Is lensing of point sources a problem for future CMB experiments?

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Lensing of Point Sources a Problem for Future Cmb Experiments ?

Weak gravitational lensing from large-scale structure enhances and reduces the fluxes from extragalactic point sources with an r.m.s. amplitude of order 15%. In cosmic microwave background (CMB) experiments, sources exceeding some flux threshold φc are removed, which means that lensing will modulate the brightness map of the remaining unresolved sources. Since this mean brightness is of order 1...

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No. Weak gravitational lensing from large-scale structure enhances and reduces the fluxes from extragalactic point sources with an r.m.s. amplitude of order 15%. In cosmic microwave background (CMB) experiments, all sources exceeding some flux threshold φc are removed, which means that lensing will modulate the brightness map of the remaining unresolved sources. Since this mean brightness is of...

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Weak gravitational lensing from large-scale structure enhances and reduces the fluxes from extragalactic point sources with an r.m.s. amplitude of order 15%. In cosmic microwave background (CMB) experiments, sources exceeding some flux threshold φc are removed, which means that lensing will modulate the brightness map of the remaining unresolved sources. Since this mean brightness is of order 1...

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ژورنال

عنوان ژورنال: Monthly Notices of the Royal Astronomical Society

سال: 1997

ISSN: 0035-8711,1365-2966

DOI: 10.1093/mnras/289.1.169