IVOA KDD-IG: A user guide for Data Mining in Astronomy

Who's interested?


Purpose of this Guide

The purpose of this guide is to show how the techniques of data mining, a large well-known field with a wide array of applications, can be used within astronomy to improve the science that is done with the available data. It is written with the typical astronomer in mind, i.e., one whose first priority is to get good science done.

Table of contents


  • Nick Ball is an active participant in the Next Generation Virgo Cluster Survey at the Herzberg Institute for Astrophysics in Victoria, British Columbia, Canada. His research interests include the galaxy luminosity function, galaxy, AGN, and quasar properties versus environment, photometric redshifts and classification, and data mining.

  • Sabine McConnell (main author of sections 3 and 4) is an Assistant Professor in the Department of Computing and Information Systems at Trent University, Peterborough, Ontario, Canada.

-- NickBall - 18 Mar 2011
-- NickBall - 23 Sep 2011

Edit | Attach | Watch | Print version | History: r13 < r12 < r11 < r10 < r9 | Backlinks | Raw View | Raw edit | More topic actions
Topic revision: r13 - 2011-09-24 - NickBall
This site is powered by the TWiki collaboration platform Powered by Perl This site is powered by the TWiki collaboration platformCopyright © 2008-2024 by the contributing authors. All material on this collaboration platform is the property of the contributing authors.
Ideas, requests, problems regarding TWiki? Send feedback