  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: Network Monitoring Experiment
 Exp. Code:  N08M1   


Schedule Version:       2.00                                              
Processed by SCHED version:   6.05  June 2006                             

PI:       Stefanie Muehle                                                 

Address:  JIVE                                                            
          Postbus 2                                                       
          7990 AA Dwingeloo                                               
          The Netherlands                                                 

Phone:    +31-521-596508                                                  
EMAIL:    muehle@jive.nl                                                  
Fax:                                                                      
Phone during observation: +31-521-596508                                  

Observing mode:                                                           

Notes:    Please DO NOT use the phase cal signal.                         
          Please send the disk pack by express to JIVE                    
                                                                          
                                                                          

Schedule for HART      (Code Hh )                                   Page   2
               Network Monitoring Experiment
  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
----------------------------------------------------------------------------------------

 --- Fri  14 Mar 2008   Day  74 ---

 Next scan frequencies:  6644.52  6644.52  6644.52  6644.52  6660.52  6660.52
                         6660.52  6660.52
 Next BBC frequencies:    134.52   134.52   134.52   134.52   150.52   150.52
                          150.52   150.52
 Next scan bandwidths:      8.00     8.00     8.00     8.00     8.00     8.00
                            8.00     8.00

10 00 00  3C454.3      23 20 19  47.4 350.8  0.4       0.0     0   1  1      0  10 00 00
10 05 00  ---          23 25 19  47.3 349.0  0.5       0.0   300   F  1     10  10 00 04

10 06 00  3C454.3      23 26 20  47.2 348.7  0.5       0.0    36   1  1     10  10 06 00
10 16 00  ---          23 36 21  46.7 345.2  0.7       0.0   600   F  1     29  10 06 04

10 18 00  J2212+2355   23 38 22  36.0 335.6  1.4       0.0    71   1  1     29  10 18 00
10 20 00  =2209+236    23 40 22  35.8 335.1  1.5       0.0   120   F  1     33  10 18 04

10 20 00  J2210+2013   23 40 22  39.0 332.7  1.5       0.0   -34   1  1     33  10 20 00
10 24 00  ---          23 44 23  38.6 331.7  1.6       0.0   206   F  1     41  10 20 04

10 24 00  J2212+2355   23 44 23  35.4 334.0  1.5       0.0   -34   1  1     41  10 24 00
10 26 00  =2209+236    23 46 23  35.2 333.5  1.6       0.0    86   F  1     45  10 24 04

10 26 00  J2210+2013   23 46 23  38.4 331.1  1.6       0.0   -34   1  1     45  10 26 00
10 30 00  ---          23 50 24  38.0 330.1  1.7       0.0   206   F  1     52  10 26 04

10 31 00  J2212+2355   23 51 24  34.7 332.3  1.6       0.0    26   1  1     52  10 31 00
10 33 00  =2209+236    23 53 24  34.5 331.8  1.7       0.0   120   F  1     56  10 31 04

10 33 00  J2210+2013   23 53 24  37.6 329.3  1.7       0.0   -34   1  1     56  10 33 00
10 37 00  ---          23 57 25  37.1 328.3  1.8       0.0   206   F  1     64  10 33 04

10 37 00  J2212+2355   23 57 25  34.1 330.8  1.7       0.0   -34   1  1     64  10 37 00
10 39 00  =2209+236    23 59 25  33.8 330.3  1.8       0.0    86   F  1     68  10 37 04

10 39 00  J2210+2013   23 59 25  36.9 327.8  1.8       0.0   -34   1  1     68  10 39 00
10 43 00  ---          00 03 26  36.4 326.8  1.9       0.0   206   F  1     75  10 39 04

10 44 00  J2212+2355   00 04 26  33.3 329.1  1.9       0.0    26   1  1     75  10 44 00
10 46 00  =2209+236    00 06 26  33.0 328.7  1.9       0.0   120   F  1     79  10 44 04

10 46 00  J2210+2013   00 06 26  36.0 326.0  1.9       0.0   -34   1  1     79  10 46 00
10 50 00  ---          00 10 27  35.5 325.0  2.0       0.0   206   F  1     87  10 46 04
Schedule for HART      (Code Hh )                                   Page   3
               Network Monitoring Experiment
  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
----------------------------------------------------------------------------------------

 --- Fri  14 Mar 2008   Day  74 ---

10 50 00  J2212+2355   00 10 27  32.6 327.7  2.0       0.0   -34   1  1     87  10 50 00
10 52 00  =2209+236    00 12 27  32.3 327.3  2.0       0.0    86   F  1     91  10 50 04

10 52 00  J2210+2013   00 12 27  35.3 324.6  2.0       0.0   -34   1  1     91  10 52 00
10 56 00  ---          00 16 28  34.7 323.6  2.1       0.0   206   F  1     99  10 52 04

