  COVER INFORMATION 

 Station:    URUMQI    (Code Ur ) 
 Experiment: K band NME+FTP-FT Experiment N12K1
 Exp. Code:  N12K1   


Schedule Version:       1.00
Processed by SCHED version:  10.00  Release Sept. 15, 2011

PI:       Jun YANG

Address:  JIVE, The Netherlands
 
 
 

Phone:    +31 521 596 507
EMAIL:    yang@jive.nl
Fax:
Phone during observation:

Observing mode: 512-16-2

Notes:    512 Mbps, 16 x 8 MHz, 2 bit sampling
          Check antenna pointing, Please
          Three FTP-FT scans scheduled.
          Skype group chat will be iniated

Schedule for URUMQI    (Code Ur )                                   Page   2
               K band NME+FTP-FT Experiment N12K1
  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
----------------------------------------------------------------------------------------

 --- Wed  29 Feb 2012   Day  60 ---

 Next scan frequencies: 22211.49 22211.49 22211.49 22211.49 22227.49 22227.49
                        22227.49 22227.49 22243.49 22243.49 22243.49 22243.49
                        22259.49 22259.49 22259.49 22259.49
 Next BBC frequencies:    211.49   211.49   211.49   211.49   227.49   227.49
                          227.49   227.49   243.49   243.49   243.49   243.49
                          259.49   259.49   259.49   259.49
 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

12 30 00  3C84         04 53 37  72.8 271.6  1.5      75.8     0        0   12 30 00
12 38 00  ---          05 01 38  71.4 272.8  1.7      75.6   480       31   12 30 01

12 42 00  3C84         05 05 39  70.6 273.4  1.8      75.5   238       31   12 42 00
12 50 00  ---          05 13 40  69.2 274.5  1.9      75.2   480       62   12 42 01

12 52 00  3C84         05 15 41  68.8 274.8  1.9      75.1   118       62   12 52 00
13 00 00  ---          05 23 42  67.4 275.8  2.1      74.8   480       93   12 52 01

13 02 00  3C84         05 25 42  67.0 276.1  2.1      74.7   118       93   13 02 00
13 10 00  ---          05 33 44  65.6 277.1  2.2      74.2   480      124   13 02 01

13 12 00  3C84         05 35 44  65.2 277.3  2.3      74.1   118      124   13 12 00
13 20 00  ---          05 43 45  63.8 278.3  2.4      73.7   480      155   13 12 01

13 22 00  3C84         05 45 46  63.4 278.5  2.4      73.6   118      155   13 22 00
13 30 00  ---          05 53 47  62.0 279.5  2.6      73.1   480      186   13 22 01

13 32 00  0528+134     05 55 47  59.6 191.7  0.4       8.7    28      186   13 32 00
13 40 00  ---          06 03 49  59.3 195.4  0.5      11.5   480      217   13 32 01

13 42 00  0528+134     06 05 49  59.2 196.4  0.6      12.1   118      217   13 42 00
13 50 00  ---          06 13 50  58.7 200.0  0.7      14.8   480      248   13 42 01

13 52 00  0528+134     06 15 51  58.6 201.0  0.7      15.5   118      248   13 52 00
14 00 00  ---          06 23 52  58.0 204.5  0.9      18.0   480      279   13 52 01

14 02 00  0528+134     06 25 52  57.9 205.4  0.9      18.7   118      279   14 02 00
14 10 00  ---          06 33 54  57.2 208.8  1.0      21.1   480      310   14 02 01

14 12 00  0528+134     06 35 54  57.0 209.6  1.1      21.7   118      310   14 12 00
14 20 00  ---          06 43 55  56.3 212.9  1.2      23.9   480      341   14 12 01
Schedule for URUMQI    (Code Ur )                                   Page   3
               K band NME+FTP-FT Experiment N12K1
  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
----------------------------------------------------------------------------------------

 --- Wed  29 Feb 2012   Day  60 ---

14 22 00  0528+134     06 45 56  56.1 213.7  1.2      24.5   118      341   14 22 00
14 30 00  ---          06 53 57  55.2 216.8  1.4      26.6   480      372   14 22 01

14 32 00  0528+134     06 55 57  55.0 217.6  1.4      27.1   118      372   14 32 00
14 40 00  ---          07 03 59  54.1 220.6  1.5      29.0   480      403   14 32 01

14 42 00  0528+134     07 05 59  53.9 221.3  1.6      29.5   118      403   14 42 00
14 50 00  ---          07 14 00  52.9 224.1  1.7      31.3   480      434   14 42 01

14 52 00  0528+134     07 16 01  52.6 224.8  1.7      31.7   118      434   14 52 00
15 00 00  ---          07 24 02  51.6 227.5  1.9      33.4   480      464   14 52 01

15 02 00  0528+134     07 26 02  51.3 228.1  1.9      33.8   118      464   15 02 00
15 10 00  ---          07 34 03  50.2 230.6  2.0      35.3   480      495   15 02 01

15 12 00  0528+134     07 36 04  49.9 231.3  2.1      35.6   118      495   15 12 00
15 20 00  ---          07 44 05  48.8 233.7  2.2      37.0   480      526   15 12 01

15 22 00  0528+134     07 46 05  48.5 234.3  2.2      37.3   118      526   15 22 00
15 30 00  ---          07 54 07  47.3 236.6  2.4      38.5   480      557   15 22 01


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


 Setup file: sess112.K512
   Matching groups in /aps3/sched10.0/catalogs/freq.dat:
     ur1cmd          Dummy dual-pol entry, only LCP available (CR 2Jul02).

   Setup group:    9         Station: URUMQI            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=  22000.00  22000.00  22000.00  22000.00  22000.00  22000.00  22000.00  22000.00
            22000.00  22000.00  22000.00  22000.00  22000.00  22000.00  22000.00  22000.00
   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:   8  Setup file default.
   LO sum=   22211.49  22211.49  22211.49  22211.49  22227.49  22227.49  22227.49  22227.49
             22243.49  22243.49  22243.49  22243.49  22259.49  22259.49  22259.49  22259.49
   BBC fr=     211.49    211.49    211.49    211.49    227.49    227.49    227.49    227.49
               243.49    243.49    243.49    243.49    259.49    259.49    259.49    259.49
   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
    Matching frequency sets:   8

   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 --                         K band NME+FTP-FT Experiment N12K1
     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)

   J0319+4130        03 16 29.567258   * 03 19 48.160088     03 20 37.528179       1.66
   0316+413          41 19 51.91695    * 41 30 42.10408      41 33 27.24171        2.78
 * 3C84              /aps3/sched10.0/catalogs/sources.vlba
   J0319+41          GSFC 2010a astro solution     10264 Observations
                        0.800 scan and     40.000 baseline hours in setup: sess112.K512
                     Frequency sets (dups not shown):   1  2  3  4  5  6  8  9 10 11

   J0530+1331        05 28 06.759216   * 05 30 56.416747     05 31 39.196033       0.21
 * 0528+134          13 29 42.28887    * 13 31 55.14954      13 32 20.59559        0.23
   J0530+13          /aps3/sched10.0/catalogs/sources.vlba
                     GSFC 2010a astro solution    133158 Observations
                        1.600 scan and     87.265 baseline hours in setup: sess112.K512
                     Frequency sets (dups not shown):   1  2  3  4  5  6  8  9 10 11



  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) 
   3C84                79.3
   0528+134           102.4

  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 

