  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: Parsec scale radio nuclei in nearby Seyfert galaxies from a complete sam
 Exp. Code:  EG037D  


Schedule Version:       1.00                                              
Processed by SCHED version:   6.05  June 2006                             

PI:       M. Giroletti                                                    

Address:  INAF Istituto di Radioastronomia                                
          Via Gobetti 101                                                 
          40129 Bologna                                                   
          Italy                                                           

Phone:    +39 051 639 9394                                                
EMAIL:    giroletti@ira.inaf.it                                           
Fax:      +39 051 639 9431                                                
Phone during observation: +39 347 906 6221                                

Observing mode: Phase-referencing of low dec sources at 6cm (1 Gb/s)      

Notes:                                                                    
                                                                          
                                                                          
                                                                          

Schedule for HART      (Code Hh )                                   Page   2
               Parsec scale radio nuclei in nearby Seyfert galaxies from a complete sam
  UP:  D => Below limits;  H => Below horizon mask.  blank => Up.
  Early: Seconds between end of slew and start.   Dwell: On source seconds. 
  Tapes: Drive, Index, Start footage / Direction, Head Group, End footage.
         For disks, the footages are really the GBytes
  TPStart:  Tape motion start time.  Frequencies are LO sum (band edge).
  SYNC: Time correlator is expected to sync up.
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)   SYNC
----------------------------------------------------------------------------------------

 --- Mon  10 Mar 2008   Day  70 ---

 Next scan frequencies:  4942.49  4942.49  4942.49  4942.49  4974.49  4974.49
                         4974.49  4974.49  5006.49  5006.49  5006.49  5006.49
                         5038.49  5038.49  5038.49  5038.49
 Next BBC frequencies:    342.49   342.49   342.49   342.49   374.49   374.49
                          374.49   374.49   406.49   406.49   406.49   406.49
                          438.49   438.49   438.49   438.49
 Next scan bandwidths:     16.00    16.00    16.00    16.00    16.00    16.00
                           16.00    16.00    16.00    16.00    16.00    16.00
                           16.00    16.00    16.00    16.00

20 30 00  J1225+1253   09 36 16  33.5  51.9 -2.8       0.0     0   1  1      0  20 30 00
20 31 40  =M84         09 37 56  33.8  51.6 -2.8       0.0   100   F  1     13  20 30 04

20 31 40  NGC4388      09 37 56  33.8  51.9 -2.8       0.0   -24   1  1     13  20 31 40
20 35 40  ---          09 41 57  34.5  51.1 -2.7       0.0   216   F  1     44  20 31 44

20 36 05  J1225+1253   09 42 22  34.5  50.6 -2.7       0.0     1   1  1     44  20 36 05
20 37 45  =M84         09 44 02  34.8  50.3 -2.7       0.0   100   F  1     57  20 36 09

20 37 45  NGC4388      09 44 02  34.9  50.6 -2.7       0.0   -24   1  1     57  20 37 45
20 41 45  ---          09 48 03  35.6  49.8 -2.6       0.0   216   F  1     88  20 37 49

20 41 45  J1225+1253   09 48 03  35.5  49.5 -2.6       0.0   -24   1  1     88  20 41 45
20 43 45  =M84         09 50 03  35.9  49.0 -2.6       0.0    96   F  1    103  20 41 49

20 43 45  NGC4501      09 50 03  33.6  49.2 -2.7       0.0   -30   1  1    103  20 43 45
20 47 45  ---          09 54 04  34.3  48.3 -2.6       0.0   210   F  1    134  20 43 49

20 48 10  J1225+1253   09 54 29  36.6  48.1 -2.5       0.0    -5   1  1    134  20 48 10
20 49 50  =M84         09 56 09  36.9  47.7 -2.5       0.0    95   F  1    147  20 48 14

20 49 50  NGC4501      09 56 09  34.6  47.9 -2.6       0.0   -30   1  1    147  20 49 50
20 53 50  ---          10 00 10  35.3  47.0 -2.5       0.0   210   F  1    178  20 49 54

20 53 50  J1225+1253   10 00 10  37.6  46.8 -2.4       0.0   -30   1  1    178  20 53 50
20 55 50  =M84         10 02 10  37.9  46.3 -2.4       0.0    90   F  1    194  20 53 54

20 55 50  NGC4388      10 02 10  37.9  46.7 -2.4       0.0   -24   1  1    194  20 55 50
20 59 50  ---          10 06 11  38.6  45.7 -2.3       0.0   216   F  1    225  20 55 54

