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A&A 445, 795-804 (2006)
DOI: 10.1051/0004-6361:20041950
A method to search for topological signatures in the angular distribution of cosmic objects
A. Bernui and T. VillelaInstituto Nacional de Pesquisas Espaciais, Divisão de Astrofísica, Av. dos Astronautas 1758, 12227-010, São José dos Campos, SP, Brazil
e-mail: [bernui;thyrso]@das.inpe.br
(Received 5 September 2004 / Accepted 30 September 2004 )
Abstract
We present a method to search for large angular-scale
correlations, termed topological signatures, in the angular
distribution of cosmic objects, which does not depend on
cosmological models or parameters and is based only on the
angular coordinates of the objects.
In order to explore Cosmic Microwave Background temperature
fluctuations data, we applied this method to simulated
distributions of objects in thin spherical shells located
in three dif ferent multiply-connected Euclidean 3-spaces
(T3,
, and G6), and found that the topological
signatures due to these topologies can be revealed even if
their intensities are small.
We show how to detect such signatures for the cases of
full-sky and partial-sky distributions of objects.
This method can also be applied to other ensembles of
cosmic objects, like galaxies or quasars, in order to
reveal possible angular-scale correlations in their
distributions.
Key words: cosmology -- cosmology: large-scale structure of Universe -- cosmology: cosmic microwave background -- methods: data analysis
© ESO 2006
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