  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: EVN observations of a new sample of faint blazars
 Exp. Code:  EM077F  


Schedule Version:       1.00
Processed by SCHED version:   9.40  Release Jan. 13, 2011.

PI:       Franco Mantovani

Address:  Istituto di Radioastronomia
          Via P. Gobetti, 101
          I-40129 Bologna
          Italy

Phone:    +39 51 6399377
EMAIL:    fmantovani@ira.inaf.it
Fax:      +39 51 6399431
Phone during observation:

Observing mode: Continuum

Notes:
 
 
 

Schedule for HART      (Code Hh )                                   Page   2
               EVN observations of a new sample of faint blazars
  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
----------------------------------------------------------------------------------------

 --- Tue  31 May 2011   Day 151 ---

 Next scan frequencies:  4966.49  4966.49  4966.49  4966.49  4982.49  4982.49
                         4982.49  4982.49  4998.49  4998.49  4998.49  4998.49
                         5014.49  5014.49  5014.49  5014.49
 Next BBC frequencies:    366.49   366.49   366.49   366.49   382.49   382.49
                          382.49   382.49   398.49   398.49   398.49   398.49
                          414.49   414.49   414.49   414.49
 Next scan bandwidths:      8.00     8.00     8.00     8.00     8.00     8.00
                            8.00     8.00     8.00     8.00     8.00     8.00
                            8.00     8.00     8.00     8.00

16 00 00  3C273        10 25 57  49.1  51.7 -2.1       0.0     0        0   15 59 55
16 10 00  ---          10 35 59  50.8  48.9 -1.9       0.0   600       39   15 59 59

16 11 00 J1204.2-0710  10 36 59  62.0  52.2 -1.5       0.0    15       39   16 10 55
16 17 00  ---          10 43 00  63.0  49.9 -1.4       0.0   360       63   16 10 59

16 18 30 J1223.9+0650  10 44 30  49.3  40.1 -1.7       0.0    35       63   16 18 25
16 24 30  ---          10 50 31  50.2  38.2 -1.6       0.0   360       86   16 18 29

16 24 55 J1225.5+0715  10 50 56  49.6  38.2 -1.6       0.0     0       86   16 24 50
16 30 55  ---          10 56 57  50.5  36.2 -1.5       0.0   360      110   16 24 54

16 33 15 J1311.3-0521  10 59 18  52.3  62.9 -2.2       0.0    88      110   16 33 10
16 39 15  ---          11 05 19  53.5  61.4 -2.1       0.0   360      133   16 33 14

16 40 02 J1320.4+0140  11 06 06  47.3  55.0 -2.2       0.0     6      133   16 39 57
16 46 02  ---          11 12 07  48.4  53.5 -2.1       0.0   360      157   16 40 01

16 50 02 J1224.5+2613  11 16 08  35.4  19.1 -1.2       0.0   164      157   16 49 57
16 56 02  ---          11 22 09  35.8  17.5 -1.1       0.0   360      180   16 50 01

16 56 33 J1229.5+2711  11 22 39  34.5  18.3 -1.1       0.0     2      180   16 56 28
17 02 33  ---          11 28 40  34.9  16.7 -1.0       0.0   360      204   16 56 32

17 03 03 J1231.7+2848  11 29 11  33.3  16.6 -1.1       0.0     1      204   17 02 58
17 09 03  ---          11 35 12  33.7  15.1 -1.0       0.0   360      227   17 03 02

17 10 13 J1315.1+2841  11 36 22  30.5  25.4 -1.7       0.0    21      227   17 10 08
17 16 13  ---          11 42 23  31.1  24.0 -1.6       0.0   360      251   17 10 12

17 18 19 J1213.2+1443  11 44 30  48.8  10.8 -0.5       0.0    68      251   17 18 14
17 24 19  ---          11 50 31  49.0   8.6 -0.4       0.0   360      274   17 18 18
Schedule for HART      (Code Hh )                                   Page   3
               EVN observations of a new sample of faint blazars
  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
----------------------------------------------------------------------------------------

 --- Tue  31 May 2011   Day 151 ---

17 26 59 J1204.2-0710  11 53 11  71.1   9.0 -0.2       0.0    89      274   17 26 54
17 32 59  ---          11 59 12  71.3   4.4 -0.1       0.0   360      298   17 26 58

