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- W3088976049 abstract "We present a model to estimate the effect of differential magnification on the SED of high-z ULIRGs. It is found that the ratio of the high temperature component to the low temperature component can vary with up to a factor of ten with source position on very small angular scales ~0.01. This means that a correction for differential magnification is needed when deriving dust properties from strongly lensed sources." @default.
- W3088976049 created "2020-10-01" @default.
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- W3088976049 date "1999-09-21" @default.
- W3088976049 modified "2023-09-26" @default.
- W3088976049 title "Distortion of the SED of High-z Luminous Infrared Galaxies by Strong Lensing" @default.
- W3088976049 doi "https://doi.org/10.48550/arxiv.astro-ph/9909352" @default.
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