Fitting the spectral energy distributions (SEDs) of galaxies is an almost universally used
technique that has matured significantly in the last decade. Model predictions and fitting …

Abstract Anomalous Microwave Emission (AME) is a component of diffuse Galactic radiation
observed at frequencies in the range≈ 10–60 GHz. AME was first detected in 1996 and …

We present the characteristics of 2 mm selected sources from the largest Atacama Large
Millimeter/submillimeter Array (ALMA) blank-field contiguous survey conducted to date, the …

We present a simple, largely empirical but physically motivated model to interpret the mid-
and far-infrared spectral energy distributions of galaxies consistently with the emission at …

Context. The evolution of amorphous hydrocarbon materials, aC (: H), principally resulting
from ultraviolet (UV) photon absorption-induced processing, are likely at the heart of the …

We present a quantitative model for the infrared emission from dust in the diffuse interstellar
medium. The model consists of a mixture of amorphous silicate grains and carbonaceous …

We present models of photometric evolution of galaxies in which the effects of a dusty
interstellar medium have been included with particular care. A chemical evolution code …

New far-infrared and submillimeter data are used to solidify and to extend to long
wavelengths the empirical calibration of the infrared spectral energy distribution (SED) of …

The Planck and Herschel missions are currently measuring the far-infrared to millimeter
emission of dust, which combined with existing IR data, will for the first time provide the full …

Solid particles with the composition of interstellar dust and power-law size distribution
dn/da∝ ap (for a≤ a max with a max≳ 3λ and 3< p< 4) will have submillimeter opacity …