Search
Now showing items 1-10 of 13
The ALPINE-ALMA [CII] Survey: A Triple Merger at z ~ 4.56
(Royal Astronomical Society, 2020)
We report the detection of [C II] λ158 μm emission from a system of three closely separated sources in the Cosmic Evolution Survey (COSMOS) field at z ∼ 4.56 , as part of the Atacama Large Millimeter/submillimeter Array ...
The ALPINE-ALMA [C II] survey: Molecular gas budget in the Early Universe as traced by [C II]
(European Southern Observatory, 2020)
The molecular gas content of normal galaxies at z > 4 is poorly constrained because the commonly used molecular gas tracers become hard to detect at these high redshifts. We use the [C II] 158 μm luminosity, which was ...
The ALPINE-ALMA [CII] survey: Dust attenuation properties and obscured star formation at z ~ 4:4 - 5:8
(European Southern Observatory, 2020)
We present dust attenuation properties of spectroscopically confirmed star forming galaxies on the main sequence at a redshift of ∼4.4 − 5.8. Our analyses are based on the far infrared continuum observations of 118 galaxies ...
SCUBA-2 overdensities associated with candidate protoclusters selected from Planck data
(Royal Astronomical Society, 2020)
We measure the 850-μm source densities of 46 candidate protoclusters selected
from the Planck High-z catalogue (PHz) and the Planck Catalogue of Compact Sources
(PCCS) that were followed up with Herschel -SPIRE and ...
The ALPINE-ALMA [CII] Survey: On the nature of an extremely obscured serendipitous galaxy
(Royal Astronomical Society, 2020)
We report the serendipitous discovery of a dust-obscured galaxy observed as part of the
Atacama Large Millimeter Array (ALMA) Large Program to INvestigate [CII] at Early times
(ALPINE). While this galaxy is detected both ...
The ALPINE-ALMA [CII] survey: Data processing, catalogs, and statistical source properties
(European Southern Observatory, 2020)
The Atacama Large Millimeter Array (ALMA) Large Program to INvestigate [CII] at Early times (ALPINE) targets the [CII] 158 m line and the far-infrared continuum in 118 spectroscopically confirmed star-forming galaxies ...
The e-MERGE Survey (e-MERLIN Galaxy Evolution Survey): overview and survey description
(Royal Astronomical Society, 2020)
We present an overview and description of the e-MERGE Survey (e-MERLIN Galaxy Evolution Survey) Data Release 1 (DR1), a large program of high-resolution 1.5-GHz radio observations of the GOODS-N field comprising ∼140 h of ...
The ALPINE-ALMA [C II] Survey: [C II] 158micron Emission Line Luminosity Functions at z∼4−6
(American Astronomical Society, 2020)
We present the [C II] 158 μm line luminosity functions (LFs) at z ~ 4–6 using the ALMA observations of 118 sources, which are selected to have UV luminosity M1500Å < −20.2 and optical spectroscopic redshifts in COSMOS and ...
From Peculiar Morphologies to Hubble–type Spirals: The relation between galaxy dynamics and morphology in star–forming galaxies at z ∼ 1.5
(Royal Astronomical Society, 2020)
We present an analysis of the gas dynamics of star-forming galaxies at z ∼ 1.5 using data from the KMOS Galaxy Evolution Survey. We quantify the morphology of the galaxies using HSTCANDELS imaging parametrically and ...
The ALPINE-ALMA [CII] survey: Star-formation-driven outflows and circumgalactic enrichment in the early Universe
(The European Southern Observatory (ESO), 2020)
We study the efficiency of galactic feedback in the early Universe by stacking the [C II] 158 µm emission in a large sample of normal star-forming galaxies at 4 < z < 6 from the ALMA Large Program to INvestigate [C II] at ...