Issue |
Astron. Astrophys. Suppl. Ser.
Volume 127, Number 2, January II 1998
|
|
---|---|---|
Page(s) | 319 - 325 | |
DOI | https://doi.org/10.1051/aas:1998370 | |
Published online | 15 January 1998 |
Covered data structures I
The algorithm
Institut für Astronomie der Leopold–Franzens–Universität Innsbruck, Technikerstraße 25, A–6020 Innsbruck, Austria http://astro.uibk.ac.at
Send offprint request to: S. Kimeswenger
Received:
13
September
1996
Accepted:
26
May
1997
Many algorithms separating or detecting groups of similiar
objects (for example the extraction of groups lying in a
color–color–diagram)
are based on two statistical methods: the Kernel Method
(Silverman 1986) or the
Likelihood Statistic (van der Waerden 1957).
These standard methods have one or more
restrictions (e.g. known number or
differentiability of the groups, ). We present here a
new powerful algorithm and show results worked out with
artificial data sets.
The algorithm is based on Recursive Restoration Methods (neither on the
Likelihood Statistic (Sutherland & Saunders 1992) nor on the
Kernel Method (De Jager et al. 1986) and
allows to detect substructures in a data set, even if they are overlapped or
superimposed by any kind of dominating main structure. In comparison to the
other methods mentioned above there are
no restrictions concerning the form and the dimension of the components
lying in the data set.
The algorithm is easy to handle and therefore opens a wide
range of applications for many fields of science (see Boller et al.
1992).
Key words: methods: statistical / astronomical data bases: miscellaneous
© European Southern Observatory (ESO), 1998