  COVER INFORMATION 

 Station:    SHANGHAI  (Code Sh ) 
 Experiment: Network Monitoring Experiment
 Exp. Code:  N13L2   


Schedule Version:       1.00
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 2/2013
          512 Mbps, 2-bit sampling, 8 MHz filters
          Send the disk pack by express to JIVE
          DBBC testing data from On, Hh, Nt, Mc, Tr, Jb are expected.


COVER LETTER:


Dear EVN friends,

This is the schedule for the 18cm NME on June 7 2013,
involving 13 antennas: Eb Wb Jb1 On25 Mc Nt Tr Sv Zc Bd Ur Sh Hh.
The NME uses a standard setup with 512 Mbps and consists of
2 phase-referencing cycles on strong calibrators (DA193
 and 0528+134) with continuum sources as targets (J0552+3754 and J0539+1433).

*No* ftp tests are scheduled (the NME comes after all the user experiments in L-band).

Ciriaco

Schedule for SHANGHAI  (Code Sh )                                   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
----------------------------------------------------------------------------------------

 --- Fri   7 Jun 2013   Day 158 ---

 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:    665.51   665.51   665.51   665.51   649.51   649.51   649.51   649.51
                          633.51   633.51   633.51   633.51   617.51   617.51   617.51   617.51
 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

06 00 00  DA193        07 08 00  73.1 -54.1  1.2     115.4     0        0   06 00 00
06 02 00  ---          07 10 00  72.7 -54.7  1.2     114.6   120        8   06 00 01

06 03 00  J0552+3754   07 11 00  72.6 -61.6  1.3     107.2    49        8   06 03 00
06 09 00  =0548+378    07 17 01  71.5 -62.7  1.4     105.3   360       31   06 03 01

06 10 00  DA193        07 18 02  71.3 -56.6  1.4     111.4    50       31   06 10 00
06 12 00  ---          07 20 02  70.9 -57.0  1.4     110.7   120       39   06 10 01

06 13 00  J0552+3754   07 21 02  70.7 -63.3  1.5     104.1    50       39   06 13 00
06 19 00  =0548+378    07 27 03  69.6 -64.1  1.6     102.4   360       62   06 13 01

06 20 00  DA193        07 28 03  69.5 -58.6  1.5     108.0    50       62   06 20 00
06 22 00  ---          07 30 04  69.1 -58.9  1.6     107.4   120       70   06 20 01

06 23 00  J0552+3754   07 31 04  68.8 -64.6  1.6     101.4    50       70   06 23 00
06 29 00  =0548+378    07 37 05  67.6 -65.2  1.7      99.9   360       93   06 23 01

06 30 00  DA193        07 38 05  67.6 -60.1  1.7     105.0    51       93   06 30 00
06 32 00  ---          07 40 05  67.3 -60.3  1.7     104.4   120      101   06 30 01

06 33 00  J0552+3754   07 41 05  66.8 -65.5  1.8      99.0    51      101   06 33 00
06 39 00  =0548+378    07 47 06  65.7 -66.0  1.9      97.7   360      124   06 33 01

06 40 00  DA193        07 48 07  65.8 -61.2  1.9     102.3    51      124   06 40 00
06 42 00  ---          07 50 07  65.4 -61.4  1.9     101.8   120      132   06 40 01

06 43 00  J0552+3754   07 51 07  64.9 -66.2  2.0      96.8    51      132   06 43 00
06 49 00  =0548+378    07 57 08  63.7 -66.5  2.1      95.6   360      155   06 43 01

06 50 00  DA193        07 58 08  63.9 -62.1  2.0      99.9    52      155   06 50 00
06 52 00  ---          08 00 09  63.5 -62.2  2.1      99.5   120      163   06 50 01

06 53 00  J0552+3754   08 01 09  62.9 -66.6  2.1      94.9    52      163   06 53 00
06 59 00  =0548+378    08 07 10  61.7 -66.8  2.2      93.8   360      186   06 53 01

07 00 00  DA193        08 08 10  62.0 -62.7  2.2      97.8    52      186   07 00 00
07 02 00  ---          08 10 10  61.6 -62.8  2.2      97.3   120      194   07 00 01
Schedule for SHANGHAI  (Code Sh )                                   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
----------------------------------------------------------------------------------------

 --- Fri   7 Jun 2013   Day 158 ---

07 05 00  0528+134     08 13 11  49.0 253.9  2.7      57.8  -141      194   07 05 00
07 07 30  ---          08 15 41  48.5 254.4  2.7      58.0     9      203   07 05 01

07 08 30  J0539+1433   08 16 41  50.7 254.2  2.6      58.3    52      203   07 08 30
07 14 30  =0536+145    08 22 42  49.4 255.4  2.7      58.9   360      226   07 08 31

07 15 30  0528+134     08 23 42  46.9 255.9  2.9      58.7    52      226   07 15 30
07 18 00  ---          08 26 13  46.3 256.3  2.9      58.9   150      236   07 15 31

07 19 00  J0539+1433   08 27 13  48.5 256.2  2.8      59.2    52      236   07 19 00
07 25 00  =0536+145    08 33 14  47.2 257.3  2.9      59.7   360      259   07 19 01

