  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: Network Monitoring Experiment
 Exp. Code:  N13L1   


Schedule Version:       3.00
Processed by SCHED version:  10.20  Release of about July 12, 2012

PI:       Ciriaco Goddi

Address:  JIVE
          Postbus 2
          7990 AA Dwingeloo
          The Netherlands

Phone:    +31-521-596548
EMAIL:    goddi@jive.nl
Fax:
Phone during observation: +31-521-596548

Observing mode:

Notes:    18cm NME for session 1/2013
          512 Mbps, 2-bit sampling, 8 MHz filters
          Send the disk pack by express to JIVE
          DBBC testing data from On, Hh, Nt and Ir are expected.


COVER LETTER:


Dear EVN friends,

This is the schedule for the 18cm NME and ftp fringe-test on 11 March 2013,
involving 14 antennas: Eb Wb Jb1 On25 Mc Nt Tr Ys Sv Zc Bd Ur Sh Hh Ir.
The NME uses a standard setup with 512 Mbps and consists of long
integrations on strong calibrators like DA193
 and 0528+134 as well as phase-referencing cycles with
continuum sources as targets.

Three ftp tests are scheduled:
(1) 14:09:00 UT (scan  2, 2 sec, DA193)
(2) 15:05:00 UT (scan  15, 2 sec, 0528+134)
(3) 15:57:00 UT (scan 30, 2 sec, 0528+134)
Please make sure that the autoftp is set up correctly.

Good luck with the session!

Ciriaco

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
----------------------------------------------------------------------------------------

 --- Mon  11 Mar 2013   Day  70 ---

 Next scan frequencies:  1634.49  1634.49  1634.49  1634.49  1650.49  1650.49  1650.49  1650.49
                         1666.49  1666.49  1666.49  1666.49  1682.49  1682.49  1682.49  1682.49
 Next BBC frequencies:    124.49   124.49   124.49   124.49   140.49   140.49   140.49   140.49
                          156.49   156.49   156.49   156.49   172.49   172.49   172.49   172.49
 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

14 00 00  DA193        03 08 19  13.5  31.9 -2.8       0.0     0        0   14 00 00
14 04 00  ---          03 12 19  14.0  31.3 -2.7       0.0   240       15   14 00 04

14 06 00  DA193        03 14 20  14.2  31.0 -2.7       0.0    99       15   14 06 00
14 10 00  ---          03 18 20  14.7  30.4 -2.6       0.0   240       31   14 06 04

14 10 30  DA193        03 18 50  14.7  30.3 -2.6       0.0     9       31   14 10 30
14 17 00  ---          03 25 21  15.5  29.2 -2.5       0.0   390       56   14 10 34

14 18 00  DA193        03 26 21  15.6  29.1 -2.5       0.0    39       56   14 18 00
14 20 00  ---          03 28 22  15.8  28.7 -2.5       0.0   120       64   14 18 04

14 20 30  DA193        03 28 52  15.8  28.6 -2.5       0.0     9       64   14 20 30
14 22 30  ---          03 30 52  16.1  28.3 -2.4       0.0   120       72   14 20 34

14 23 00  J0552+3754   03 31 22  18.0  28.8 -2.4       0.0     0       72   14 23 00
14 27 00  =0548+378    03 35 23  18.5  28.1 -2.3       0.0   240       87   14 23 04

14 27 30  DA193        03 35 53  16.6  27.5 -2.3       0.0     0       87   14 27 30
14 29 30  ---          03 37 53  16.8  27.1 -2.3       0.0   120       95   14 27 34

14 30 00  J0552+3754   03 38 23  18.8  27.6 -2.2       0.0     0       95   14 30 00
14 34 00  =0548+378    03 42 24  19.2  26.8 -2.2       0.0   240      110   14 30 04

14 34 30  DA193        03 42 54  17.3  26.3 -2.2       0.0     0      110   14 34 30
14 36 30  ---          03 44 55  17.5  25.9 -2.2       0.0   120      118   14 34 34

14 37 00  J0552+3754   03 45 25  19.5  26.3 -2.1       0.0     0      118   14 37 00
14 41 00  =0548+378    03 49 25  19.9  25.6 -2.1       0.0   240      134   14 37 04