17 34 35 J1223.9+0650  12 00 48  56.8  10.8 -0.4       0.0    41      298   17 34 30
17 40 35  ---          12 06 49  57.1   8.1 -0.3       0.0   360      322   17 34 34

17 41 00 J1225.5+0715  12 07 14  56.6   8.5 -0.3       0.0     0      322   17 40 55
17 47 00  ---          12 13 15  56.8   5.8 -0.2       0.0   360      345   17 40 59

17 49 20 J1311.3-0521  12 15 35  65.5  35.7 -0.9       0.0    88      345   17 49 15
17 55 20  ---          12 21 36  66.3  32.6 -0.8       0.0   360      369   17 49 19

17 56 12 J1320.4+0140  12 22 28  59.1  29.5 -1.0       0.0    11      369   17 56 07
18 02 12  ---          12 28 29  59.7  26.8 -0.9       0.0   360      392   17 56 11

18 06 12 J1224.5+2613  12 32 30  37.9 357.9  0.1       0.0   164      392   18 06 07
18 12 12  ---          12 38 31  37.9 356.2  0.2       0.0   360      416   18 06 11

18 12 45 J1229.5+2711  12 39 04  36.9 357.5  0.1       0.0     5      416   18 12 40
18 18 45  ---          12 45 05  36.9 355.9  0.2       0.0   360      439   18 12 44

18 19 16 J1231.7+2848  12 45 36  35.3 356.4  0.2       0.0     1      439   18 19 11
18 25 16  ---          12 51 37  35.2 354.8  0.3       0.0   360      463   18 19 15

18 26 36 J1315.1+2841  12 52 57  35.2   6.1 -0.4       0.0    31      463   18 26 31
18 32 36  ---          12 58 58  35.3   4.5 -0.3       0.0   360      486   18 26 35

18 34 59 J1213.2+1443  13 01 22  47.8 342.7  0.8       0.0    85      486   18 34 54
18 40 59  ---          13 07 22  47.4 340.7  0.9       0.0   360      510   18 34 58

18 43 49 J1400.7+0425  13 10 13  57.3  24.1 -0.9       0.0    90      510   18 43 44
18 49 49  ---          13 16 14  57.8  21.5 -0.8       0.0   360      534   18 43 48

18 50 41 J1416.4+1242  13 17 06  48.8  22.5 -1.0       0.0     9      534   18 50 36
18 56 41  ---          13 23 07  49.3  20.4 -0.9       0.0   360      557   18 50 40

18 57 51 J1419.1+0603  13 24 18  55.4  24.8 -0.9       0.0    30      557   18 57 46
19 03 51  ---          13 30 19  55.9  22.3 -0.8       0.0   360      581   18 57 50

19 04 18 J1420.6+0650  13 30 45  55.1  22.3 -0.8       0.0     0      581   19 04 13
19 10 18  ---          13 36 46  55.6  19.8 -0.7       0.0   360      604   19 04 17

19 13 08  3C273        13 39 37  57.4 326.2  1.2       0.0    87      604   19 13 03
19 19 08  ---          13 45 38  56.6 323.8  1.3       0.0   360      628   19 13 07
Schedule for HART      (Code Hh )                                   Page   4
               EVN observations of a new sample of faint blazars
  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
----------------------------------------------------------------------------------------

 --- Tue  31 May 2011   Day 151 ---

19 20 38 J1204.2-0710  13 47 08  59.3 303.0  1.7       0.0    45      628   19 20 33
19 26 38  ---          13 53 09  58.2 301.1  1.8       0.0   360      651   19 20 37

19 28 32 J1223.9+0650  13 55 04  50.6 322.9  1.5       0.0    59      651   19 28 27
19 34 32  ---          14 01 05  49.8 321.0  1.6       0.0   360      675   19 28 31

19 34 57 J1225.5+0715  14 01 30  49.6 321.8  1.6       0.0     0      675   19 34 52
19 40 57  ---          14 07 31  48.8 319.9  1.7       0.0   360      698   19 34 56

19 43 07 J1311.3-0521  14 09 41  65.3 323.5  1.0       0.0    78      698   19 43 02
19 49 07  ---          14 15 42  64.5 320.6  1.1       0.0   360      722   19 43 06

19 50 08 J1320.4+0140  14 16 43  59.4 331.8  0.9       0.0    20      722   19 50 03
19 56 08  ---          14 22 44  58.7 329.2  1.0       0.0   360      745   19 50 07