21 00 15  J1225+1253   10 06 36  38.6  45.3 -2.3       0.0     1   1  1    225  21 00 15
21 01 55  =M84         10 08 16  38.9  44.9 -2.3       0.0   100   F  1    237  21 00 19
Schedule for HART      (Code Hh )                                   Page   3
               Parsec scale radio nuclei in nearby Seyfert galaxies from a complete sam
  UP:  D => Below limits;  H => Below horizon mask.  blank => Up.
  Early: Seconds between end of slew and start.   Dwell: On source seconds. 
  Tapes: Drive, Index, Start footage / Direction, Head Group, End footage.
         For disks, the footages are really the GBytes
  TPStart:  Tape motion start time.  Frequencies are LO sum (band edge).
  SYNC: Time correlator is expected to sync up.
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)   SYNC
----------------------------------------------------------------------------------------

 --- Mon  10 Mar 2008   Day  70 ---

21 01 55  NGC4388      10 08 16  38.9  45.3 -2.3       0.0   -24   1  1    237  21 01 55
21 05 55  ---          10 12 17  39.6  44.3 -2.2       0.0   216   F  1    268  21 01 59

21 05 55  J1225+1253   10 12 17  39.5  43.9 -2.2       0.0   -24   1  1    268  21 05 55
21 07 55  =M84         10 14 17  39.8  43.4 -2.2       0.0    96   F  1    284  21 05 59

21 07 55  NGC4501      10 14 17  37.6  43.8 -2.3       0.0   -30   1  1    284  21 07 55
21 11 55  ---          10 18 18  38.2  42.9 -2.2       0.0   210   F  1    315  21 07 59

21 12 20  J1225+1253   10 18 43  40.5  42.3 -2.1       0.0    -5   1  1    315  21 12 20
21 14 00  =M84         10 20 23  40.7  41.9 -2.1       0.0    95   F  1    328  21 12 24

21 14 00  NGC4501      10 20 23  38.5  42.4 -2.2       0.0   -30   1  1    328  21 14 00
21 18 00  ---          10 24 24  39.1  41.4 -2.1       0.0   210   F  1    359  21 14 04

21 18 00  J1225+1253   10 24 24  41.3  40.9 -2.0       0.0   -30   1  1    359  21 18 00
21 20 00  =M84         10 26 24  41.6  40.4 -2.0       0.0    90   F  1    374  21 18 04

21 20 00  NGC4388      10 26 24  41.7  40.7 -2.0       0.0   -24   1  1    374  21 20 00
21 24 00  ---          10 30 25  42.3  39.7 -1.9       0.0   216   F  1    405  21 20 04

21 24 25  J1225+1253   10 30 50  42.3  39.2 -1.9       0.0     1   1  1    405  21 24 25
21 26 05  =M84         10 32 30  42.5  38.8 -1.9       0.0   100   F  1    418  21 24 29

21 26 05  NGC4388      10 32 30  42.6  39.1 -1.9       0.0   -24   1  1    418  21 26 05
21 30 05  ---          10 36 31  43.1  38.0 -1.8       0.0   216   F  1    449  21 26 09

21 30 05  J1225+1253   10 36 31  43.1  37.7 -1.8       0.0   -24   1  1    449  21 30 05
21 32 05  =M84         10 38 31  43.3  37.1 -1.8       0.0    96   F  1    464  21 30 09

21 32 05  NGC4501      10 38 31  41.1  37.8 -1.9       0.0   -30   1  1    464  21 32 05
21 36 05  ---          10 42 32  41.7  36.7 -1.8       0.0   210   F  1    495  21 32 09

21 36 30  J1225+1253   10 42 57  43.9  35.9 -1.7       0.0    -5   1  1    495  21 36 30
21 38 10  =M84         10 44 37  44.1  35.4 -1.7       0.0    95   F  1    508  21 36 34

21 38 10  NGC4501      10 44 37  41.9  36.2 -1.8       0.0   -30   1  1    508  21 38 10
21 42 10  ---          10 48 38  42.5  35.1 -1.7       0.0   210   F  1    539  21 38 14

21 42 10  J1225+1253   10 48 38  44.7  34.2 -1.6       0.0   -30   1  1    539  21 42 10
21 44 10  =M84         10 50 38  44.9  33.6 -1.6       0.0    90   F  1    555  21 42 14

