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- W2066339966 abstract "We consider the effect of lensing by galaxy clusters on the angular distribution of submillimeter wavelength objects. While lensing does not change the total flux and number counts of submillimeter sources, it can affect the number counts and fluxes of flux-limited samples. Therefore imposing a flux cut on point sources not only reduces the overall Poisson noise, but imprints the correlations between lensing clusters on the unresolved flux distribution. Using a simple model, we quantify the lensing anisotropy induced in flux-limited samples and compare this to Poisson noise. We find that while the level of induced anisotropies on the scale of the cluster angular correlation length is comparable to Poisson noise for a slowly evolving cluster model, it is negligible for more realistic models of cluster evolution. Thus the removal of point sources is not expected to induce measurable structure in the microwave or far-infrared backgrounds." @default.
- W2066339966 created "2016-06-24" @default.
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- W2066339966 date "2000-01-20" @default.
- W2066339966 modified "2023-09-23" @default.
- W2066339966 title "Lensing‐induced Structure of Submillimeter Sources: Implications for the Microwave Background" @default.
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- W2066339966 doi "https://doi.org/10.1086/308235" @default.
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