19 59 34 J1224.5+2613  14 26 11  30.3 328.4  2.0       0.0   130      745   19 59 29
20 05 34  ---          14 32 12  29.6 327.1  2.1       0.0   360      769   19 59 33

20 06 34 J1229.5+2711  14 33 12  29.3 328.6  2.1       0.0    32      769   20 06 29
20 12 34  ---          14 39 13  28.5 327.3  2.2       0.0   360      793   20 06 33

20 13 04 J1231.7+2848  14 39 42  27.4 328.6  2.1       0.0     0      793   20 12 59
20 19 04  ---          14 45 43  26.7 327.3  2.2       0.0   360      816   20 13 03

20 20 47 J1315.1+2841  14 47 27  31.2 336.4  1.5       0.0    54      816   20 20 42
20 26 47  ---          14 53 28  30.7 335.1  1.6       0.0   360      840   20 20 46

20 29 07 J1213.2+1443  14 55 48  33.5 311.2  2.7       0.0    82      840   20 29 02
20 35 07  ---          15 01 49  32.4 309.9  2.8       0.0   360      863   20 29 06

20 39 22 J1539.1-0658  15 06 05  69.5  24.5 -0.6       0.0   126      863   20 39 17
20 45 22  ---          15 12 06  70.0  20.5 -0.5       0.0   360      887   20 39 21

20 48 26 J1543.6+1847  15 15 10  44.8   9.7 -0.5       0.0   105      887   20 48 21
20 54 26  ---          15 21 11  45.0   7.7 -0.4       0.0   360      910   20 48 25

20 55 16 J1606.0+2031  15 22 02  42.4  14.2 -0.7       0.0    12      910   20 55 11
21 01 16  ---          15 28 03  42.7  12.3 -0.6       0.0   360      934   20 55 15

21 02 04 J1629.7+2117  15 28 51  40.5  19.0 -1.0       0.0    10      934   21 01 59
21 08 04  ---          15 34 52  41.0  17.2 -0.9       0.0   360      957   21 02 03

21 18 04  3C345        15 44 54  22.9  12.2 -1.0       0.0   536      957   21 17 59
21 24 04  ---          15 50 55  23.2  10.9 -0.9       0.0   360      981   21 18 03
Schedule for HART      (Code Hh )                                   Page   5
               EVN observations of a new sample of faint blazars
  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
----------------------------------------------------------------------------------------

 --- Tue  31 May 2011   Day 151 ---

21 31 57 J1204.2-0710  15 58 48  31.4 277.6  3.9       0.0   305      981   21 31 52
21 37 57  ---          16 04 49  30.1 276.9  4.0       0.0   360     1004   21 31 56

21 39 58 J1223.9+0650  16 06 52  27.0 293.2  3.7       0.0    67     1004   21 39 53
21 45 58  ---          16 12 53  25.7 292.3  3.8       0.0   360     1028   21 39 57

21 46 23 J1225.5+0715  16 13 18  25.7 292.9  3.8       0.0     0     1028   21 46 18
21 52 23  ---          16 19 19  24.5 292.0  3.9       0.0   360     1052   21 46 22

21 53 48 J1311.3-0521  16 20 43  40.5 286.1  3.1       0.0    32     1052   21 53 43
21 59 48  ---          16 26 44  39.2 285.1  3.2       0.0   360     1075   21 53 47

22 00 54 J1320.4+0140  16 27 51  37.2 294.1  3.1       0.0    25     1075   22 00 49
22 06 54  ---          16 33 52  35.9 293.0  3.2       0.0   360     1099   22 00 53

22 09 34 J1224.5+2613  16 36 32  10.1 305.8  4.2       0.0    84     1099   22 09 29
22 15 34  ---          16 42 33   9.0 305.0  4.3       0.0   360     1122   22 09 33

22 16 03 J1229.5+2711  16 43 02   9.3 306.4  4.2       0.0     0     1122   22 15 58
22 22 03  ---          16 49 03   8.2 305.6  4.3       0.0   360     1146   22 16 02

22 29 59 J1315.1+2841  16 57 00  13.9 312.0  3.7       0.0   426     1146   22 29 54
22 35 59  ---          17 03 01  12.9 311.1  3.8       0.0   360     1169   22 29 58

