Discriminating between unresolved point sources and "negative" SZ clusters in CMB maps
Clusters of galaxies produce negative features at wavelengths $\lambda > 1.25$ mm in CMB maps, by means of the thermal SZ effect, while point radio sources produce positive peaks. This fact implies that a distribution of unresolved SZ clusters could be detected using the negative asymmetry introd...
Main Authors: | , |
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Language: | English |
Published: |
2002
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Subjects: | |
Online Access: | http://cds.cern.ch/record/592327 |