14 41 30  DA193        03 49 55  18.0  25.1 -2.1       0.0     0      134   14 41 30
14 43 30  ---          03 51 56  18.2  24.7 -2.1       0.0   120      141   14 41 34

14 44 00  J0552+3754   03 52 26  20.2  25.0 -2.0       0.0     0      141   14 44 00
14 48 00  =0548+378    03 56 26  20.6  24.3 -1.9       0.0   240      157   14 44 04

14 48 30  DA193        03 56 56  18.6  23.8 -2.0       0.0     0      157   14 48 30
14 50 30  ---          03 58 57  18.8  23.5 -2.0       0.0   120      165   14 48 34
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
----------------------------------------------------------------------------------------

 --- Mon  11 Mar 2013   Day  70 ---

14 51 00  J0552+3754   03 59 27  20.8  23.7 -1.9       0.0     0      165   14 51 00
14 55 00  =0548+378    04 03 28  21.2  23.0 -1.8       0.0   240      180   14 51 04

14 58 00  0528+134     04 06 28  45.4  30.2 -1.4       0.0   104      180   14 58 00
15 02 00  ---          04 10 29  45.9  29.0 -1.4       0.0   240      195   14 58 04

15 04 00  0528+134     04 12 29  46.1  28.4 -1.3       0.0    99      195   15 04 00
15 06 00  ---          04 14 29  46.3  27.7 -1.3       0.0   120      203   15 04 04

15 07 00  0528+134     04 15 30  46.4  27.4 -1.3       0.0    39      203   15 07 00
15 09 00  ---          04 17 30  46.6  26.8 -1.2       0.0   120      211   15 07 04

15 09 30  0528+134     04 18 00  46.7  26.6 -1.2       0.0     9      211   15 09 30
15 11 30  ---          04 20 00  46.9  26.0 -1.2       0.0   120      219   15 09 34

15 12 00  J0539+1433   04 20 30  45.1  28.0 -1.3       0.0    -1      219   15 12 00
15 16 00  =0536+145    04 24 31  45.5  26.7 -1.3       0.0   239      234   15 12 04

15 16 30  0528+134     04 25 01  47.4  24.3 -1.1       0.0    -1      234   15 16 30
15 18 30  ---          04 27 01  47.5  23.6 -1.1       0.0   119      242   15 16 34

15 19 00  J0539+1433   04 27 31  45.8  25.8 -1.2       0.0    -1      242   15 19 00
15 23 00  =0536+145    04 31 32  46.2  24.5 -1.1       0.0   239      257   15 19 04

15 23 30  0528+134     04 32 02  48.0  22.0 -1.0       0.0    -1      257   15 23 30
15 25 30  ---          04 34 03  48.1  21.3 -1.0       0.0   119      265   15 23 34

15 26 00  J0539+1433   04 34 33  46.5  23.5 -1.1       0.0    -1      265   15 26 00
15 30 00  =0536+145    04 38 33  46.8  22.2 -1.0       0.0   239      281   15 26 04

15 30 30  0528+134     04 39 03  48.5  19.5 -0.9       0.0    -1      281   15 30 30
15 32 30  ---          04 41 04  48.7  18.8 -0.8       0.0   119      288   15 30 34

15 33 00  J0539+1433   04 41 34  47.1  21.2 -1.0       0.0    -1      288   15 33 00
15 37 00  =0536+145    04 45 34  47.4  19.8 -0.9       0.0   239      304   15 33 04

15 37 30  0528+134     04 46 05  49.0  17.1 -0.8       0.0    -1      304   15 37 30
15 39 30  ---          04 48 05  49.2  16.3 -0.7       0.0   119      312   15 37 34

15 40 00  J0539+1433   04 48 35  47.6  18.8 -0.9       0.0    -1      312   15 40 00
15 44 00  =0536+145    04 52 36  47.9  17.4 -0.8       0.0   239      327   15 40 04

15 44 30  0528+134     04 53 06  49.5  14.5 -0.6       0.0    -1      327   15 44 30
15 46 30  ---          04 55 06  49.6  13.8 -0.6       0.0   119      335   15 44 34
Schedule for HART      (Code Hh )                                   Page   4
               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
----------------------------------------------------------------------------------------