22 38 38 J1213.2+1443  17 05 41   8.3 290.8  4.9       0.0   101     1169   22 38 33
22 44 38  ---          17 11 42   7.0 290.1  5.0  D    0.0     0     1193   22 38 37

22 47 38 J1204.2-0710  17 14 42  14.4 268.9  5.2       0.0   109     1193   22 47 33
22 53 38  ---          17 20 43  13.1 268.2  5.3       0.0   360     1216   22 47 37

22 56 31 J1400.7+0425  17 23 37  32.5 294.1  3.4       0.0    88     1216   22 56 26
23 02 31  ---          17 29 38  31.2 293.2  3.5       0.0   360     1240   22 56 30

23 04 01 J1416.4+1242  17 31 08  29.1 303.2  3.2       0.0    46     1240   23 03 56
23 10 01  ---          17 37 09  27.9 302.2  3.3       0.0   360     1263   23 04 00

23 11 00 J1419.1+0603  17 38 08  32.3 296.4  3.3       0.0    18     1263   23 10 55
23 17 00  ---          17 44 09  31.1 295.4  3.4       0.0   360     1287   23 10 59

23 17 27 J1420.6+0650  17 44 36  30.8 296.3  3.4       0.0     0     1287   23 17 22
23 23 27  ---          17 50 37  29.6 295.3  3.5       0.0   360     1311   23 17 26

23 25 37 J1539.1-0658  17 52 47  53.1 294.9  2.2       0.0    64     1311   23 25 32
23 31 37  ---          17 58 48  51.9 293.5  2.3       0.0   360     1334   23 25 36
Schedule for HART      (Code Hh )                                   Page   6
               EVN observations of a new sample of faint blazars
  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
----------------------------------------------------------------------------------------

 --- Tue  31 May 2011   Day 151 ---

23 35 01 J1543.6+1847  18 02 13  34.2 319.6  2.3       0.0   126     1334   23 34 56
23 41 01  ---          18 08 14  33.3 318.3  2.4       0.0   360     1358   23 35 00

23 41 53 J1606.0+2031  18 09 06  34.9 324.4  2.0       0.0    13     1358   23 41 48
23 47 53  ---          18 15 07  34.1 323.0  2.1       0.0   360     1381   23 41 52

23 49 03 J1629.7+2117  18 16 17  36.3 328.9  1.8       0.0    31     1381   23 48 58
23 55 03  ---          18 22 18  35.6 327.5  1.9       0.0   360     1405   23 49 02

 --- Wed   1 Jun 2011   Day 152 ---

00 05 03  3C345        18 32 20  19.6 338.1  1.8       0.0   536     1405   00 04 58
00 11 03  ---          18 38 21  19.1 337.0  1.9       0.0   360     1428   00 05 02

02 17 41 J1539.1-0658  20 45 19  15.3 269.5  5.1       0.0  7477     1428   02 17 36
02 29 41  ---          20 57 21  12.6 268.2  5.3       0.0   720     1475   02 17 40


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


 Setup file: sess211.C512
   Matching groups in /irasoft/sched/catalogs/freq.dat:
     hh6cm           Values confirmed by E-mail Jonathan Quick 221105 (CR)

   Setup group:    8         Station: HART              Total bit rate:  512
   Format: MKIV1:2           Bits per sample: 2         Sample rate: 16.000
   Number of channels: 16    DBE type:                  Speedup factor:   1.00

   Disk used to record data.

   1st LO=   4600.00   4600.00   4600.00   4600.00   4600.00   4600.00   4600.00   4600.00
             4600.00   4600.00   4600.00   4600.00   4600.00   4600.00   4600.00   4600.00
   Net SB=         L         L         U         U         L         L         U         U
                   L         L         U         U         L         L         U         U
   Pol.  =      RCP       LCP       RCP       LCP       RCP       LCP       RCP       LCP 
                RCP       LCP       RCP       LCP       RCP       LCP       RCP       LCP 
   BBC   =         2         1         2         1         4         3         4         3
                   6         5         6         5         8         7         8         7
   BBC SB=         L         L         U         U         L         L         U         U
                   L         L         U         U         L         L         U         U
   IF    =        2N        1N        2N        1N        2N        1N        2N        1N
                  2N        1N        2N        1N        2N        1N        2N        1N

  The following frequency sets based on this setup were used.

