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The TIMING mode of spiros is again easy to use as it does not
search for sources but gets their locations from an input catalog as in
SPECTRAL mode. The idea is that the user will bin count data over
some observation period in as many energy bins as desired and that
spiros will calculate source flux values at a sequence of MJD times
over some integration time interval to be given by the user. Note that
the data at this level are already grouped into pointings, thus no
timing analysis can be performed on time scales shorter than the
pointing duration.
At present TIMING mode has three forms of analysis
- QUICKLOOK
This computes the flux for all sources and background in small groups
of pointing exposures covering the integration time interval, in parameter
source-timing-scale, and in each count spectrum energy bin.
- WINDOW
This mode assumes a mean count modulation model (MCM), or known background variations and computes source flux
values simultaneously in a sequence of integration time intervals spanning the period
of observation. For a large number of integration intervals and energy bins this
might take some time to calculate.
- TRANSIENT
This upgraded mode is similar to WINDOW mode but allows the removal of the
discontinuous nature of the HAT like time bin functions to return an implicitly
smoothed light curve. The integration time intervals spanning the period of observation
are used here to create a sequence of splining nodes, or knot points, which will
define a sequence of piecewise or smoothly continuous B-spline functions.
Select either TRANSIENT-HAT, TRANSIENT-LINEAR,
TRANSIENT-QUADR, or TRANSIENT-CUBIC. If no -XXXX function is appended a simple
HAT type is selected and the results should be the same as in WINDOW mode.
These functions are actually created by taking a HAT function covering each time
interval and smoothing it with a HAT filter several times over to create LINEAR,
QUADRATIC or CUBIC B-spline functions, a sequence which will tend towards a Gaussian
shape with each further smoothing.
Next: Parameter list
Up: Image reconstruction and spectral
Previous: SPECTRAL extraction mode
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