  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: Network Monitoring Experiment
 Exp. Code:  N11M1   


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

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:    5cm NME and ftp fringe test for session 1/2011
          (512 Mbps, L+R, 2-bit sampling, 8 MHz filters)
          Please send the disk pack by express to JIVE
          Please DO NOT use the phase cal signal.


COVER LETTER:

This is the schedule for the 5cm NME and ftp fringe-test on 01 March 2011.
The NME uses a setup typical for methanol spectral line experiments, but
with 16 channels, i.e. using both sidebands of all BBCs, and 8 MHz filters.
The schedule consists of long integrations on strong calibrators like
3C454.3 and DA193 as well as phase-referencing parts with a methanol maser
and a continuum source as targets, respectively.

Five ftp-fringe tests are scheduled throughout the experiment:
~12:15 (scan 02, 4 sec, 0234+285)
~12:50 (scan 09, 4 sec, 3C454.3, no Sh)
~13:21 (scan 12, 4 sec, DA193, no Hh)
~14:14 (scan 21, 4 sec, 0234+285, no Sh?)
~14:53 (scan 32, 8 sec, DA193, no Hh?)

Please make sure that the autoftp is set up correctly. Thanks!

Since this schedule includes a spectral line part (W75A), please switch OFF
the phase cal signal!

Good luck with the session!

Stefanie

Schedule for HART      (Code Hh )                                   Page   2
               Network Monitoring Experiment
  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   1 Mar 2011   Day  60 ---

 Next scan frequencies:  6640.52  6640.52  6640.52  6640.52  6656.52  6656.52
                         6656.52  6656.52  6672.52  6672.52  6672.52  6672.52
                         6688.52  6688.52  6688.52  6688.52
 Next BBC frequencies:    130.52   130.52   130.52   130.52   146.52   146.52
                          146.52   146.52   162.52   162.52   162.52   162.52
                          178.52   178.52   178.52   178.52
 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

12 00 00  0234+285     00 26 31  26.7  32.3 -2.2       0.0     0        0   12 00 00
12 10 00  ---          00 36 33  27.9  30.2 -2.0       0.0   600       39   12 00 04

12 11 00  0234+285     00 37 33  28.0  30.0 -2.0       0.0    39       39   12 11 00
12 16 00  ---          00 42 34  28.6  28.9 -1.9       0.0   300       58   12 11 04

12 20 00  0234+285     00 46 35  29.0  28.0 -1.9       0.0   219       58   12 20 00
12 21 30  ---          00 48 05  29.2  27.7 -1.8       0.0    90       64   12 20 04

12 21 30  J0258+2900   00 48 05  26.6  32.1 -2.2       0.0   -37       64   No stop 
12 25 00  =0255+288    00 51 35  27.1  31.4 -2.1       0.0   173       77   12 21 34

12 25 00  0234+285     00 51 35  29.5  26.9 -1.8       0.0   -38       77   No stop 
12 26 30  ---          00 53 06  29.7  26.6 -1.8       0.0    52       83   12 25 04

12 26 30  J0258+2900   00 53 06  27.2  31.0 -2.1       0.0   -37       83   No stop 
12 30 00  =0255+288    00 56 36  27.6  30.3 -2.0       0.0   173       97   12 26 34

12 30 00  0234+285     00 56 36  30.0  25.8 -1.7       0.0   -38       97   No stop 
12 31 30  ---          00 58 06  30.2  25.5 -1.7       0.0    52      103   12 30 04

12 36 30  3C454.3      01 03 07  37.6 319.9  2.1       0.0   160      103   12 36 30
12 46 30  ---          01 13 09  36.1 317.5  2.3       0.0   600      141   12 36 34

12 47 30  3C454.3      01 14 09  35.9 317.3  2.3       0.0    39      141   12 47 30
12 52 30  ---          01 19 10  35.1 316.1  2.4       0.0   300      161   12 47 34

14 04 00  0234+285     02 30 52  35.2   2.1 -0.1       0.0  4152      161   14 04 00
14 09 00  ---          02 35 52  35.3   0.7  0.0       0.0   300      180   14 04 04

14 10 00  0234+285     02 36 53  35.3   0.4  0.0       0.0    39      180   14 10 00
14 15 00  ---          02 41 53  35.3 359.1  0.1       0.0   300      199   14 10 04
Schedule for HART      (Code Hh )                                   Page   3
               Network Monitoring Experiment
  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   1 Mar 2011   Day  60 ---

14 19 00  0234+285     02 45 54  35.2 358.0  0.1       0.0   219      199   14 19 00
14 20 30  ---          02 47 24  35.2 357.6  0.1       0.0    90      205   14 19 04

14 20 30  J0258+2900   02 47 24  35.0   3.3 -0.2       0.0   -37      205   No stop 
14 24 00  =0255+288    02 50 55  35.0   2.3 -0.1       0.0   173      219   14 20 34

14 24 00  0234+285     02 50 55  35.2 356.7  0.2       0.0   -38      219   No stop 
14 25 30  ---          02 52 25  35.2 356.3  0.2       0.0    52      225   14 24 04

