Infrared and Submillimeter Space Astronomy
C. Aime and R. Soummer (eds)
EAS Publications Series, Vol. 8, 2003
DOI: 10.1051/eas:2003057
A brief introduction to detection problems and illustration
O. Michel and A. FerrariLUAN UMR 6525, Université de Nice Sophia Antipolis, Parc Valrose, 06108 Nice Cedex 2, France; omichel@unice.fr
ferrari@unice.fr
Abstract
In this paper, some basics concepts in statistical approaches
for detection of signals embedded in noise are briefly
reviewed. Though most material presented in the first part of
the paper is well documented in the litterature (see
references), some effort is made to provide a self-contained
and concise introduction to the subject. The importance and
relevance of the likelihood ratio is highlighted from a
Bayesian formulation of the problem; the optimal (in the sense
of maximized detection probability for given false alarm rates)
Neyman Pearson test and likelihood ratio test are discussed in
the general framework of test performance studies. Therefore,
the usefullness of the ROCs (Receiver Operating
Characteristics) is illustrated on simple examples. When some
unknown parameters must be taken into account, extension of the
previous approaches are mentionned, with some emphasis put on
the GLRT (generalized likelihood ratio test). Most results
introduced in this tutorial are then applied and discussed in
the framework of the extra-solar planet detection problem. A
observation model involving Poisson random variables is
studied. A thorough study in performed, and the Gaussian
asymptotics are discussed in the case where all parameters of
the model are assumed. In a more realistic situation where some
parameters must be estimated, the GLRT is derived and its
performances are evaluated by Monte Carlo simulation.
© EAS, EDP Sciences 2003


Document