Active galactic nuclei (AGN) are energetic astrophysical sources powered by accretion onto
supermassive black holes in galaxies, and present unique observational signatures that …

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 …

ABSTRACT ALMA observations have revealed the presence of dust in the first generations
of galaxies in the Universe. However, the dust temperature T d remains mostly …

ABSTRACT A two-parameter semi-empirical model is presented for the spectral energy
distributions of galaxies with contributions to their infrared–submillimeter–radio emission …

We review results from cosmic X-ray surveys of active galactic nuclei (AGNs) over the past
≈ 15≈ 15 years that have dramatically improved our understanding of growing …

The total star formation budget of galaxies consists of the sum of the unobscured star
formation, as observed in the rest-frame ultraviolet (UV), together with the obscured …

Dust temperature is an important property of the interstellar medium (ISM) of galaxies. It is
required when converting (sub) millimetre broad-band flux to total infrared luminosity (L IR) …

We use deep panchromatic data sets in the GOODS-N field, from GALEX to the deepest
Herschel far-infrared (FIR) and VLA radio continuum imaging, to explore the evolution of star …

Environment is one of the primary drivers of galaxy evolution; via multiple mechanisms, it
can control the critical process of transforming galaxies from star forming to quiescent …

We characterize infrared spectral energy distributions of 343 (ultra) luminous infrared
galaxies from z= 0.3–2.8. We diagnose the presence of an active galactic nucleus (AGN) by …