Laurent Verstraete

TL;DR: In this article, the authors presented an all-sky model of dust emission from the Planck 857, 545 and 353 GHz, and IRAS 100 micron data.

TL;DR: In this article, the authors used the spectral energy distribution (SED) of the galactic interstellar medium dust emission, from the mid-IR to the mm range, with an unprecedented sensitivity and down to spatial scales ∼30 ��.

TL;DR: In this paper, the authors present a numerical tool, DustEM, that predicts the emission and extinction of dust given their size distribution and their optical and thermal properties, which is used to model the dust SED and extinction in the diffuse interstellar medium at high-galactic latitude (DHGL), a natural reference SED.

TL;DR: In this article, the authors present an early analysis of the Taurus molecular complex, on line-of-sight-averaged data and without component separation, and derive maps of the dust temperature T, the dust spectral emissivity index β, and the dust optical depth at 250 μm τ250.

TL;DR: In this paper, the authors constructed spectra for two known AME regions: the Perseus and ρ Ophiuchi molecular clouds using Planck maps and multi-frequency ancillary data.