21 44 10  NGC4388      10 50 38  45.0  34.0 -1.6       0.0   -24   1  1    555  21 44 10
21 48 10  ---          10 54 39  45.5  32.8 -1.5       0.0   216   F  1    586  21 44 14
Schedule for HART      (Code Hh )                                   Page   4
               Parsec scale radio nuclei in nearby Seyfert galaxies from a complete sam
  UP:  D => Below limits;  H => Below horizon mask.  blank => Up.
  Early: Seconds between end of slew and start.   Dwell: On source seconds. 
  Tapes: Drive, Index, Start footage / Direction, Head Group, End footage.
         For disks, the footages are really the GBytes
  TPStart:  Tape motion start time.  Frequencies are LO sum (band edge).
  SYNC: Time correlator is expected to sync up.
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)   SYNC
----------------------------------------------------------------------------------------

 --- Mon  10 Mar 2008   Day  70 ---

21 48 35  J1225+1253   10 55 04  45.5  32.3 -1.5       0.0     1   1  1    586  21 48 35
21 50 15  =M84         10 56 44  45.7  31.8 -1.5       0.0   100   F  1    599  21 48 39

21 50 15  NGC4388      10 56 44  45.8  32.2 -1.5       0.0   -24   1  1    599  21 50 15
21 54 15  ---          11 00 45  46.2  30.9 -1.4       0.0   216   F  1    630  21 50 19

21 54 15  J1225+1253   11 00 45  46.1  30.6 -1.4       0.0   -24   1  1    630  21 54 15
21 56 15  =M84         11 02 45  46.3  29.9 -1.4       0.0    96   F  1    645  21 54 19

21 56 15  NGC4501      11 02 45  44.2  31.0 -1.5       0.0   -30   1  1    645  21 56 15
22 00 15  ---          11 06 46  44.7  29.8 -1.4       0.0   210   F  1    676  21 56 19

22 00 40  J1225+1253   11 07 11  46.8  28.5 -1.3       0.0    -5   1  1    676  22 00 40
22 02 20  =M84         11 08 51  47.0  28.0 -1.3       0.0    95   F  1    689  22 00 44

22 02 20  NGC4501      11 08 51  44.9  29.2 -1.4       0.0   -30   1  1    689  22 02 20
22 06 20  ---          11 12 52  45.3  28.0 -1.3       0.0   210   F  1    720  22 02 24

22 06 20  J1225+1253   11 12 52  47.4  26.7 -1.2       0.0   -30   1  1    720  22 06 20
22 08 20  =M84         11 14 52  47.6  26.0 -1.2       0.0    90   F  1    735  22 06 24

22 53 34  J1225+1253   12 00 14  50.8   9.8 -0.4       0.0  2664   1  1    735  22 53 34
22 55 14  =M84         12 01 54  50.8   9.1 -0.4       0.0   100   F  1    748  22 53 38

22 55 14  NGC4388      12 01 54  51.0   9.5 -0.4       0.0   -24   1  1    748  22 55 14
22 59 14  ---          12 05 55  51.2   7.9 -0.3       0.0   216   F  1    779  22 55 18

22 59 39  J1225+1253   12 06 20  51.0   7.4 -0.3       0.0     1   1  1    779  22 59 39
23 01 19  =M84         12 08 00  51.0   6.8 -0.3       0.0   100   F  1    792  22 59 43

23 01 19  NGC4388      12 08 00  51.2   7.1 -0.3       0.0   -24   1  1    792  23 01 19
23 05 19  ---          12 12 01  51.3   5.6 -0.2       0.0   216   F  1    823  23 01 23

23 05 19  J1225+1253   12 12 01  51.1   5.2 -0.2       0.0   -24   1  1    823  23 05 19
23 07 19  =M84         12 14 01  51.2   4.5 -0.2       0.0    96   F  1    839  23 05 23

23 07 19  NGC4501      12 14 01  49.5   6.9 -0.3       0.0   -30   1  1    839  23 07 19
23 11 19  ---          12 18 02  49.6   5.4 -0.2       0.0   210   F  1    870  23 07 23

23 11 44  J1225+1253   12 18 27  51.2   2.8 -0.1       0.0    -5   1  1    870  23 11 44
23 13 24  =M84         12 20 07  51.3   2.1 -0.1       0.0    95   F  1    883  23 11 48

