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When the analysis yields a large number of parameters for each object,
it is difficult to overview relations between the individual variable.
Multivariate statistical methods can be applied in such a situation to
give an objective description of the data. The Principal Components
Analysis is used to determine the true dimensionality of the data set
and find the best linear combination of the parameter for following
studies (see Chatfield and Collins 1980). A typical example of such
analysis was performed by Okamura (1985) on photometric data from
Virgo Cluster galaxies.
Structures and groups in large data sets can be located by means of a
Cluster Analysis which constructs a set of groups in the data using a
given distance measure. A large variety of methods for clustering are
available with different distance definitions providing both
hierarchical and non-hierarchical groups (see Murtagh 1986 and
references therein). These techniques are used especially for
classification problems in astronomy.
References
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the Physical Sciences, McGraw-Hill, New York.
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- Chatfield, C., Collins, A.J. : 1980, Introduction to Multivariate
Analysis, Chapman and Hall.
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Osservatorio Astronomico di Trieste, p. 211.
- Murtagh, F. : 1986, ESO Preprint No. 448
- Newell, E.B. : 1979, Image Processing in Astronomy,
Eds. G. Sedmark, M. Capaccioli, R.J. Allen,
Osservatorio Astronomico di Trieste, p. 100.
- Newell, B., O'Neil, Jr., E.J. : 1977, Pub. Astron. Soc. Pac.
89, 925.
- Okamura, S. : 1985, Proc. of ESO Workshop on The Virgo Cluster,
Eds. O.-G. Richter and B. Binggeli, ESO, p. 201.
- Pratt, N.M. : 1977, Vistas in Astronomy 21, 1.
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New York.
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Vol. 1-2, Academic Press, New York.
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Reading, Mass.
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=31 =3 =1999
Next: CCD Reductions
Up: Analysis of Results
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Petra Nass
1999-06-15