In cases where data is more poorly sampled or noisier than those
examined here, convergence times may become longer than the few
minutes or so typical of the examples shown. It is clear from the
CPU times () given in Tables 1 and 2 that although
Ga-GA is not as "fast" as CURVEFIT we can see that the
user must compromise between run time and the degree of accuracy
required since Ga-GA has clearly demonstrated its
usefulness in the presence of quite severe noise. Presumably there
is also a trade-off between poorer sampling (i.e. fewer points)
saving on floating point operations, and noisier data leading to
many more fitting attempts. Monitoring the convergence of the GA in
the cases examined here indicates that it is adept at rapidly
fitting the large scale spectral features, and progressively slower
at smaller scales. This cascading nature is central to the
operation of a GA, and underpins its stability in the face of noisy
data (the noise being on the smallest scale is fitted last).
Increasing the scale of the computation is straightforward since
the generation of each child is an independent calculation
(strictly, the generation of each pair of derived strings), and so
the algorithm lends itself naturally to parallelisation. It is also
clear that a GA routine like Ga-GA could form part of a
suite of line analysis codes, with the GA offering a best initial
estimate of the profile for more conventional processing methods
which require a "good" initial guess.
We acknowledge the support of finance from the UK PPARC (Research
grants to JCB, DAD and JI, Studentship - SMc, Visitor Grant - PGJ) and
software/hardware supplied by the STARLINK project. JCB and SMc also
acknowledge the support of the HAO Visitor program. SMc would like to
thank PC for introducing him to the freely available PIKAIA
Genetic Algorithm.
We would also like to thank Dr. B. Plez for helpful comments and
suggestions made about this text during the refereeing process.
Copyright The European Southern Observatory (ESO)