23 13 24  NGC4501      12 20 07  49.6   4.6 -0.2       0.0   -30   1  1    883  23 13 24
23 17 24  ---          12 24 08  49.7   3.1 -0.1       0.0   210   F  1    913  23 13 28
Schedule for HART      (Code Hh )                                   Page   5
               Parsec scale radio nuclei in nearby Seyfert galaxies from a complete sam
  UP:  D => Below limits;  H => Below horizon mask.  blank => Up.
  Early: Seconds between end of slew and start.   Dwell: On source seconds. 
  Tapes: Drive, Index, Start footage / Direction, Head Group, End footage.
         For disks, the footages are really the GBytes
  TPStart:  Tape motion start time.  Frequencies are LO sum (band edge).
  SYNC: Time correlator is expected to sync up.
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)   SYNC
----------------------------------------------------------------------------------------

 --- Mon  10 Mar 2008   Day  70 ---

23 17 24  J1225+1253   12 24 08  51.3   0.5  0.0       0.0   -30   1  1    913  23 17 24
23 19 24  =M84         12 26 08  51.3 359.8  0.0       0.0    90   F  1    929  23 17 28

23 19 24  NGC4388      12 26 08  51.5   0.0  0.0       0.0   -24   1  1    929  23 19 24
23 23 24  ---          12 30 09  51.5 358.5  0.1       0.0   216   F  1    960  23 19 28

23 23 49  J1225+1253   12 30 34  51.3 358.0  0.1       0.0     1   1  1    960  23 23 49
23 25 29  =M84         12 32 14  51.2 357.4  0.1       0.0   100   F  1    973  23 23 53

23 25 29  NGC4388      12 32 14  51.5 357.6  0.1       0.0   -24   1  1    973  23 25 29
23 29 29  ---          12 36 15  51.4 356.1  0.2       0.0   216   F  1   1004  23 25 33

23 29 29  J1225+1253   12 36 15  51.2 355.8  0.2       0.0   -24   1  1   1004  23 29 29
23 31 29  =M84         12 38 15  51.1 355.0  0.2       0.0    96   F  1   1019  23 29 33

23 31 29  NGC4501      12 38 15  49.7 357.8  0.1       0.0   -30   1  1   1019  23 31 29
23 35 29  ---          12 42 16  49.7 356.3  0.2       0.0   210   F  1   1050  23 31 33

23 35 54  J1225+1253   12 42 41  51.0 353.3  0.3       0.0    -5   1  1   1050  23 35 54
23 37 34  =M84         12 44 21  51.0 352.7  0.3       0.0    95   F  1   1063  23 35 58

23 37 34  NGC4501      12 44 21  49.6 355.5  0.2       0.0   -30   1  1   1063  23 37 34
23 41 34  ---          12 48 22  49.6 354.0  0.3       0.0   210   F  1   1094  23 37 38

23 41 34  J1225+1253   12 48 22  50.9 351.2  0.4       0.0   -30   1  1   1094  23 41 34
23 43 34  =M84         12 50 22  50.8 350.4  0.4       0.0    90   F  1   1110  23 41 38

23 43 34  NGC4388      12 50 22  51.1 350.6  0.4       0.0   -24   1  1   1110  23 43 34
23 47 34  ---          12 54 23  50.9 349.1  0.5       0.0   216   F  1   1141  23 43 38

23 47 59  J1225+1253   12 54 48  50.6 348.7  0.5       0.0     1   1  1   1141  23 47 59
23 49 39  =M84         12 56 28  50.5 348.1  0.5       0.0   100   F  1   1153  23 48 03

23 49 39  NGC4388      12 56 28  50.8 348.3  0.5       0.0   -24   1  1   1153  23 49 39
23 53 39  ---          13 00 29  50.6 346.8  0.6       0.0   216   F  1   1184  23 49 43

23 53 39  J1225+1253   13 00 29  50.3 346.6  0.6       0.0   -24   1  1   1184  23 53 39
23 55 39  =M84         13 02 29  50.2 345.8  0.6       0.0    96   F  1   1200  23 53 43

23 55 39  NGC4501      13 02 29  49.1 348.9  0.5       0.0   -30   1  1   1200  23 55 39
23 59 39  ---          13 06 30  48.9 347.4  0.6       0.0   210   F  1   1231  23 55 43
Schedule for HART      (Code Hh )                                   Page   6
               Parsec scale radio nuclei in nearby Seyfert galaxies from a complete sam
  UP:  D => Below limits;  H => Below horizon mask.  blank => Up.
  Early: Seconds between end of slew and start.   Dwell: On source seconds. 
  Tapes: Drive, Index, Start footage / Direction, Head Group, End footage.
         For disks, the footages are really the GBytes
  TPStart:  Tape motion start time.  Frequencies are LO sum (band edge).
  SYNC: Time correlator is expected to sync up.
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)   SYNC
----------------------------------------------------------------------------------------