10 57 00  J2212+2355   00 17 28  31.7 326.1  2.1       0.0    26   1  1     99  10 57 00
10 59 00  =2209+236    00 19 28  31.4 325.7  2.1       0.0   120   F  1    103  10 57 04

10 59 00  J2210+2013   00 19 28  34.3 322.9  2.1       0.0   -34   1  1    103  10 59 00
11 03 00  ---          00 23 29  33.8 322.0  2.2       0.0   206   F  1    110  10 59 04

11 03 00  J2212+2355   00 23 29  30.9 324.8  2.2       0.0   -34   1  1    110  11 03 00
11 05 00  =2209+236    00 25 29  30.7 324.4  2.2       0.0    86   F  1    114  11 03 04

11 05 00  J2210+2013   00 25 29  33.5 321.5  2.2       0.0   -34   1  1    114  11 05 00
11 09 00  ---          00 29 30  32.9 320.6  2.3       0.0   206   F  1    122  11 05 04

11 10 00  J2212+2355   00 30 30  30.0 323.3  2.3       0.0    26   1  1    122  11 10 00
11 12 00  =2209+236    00 32 30  29.7 322.9  2.3       0.0   120   F  1    126  11 10 04

11 12 00  J2210+2013   00 32 30  32.5 320.0  2.4       0.0   -34   1  1    126  11 12 00
11 16 00  ---          00 36 31  31.9 319.1  2.4       0.0   206   F  1    134  11 12 04

11 16 00  J2212+2355   00 36 31  29.2 322.0  2.4       0.0   -34   1  1    134  11 16 00
11 18 00  =2209+236    00 38 31  28.9 321.6  2.4       0.0    86   F  1    137  11 16 04

11 18 00  J2210+2013   00 38 31  31.6 318.7  2.5       0.0   -34   1  1    137  11 18 00
11 22 00  ---          00 42 32  31.0 317.8  2.5       0.0   206   F  1    145  11 18 04

11 23 00  J2212+2355   00 43 32  28.2 320.6  2.5       0.0    26   1  1    145  11 23 00
11 25 00  =2209+236    00 45 33  27.9 320.2  2.6       0.0   120   F  1    149  11 23 04

11 25 00  J2210+2013   00 45 33  30.6 317.2  2.6       0.0   -34   1  1    149  11 25 00
11 29 00  ---          00 49 33  30.0 316.4  2.6       0.0   206   F  1    157  11 25 04

11 29 00  J2212+2355   00 49 33  27.3 319.4  2.6       0.0   -34   1  1    157  11 29 00
11 31 00  =2209+236    00 51 34  27.0 319.0  2.7       0.0    86   F  1    161  11 29 04

11 31 00  J2210+2013   00 51 34  29.6 316.0  2.7       0.0   -34   1  1    161  11 31 00
11 35 00  ---          00 55 34  29.0 315.2  2.7       0.0   206   F  1    168  11 31 04

11 37 00  3C454.3      00 57 35  38.3 321.2  2.1       0.0    72   1  1    168  11 37 00
11 42 00  ---          01 02 35  37.6 319.9  2.1       0.0   300   F  1    178  11 37 04
Schedule for HART      (Code Hh )                                   Page   4
               Network Monitoring Experiment
  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
----------------------------------------------------------------------------------------

 --- Fri  14 Mar 2008   Day  74 ---

11 43 00  3C454.3      01 03 36  37.5 319.7  2.2       0.0    36   1  1    178  11 43 00
11 53 00  ---          01 13 37  36.0 317.3  2.3       0.0   600   F  1    197  11 43 04

11 57 30  0234+285     01 18 08  32.0  20.7 -1.3       0.0   133   1  1    197  11 57 30
12 07 30  ---          01 28 10  32.7  18.3 -1.2       0.0   600   F  1    217  11 57 34

12 08 00  0234+285     01 28 40  32.8  18.2 -1.2       0.0     7   1  1    217  12 08 00
12 18 00  ---          01 38 41  33.4  15.7 -1.0       0.0   600   F  1    236  12 08 04

12 18 30  0234+285     01 39 11  33.5  15.5 -1.0       0.0     7   1  1    236  12 18 30
12 28 30  ---          01 49 13  34.0  13.0 -0.8       0.0   600   F  1    255  12 18 34

12 29 00  0234+285     01 49 43  34.0  12.9 -0.8       0.0     7   1  1    255  12 29 00
12 39 00  ---          01 59 45  34.5  10.3 -0.6       0.0   600   F  1    275  12 29 04

12 39 30  0234+285     02 00 15  34.5  10.1 -0.6       0.0     7   1  1    275  12 39 30
12 49 30  ---          02 10 17  34.9   7.5 -0.5       0.0   600   F  1    294  12 39 34

12 50 00  0234+285     02 10 47  34.9   7.4 -0.5       0.0     7   1  1    294  12 50 00
13 00 00  ---          02 20 48  35.1   4.7 -0.3       0.0   600   F  1    314  12 50 04

