The Kohonen Map: Chaos to Order in 17000 Easy Steps

Successful use of the Kohonen Self-Organising Map scheme in the area of lightcurve classification is presented along with preliminary results of the method applied to analysis of the XMM-Subaru x-ray and optical-counterpart deep-field data.

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Author and article information

Conference

Publication date: April 2004

Publication date (Print): April 2004

Pages: 1-2

Affiliations

[0001]University of Leicester, UK

Article

DOI: 10.14236/ewic/ADA-III2004.5

SO-VID: c5d3b4bb-ccfe-4dd8-ada2-d93d7369db60

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This work is licensed under a Creative Commons Attribution 4.0 Unported License. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/

Conference name: ADA-III - Astronomical Data Analysis III Conference

Conference acronym: ADA

Conference number: 3

Conference location: Sant' Agata sui due Golfi, Italy

Conference date: 29 April - 1 May 2004

Conference sponsor: Electronic Workshops in Computing (eWiC)

Conference theme: Astronomical Data Analysis

History

Product

1477-9358 BCS Learning & Development

Self URI (article page): https://www.scienceopen.com/hosted-document?doi=10.14236/ewic/ADA-III2004.5

Self URI (journal page): https://ewic.bcs.org/

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The Kohonen Map: Chaos to Order in 17000 Easy Steps

Abstract