Volume 390, Issue 4 pp. 1339-1348

ISINA: INTEGRAL Source Identification Network Algorithm

S. Scaringi

Corresponding Author

S. Scaringi

Department of Physics and Astronomy, University of Southampton, Highfield SO17 1BJ

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A. J. Bird

A. J. Bird

Department of Physics and Astronomy, University of Southampton, Highfield SO17 1BJ

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D. J. Clark

D. J. Clark

Department of Physics and Astronomy, University of Southampton, Highfield SO17 1BJ

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A. J. Dean

A. J. Dean

Department of Physics and Astronomy, University of Southampton, Highfield SO17 1BJ

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A. B. Hill

A. B. Hill

Department of Physics and Astronomy, University of Southampton, Highfield SO17 1BJ

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V. A. McBride

V. A. McBride

Department of Physics and Astronomy, University of Southampton, Highfield SO17 1BJ

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S. E. Shaw

S. E. Shaw

Department of Physics and Astronomy, University of Southampton, Highfield SO17 1BJ

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First published: 27 October 2008
Citations: 1

Based on observations with INTEGRAL, an ESA project with instruments and science data centre funded by ESA member states (especially the PI countries: Denmark, France, Germany, Italy, Spain), Czech Republic and Poland, and the participation of Russia and the USA.

ABSTRACT

We give an overview of ISINA: INTEGRAL Source Identification Network Algorithm. This machine learning algorithm, using random forests, is applied to the IBIS/ISGRI data set in order to ease the production of unbiased future soft gamma-ray source catalogues. First, we introduce the data set and the problems encountered when dealing with images obtained using the coded mask technique. The initial step of source candidate searching is introduced and an initial candidate list is created. A description of the feature extraction on the initial candidate list is then performed together with feature merging for these candidates. Three training and testing sets are created in order to deal with the diverse time-scales encountered when dealing with the gamma-ray sky. Three independent random forests are built: one dealing with faint persistent source recognition, one dealing with strong persistent sources and a final one dealing with transients. For the latter, a new transient detection technique is introduced and described: the transient matrix. Finally the performance of the network is assessed and discussed using the testing set and some illustrative source examples.

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