07 26 00  0528+134     08 34 14  44.7 257.8  3.0      59.4    52      259   07 26 00
07 28 30  ---          08 36 45  44.1 258.2  3.1      59.6   150      269   07 26 01

07 29 30  J0539+1433   08 37 45  46.3 258.1  3.0      60.0    52      269   07 29 30
07 35 30  =0536+145    08 43 46  45.0 259.2  3.1      60.3   360      292   07 29 31

07 36 30  0528+134     08 44 46  42.5 259.6  3.2      60.0    52      292   07 36 30
07 39 00  ---          08 47 16  41.9 260.0  3.3      60.1   150      302   07 36 31

07 40 00  J0539+1433   08 48 16  44.1 259.9  3.1      60.6    52      302   07 40 00
07 46 00  =0536+145    08 54 17  42.8 260.9  3.2      60.9   360      325   07 40 01

07 47 00  0528+134     08 55 18  40.2 261.2  3.4      60.5    52      325   07 47 00
07 49 30  ---          08 57 48  39.7 261.6  3.4      60.6   150      335   07 47 01

07 50 30  J0539+1433   08 58 48  41.9 261.6  3.3      61.1    52      335   07 50 30
07 56 30  =0536+145    09 04 49  40.6 262.5  3.4      61.3   360      358   07 50 31

07 57 30  0528+134     09 05 49  38.0 262.9  3.6      60.9    52      358   07 57 30
08 00 00  ---          09 08 20  37.5 263.2  3.6      61.0   150      368   07 57 31


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


 ======== Setup file: sess213.L512
   Matching groups in /aps3/sched10.2/catalogs/freq.dat:
     sh18cm          Huang Xinyong 27Sept05

   Setup group:   10         Station: SHANGHAI          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=   2300.00   2300.00   2300.00   2300.00   2300.00   2300.00   2300.00   2300.00
             2300.00   2300.00   2300.00   2300.00   2300.00   2300.00   2300.00   2300.00
   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   =         1         2         1         2         3         4         3         4
                   5         6         5         6         7         8         7         8
   BBC SB=         U         U         L         L         U         U         L         L
                   U         U         L         L         U         U         L         L
   IF    =        C         A         C         A         C         A         C         A 
                  C         A         C         A         C         A         C         A 

  The following frequency sets based on these setups were used.

   Frequency Set:  11  Setup file default.  Used pcal sets:   1
   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=    665.51   665.51   665.51   665.51   649.51   649.51   649.51   649.51
              633.51   633.51   633.51   633.51   617.51   617.51   617.51   617.51
   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:  11

  The following pulse cal sets were used with this setup:

   Pulse cal detection set:   1  PCAL = 1MHZ
    PCALXB1=   S1    S3    S5    S7    S9    S11   S13   S15
    PCALXB2=   S2    S4    S6    S8    S10   S12   S14   S16
    PCALFR1=   490   510   490   510   490   510   490   510
    PCALFR2=   490   510   490   510   490   510   490   510

   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 41.442909       0.10
 * 0528+134          13 29 42.28877    * 13 31 55.14944      13 32 20.90681        0.10
   J0530+13          /aps3/sched10.2/catalogs/sources.vlba
                     rfc_2012b Petrov, 2012, unpublished 138123 observations
                        0.250 scan and     42.044 baseline hours in setup: sess213.L512
                     Frequency sets (dups not shown):   1  2  3  4  5  6  7  8 11 12 13 14 15 16 17 19

 * J0539+1433        05 36 51.361474   * 05 39 42.365992     05 40 27.753893       0.10
   0536+145          14 32 10.73036    * 14 33 45.56166      14 34 01.11238        0.10
   J0539+14          /aps3/sched10.2/catalogs/sources.vlba
                     rfc_2012b Petrov, 2012, unpublished 2596 observations
                        0.500 scan and     85.500 baseline hours in setup: sess213.L512
                     Frequency sets (dups not shown):   1  2  3  4  5  6  7  8 11 12 13 14 15 16 17 19

 * J0552+3754        05 48 52.231755   * 05 52 17.936920     05 53 12.513332       0.13
   0548+378          37 53 44.15048    * 37 54 25.28236      37 54 27.74959        0.11
                     /aps3/sched10.2/catalogs/sources.vlba
                     rfc_2012b Petrov, 2012, unpublished 889 observations
                        0.600 scan and     76.800 baseline hours in setup: sess213.L512
                     Frequency sets (dups not shown):   1  2  3  4  5  6  7  8 11 12 13 14 15 16 17

   J0555+3948        05 52 01.407174   * 05 55 30.805616     05 56 26.343500       0.13
   0552+398          39 48 21.94578    * 39 48 49.16493      39 48 48.09541        0.10
 * DA193             /aps3/sched10.2/catalogs/sources.vlba
   J0555+39          rfc_2012b Petrov, 2012, unpublished 376994 observations
                        0.233 scan and     30.133 baseline hours in setup: sess213.L512
                     Frequency sets (dups not shown):   1  2  3  4  5  6  7  8 11 12 13 14 15 16 17



  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            11.6
   J0539+1433          12.2
   J0552+3754          18.7
   DA193               20.5

  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 

