The experiment is a standard style observation of the 12.2 GHz
methanol maser 335.79+0.17, so it is long scans on the program 
source, with a fringe finder scans every few hours.

Schedules for v034b2 are available via anonymous FTP in 
ftp://kerr.phys.utas.edu.au/vlbobs/incoming.  There is an
SCHED command file and catalogue for AT/Mopra (untested) and
snap/procedure files for Hobart (ho), Parkes (pk) and Hart (hh).

Times : 1999 353/2300 - 354/0830 Hobart, AT, Mopra
             353/2300 - 354/0600 Parkes
             354/0230 - 354/0830 Hart
Sky frequency : 12179-12183 MHz (4 MHz, 12181.0 Centre frequency)
DAS : profile = mp4s_f.pro (for non-inverted input at 96 MHz)
             or at4s_n.pro
      jumper = IN! (except Hart)
S2 mode : 8x4-2 (2 tapes recording), LP (Everywhere except Hart)
          8x2-2 (1 tape recording), LP (Hart)
Polarization : RCP,LCP (Hart LCP only)
Tapes : 3x2, (Hart 2x1)
        Only recording in LP, so can use Maxwell.
        group 0 : 353/2300 - 354/0300
        group 1 : 354/0300 - 354/0700
        group 2 : 354/0700 - 354/0830
Schedules : v034b2.snp - PCFS snap file
            v034b2.com - A command file for SCHED (untested)
            v034b.cat  - A catalogue file for SCHED (format might not
                         be quite right).
 
Please don't make system temperature measurements more frequently 
than once every half hour, except if it doesn't interfer with the 
recorded data.  Amplitude calibration can be done more accurately 
from the autocorrelations on the maser source anyway.
 
Observations of 3C273B, 1549-790 and 1921-293 have been included for 
fringe finding - if problems occur, please try and ensure that your
antenna participates in at least one of these scans.

If there are any problems with the schedule call me (Simon) at
Ceduna (08 8624 1501)