Distortion of the SED of High-z Luminous Infrared Galaxies by Strong Lensing

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dc.creatorPontoppidan, K. M.
dc.creatorWiklind, T.
dc.date1999-09-21
dc.date.accessioned2026-07-07T02:33:24Z
dc.date.available2026-07-07T02:33:24Z
dc.descriptionWe 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.
dc.description2 pages, 2 figures, uses paspconf.sty. Poster contribution to "Gravitational Lensing: Recent Progress and Future Goals", Boston University 1999, eds. T. G. Brainerd and C. S. Kochanek
dc.identifierhttps://arxiv.org/abs/astro-ph/9909352
dc.identifierhttp://arxiv.org/abs/astro-ph/9909352
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14826
dc.subjectAstrophysics
dc.titleDistortion of the SED of High-z Luminous Infrared Galaxies by Strong Lensing
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