Roughly half of the radiation from evolving galaxies in the early Universe reaches us in the
far-infrared and submillimeter wavelength ranges. Recent major advances in observing …

This paper presents an all-sky model of dust emission from the Planck 353, 545, and 857
GHz, and IRAS 100 μm data. Using a modified blackbody fit to the data we present all-sky …

Aims. We present the first public release of high-quality data products (DR1) from Hi-GAL,
the Herschel infrared Galactic Plane Survey. Hi-GAL is the keystone of a suite of continuum …

ABSTRACT Spitzer Space Telescope and Herschel Space Observatory imaging of M31 is
used, with a physical dust model, to construct maps of dust surface density, dust-to-gas ratio …

We present new measurements of cosmic infrared background (CIB) anisotropies using
Planck. Combining HFI data with IRAS, the angular auto-and cross-frequency power …

The relative importance of primordial molecular cloud fragmentation versus large-scale
accretion still remains to be assessed in the context of massive core/star formation. Studying …

Though half of cosmic starlight is absorbed by dust and reradiated at long wavelengths (3
μm–3 mm), constraints on the infrared through the millimeter galaxy luminosity function (or …

ABSTRACT A key parameter to the description of all star formation processes is the density
structure of the gas. In this Letter, we make use of probability distribution functions (PDFs) of …

Planck allows unbiased mapping of Galactic sub-millimetre and millimetre emission from the
most diffuse regions to the densest parts of molecular clouds. We present an early analysis …

ABSTRACT ALMA observations have revealed the presence of dust in galaxies in the Epoch
of Reionization (EoR; redshift z> 6). However, the dust temperature, T d, remains …