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 …

Nearby galaxies offer unique laboratories allowing multi-wavelength spatially resolved
studies of the interstellar medium, star formation and nuclear activity across a broad range of …

We introduce serra, a suite of zoom-in high-resolution (, at z= 7.7) cosmological simulations
including non-equilibrium chemistry and on-the-fly radiative transfer. The outputs are post …

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 present ALMA Band 9 observations of the [C ii] 158 m emission for a sample of 10 main-
sequence galaxies at redshift∼ 2, with typical stellar masses (log M⋆/M⊙∼ 10.0–10.9) and …

Aims. We analyze the applicability of far-infrared fine-structure lines [Cii] 158 μm,[Oi] 63 μm,
and [Oiii] 88 μm to reliably trace the star formation rate (SFR) in a sample of low-metallicity …

The existence of massive (1011 solar masses) elliptical galaxies by redshift z≈ 4 (refs,,;
when the Universe was 1.5 billion years old) necessitates the presence of galaxies with star …

We present ALMA detections of the [C ii] 158 μm emission line and the underlying far-
infrared (FIR) continuum of three quasars at 6.6< z< 6.9 selected from the VIKING survey …

Context. The far-infrared (FIR) lines are important tracers of the cooling and physical
conditions of the interstellar medium (ISM) and are rapidly becoming workhorse diagnostics …