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Professor of Astronomy
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Gamma-ray bursts (GRB) do not easily subdivide into classes; there is
tremendous overlap in their behaviors. However, it is difficult to imagine
how one mechanism produces the large range of observed GRB temporal and
spectral characteristics. There is strong evidence for two GRB classes
and weaker (but statistically meaningful) evidence for the existence of
a third class using BATSE data. We are applying pattern recognition algorithms
from the artificial intelligence (AI) branch of computer science to GRB
classification. In addition to science, our
eventual goal is to produce an online AI program library and a detailed
GRB database. This approach has already allowed us to discover that the
properties of the third class do not require the existence of a new source
population but can be manufactured from one of the other classes
via a combination of instrumental biases and data correlations.
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