  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: NME and FTP Fringe Test at S/X band in Session 1/2011
 Exp. Code:  N11SX1  


Schedule Version:       1.00
Processed by SCHED version:   9.30  Release near March 23, 2010

PI:       Jun Yang

Address:  JIVE
          Postbus 2
          7990AA Dwingeloo
          The Netherlands

Phone:    +31-521-596507
EMAIL:    yang@jive.nl
Fax:
Phone during observation:

Observing mode: 3.6/13 cm, 512-16-2

Notes:    Only RCP, 512 Mbps, 8 BBCs (USB & LSB), 2-bit sampling.
          Check autoftp settings and pointing, please
          On, Hh, and Mc request a mixed BBC patching.
 


COVER LETTER:


Dear EVN friends,

This is the schedule file for N11SX1. Four ftp scans are
scheduled in N11SX1.

(1) 12h07m UT, 2 second, 128 MB data, source 3C454.3
(2) 13h07m UT, 2 second, 128 MB data, source 3C454.3
(3) 13h59m UT, 2 second, 128 MB data, source DA193
(4) 14h59m UT, 2 second, 128 MB data, source DA193

The Kunming 40m radio telescope will participate in the NME and
the last two ftp-fringe tests to test its Mark4 backend.

Good Luck!

Jun Yang
skype account: uaoagn

Schedule for HART      (Code Hh )                                   Page   2
               NME and FTP Fringe Test at S/X band in Session 1/2011
  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  15 Mar 2011   Day  74 ---

 Next scan frequencies:  2234.99  2234.99  2250.99  2250.99  2266.99  2266.99
                         2282.99  2282.99  8384.99  8384.99  8400.99  8400.99
                         8416.99  8416.99  8432.99  8432.99
 Next BBC frequencies:    214.99   214.99   230.99   230.99   246.99   246.99
                          262.99   262.99   304.99   304.99   320.99   320.99
                          336.99   336.99   352.99   352.99
 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  3C454.3      01 21 43  34.7 315.6  2.5       0.0     0   1  1      0  12 00 00
12 08 00  ---          01 29 44  33.5 313.8  2.6       0.0   480   F  1     31  12 00 04

12 10 00  3C454.3      01 31 45  33.1 313.4  2.6       0.0    95   1  1     31  12 10 00
12 18 00  ---          01 39 46  31.8 311.8  2.8       0.0   480   F  1     62  12 10 04

12 20 00  3C454.3      01 41 46  31.5 311.4  2.8       0.0    95   1  1     62  12 20 00
12 28 00  ---          01 49 48  30.1 309.8  2.9       0.0   480   F  1     93  12 20 04

12 30 00  3C454.3      01 51 48  29.7 309.4  3.0       0.0    95   1  1     93  12 30 00
12 38 00  ---          01 59 49  28.3 307.9  3.1       0.0   480   F  1    124  12 30 04

12 40 00  3C454.3      02 01 50  28.0 307.5  3.1       0.0    95   1  1    124  12 40 00
12 48 00  ---          02 09 51  26.5 306.1  3.3       0.0   480   F  1    155  12 40 04

12 50 00  3C454.3      02 11 51  26.2 305.7  3.3       0.0    95   1  1    155  12 50 00
12 58 00  ---          02 19 53  24.7 304.4  3.4       0.0   480   F  1    186  12 50 04

13 00 00  3C454.3      02 21 53  24.3 304.0  3.5       0.0    95   1  1    186  13 00 00
13 08 00  ---          02 29 54  22.8 302.7  3.6       0.0   480   F  1    217  13 00 04

13 12 00  DA193        02 33 55   9.1  37.0 -3.4       0.0     4   1  1    217  13 12 00
13 20 00  ---          02 41 56  10.2  35.8 -3.2       0.0   480   F  1    248  13 12 04

13 22 00  DA193        02 43 57  10.5  35.5 -3.2       0.0    95   1  1    248  13 22 00
13 30 00  ---          02 51 58  11.5  34.4 -3.1       0.0   480   F  1    279  13 22 04

13 32 00  DA193        02 53 58  11.8  34.1 -3.0       0.0    95   1  1    279  13 32 00
13 40 00  ---          03 01 59  12.8  32.9 -2.9       0.0   480   F  1    310  13 32 04

13 42 00  DA193        03 04 00  13.0  32.6 -2.9       0.0    95   1  1    310  13 42 00
13 50 00  ---          03 12 01  14.0  31.3 -2.7       0.0   480   F  1    341  13 42 04
Schedule for HART      (Code Hh )                                   Page   3
               NME and FTP Fringe Test at S/X band in Session 1/2011
  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  15 Mar 2011   Day  74 ---

