Specifies which models to include in the iterative process, and the order in which
they are evaluated MODELORDER
’ ast’ will not be calculated for the first time until the second
iteration:
dks: fit and remove dark squid for the column
com: remove common-mode signal
gai: if com specified, fit gain/offset of common mode
ext: apply extinction correction
ast: estimate the map and astronomical signal
flt: apply filter to time streams
noi: estimate time-domain variance
smo: time series smoothing using a median or mean boxcar filter
ssn: scan-synchronous (i.e. azimuth dependent) noise removal
pln: remove plane from each time slice
tmp: remove externally define template such as azimuth [(com,gai,ext,flt,ast,noi)]