   Frequency Set:  12  Setup file default.
   LO sum=    4966.49   4966.49   4966.49   4966.49   4982.49   4982.49   4982.49   4982.49
              4998.49   4998.49   4998.49   4998.49   5014.49   5014.49   5014.49   5014.49
   BBC fr=     366.49    366.49    366.49    366.49    382.49    382.49    382.49    382.49
               398.49    398.49    398.49    398.49    414.49    414.49    414.49    414.49
   Bandwd=      8.000     8.000     8.000     8.000     8.000     8.000     8.000     8.000
                8.000     8.000     8.000     8.000     8.000     8.000     8.000     8.000

   Track assignments are: 
    track1=   2, 10, 18, 26,  3, 11, 19, 27, 66, 74, 82, 90, 67, 75, 83, 91
    barrel=roll_off 
 SOURCES USED IN RECORDING SCANS --                         EVN observations of a new sample of faint blazars
     Catalog positions marked with *. 
     Precession of date coordinates is based on stop time of first scan.
     Names used in schedule marked with *. 
     Short names used in VLA and SNAP files marked with +. 
     Observation date used in B1950/J2000 coordinate conversion (PRECDATE):  1979.900
     No adjustments are made for rates (DRA, DDEC).
     Scan hours are for recording scans only. 
     Baseline hours are only counted for scans above horizon at both ends.

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

 * J1204.2-0710      12 01 42.796323   * 12 04 16.665000     12 04 53.263862       0.00
                    -06 53 26.73304    *-07 10 08.79000     -07 14 09.05071        0.00
                     From catalog imbedded in main SCHED input file.
                        0.500 scan and     28.400 baseline hours in setup: sess211.C512

 * J1213.2+1443      12 10 41.961642   * 12 13 14.797000     12 13 51.141854       0.00
                     15 00 41.07847    * 14 44 00.43000      14 40 07.70049        0.00
                     From catalog imbedded in main SCHED input file.
                        0.500 scan and     27.899 baseline hours in setup: sess211.C512

 * J1223.9+0650      12 21 21.662720   * 12 23 54.620000     12 24 31.066577       0.00
                     07 06 39.91652    * 06 50 02.74000      06 46 08.35095        0.00
                     From catalog imbedded in main SCHED input file.
                        0.500 scan and     31.800 baseline hours in setup: sess211.C512

 * J1224.5+2613      12 22 04.021031   * 12 24 34.421000     12 25 10.262486       0.00
                     26 29 53.43014    * 26 13 16.66000      26 09 28.45668        0.00
                     From catalog imbedded in main SCHED input file.
                        0.500 scan and     35.100 baseline hours in setup: sess211.C512

 * J1225.5+0715      12 22 58.400584   * 12 25 31.247000     12 26 07.675481       0.00
                     07 32 30.02458    * 07 15 53.57000      07 11 59.50022        0.00
                     From catalog imbedded in main SCHED input file.
                        0.500 scan and     31.800 baseline hours in setup: sess211.C512

 * J1229.5+2711      12 27 04.760348   * 12 29 34.266000     12 30 09.930216       0.00
                     27 28 30.61441    * 27 11 56.31000      27 08 08.95575        0.00
                     From catalog imbedded in main SCHED input file.
                        0.500 scan and     35.100 baseline hours in setup: sess211.C512

 * J1231.7+2848      12 29 14.726915   * 12 31 43.592000     12 32 19.122986       0.00
                     29 04 22.79739    * 28 47 49.71000      28 44 03.10256        0.00
                     From catalog imbedded in main SCHED input file.
                        0.500 scan and     34.100 baseline hours in setup: sess211.C512

 * J1311.3-0521      13 08 42.241929   * 13 11 17.846000     13 11 55.197550       0.00
                    -05 05 24.28988    *-05 21 20.04000     -05 25 07.74430        0.00
                     From catalog imbedded in main SCHED input file.
                        0.500 scan and     30.000 baseline hours in setup: sess211.C512

 * J1315.1+2841      13 12 51.421408   * 13 15 13.523000     13 15 47.725472       0.00
                     28 56 43.67856    * 28 40 53.58000      28 37 16.55445        0.00
                     From catalog imbedded in main SCHED input file.
                        0.500 scan and     35.100 baseline hours in setup: sess211.C512

