flag 1,2,5,6,9,11,13,14,15,16,17,20,21,22

# Specify the directory where the raw data files are to be found
datapath ~/data/saboca

# Specify the project-id (case sensitive!)
project T-081.F-0001-2008

# Give the conversion factor from uV to Jy that is to be used. In this case
# 1 mV = 5.55 Jy +- 1.2% (~5% rms on integrated Uranus) 6.40 Jy +- 1.3%
# This is the convesion factor for using aperture fluxes.
# For peak fluxes, use the factor found in 'deep.cfg' here...
jansky 5.55e-3

# The stability time-scale of the detectors in seconds (1 / 2fc).
stability 30.0

# A value by which taus obtained from skydip data (laboca-taus-master.dat)
# ought to be multiplied.
#skydipfactor 1.00

# Specify the units in which the ouput map should be written. Use 'uV/beam'
# to get uncalibrated data in detector voltage units, or 'Jy/beam' to write
# calibrated data, with the calibration factor defined via the 'jansky' option
# above
unit Jy/beam

# Set the instrument beam FWHM in arcsec
beam 7.5

# Set the map grid at 1/5 beam, i.e. ~1.5 arcsec
grid 1.5

# Clip data where the scan velocity on the field is below 100.0 "/s.
vclip 5.0 100.0

# Clip data where the telescope acceleration exceeds 8'/s^2.
aclip 480.0

# Smooth source maps to 4". This is not necessarily the smoothing of the 
# final map, but it is aimed at creating some redundancy in the data, by
# coupling nearby map positions.
#smooth 4.0

# Use He3 temperatures to correct data from 'thermistor' or 'blinds'
#He3 blinds

# Decorrelate on the squid amplifiers 
#amps

# Smooth the final map by a 4" FWHM Gaussian.
#iteration:last smooth 4.0

# Only make maps from the scans, in the advanced iterations, if the NEFD is 
# within the specified range (in units of 'Jy sqrt(s)')
#iteration:last-2 nefd-range 0.035--0.150

# options for 'extended' reduction mode
#extendedopt forget amps
#extendedopt iteration.4 amps