 --- Tue  11 Mar 2008   Day  71 ---

00 00 04  J1225+1253   13 06 55  50.0 344.2  0.7       0.0    -5   1  1   1231  00 00 04
00 01 44  =M84         13 08 35  49.9 343.6  0.7       0.0    95   F  1   1244  00 00 08

00 01 44  NGC4501      13 08 35  48.8 346.6  0.6       0.0   -30   1  1   1244  00 01 44
00 05 44  ---          13 12 36  48.6 345.2  0.7       0.0   210   F  1   1275  00 01 48

00 05 44  J1225+1253   13 12 36  49.6 342.1  0.8       0.0   -30   1  1   1275  00 05 44
00 07 44  =M84         13 14 36  49.5 341.4  0.8       0.0    90   F  1   1290  00 05 48

00 11 44  3C345        13 18 37   8.9  37.3 -3.4       0.0    86   1  1   1290  00 11 44
00 21 44  ---          13 28 38  10.2  35.9 -3.2       0.0   600   F  1   1368  00 11 48

01 08 15  J1225+1253   14 15 16  43.0 322.1  1.8       0.0  2611   1  1   1368  01 08 15
01 09 55  =M84         14 16 56  42.7 321.7  1.9       0.0   100   F  1   1381  01 08 19

01 09 55  NGC4388      14 16 56  43.0 321.7  1.8       0.0   -24   1  1   1381  01 09 55
01 13 55  ---          14 20 57  42.4 320.6  1.9       0.0   216   F  1   1412  01 09 59

01 14 20  J1225+1253   14 21 22  42.1 320.5  1.9       0.0     1   1  1   1412  01 14 20
01 16 00  =M84         14 23 02  41.9 320.0  2.0       0.0   100   F  1   1424  01 14 24

01 16 00  NGC4388      14 23 02  42.1 320.0  1.9       0.0   -24   1  1   1424  01 16 00
01 20 00  ---          14 27 03  41.6 319.0  2.0       0.0   216   F  1   1455  01 16 04

01 20 00  J1225+1253   14 27 03  41.3 319.0  2.0       0.0   -24   1  1   1455  01 20 00
01 22 00  =M84         14 29 03  41.0 318.5  2.1       0.0    96   F  1   1471  01 20 04

01 22 00  NGC4501      14 29 03  40.7 321.5  1.9       0.0   -30   1  1   1471  01 22 00
01 26 00  ---          14 33 04  40.2 320.4  2.0       0.0   210   F  1   1502  01 22 04

01 26 25  J1225+1253   14 33 29  40.3 317.4  2.1       0.0    -5   1  1   1502  01 26 25
01 28 05  =M84         14 35 09  40.1 316.9  2.2       0.0    95   F  1   1515  01 26 29

01 28 05  NGC4501      14 35 09  39.9 319.9  2.0       0.0   -30   1  1   1515  01 28 05
01 32 05  ---          14 39 10  39.3 318.9  2.1       0.0   210   F  1   1546  01 28 09

01 32 05  J1225+1253   14 39 10  39.4 316.0  2.2       0.0   -30   1  1   1546  01 32 05
01 34 05  =M84         14 41 10  39.1 315.5  2.3       0.0    90   F  1   1561  01 32 09

01 34 05  NGC4388      14 41 10  39.4 315.5  2.2       0.0   -24   1  1   1561  01 34 05
01 38 05  ---          14 45 11  38.8 314.5  2.3       0.0   216   F  1   1592  01 34 09

01 38 30  J1225+1253   14 45 36  38.4 314.4  2.3       0.0     1   1  1   1592  01 38 30
01 40 10  =M84         14 47 16  38.1 314.0  2.4       0.0   100   F  1   1605  01 38 34
Schedule for HART      (Code Hh )                                   Page   7
               Parsec scale radio nuclei in nearby Seyfert galaxies from a complete sam
  UP:  D => Below limits;  H => Below horizon mask.  blank => Up.
  Early: Seconds between end of slew and start.   Dwell: On source seconds. 
  Tapes: Drive, Index, Start footage / Direction, Head Group, End footage.
         For disks, the footages are really the GBytes
  TPStart:  Tape motion start time.  Frequencies are LO sum (band edge).
  SYNC: Time correlator is expected to sync up.
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)   SYNC
----------------------------------------------------------------------------------------