14 25 30  J0258+2900   02 52 25  35.0   1.9 -0.1       0.0   -37      225   No stop 
14 29 00  =0255+288    02 55 56  35.1   1.0 -0.1       0.0   173      238   14 25 34

14 30 00  0234+285     02 56 56  35.1 355.1  0.3       0.0    22      238   14 30 00
14 31 30  ---          02 58 26  35.0 354.7  0.3       0.0    90      244   14 30 04

14 31 30  J0258+2900   02 58 26  35.1   0.3  0.0       0.0   -37      244   No stop 
14 35 00  =0255+288    03 01 57  35.1 359.4  0.0       0.0   173      257   14 31 34

14 35 00  0234+285     03 01 57  35.0 353.7  0.4       0.0   -38      257   No stop 
14 36 30  ---          03 03 27  34.9 353.3  0.4       0.0    52      263   14 35 04

14 36 30  J0258+2900   03 03 27  35.1 359.0  0.1       0.0   -37      263   No stop 
14 40 00  =0255+288    03 06 58  35.0 358.0  0.1       0.0   173      277   14 36 34

14 40 00  0234+285     03 06 58  34.8 352.4  0.5       0.0   -38      277   No stop 
14 41 30  ---          03 08 28  34.8 352.0  0.5       0.0    52      283   14 40 04

14 45 30  DA193        03 12 28  14.0  31.3 -2.7       0.0   115      283   14 45 30
14 50 30  ---          03 17 29  14.6  30.5 -2.6       0.0   300      302   14 45 34

14 51 30  DA193        03 18 29  14.7  30.3 -2.6       0.0    39      302   14 51 30
14 54 30  ---          03 21 30  15.0  29.8 -2.6       0.0   180      314   14 51 34

14 58 00  DA193        03 25 01  15.4  29.3 -2.5       0.0   189      314   14 58 00
15 00 00  ---          03 27 01  15.7  28.9 -2.5       0.0   120      321   14 58 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
   Matching groups in ./n11m1_freq.dat:
     hh4.5cm_S2      Values confirmed by E-mail Jonathan Quick 291100 (CR)
    ****** Only   64.00 of  128.00 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:  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=   6510.00   6510.00   6510.00   6510.00   6510.00   6510.00   6510.00   6510.00
             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
                   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.
   LO sum=    6640.52   6640.52   6640.52   6640.52   6656.52   6656.52   6656.52   6656.52
              6672.52   6672.52   6672.52   6672.52   6688.52   6688.52   6688.52   6688.52
   BBC fr=     130.52    130.52    130.52    130.52    146.52    146.52    146.52    146.52
               162.52    162.52    162.52    162.52    178.52    178.52    178.52    178.52
   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 --                         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)

 * W75A              20 36 49.966274   * 20 38 36.410000     20 38 59.400836       0.00
                     42 26 58.84751    * 42 37 35.25000      42 39 50.71238        0.00
                     From catalog imbedded in main SCHED input file.
                        0.250 scan and      6.414 baseline hours in setup: nme.5cm

   J0237+2848        02 34 55.589590   * 02 37 52.405677     02 38 32.551569       0.01
 * 0234+285          28 35 11.40778    * 28 48 08.99003      28 51 08.76912        0.01
   J0237+28          /aps3/sched9.4/catalogs/sources.vlba
                     GSFC 2010a astro solution     53368 Observations
                        0.617 scan and     25.094 baseline hours in setup: nme.5cm

 * J0258+2900        02 55 55.645344   * 02 58 55.181143     02 59 36.072829       0.69
   0255+288          28 48 05.18438    * 29 00 01.60798      29 02 47.60032        0.94
                     /aps3/sched9.4/catalogs/sources.vlba
                     GSFC 2010a astro solution        18 Observations
                        0.350 scan and     12.989 baseline hours in setup: nme.5cm

   J0555+3948        05 52 01.407170   * 05 55 30.805612     05 56 19.694693       0.01
   0552+398          39 48 21.94583    * 39 48 49.16498      39 48 59.20433        0.01
 * DA193             /aps3/sched9.4/catalogs/sources.vlba
   J0555+39          GSFC 2010a astro solution    355917 Observations
                        0.500 scan and     19.500 baseline hours in setup: nme.5cm

 * J2007+4029        20 05 59.558904   * 20 07 44.944855     20 08 07.861479       0.42
   2005+403          40 21 01.80230    * 40 29 48.60415      40 31 37.47739        0.31
   J2007+40          /aps3/sched9.4/catalogs/sources.vlba
                     GSFC 2010a astro solution       129 Observations
                        0.133 scan and      2.839 baseline hours in setup: nme.5cm

   J2253+1608        22 51 29.519738   * 22 53 57.747937     22 54 30.603435       0.76
 * 3C454.3           15 52 54.34811    * 16 08 53.56094      16 12 28.19296        0.74
   2251+158          /aps3/sched9.4/catalogs/sources.vlba
   J2253+16          GSFC 2010a astro solution     39550 Observations
                        0.250 scan and      9.000 baseline hours in setup: nme.5cm



  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) 
   W75A                58.2
   0234+285            66.3
   J0258+2900          70.6
   DA193              107.9
   J2007+4029          60.6
   3C454.3             23.8

  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 

