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It is the recommendation to use the mean
values
presented in the previous section to calibrate your data. However, if
it is desired to produce an individual FCF from the night of a
particular set of science observations, then the method is described
here.
- Reduce the selected calibration observation using the
dimmconfig_bright_compact.lis config file.
- Use PICARD's recipe SCUBA2_FCFNEFD on your reduced calibration
observation. This will produce information to the screen and a
logfile log.fcfnefd with the FCFs as mentioned above, and an NEFD
for the observation. PICARD by default uses fixed FCF's to
calculate the NEFD. (450μm: 400 Jy/beam/pW and 850μm: 500
Jy/beam/pW). If you wish to get an NEFD using the FCF calculated
for the individual calibrator you are reducing, add USEFCF=1 to
your parameter file.
- Take your selected FCF and multiply your map by it using KAPPA cmult.
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Up: Notes on Shared Risk Observing
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The SMURF SCUBA-2 SRO Data Reduction Cookbook
Starlink Cookbook 19
Edward Chapin, Jessica Dempsey, Tim Jenness, Douglas Scott, Holly Thomas & Remo Tilanus
3 August 2010
E-mail:starlink@jiscmail.ac.uk
Copyright © 2009-2010 University of British Columbia \
Copyright © 2009-2010 Science \& Technology Facilities Council