Eli Dwek

TL;DR: In this paper, the dust properties of galaxies in the redshift range 0.1 0.5 with L_IR>5x10^{10} L_\odot, appears to be 2-5 K colder than that of AKARI-selected local galaxies with similar luminosities.

TL;DR: In this article, the authors report observations of the IR/SMM emission from the Lockman North field and the Great Observatories Origins Deep Survey Field-North (GOSF-North).

TL;DR: In this paper, the authors presented analytical approximations for calculating the scattering, absorption and escape of nonionizing photons from a spherically symmetric two-phase clumpy medium, with either a central point source of isotropic radiation, a uniform distribution of IS emitters, or uniformly illuminated by external sources.

TL;DR: In this paper, the relation between dust and several fundamental properties of simulated galaxies using the Dusty SAGE semi-analytic model is explored. But the authors do not consider the properties of the galaxies themselves.

TL;DR: In this article, the authors used the Herschel Hi-GAL data to model the dust emission across the Galactic center and found that a single-temperature fit can describe the 160 − 500 µm emission for most lines of sight, if the long-wavelength dust emissivity scales as γ − β with β ≈ 2.25 µm.