 * J1320.4+0140      13 17 53.715455   * 13 20 26.770000     13 21 03.540161       0.00
                     01 56 19.48932    * 01 40 36.60000      01 36 53.93876        0.00
                     From catalog imbedded in main SCHED input file.
                        0.500 scan and     33.100 baseline hours in setup: sess211.C512

 * J1400.7+0425      13 58 17.298374   * 14 00 48.424000     14 01 24.908765       0.00
                     04 39 59.85370    * 04 25 31.05000      04 22 06.78603        0.00
                     From catalog imbedded in main SCHED input file.
                        0.500 scan and     20.800 baseline hours in setup: sess211.C512

 * J1416.4+1242      14 14 03.338535   * 14 16 28.652000     14 17 03.833126       0.00
                     12 56 06.08530    * 12 42 13.59000      12 38 59.65452        0.00
                     From catalog imbedded in main SCHED input file.
                        0.500 scan and     23.000 baseline hours in setup: sess211.C512

 * J1419.1+0603      14 16 39.577962   * 14 19 09.262000     14 19 45.475130       0.00
                     06 17 14.76038    * 06 03 28.71000      06 00 14.90893        0.00
                     From catalog imbedded in main SCHED input file.
                        0.400 scan and     20.200 baseline hours in setup: sess211.C512

 * J1420.6+0650      14 18 11.782977   * 14 20 40.893000     14 21 16.976416       0.00
                     07 04 41.89586    * 06 50 59.66000      06 47 46.91843        0.00
                     From catalog imbedded in main SCHED input file.
                        0.400 scan and     20.200 baseline hours in setup: sess211.C512

 * J1539.1-0658      15 36 29.290851   * 15 39 09.648000     15 39 48.601904       0.00
                    -06 49 00.92288    *-06 58 43.49000     -07 01 01.23628        0.00
                     From catalog imbedded in main SCHED input file.
                        0.400 scan and     19.300 baseline hours in setup: sess211.C512

 * J1543.6+1847      15 41 28.887031   * 15 43 43.819000     15 44 16.829303       0.00
                     18 56 45.52225    * 18 47 20.20000      18 45 08.73594        0.00
                     From catalog imbedded in main SCHED input file.
                        0.500 scan and     26.500 baseline hours in setup: sess211.C512

 * J1606.0+2031      16 03 54.143619   * 16 06 05.908000     16 06 38.219250       0.00
                     20 40 11.01838    * 20 32 09.11000      20 30 16.83621        0.00
                     From catalog imbedded in main SCHED input file.
                        0.500 scan and     27.400 baseline hours in setup: sess211.C512

 * J1629.7+2117      16 27 37.816457   * 16 29 47.541000     16 30 19.398708       0.00
                     21 23 46.72279    * 21 17 18.12000      21 15 47.14984        0.00
                     From catalog imbedded in main SCHED input file.
                        0.500 scan and     28.300 baseline hours in setup: sess211.C512

   J1229+0203        12 26 33.245835   * 12 29 06.699731     12 29 43.303561       1.04
 * 3C273             02 19 43.30577    * 02 03 08.59827      01 59 13.32982        1.33
   3C273B            /irasoft/sched/catalogs/sources.vlba
   1226+023          GSFC 2010a astro solution     32199 Observations
   J1229+02             0.267 scan and     21.767 baseline hours in setup: sess211.C512

   J1642+3948        16 41 17.606228   * 16 42 58.809965     16 43 24.270069       0.81
 * 3C345             39 54 10.81494    * 39 48 36.99400      39 47 18.69526        0.54
   1641+399          /irasoft/sched/catalogs/sources.vlba
   J1642+39          GSFC 2010a astro solution     52595 Observations
                        0.300 scan and     18.900 baseline hours in setup: sess211.C512



  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) 
   J1204.2-0710       113.8
   J1213.2+1443       106.5
   J1223.9+0650       112.5
   J1224.5+2613       102.9
   J1225.5+0715       112.7
   J1229.5+2711       103.3
   J1231.7+2848       102.8
   J1311.3-0521       128.5
   J1315.1+2841       110.4
   J1320.4+0140       127.4
   J1400.7+0425       134.3
   J1416.4+1242       131.8
   J1419.1+0603       136.9
   J1420.6+0650       136.6
   J1539.1-0658       160.2
   J1543.6+1847       137.5
   J1606.0+2031       137.0
   J1629.7+2117       136.8
   3C273              115.8
   3C345              118.2

  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 