 --- Tue  11 Mar 2008   Day  71 ---

01 40 10  NGC4388      14 47 16  38.4 314.0  2.4       0.0   -24   1  1   1605  01 40 10
01 44 10  ---          14 51 17  37.8 313.1  2.4       0.0   216   F  1   1636  01 40 14

01 44 10  J1225+1253   14 51 17  37.5 313.1  2.4       0.0   -24   1  1   1636  01 44 10
01 46 10  =M84         14 53 17  37.2 312.7  2.5       0.0    96   F  1   1652  01 44 14

01 46 10  NGC4501      14 53 17  37.1 315.5  2.3       0.0   -30   1  1   1652  01 46 10
01 50 10  ---          14 57 18  36.5 314.6  2.4       0.0   210   F  1   1682  01 46 14

01 50 35  J1225+1253   14 57 43  36.4 311.7  2.5       0.0    -5   1  1   1682  01 50 35
01 52 15  =M84         14 59 23  36.1 311.3  2.6       0.0    95   F  1   1695  01 50 39

01 52 15  NGC4501      14 59 23  36.2 314.1  2.4       0.0   -30   1  1   1695  01 52 15
01 56 15  ---          15 03 24  35.5 313.2  2.5       0.0   210   F  1   1726  01 52 19

01 56 15  J1225+1253   15 03 24  35.5 310.5  2.6       0.0   -30   1  1   1726  01 56 15
01 58 15  =M84         15 05 24  35.1 310.0  2.7       0.0    90   F  1   1742  01 56 19

01 58 15  NGC4388      15 05 24  35.4 310.0  2.7       0.0   -24   1  1   1742  01 58 15
02 02 15  ---          15 09 25  34.7 309.1  2.7       0.0   216   F  1   1773  01 58 19

02 02 40  J1225+1253   15 09 50  34.3 309.1  2.7       0.0     1   1  1   1773  02 02 40
02 04 20  =M84         15 11 30  34.1 308.8  2.8       0.0   100   F  1   1786  02 02 44

02 04 20  NGC4388      15 11 30  34.3 308.7  2.8       0.0   -24   1  1   1786  02 04 20
02 08 20  ---          15 15 31  33.6 307.9  2.8       0.0   216   F  1   1817  02 04 24

02 08 20  J1225+1253   15 15 31  33.3 308.0  2.8       0.0   -24   1  1   1817  02 08 20
02 10 20  =M84         15 17 31  33.0 307.6  2.9       0.0    96   F  1   1832  02 08 24

02 10 20  NGC4501      15 17 31  33.1 310.3  2.8       0.0   -30   1  1   1832  02 10 20
02 14 20  ---          15 21 32  32.4 309.5  2.8       0.0   210   F  1   1863  02 10 24

02 14 45  J1225+1253   15 21 57  32.2 306.7  2.9       0.0    -5   1  1   1863  02 14 45
02 16 25  =M84         15 23 37  31.9 306.4  3.0       0.0    95   F  1   1876  02 14 49

02 16 25  NGC4501      15 23 37  32.1 309.0  2.9       0.0   -30   1  1   1876  02 16 25
02 20 25  ---          15 27 38  31.4 308.3  2.9       0.0   210   F  1   1907  02 16 29

02 20 25  J1225+1253   15 27 38  31.2 305.6  3.0       0.0   -30   1  1   1907  02 20 25
02 22 25  =M84         15 29 38  30.8 305.2  3.1       0.0    90   F  1   1922  02 20 29

03 08 16  3C345        16 15 37  24.0   5.8 -0.5       0.0  2618   1  1   1922  03 08 16
03 18 16  ---          16 25 38  24.2   3.7 -0.3       0.0   600   F  1   2000  03 08 20
Schedule for HART      (Code Hh )                                   Page   8
               Parsec scale radio nuclei in nearby Seyfert galaxies from a complete sam
  UP:  D => Below limits;  H => Below horizon mask.  blank => Up.
  Early: Seconds between end of slew and start.   Dwell: On source seconds. 
  Tapes: Drive, Index, Start footage / Direction, Head Group, End footage.
         For disks, the footages are really the GBytes
  TPStart:  Tape motion start time.  Frequencies are LO sum (band edge).
  SYNC: Time correlator is expected to sync up.
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)   SYNC
----------------------------------------------------------------------------------------

