Galaxy angular power spectrum analysis of the FLAMEX survey

Details Galaxy angular power spectrum analysis of the FLAMEX survey Galaxy angular power spectrum analysis of the FLAMEX survey

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aas...20717004n&link_type=abstract

American Astronomical Society Meeting 207, #170.04; Bulletin of the American Astronomical Society, Vol. 37, p.1427

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The galaxy angular power spectrum, Cl, is a powerful tool to probe the large scale structure and to constrain cosmological parameters (Cooray et al. 2001; Tegmark et al. 2002; Blake et al. 2004). Here, we construct the galaxy angular power spectrum within redshift shells extending beyond z=1 using the catalogues produced from the FLAMEX survey (FLAMINGOS Extragalactic Survey). We employ a spherical harmonic analysis (Peebles 1973; Blake et al. 2004) that incorporates the appropriate window functions describing the partial sky coverage. The FLAMEX survey will eventually covers about 7 square degrees using the deep J and Ks band imaging with corresponding multiband optical coverage available from NDWFS (the data reduction of the Bootes region is completed). Preliminary results will be presented.

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