 20  1253-055     11 15 47  58.6  54.8 -1.7       0.0    17      363   17 55 20
17 59 20  ---          11 19 47  59.3  53.5 -1.6       0.0   240      370   17 55 21

18 01 00  1228+126     11 21 28  48.2  26.2 -1.2       0.0    37      370   18 01 00
18 04 20  ---          11 24 48  48.5  25.1 -1.1       0.0   200      377   18 01 01
Schedule for HART      (Code Hh )                                   Page   4
               Fine-scale imaging of M87
  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
----------------------------------------------------------------------------------------

 --- Mon  14 May 2018   Day 134 ---

 ---------- K-band VLBI scans. Space segment 03: 1228+126 ----------

18 05 00  1228+126     11 25 28  48.6  24.9 -1.1       0.0    19      377   18 05 00
18 25 00  ---          11 45 32  50.2  17.8 -0.8       0.0  1200      415   18 05 01

18 25 40  1228+126     11 46 12  50.2  17.6 -0.8       0.0    19      415   18 25 40
18 45 00  ---          12 05 35  51.3  10.3 -0.4       0.0  1160      453   18 25 41

 ---------- K-band VLBI scans. Ground segment 04: ----------

18 45 40  1228+126     12 06 15  51.3  10.0 -0.4       0.0    19      453   18 45 40
18 55 00  ---          12 15 37  51.6   6.4 -0.3       0.0   560      471   18 45 41

18 56 40  1156+295     12 17 17  34.8 355.5  0.3       0.0    39      471   18 56 40
19 00 10  ---          12 20 47  34.7 354.6  0.3       0.0   210      478   18 56 41

19 01 40  1228+126     12 22 18  51.7   3.7 -0.2       0.0    29      478   19 01 40
19 09 40  ---          12 30 19  51.8   0.6 -0.0       0.0   480      493   19 01 41

19 11 10  1253-055     12 31 49  69.1  17.9 -0.4       0.0    27      493   19 11 10
19 14 40  ---          12 35 20  69.3  15.5 -0.4       0.0   210      500   19 11 11

19 16 20  1228+126     12 37 00  51.8 357.9  0.1       0.0    37      500   19 16 20
19 24 40  ---          12 45 22  51.7 354.6  0.2       0.0   500      516   19 16 21

 ---------- K-band VLBI scans. Ground segment 04: ----------

19 25 40  1228+126     12 46 22  51.7 354.2  0.2       0.0    39      516   19 25 40
19 34 40  ---          12 55 23  51.4 350.7  0.4       0.0   540      533   19 25 41

19 35 50  1226+023     12 56 33  61.4 346.0  0.4       0.0    22      533   19 35 50
19 39 40  ---          13 00 24  61.2 344.1  0.5       0.0   230      541   19 35 51

19 40 50  1228+126     13 01 34  51.1 348.3  0.5       0.0    22      541   19 40 50
19 49 40  ---          13 10 26  50.7 345.0  0.6       0.0   530      558   19 40 51

19 51 10  1156+295     13 11 56  32.4 341.5  1.2       0.0    29      558   19 51 10
19 54 50  ---          13 15 36  32.1 340.6  1.3       0.0   220      565   19 51 11

19 56 20  1228+126     13 17 07  50.3 342.5  0.8       0.0    29      565   19 56 20
20 05 00  ---          13 25 48  49.6 339.4  0.9       0.0   520      582   19 56 21

20 06 40  1253-055     13 27 28  68.7 338.8  0.5       0.0    37      582   20 06 40
20 10 00  ---          13 30 49  68.4 336.7  0.6       0.0   200      588   20 06 41
Schedule for HART      (Code Hh )                                   Page   5
               Fine-scale imaging of M87
  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
----------------------------------------------------------------------------------------

 --- Mon  14 May 2018   Day 134 ---

20 11 40  1228+126     13 32 29  49.1 337.0  1.0       0.0    37      588   20 11 40
20 20 00  ---          13 40 51  48.3 334.2  1.2       0.0   500      604   20 11 41