 --- Tue  11 Mar 2008   Day  71 ---

03 26 28  J1225+1253   16 33 53  18.3 294.9  4.1       0.0   333   1  1   2000  03 26 28
03 28 28  =M84         16 35 53  17.9 294.6  4.2       0.0   120   F  1   2015  03 26 32

03 28 28  NGC4388      16 35 53  18.1 294.5  4.2       0.0   -24   1  1   2015  03 28 28
03 32 28  ---          16 39 54  17.3 293.9  4.2       0.0   216   F  1   2046  03 28 32

03 32 53  J1225+1253   16 40 19  17.0 294.0  4.2       0.0     1   1  1   2046  03 32 53
03 34 33  =M84         16 41 59  16.6 293.7  4.3       0.0   100   F  1   2059  03 32 57

03 34 33  NGC4501      16 41 59  17.2 296.0  4.2       0.0   -30   1  1   2059  03 34 33
03 38 33  ---          16 46 00  16.4 295.5  4.2       0.0   210   F  1   2090  03 34 37

03 38 33  J1225+1253   16 46 00  15.8 293.2  4.3       0.0   -30   1  1   2090  03 38 33
03 40 33  =M84         16 48 00  15.4 292.9  4.4       0.0    90   F  1   2106  03 38 37

03 40 33  NGC4388      16 48 00  15.6 292.8  4.4       0.0   -24   1  1   2106  03 40 33
03 44 33  ---          16 52 01  14.8 292.3  4.4       0.0   216   F  1   2137  03 40 37

03 44 58  J1225+1253   16 52 26  14.4 292.3  4.4       0.0     1   1  1   2137  03 44 58
03 46 38  =M84         16 54 06  14.1 292.1  4.5       0.0   100   F  1   2150  03 45 02

03 46 38  NGC4501      16 54 06  14.7 294.4  4.4       0.0   -30   1  1   2150  03 46 38
03 50 38  ---          16 58 07  13.9 293.8  4.4       0.0   210   F  1   2181  03 46 42

03 50 38  J1225+1253   16 58 07  13.3 291.6  4.5       0.0   -30   1  1   2181  03 50 38
03 52 38  =M84         17 00 07  12.8 291.3  4.6       0.0    90   F  1   2196  03 50 42

03 52 38  NGC4388      17 00 07  13.1 291.2  4.6       0.0   -24   1  1   2196  03 52 38
03 56 38  ---          17 04 08  12.3 290.7  4.6       0.0   216   F  1   2227  03 52 42

03 57 03  J1225+1253   17 04 33  11.9 290.8  4.7       0.0     1   1  1   2227  03 57 03
03 58 43  =M84         17 06 13  11.6 290.6  4.7       0.0   100   F  1   2240  03 57 07

03 58 43  NGC4501      17 06 13  12.2 292.8  4.6       0.0   -30   1  1   2240  03 58 43
04 02 43  ---          17 10 14  11.4 292.3  4.6       0.0   210   F  1   2271  03 58 47

04 02 43  J1225+1253   17 10 14  10.7 290.1  4.7       0.0   -30   1  1   2271  04 02 43
04 04 43  =M84         17 12 14  10.3 289.8  4.8       0.0    90   F  1   2286  04 02 47

04 04 43  NGC4388      17 12 14  10.6 289.7  4.8       0.0   -24   1  1   2286  04 04 43
04 08 43  ---          17 16 15   9.7 289.2  4.8       0.0   216   F  1   2317  04 04 47

04 09 08  J1225+1253   17 16 40   9.4 289.3  4.9       0.0     1   1  1   2317  04 09 08
04 10 48  =M84         17 18 20   9.0 289.1  4.9       0.0   100   F  1   2330  04 09 12
Schedule for HART      (Code Hh )                                   Page   9
               Parsec scale radio nuclei in nearby Seyfert galaxies from a complete sam
  UP:  D => Below limits;  H => Below horizon mask.  blank => Up.
  Early: Seconds between end of slew and start.   Dwell: On source seconds. 
  Tapes: Drive, Index, Start footage / Direction, Head Group, End footage.
         For disks, the footages are really the GBytes
  TPStart:  Tape motion start time.  Frequencies are LO sum (band edge).
  SYNC: Time correlator is expected to sync up.
----------------------------------------------------------------------------------------
Start UT  Source               Start / Stop                 Early    Tapes      TPStart
Stop UT                  LST      EL    AZ   HA  UP   ParA  Dwell  (see above)   SYNC
----------------------------------------------------------------------------------------

