Filtering techniques for the detection of Sunyaev-Zel'dovich clusters in multifrequency maps

被引:111
作者
Herranz, D
Sanz, JL
Hobson, MP
Barreiro, RB
Diego, JM
Martínez-González, E
Lasenby, AN
机构
[1] Fac Ciencias, Inst Fis Cantabria, Santander 39005, Spain
[2] Univ Cantabria, Dept Fis Moderna, E-39005 Santander, Spain
[3] Univ Cambridge, Cavendish Lab, Astrophys Grp, Cambridge CB3 0HE, England
[4] Univ Oxford, Dept Astrophys, Oxford OX1 3RH, England
关键词
methods : analytical; methods : data analysis; techniques : image processing; galaxies : clusters : general; cosmic microwave background;
D O I
10.1046/j.1365-8711.2002.05704.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The problem of detecting Sunyaev-Zel'dovich (SZ) clusters in multifrequency CMB observations is investigated using a number of filtering techniques. A multifilter approach is introduced that optimizes the detection of SZ clusters on microwave maps. An alternative method is also investigated in which maps at different frequencies are combined in an optimal manner so that existing filtering techniques can be applied to the single combined map. The SZ profiles are approximated by the circularly-symmetric template tau(x) = [1 + (x/r(c))(2)](-lambda), with lambda similar or equal to 1/2 and x = |x |, where the core radius r(c) and the overall amplitude of the effect are not fixed a priori, but are determined from the data. The background emission is modelled by a homogeneous and isotropic random field, characterized by a cross-power spectrum P-nu1nu2 (q) with q=\q |. The filtering methods are illustrated by application to simulated Planck observations of a 12.8degrees x 12.8degrees patch of sky in 10 frequency channels. Our simulations suggest that the Planck instrument should detect approximate to10 000 SZ clusters in 2/3 of the sky. Moreover, we find the catalogue to be complete for fluxes S > 170 mJy at 300 GHz.
引用
收藏
页码:1057 / 1068
页数:12
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