20 20 40  1228+126     13 41 31  48.2 333.9  1.2       0.0    19      604   20 20 40
20 25 00  ---          13 45 51  47.8 332.5  1.2       0.0   260      613   20 20 41

 ---------- K-band VLBI scans. Ground segment 04: ----------

20 26 20  1228+126     13 47 12  47.6 332.0  1.3       0.0    59      613   20 26 20
20 35 30  ---          13 56 23  46.6 329.1  1.4       0.0   550      630   20 26 21

20 36 50  1156+295     13 57 43  28.2 331.0  2.0       0.0    19      630   20 36 50
20 40 30  ---          14 01 24  27.8 330.2  2.0       0.0   220      637   20 36 51

20 41 50  1228+126     14 02 44  45.9 327.1  1.5       0.0    19      637   20 41 50
20 50 30  ---          14 11 26  44.8 324.6  1.7       0.0   520      654   20 41 51

20 51 50  1226+023     14 12 46  52.7 314.4  1.7       0.0    32      654   20 51 50
20 55 30  ---          14 16 26  52.1 313.2  1.8       0.0   220      661   20 51 51

20 56 50  1228+126     14 17 47  43.9 322.7  1.8       0.0    32      661   20 56 50
21 05 30  ---          14 26 28  42.7 320.4  1.9       0.0   520      678   20 56 51

21 07 00  1253-055     14 27 58  60.5 308.8  1.5       0.0    27      678   21 07 00
21 10 30  ---          14 31 29  59.9 307.5  1.6       0.0   210      685   21 07 01

21 12 00  1228+126     14 32 59  41.8 318.6  2.0       0.0    27      685   21 12 00
21 20 30  ---          14 41 31  40.5 316.5  2.2       0.0   510      701   21 12 01

21 21 10  1228+126     14 42 11  40.4 316.3  2.2       0.0    19      701   21 21 10
21 30 00  ---          14 51 02  39.0 314.2  2.3       0.0   530      718   21 21 11

21 30 40  1228+126     14 51 42  38.8 314.0  2.3       0.0    19      718   21 30 40
21 39 00  ---          15 00 04  37.5 312.1  2.5       0.0   500      734   21 30 41

 ---------- K-band VLBI scans. Space segment 04: 1228+126 ----------

21 40 00  1228+126     15 01 04  37.3 311.9  2.5       0.0    39      734   21 40 00
21 56 40  ---          15 17 46  34.4 308.3  2.8       0.0  1000      766   21 40 01

21 57 20  1228+126     15 18 27  34.3 308.1  2.8       0.0    19      766   21 57 20
22 13 20  ---          15 34 29  31.4 305.0  3.0       0.0   960      797   21 57 21

22 14 00  1228+126     15 35 09  31.3 304.9  3.1       0.0    19      797   22 14 00
22 30 00  ---          15 51 12  28.3 302.0  3.3       0.0   960      828   22 14 01
Schedule for HART      (Code Hh )                                   Page   6
               Fine-scale imaging of M87
  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
----------------------------------------------------------------------------------------

 --- Mon  14 May 2018   Day 134 ---

22 31 20  1253-055     15 52 32  43.6 287.8  2.9       0.0    17      828   22 31 20
22 33 20  ---          15 54 32  43.2 287.4  3.0       0.0   120      832   22 31 21

22 35 00  1156+295     15 56 13  11.1 310.3  3.9       0.0     3      832   22 35 00
22 37 00  ---          15 58 13  10.8 310.0  4.0       0.0   120      836   22 35 01

22 38 40  1228+126     15 59 53  26.6 300.5  3.5       0.0    39      836   22 38 40
22 42 40  ---          16 03 54  25.8 299.9  3.5       0.0   240      844   22 38 41

22 43 30  1228+126     16 04 44  25.7 299.7  3.5       0.0    29      844   22 43 30
22 52 00  ---          16 13 16  24.0 298.4  3.7       0.0   510      860   22 43 31