 --- Tue  11 Mar 2008   Day  71 ---

04 10 48  NGC4501      17 18 20   9.7 291.3  4.8       0.0   -30   1  1   2330  04 10 48
04 14 48  ---          17 22 21   8.9 290.8  4.8       0.0   210   F  1   2361  04 10 52

04 14 48  J1225+1253   17 22 21   8.1 288.6  4.9       0.0   -30   1  1   2361  04 14 48
04 16 48  =M84         17 24 21   7.7 288.4  5.0  D    0.0     0   F  1   2377  04 14 52


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


 Setup file: eg037d.6cm
   Matches group hh6cm in /irasoft/sched/catalogs/freq.dat
    Values confirmed by E-mail Jonathan Quick 221105 (CR)

   Setup group:    9         Station: HART              Total bit rate: 1024
   Format: MKIV1:2           Bits per sample: 2         Sample rate: 32.000
   Number of channels: 16                               Speedup factor:   0.50

   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:   9  Setup file default.  No pcal detection.
   LO sum=    4942.49   4942.49   4942.49   4942.49   4974.49   4974.49   4974.49   4974.49
              5006.49   5006.49   5006.49   5006.49   5038.49   5038.49   5038.49   5038.49
   BBC fr=     342.49    342.49    342.49    342.49    374.49    374.49    374.49    374.49
               406.49    406.49    406.49    406.49    438.49    438.49    438.49    438.49
   Bandwd=     16.000    16.000    16.000    16.000    16.000    16.000    16.000    16.000
               16.000    16.000    16.000    16.000    16.000    16.000    16.000    16.000

   Track assignments are: 
    track1=   2, 10, 18, 26,  3, 11, 19, 27, 66, 74, 82, 90, 67, 75, 83, 91
    barrel=roll_off 
 SOURCE LIST -- Parsec scale radio nuclei in nearby Seyfert galaxies from a complete sam
     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)

 * NGC4388           12 23 14.602212   * 12 25 46.745000     12 26 13.588268       0.00
                     12 56 19.81092    * 12 39 43.51000      12 36 46.55216        0.00
                     From catalog imbedded in main SCHED input file.
                        1.733 scan hours,     57.921 baseline hours above horizon.

 * NGC4501           12 29 27.678516   * 12 31 59.123300     12 32 25.863387       0.00
                     14 41 45.82552    * 14 25 12.79990      14 22 15.96128        0.00
                     From catalog imbedded in main SCHED input file.
                        1.733 scan hours,     56.857 baseline hours above horizon.

 * NGC5194           13 27 46.418171   * 13 29 52.803870     13 30 16.042931       0.00
                     47 27 07.59852    * 47 11 40.06500      47 08 48.53383        0.00
                     From catalog imbedded in main SCHED input file.
                        1.687 scan hours,     49.471 baseline hours above horizon.

 * J1225+1253        12 22 31.582015   * 12 25 03.743331     12 25 30.593934       0.32
   M84               13 09 49.76862    * 12 53 13.13923      12 50 16.14584        0.31
                     /irasoft/sched/catalogs/sources.vlba
                     VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro
                        1.706 scan hours,     49.282 baseline hours above horizon.

 * J1332+4722        13 30 39.878240   * 13 32 45.246425     13 33 08.308734       0.30
   1330+476          47 37 45.36427    * 47 22 22.66772      47 19 31.71104        0.40
                     /irasoft/sched/catalogs/sources.vlba
                     VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro
                        0.872 scan hours,     22.969 baseline hours above horizon.

   J1642+3948        16 41 17.606231   * 16 42 58.809968     16 43 16.150430       0.26
   1641+399          39 54 10.81494    * 39 48 36.99400      39 47 15.68586        0.40
 * 3C345             /irasoft/sched/catalogs/sources.vlba
   J1642+39          VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro
                        0.333 scan hours,     13.183 baseline hours above horizon.



  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) 
   NGC4388            162.7
   NGC4501            160.5
   NGC5194            128.9
   J1225+1253         162.7
   J1332+4722         128.5
   3C345              100.6

  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 