13 52 00  DA193        03 14 01  14.2  31.0 -2.7       0.0    95   1  1    341  13 52 00
14 00 00  ---          03 22 03  15.1  29.7 -2.6       0.0   480   F  1    372  13 52 04

14 02 00  DA193        03 24 03  15.3  29.4 -2.5       0.0    95   1  1    372  14 02 00
14 10 00  ---          03 32 04  16.2  28.1 -2.4       0.0   480   F  1    403  14 02 04

14 12 00  DA193        03 34 05  16.4  27.8 -2.4       0.0    95   1  1    403  14 12 00
14 20 00  ---          03 42 06  17.2  26.4 -2.2       0.0   480   F  1    434  14 12 04

14 22 00  DA193        03 44 06  17.4  26.0 -2.2       0.0    95   1  1    434  14 22 00
14 30 00  ---          03 52 08  18.2  24.6 -2.1       0.0   480   F  1    464  14 22 04

14 32 00  DA193        03 54 08  18.4  24.3 -2.0       0.0    95   1  1    464  14 32 00
14 40 00  ---          04 02 09  19.1  22.9 -1.9       0.0   480   F  1    495  14 32 04

14 42 00  DA193        04 04 10  19.3  22.5 -1.9       0.0    95   1  1    495  14 42 00
14 50 00  ---          04 12 11  20.0  21.0 -1.7       0.0   480   F  1    526  14 42 04

14 52 00  DA193        04 14 11  20.1  20.6 -1.7       0.0    95   1  1    526  14 52 00
15 00 00  ---          04 22 13  20.7  19.1 -1.6       0.0   480   F  1    557  14 52 04


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


 Setup file: n11sx1.set
   Matching groups in ./n11sx1_freq.dat:
     hhsx            Values confirmed by E-mail Jonathan Quick 291100 (CR)

   Setup group:    4         Station: HART              Total bit rate:  512
   Format: MKIV1:2           Bits per sample: 2         Sample rate: 16.000
   Number of channels: 16                               Speedup factor:   1.00

   Disk used to record data.

   1st LO=   2020.00   2020.00   2020.00   2020.00   2020.00   2020.00   2020.00   2020.00
             8080.00   8080.00   8080.00   8080.00   8080.00   8080.00   8080.00   8080.00
   Net SB=         L         U         L         U         L         U         L         U
                   L         U         L         U         L         U         L         U
   Pol.  =      RCP       RCP       RCP       RCP       RCP       RCP       RCP       RCP 
                RCP       RCP       RCP       RCP       RCP       RCP       RCP       RCP 
   BBC   =         2         2         4         4         6         6         8         8
                   1         1         3         3         5         5         7         7
   BBC SB=         L         U         L         U         L         U         L         U
                   L         U         L         U         L         U         L         U
   IF    =        2N        2N        2N        2N        2N        2N        2N        2N
                  1N        1N        1N        1N        1N        1N        1N        1N

  The following frequency sets based on this setup were used.

   Frequency Set:   3  Setup file default.
   LO sum=    2234.99   2234.99   2250.99   2250.99   2266.99   2266.99   2282.99   2282.99
              8384.99   8384.99   8400.99   8400.99   8416.99   8416.99   8432.99   8432.99
   BBC fr=     214.99    214.99    230.99    230.99    246.99    246.99    262.99    262.99
               304.99    304.99    320.99    320.99    336.99    336.99    352.99    352.99
   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 
 SOURCE LIST -- NME and FTP Fringe Test at S/X band in Session 1/2011
     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)

   J0555+3948        05 52 01.407172   * 05 55 30.805615     05 56 19.370758       0.01
   0552+398          39 48 21.94585    * 39 48 49.16500      39 48 59.45360        0.01
 * DA193             /aps3/sched9.3/catalogs/sources.vlba
   J0555+39          GSFC Nov. 2009 Solution 2009a    348030 Observations
                        1.467 scan hours,     30.295 baseline hours above horizon.

   J2253+1608        22 51 29.519743   * 22 53 57.747942     22 54 30.705501       0.01
 * 3C454.3           15 52 54.34806    * 16 08 53.56089      16 12 26.86945        0.01
   2251+158          /aps3/sched9.3/catalogs/sources.vlba
   J2253+16          GSFC Nov. 2009 Solution 2009a     39040 Observations
                        0.933 scan hours,     14.000 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) 
   DA193               94.5
   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 