22 52 40  1228+126     16 13 56  23.9 298.2  3.7       0.0    19      860   22 52 40
22 56 40  ---          16 17 56  23.1 297.6  3.8       0.0   240      868   22 52 41

22 57 30  1228+126     16 18 46  22.9 297.5  3.8       0.0    29      868   22 57 30
23 10 00  ---          16 31 19  20.4 295.6  4.0       0.0   750      892   22 57 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:   15         Station: HART              Total bit rate:   256
   Format: VDIF              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=  22000.00  22000.00  22000.00  22000.00
   Net SB=         U         U         L         L
   IF SB =         U         U         U         U
   Pol.  =      RCP       LCP       RCP       LCP 
   BBC   =         1         9         1         9
   BBC SB=         U         U         L         L
   IF    =        A1        C1        A1        C1

  The following frequency sets based on these setups were used.

   Frequency Set:  16  Setup file default.  Used with PCAL = 1MHz
   LO sum=   22236.00  22236.00  22236.00  22236.00
   BBC fr=     236.00    236.00    236.00    236.00
   Bandwd=      16.00     16.00     16.00     16.00
    Matching frequency sets:  16

   Track assignments are: 
    track1=   1,  2,  3,  4
    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 58.985352       0.00
                     85 16 41.77889    * 85 00 00.00000      84 54 13.48772        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 20.487542       0.10
 * 1236+077          07 46 45.39997    * 07 30 17.18902      07 24 18.52672        0.11
   J1239+07          From catalog imbedded in main SCHED input file.
                     rfc_2012b Petrov, 2012, unpublished 1855 observations

 * 1226+023          12 26 33.245835   * 12 29 06.699731     12 30 03.025117       0.00
   J1229+0203        02 19 43.30547    * 02 03 08.59797      01 57 05.87367        0.00
   3C273B            ./gs042_sources.radioastron
   3C273             AGN, rfc_2013d Petrov, 2013, unpublished 32011 observations, RA-AO4-07, RA-AO3-0

 * 1253-055          12 53 35.831289   * 12 56 11.166557     12 57 08.371431       0.00
   J1256-0547       -05 31 07.99603    *-05 47 21.52489     -05 53 17.34581        0.00
   3C279             ./gs042_sources.radioastron
                     AGN, rfc_2013d Petrov, 2013, unpublished 7924 observations, RA-AO4-07, RA-AO3-04

 * 1228+126          12 28 17.569280   * 12 30 49.423382     12 31 45.092957       0.00
   J1230+1223        12 40 01.74883    * 12 23 28.04365      12 17 28.41095        0.00
   3C274             ./gs042_sources.radioastron
   M87               AGN, rfc_2013d Petrov, 2013, unpublished 55201 observations, RA-AO3-04, RA-AO3-0
   VIR-A

 * 1156+295          11 56 57.786212   * 11 59 31.833913     12 00 28.033628       0.00
   J1159+2914        29 31 25.73868    * 29 14 43.82678      29 08 45.29167        0.00
                     ./gs042_sources.radioastron
                     AGN, MASIV, rfc_2013d Petrov, 2013, unpublished 70591 observations, RA-AO3-04, R



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            9                                 2.783     0.000
  1236+077   ra1cm2.set            1 2 3 6 7 8 11 13 14 15 16  +     0.347    16.742
  1226+023   ra1cm2.set            1 2 3 6 7 8 11 13 14 15 16  +     0.667    51.411
  1253-055   ra1cm2.set            1 2 3 6 7 8 11 13 14 15 16  +     0.597    42.278
  1228+126   ra1cm2.set            1 2 3 6 7 8 11 13 14 15 16  +     8.722   862.110
             ra7mm2.set            30 31 32                          0.350    15.750
  1156+295   ra1cm2.set            1 2 3 6 7 8 11 13 14 15 16  +     0.617    51.640


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              74.5
   1236+077           131.5
   1226+023           132.1
   1253-055           141.6
   1228+126           127.0
   1156+295           111.1

  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 

