Dept of Astrophysics
University of NSW
Sydney
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Biomolecules Project

Frequencies, schedule files and procedures for the Biomolecules project.

Observing Procedure

For an operations overview in a checklist format see the observing procedure page.

  • If something doesn't work and you can't fix it, give Maria a ring on either 02 9315 0745 or 0417 257294 in order to fix the problem quickly.
  • Observe either Sgr B2 or Orion for the Project.
  • Perform a pointing every 2 hours or so, depending on conditions.
  • The Biomolecules project is more concerned by long integration times than accurate calibration, so frequent Tsys measurements are not necessary, as in the Hot Cores project. Use your discression and your knowledge of the weather conditions. Every time you change source should be fine.
  • If the weather is good set integration times up to 2 hours (large number of repeats).
  • Total Observation time = (Cycles + 1) X 10s X Scans in Set X Repeats
  • Don't forget to close the data file after each source!

Lines and Frequencies

Lines to be observed, listed in order of priority.

Line Frequency Tuner 
(GHz)
Frequency 
TCS GUI (MHz)
Comments
Glycine II 100.332387 100332.387 Priority 1
Glycine II 92.881429 92881.429 Priority 2
Prop Oxide 98.66208 98662.08 Priority 3

Glycine I

95.990004 95990.004 Priority 4
Prop Oxide 88.348460 88348.460 Priority 5
SiO maser 86.243442 86243.442 Maser Pointing Frequency- for reference only.

Note: These lines are not preset in the tuner GUI. When choosing a line from the rest frequency box choose 'other'. Enter in one of the frequencies given above in the 'f sky' box and click the 'Set LO Frequency' button. Tune as normal (see the tuning guide).

Source Catalogs

Catalog files in a format readable by TCS

Catalog File Directory on Warrum Comment
maria.2003 /c/observer/unsw_bio/ Source list for the Biomolecules Project
Point_SiO /c/observer/unsw_bio/ Pointing sources used for the Hot Core Project

The file contains the following columns: name, ra, dec, J2000, vlsr, delimited by spaces.

Name RA DEC System VLSR
Orion 05:35:14.5 -05:22:29.6 J2000 +5.0
Sgr B2 17:47:19.8 -28:22:17.0 J2000 +65.0

These sources rise after the Hot Core sources set, so plan who is going to observe when well in advance!

Directories

Useful directories to know.

Directory Computer Use
/c/data/MPCCC_1/corr/dat/ Warrum Raw .RPF data files files are written here. Crosslinked between mpccc and warrum.
obs$0:[multi.sched] Mopra Schedule files. Use 'schedput' to ftp over new files.
/c/observer/users/ Warrum User Directories
/c/observer/unsw_bio/ Warrum Biomolecules directory
obs$0:[multi.point] Mopra sio_point looks for raw .RPF files in this directory

Schedule Files

The number of times to repeats the schedule file is not included within the schedule file for flexability reasons. Always remember to set the "repeats" box in the TCS GUI  to the value indicated below.

Schedule Correlator Config Cycles
Scans
Repeats Mode Ref Posn Use
pnt_test2 ac_64_1024_2f 2 / 6 1
5pt cross +15m lat quick pointing
pnt_test3 ac_64_1024_2f 3 / 6
1 5pt cross +15m lat more sensitive pointing

maria_bio

ac_64_1024_2 12 / 3 Set Manually
OFF-ON- OFF +1d long Biomolecules survey

Total Observation time = (Cycles + 1) X 10s X Scans in Set X Repeats

Logs

Keep the log-book up to date each observing run recording:

  • Universal Tme
  • Source name
  • RPF file name
  • Detection?
  • System Temperature (Tsys)
  • Pointing corrections (delat fx and delta fz, calculated by sio_point) and total offsets (given in camon).
  • Weather conditions

Before leaving Mopra don't forget to photocopy the log to bring back to UNSW.

Data & Reduction

The lines we are looking for here are very weak so don't expect to see anything on SPD or DFM. If you do they will probably be adjacent lines.

  • At the end of the observing run write all data to a CD-ROM and backup your data to MINOS.

Page created by Cormac Purcell and maintained by Nadia Lo. If you have any comments and suggestions, please direct your email to nlo@phys.unsw.edu.au.