13 03 00  0528+134     02 23 49  29.7  54.8 -3.1       0.0    68   1  1    314  13 03 00
13 13 00  ---          02 33 50  31.5  52.9 -3.0       0.0   600   F  1    333  13 03 04

13 13 30  0528+134     02 34 20  31.6  52.8 -3.0       0.0     7   1  1    333  13 13 30
13 23 30  ---          02 44 22  33.4  50.8 -2.8       0.0   600   F  1    352  13 13 34

13 24 00  0528+134     02 44 52  33.5  50.7 -2.8       0.0     7   1  1    352  13 24 00
13 35 30  ---          02 56 24  35.4  48.3 -2.6       0.0   690   F  1    374  13 24 04

13 39 30  3C84         03 00 25  22.4   4.0 -0.3       0.0   145   1  1    374  13 39 30
13 49 30  ---          03 10 26  22.5   2.0 -0.2       0.0   600   F  1    394  13 39 34

13 50 00  3C84         03 10 56  22.5   1.9 -0.2       0.0     7   1  1    394  13 50 00
14 00 00  ---          03 20 58  22.6 359.9  0.0       0.0   600   F  1    413  13 50 04


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


 Setup file: NME.5CM
   Matches group hh4.5cm_S2 in /aps3/sched/catalogs/freq.dat
    Values confirmed by E-mail Jonathan Quick 291100 (CR)
    ****** Only   37.04 of   64.00 MHz total bandwidth is within the IFs
           in the setup file before any FREQ or DOPPLER shifts.

   Setup group:    9         Station: HART              Total bit rate:  256
   Format: MKIV1:2           Bits per sample: 2         Sample rate: 16.000
   Number of channels:  8                               Speedup factor:   1.00

   Disk used to record data.

   1st LO=   6510.00   6510.00   6510.00   6510.00   6510.00   6510.00   6510.00   6510.00
   Net SB=         L         L         U         U         L         L         U         U
   Pol.  =      RCP       LCP       RCP       LCP       RCP       LCP       RCP       LCP 
   BBC   =         2         1         2         1         4         3         4         3
   BBC SB=         L         L         U         U         L         L         U         U
   IF    =        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=    6644.52   6644.52   6644.52   6644.52   6660.52   6660.52   6660.52   6660.52
   BBC fr=     134.52    134.52    134.52    134.52    150.52    150.52    150.52    150.52
   Bandwd=      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
    barrel=roll_off 
 SOURCE LIST -- Network Monitoring Experiment
     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)

   J0237+2848        02 34 55.589592   * 02 37 52.405679     02 38 20.929516       0.23
 * 0234+285          28 35 11.40780    * 28 48 08.99005      28 50 23.41506        0.40
   J0237+28          /aps3/sched/catalogs/sources.vlba
                     VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro
                        1.000 scan hours,     36.000 baseline hours above horizon.

   J0319+4130        03 16 29.567289   * 03 19 48.160119     03 20 20.364432       0.28
   0316+413          41 19 51.91677    * 41 30 42.10389      41 32 40.86181        0.41
 * 3C84              /aps3/sched/catalogs/sources.vlba
   J0319+41          VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro
                        0.333 scan hours,     12.000 baseline hours above horizon.

   J0530+1331        05 28 06.759218   * 05 30 56.416749     05 31 24.891679       0.31
 * 0528+134          13 29 42.28887    * 13 31 55.14954      13 32 20.77789        0.20
   J0530+13          /aps3/sched/catalogs/sources.vlba
                     VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro
                        0.525 scan hours,     18.900 baseline hours above horizon.

 * J2210+2013        22 08 29.191872   * 22 10 51.652478     22 11 14.126521       0.67
                     19 58 35.87712    * 20 13 24.05509      20 15 40.07084        0.61
                     /aps3/sched/catalogs/sources.vlba
                     VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro
                        0.800 scan hours,     25.112 baseline hours above horizon.

 * J2212+2355        22 09 45.687917   * 22 12 05.966312     22 12 28.004747       0.22
   2209+236          23 40 49.85189    * 23 55 40.54383      23 57 56.86203        0.40
   J2212+23          /aps3/sched/catalogs/sources.vlba
                     VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro
                        0.400 scan hours,     12.556 baseline hours above horizon.

   J2253+1608        22 51 29.519744   * 22 53 57.747943     22 54 21.187662       0.31
   2251+158          15 52 54.34806    * 16 08 53.56089      16 11 23.96448        0.20
 * 3C454.3           /aps3/sched/catalogs/sources.vlba
   J2253+16          VLBA Calib Survey - GSFC sols. - created L.Petrov 2005f_astro
                        0.500 scan hours,     18.000 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) 
   0234+285            53.0
   3C84                66.5
   0528+134            88.7
   J2210+2013          31.2
   J2212+2355          33.6
   3C454.3             21.5

  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 