 --- Mon  11 Mar 2013   Day  70 ---

15 47 00  J0539+1433   04 55 36  48.1  16.4 -0.7       0.0    -1      335   15 47 00
15 51 00  =0536+145    04 59 37  48.3  15.0 -0.7       0.0   239      350   15 47 04

15 53 00  0528+134     05 01 37  49.9  11.4 -0.5       0.0    89      350   15 53 00
16 00 00  ---          05 08 38  50.2   8.8 -0.4       0.0   420      377   15 53 04


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


 ======== Setup file: sess113.L512
   Matching groups in /aps3/sched10.2/catalogs/freq.dat:
     hh18cm          Values confirmed by E-mail Jonathan Quick 291100 (CR)

   Setup group:   11         Station: HART              Total bit rate:  512
   Format: MARK5B            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=   1510.00   1510.00   1510.00   1510.00   1510.00   1510.00   1510.00   1510.00
             1510.00   1510.00   1510.00   1510.00   1510.00   1510.00   1510.00   1510.00
   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 these setups were used.

   Frequency Set:   2  Setup file default.
   LO sum=   1634.49  1634.49  1634.49  1634.49  1650.49  1650.49  1650.49  1650.49
             1666.49  1666.49  1666.49  1666.49  1682.49  1682.49  1682.49  1682.49
   BBC fr=    124.49   124.49   124.49   124.49   140.49   140.49   140.49   140.49
              156.49   156.49   156.49   156.49   172.49   172.49   172.49   172.49
   Bandwd=      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
    Matching frequency sets:   2  13

   Track assignments are: 
    track1=   2,  4,  6,  8, 10, 12, 14, 16, 18, 20, 22, 24, 26, 28, 30, 32
    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)

   J0530+1331        05 28 06.759218   * 05 30 56.416749     05 31 42.227682       0.10
 * 0528+134          13 29 42.28877    * 13 31 55.14944      13 32 20.17821        0.10
   J0530+13          /aps3/sched10.2/catalogs/sources.vlba
                     rfc_2012b Petrov, 2012, unpublished 138123 observations
                        0.450 scan and     67.919 baseline hours in setup: sess113.L512
                     Frequency sets (dups not shown):   1  2  3  4  5  6  7  8  9 12 14 15 16 17 18

 * J0539+1433        05 36 51.361474   * 05 39 42.365992     05 40 28.584312       0.10
   0536+145          14 32 10.73036    * 14 33 45.56166      14 34 00.64915        0.10
   J0539+14          /aps3/sched10.2/catalogs/sources.vlba
                     rfc_2012b Petrov, 2012, unpublished 2596 observations
                        0.400 scan and     61.034 baseline hours in setup: sess113.L512
                     Frequency sets (dups not shown):   1  2  3  4  5  6  7  8  9 12 14 15 16 17 18

 * J0552+3754        05 48 52.231755   * 05 52 17.936920     05 53 13.622374       0.13
   0548+378          37 53 44.15048    * 37 54 25.28236      37 54 33.67474        0.11
                     /aps3/sched10.2/catalogs/sources.vlba
                     rfc_2012b Petrov, 2012, unpublished 889 observations
                        0.333 scan and     50.870 baseline hours in setup: sess113.L512
                     Frequency sets (dups not shown):   1  2  3  4  5  6  7  8  9 12 14 15 16 17 18

   J0555+3948        05 52 01.407174   * 05 55 30.805616     05 56 27.509602       0.13
   0552+398          39 48 21.94578    * 39 48 49.16493      39 48 54.38748        0.10
 * DA193             /aps3/sched10.2/catalogs/sources.vlba
   J0555+39          rfc_2012b Petrov, 2012, unpublished 376994 observations
                        0.442 scan and     67.488 baseline hours in setup: sess113.L512
                     Frequency sets (dups not shown):   1  2  3  4  5  6  7  8  9 12 14 15 16 17 18



  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) 
   0528+134            91.8
   J0539+1433          94.0
   J0552+3754          97.2
   DA193               97.8

  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 

