The spectral energy distributions (SEDs) of galaxies are shaped by nearly every physical
property of the system, including the star-formation history, metal content, abundance …

Over the past two decades, an avalanche of new data from multiwavelength imaging and
spectroscopic surveys has revolutionized our view of galaxy formation and evolution. Here …

We combine results from deep ALMA observations of massive (M*> 10 10 M⊙) galaxies at
different redshifts to show that the column density of their interstellar medium (ISM) rapidly …

An ALMA [C ii] Survey of 27 Quasars at z > 5.94 - IOPscience Skip to content IOP Science
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Physical Properties of 15 Quasars at z ≳ 6.5 - IOPscience This site uses cookies. By continuing
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We explore the kinematics of 27 z≳ 6 quasar host galaxies observed in [C ii] 158 μm ([C ii])
emission with the Atacama Large Millimeter/submillimeter Array at a resolution of≈ 025. We …

We present new ALMA observations and physical properties of a Lyman break galaxy at z=
7.15. Our target, B14-65666, has a bright ultra-violet (UV) absolute magnitude, M UV≈ …

We present a self-consistent cross-calibration of the three main molecular gas mass tracers
in galaxies, namely the 12CO (1–0),[C i](3 P 1–3 P 0) lines, and the submm dust continuum …

We present a new, publicly available library of dust spectral energy distributions (SEDs).
These SEDs are characterized by only three parameters: the dust mass (M dust), the dust …

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 …