Using lab-measured temperature-dependent opacities, fixed-β modified-blackbody fits overestimate high-z dust masses by 25–60% from temperature dependence alone.
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Effects of temperature-dependent optical properties on the determination of interstellar dust masses
Using lab-measured temperature-dependent opacities, fixed-β modified-blackbody fits overestimate high-z dust masses by 25–60% from temperature dependence alone.