Scale‐adaptive Filters for the Detection/Separation of Compact Sources
Author(s) -
D. Herranz,
J. L. Sanz,
R. B. Barreiro,
E. Martínez-González
Publication year - 2002
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/342651
Subject(s) - physics , isotropy , scale (ratio) , separation (statistics) , homogeneous , galaxy , spectral density , astrophysics , random field , computational physics , statistical physics , optics , mathematics , statistics , quantum mechanics
This paper presents scale-adaptive filters that optimize thedetection/separation of compact sources on a background. We assume that thesources have a multiquadric profile, i. e. $\tau (x) = {[1 +{(x/r_c)}^2]}^{-\lambda}, \lambda \geq {1/2}, x\equiv |\vec{x}|$, and abackground modeled by a homogeneous and isotropic random field, characterizedby a power spectrum $P(q)\propto q^{-\gamma}, \gamma \geq 0, q\equiv|\vec{q}|$. We make an n-dimensional treatment but consider two interestingastrophysical applications related to clusters of galaxies (Sunyaev-Zel'dovicheffect and X-ray emission).Comment: 41 pages, 7 figures, submitted to Ap
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