Far-infrared and submillimeter wavelength surveys have now established the important role
of dusty, star-forming galaxies (DSFGs) in the assembly of stellar mass and the evolution of …

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 …

Aims. We present the detailed characterisation of a sample of 56 sources serendipitously
detected in ALMA band 7 as part of the ALMA Large Program to INvestigate CII at Early …

We present results from the deepest Herschel-Photodetector Array Camera and
Spectrometer (PACS) far-infrared blank field extragalactic survey, obtained by combining …

Aims. Photometric data of galaxies covering the rest-frame wavelength range from far-UV to
far-IR make it possible to derive galaxy properties with a high reliability by fitting the …

IR emission spectra are calculated for dust heated by starlight, for mixtures of amorphous
silicate and graphitic grains, including varying amounts of PAH particles. The models are …

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 …

We present the deepest 100 to 500 μm far-infrared observations obtained with the Herschel
Space Observatory as part of the GOODS-Herschel key program, and examine the infrared …

The Herschel ATLAS is the largest open-time key project that will be carried out on the
Herschel Space Observatory. It will survey 570 deg 2 of the extragalactic sky, 4 times larger …

We present a sample of low-resolution 5-38 μm Spitzer IRS spectra of the inner few square
kiloparsecs of 59 nearby galaxies spanning a large range of star formation properties. A …