  COVER INFORMATION 

 Station:    HART      (Code Hh ) 
 Experiment: Ftp test
 Exp. Code:  F13L1   


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:
 
 
 


COVER LETTER:


This is the schedule for the L-band ftp fringe-test on 08 March 2013
involving 9 antennas: Ef Wb Jb1 On25 Nt Tr Ur Sh Hh

The ftp test uses a standard setup
and consists of long integrations on a strong source
0234+285 - a standard fringe finder.

Four ftp tests are scheduled:
~11:09 UT (scan 2, 2 sec, 0234+285)
~11:30 UT (scan 4, 2 sec, 0234+285)
~11:51 UT (scan 6, 2 sec, 0234+285)
~11:51 UT (scan 8, 2 sec, 0234+285)

Please make sure that the autoftp is set up correctly.

Good luck with the session!

Ciriaco

Schedule for HART      (Code Hh )                                   Page   2
               Ftp test
  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   8 Mar 2013   Day  67 ---

 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

12 00 00  0234+285     00 56 09  30.0  25.9 -1.7       0.0     0        0   12 00 00
12 05 00  ---          01 01 10  30.5  24.8 -1.6       0.0   300       19   12 00 04

12 06 00  0234+285     01 02 10  30.6  24.6 -1.6       0.0    39       19   12 06 00
12 11 00  ---          01 07 11  31.0  23.4 -1.5       0.0   300       39   12 06 04

12 13 00  0234+285     01 09 11  31.2  22.9 -1.5       0.0    99       39   12 13 00
12 22 00  ---          01 18 13  31.9  20.8 -1.3       0.0   540       74   12 13 04

12 24 00  0234+285     01 20 13  32.1  20.3 -1.3       0.0    99       74   12 24 00
12 33 00  ---          01 29 15  32.8  18.1 -1.2       0.0   540      108   12 24 04

12 34 00  0234+285     01 30 15  32.8  17.9 -1.1       0.0    39      108   12 34 00
12 39 00  ---          01 35 16  33.2  16.6 -1.1       0.0   300      128   12 34 04

12 41 00  0234+285     01 37 16  33.3  16.1 -1.0       0.0    99      128   12 41 00
12 50 00  ---          01 46 17  33.8  13.8 -0.9       0.0   540      163   12 41 04

12 52 00  0234+285     01 48 18  33.9  13.3 -0.8       0.0    99      163   12 52 00
13 01 00  ---          01 57 19  34.4  11.0 -0.7       0.0   540      197   12 52 04

13 02 00  0234+285     01 58 19  34.4  10.7 -0.7       0.0    39      197   13 02 00
13 07 00  ---          02 03 20  34.6   9.4 -0.6       0.0   300      217   13 02 04

13 09 00  0234+285     02 05 20  34.7   8.9 -0.6       0.0    99      217   13 09 00
13 18 00  ---          02 14 22  34.9   6.5 -0.4       0.0   540      252   13 09 04

13 20 00  0234+285     02 16 22  35.0   6.0 -0.4       0.0    99      252   13 20 00
13 29 00  ---          02 25 24  35.2   3.6 -0.2       0.0   540      286   13 20 04

13 30 00  0234+285     02 26 24  35.2   3.3 -0.2       0.0    39      286   13 30 00
13 35 00  ---          02 31 25  35.2   1.9 -0.1       0.0   300      306   13 30 04

13 37 00  0234+285     02 33 25  35.2   1.4 -0.1       0.0    99      306   13 37 00
13 46 00  ---          02 42 27  35.2 359.0  0.1       0.0   540      341   13 37 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:    6         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   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 --                         Ftp test
     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)

   J0237+2848        02 34 55.589591   * 02 37 52.405678     02 38 39.421291       0.11
 * 0234+285          28 35 11.40773    * 28 48 08.98998      28 51 34.00276        0.10
   J0237+28          /aps3/sched10.2/catalogs/sources.vlba
                     rfc_2012b Petrov, 2012, unpublished 56811 observations
                        1.467 scan and    133.467 baseline hours in setup: sess113.L512
                     Frequency sets (dups not shown):   1  2  3  4  5  6  7  9 10 11 12 13 14



  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) 
   0234+285            59.0

  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 

