PCA Tomography: how to extract information from data cubes


Autoria(s): STEINER, J. E.; MENEZES, R. B.; RICCI, T. V.; OLIVEIRA, A. S.
Contribuinte(s)

UNIVERSIDADE DE SÃO PAULO

Data(s)

19/10/2012

19/10/2012

2009

Resumo

Astronomy has evolved almost exclusively by the use of spectroscopic and imaging techniques, operated separately. With the development of modern technologies, it is possible to obtain data cubes in which one combines both techniques simultaneously, producing images with spectral resolution. To extract information from them can be quite complex, and hence the development of new methods of data analysis is desirable. We present a method of analysis of data cube (data from single field observations, containing two spatial and one spectral dimension) that uses Principal Component Analysis (PCA) to express the data in the form of reduced dimensionality, facilitating efficient information extraction from very large data sets. PCA transforms the system of correlated coordinates into a system of uncorrelated coordinates ordered by principal components of decreasing variance. The new coordinates are referred to as eigenvectors, and the projections of the data on to these coordinates produce images we will call tomograms. The association of the tomograms (images) to eigenvectors (spectra) is important for the interpretation of both. The eigenvectors are mutually orthogonal, and this information is fundamental for their handling and interpretation. When the data cube shows objects that present uncorrelated physical phenomena, the eigenvector`s orthogonality may be instrumental in separating and identifying them. By handling eigenvectors and tomograms, one can enhance features, extract noise, compress data, extract spectra, etc. We applied the method, for illustration purpose only, to the central region of the low ionization nuclear emission region (LINER) galaxy NGC 4736, and demonstrate that it has a type 1 active nucleus, not known before. Furthermore, we show that it is displaced from the centre of its stellar bulge.

FAPESP - Fundacao de Amparo a Pesquisa do Estado de Sao Paulo[06/05203-3]

FAPESP - Fundacao de Amparo a Pesquisa do Estado de Sao Paulo[05/03323-9]

Identificador

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, v.395, n.1, p.64-75, 2009

0035-8711

http://producao.usp.br/handle/BDPI/27186

10.1111/j.1365-2966.2009.14530.x

http://dx.doi.org/10.1111/j.1365-2966.2009.14530.x

Idioma(s)

eng

Publicador

WILEY-BLACKWELL PUBLISHING, INC

Relação

Monthly Notices of the Royal Astronomical Society

Direitos

restrictedAccess

Copyright WILEY-BLACKWELL PUBLISHING, INC

Palavras-Chave #methods: data analysis #methods: statistical #techniques: image processing #techniques: spectroscopic #MULTIOBJECT SPECTROGRAPH #GALACTIC NUCLEI #CLASSIFICATION #SPECTRA #Astronomy & Astrophysics
Tipo

article

original article

publishedVersion