next up previous 537
Next: SCUBA-2 Simulator
Up: Detailed operation
Previous: Using the iterate method

Configuration parameters

Table [*] summarizes the configuration parameters available for the model components used by the DIMM (see also detailed comments in appendix [*]). The default values are shown in the third column.


Table: Default parameters for the DIMM configuration file
Parameter Definition Default Value
(keyword)
General Options
numiter Either give a positive number that equals the number of 5
iterations, or give a negative number that equals the maximum
number of iterations using chi squared ($\chi^2$) stopping criterion.
chitol $\chi^2$ tolerance, requires $NOI$ model component. If the $\chi^2$ $10^{-6}$
difference $<1\times10^{-6}$, then make the current iteration the
last iteration.
varmapmethod Method of estimating variance map. If equal to zero, then use the 1
spread of values from the time-series (i.e. the raw data). If equal
to 1, then it samples the variance of data that land in each output
map pixel.
maxlen If performing the iterations in memory, this is the maximum 0
length (seconds) for concatenated data. If equal to zero, then
attempt to concatenate entire continuous chunks.
modelorder Order in which to calculate DIMM model components. (com,gai,ext,
ast,flt,noi)
exportndf An option to export DIMM model components as NDF files. It 0 (do not
exports one file per model component, per subarray. Use this export as NDF
option to view the values in these files. Can also files)
specify list of components using modelorder syntax
Pre-processing Data Cleaning Options
pad Pad beginning and end of each chunk of data with this many samples 1000
apod Apodize data at start and end over this many samples 1000
zeropad Chooses how to pad - with zeros (1) or with artificial data (0) 0
order Remove baseline polynomial of this order (0 = remove mean) 0
badfrac If this fraction (or greater) of samples are bad, ignore entire bolometer 0.05
flagstat Ignore data while telescope moving slower than this (arcsec/sec) 2
dcthresh S/N threshold for detecting DC steps -
dcbox Sample length for measuring noise for DC step finder -
spikethresh S/N threshold for detecting spikes -
spikeiter iterations for spike $\sigma$-clipper (0=until convergence) 0
filt_edgehigh, Enter low- and high-pass frequency limits in hertz (Hz). -
filt_edgelow
filt_notchhigh, Enter a range of high frequencies for filt_notchhigh and a range -
filt_notchlow of low frequencies for filt_notchlow to apply notch filters.
Control Model Component Calculation
com.niter Number of clipping iterations to use when finding common mode values 1
com.nsigma Number of standard deviations at which to clip when finding common mode values 3
noi.spikethresh Additional despiking after each iteration, within the $NOI$ 10
calculation.
noi.spikeiter Additional despiking after each iteration, within the $NOI$ 0
calculation.
flt.filt_edgehigh, Iterative filtering using $FLT$ model (see flt_* above). 0.2
flt.filt_edgelow 20
flt.filt_notchhigh, -
flt.filt_notchlow -
ext.tausrc Source of opacity data: water vapour monitor (WVMRAW), WVMRAW
$\tau_\mathrm{CSO}$ (CSOTAU), or explicit value for filter (FILTERTAU).
ext.taumethod Airmass calculation: full (separate value for each detector each ADAPTIVE
timeslice), quick (single airmass all detectors each timeslice), or
adaptive (decide dynamically to use full or quick).
ext.csotau Value of zenith $\tau_\mathrm{CSO}$ if ext.tausrc=CSOTAU. -
ext.filtertau Value of zenith optical depth for filter if ext.tausrc=FILTERTAU -




next up previous 537
Next: SCUBA-2 Simulator
Up: Detailed operation
Previous: Using the iterate method

SMURF -- the Sub-Millimetre User Reduction Facility
Starlink User Note 258
Edward Chapin, Andrew G. Gibb, Tim Jenness, David S. Berry, Douglas Scott & Remo Tilanus
14th February 2013
E-mail:starlink@jiscmail.ac.uk

Copyright © 2012 University of British Columbia \& the Science \& Technology Facilities Council