JADES initial data release for the Hubble Ultra Deep Field: revealing the faint infrared sky with deep JWST NIRCam imaging
JWST has revolutionized the field of extragalactic astronomy with its sensitive and high-
resolution infrared view of the distant Universe. Adding to the new legacy of JWST …
resolution infrared view of the distant Universe. Adding to the new legacy of JWST …
The MUSE Hubble Ultra Deep Field surveys: Data release II
R Bacon, J Brinchmann, S Conseil, M Maseda… - Astronomy & …, 2023 - aanda.org
We present the second data release of the MUSE Hubble Ultra-Deep Field surveys, which
includes the deepest spectroscopic survey ever performed. The MUSE data, with their 3D …
includes the deepest spectroscopic survey ever performed. The MUSE data, with their 3D …
High-z galaxies with JWST and local analogues–it is not only star formation
J Brinchmann - Monthly Notices of the Royal Astronomical …, 2023 - academic.oup.com
ABSTRACT I present an analysis of the JWST NIRSpec data of SMACS 0723 released as
Early Release Observations. As part of this three new redshifts are provided, bringing the …
Early Release Observations. As part of this three new redshifts are provided, bringing the …
Inside the bubble: exploring the environments of reionisation-era Lyman-α emitting galaxies with JADES and FRESCO
We present a study of the environments of 17 Lyman-α emitting galaxies (LAEs) in the
reionisation-era (5.8< z< 8) identified by JWST/NIRSpec as part of the JWST Advanced …
reionisation-era (5.8< z< 8) identified by JWST/NIRSpec as part of the JWST Advanced …
GN-z11: The environment of an active galactic nucleus at z= 10.603-New insights into the most distant Lyα detection
Recent observations with the James Webb Space Telescope (JWST) have further refined
the spectroscopic redshift of GN-z11, one of the most distant galaxies identified with the …
the spectroscopic redshift of GN-z11, one of the most distant galaxies identified with the …
(Re)Solving reionization with Lyα: how bright Lyα Emitters account for the z ≈ 2–8 cosmic ionizing background
The cosmic ionizing emissivity from star-forming galaxies has long been anchored to UV
luminosity functions. Here, we introduce an emissivity framework based on Lyα emitters …
luminosity functions. Here, we introduce an emissivity framework based on Lyα emitters …
MUSE Analysis of Gas around Galaxies (MAGG) – IV. The gaseous environment of z ∼ 3–4 Ly α emitting galaxies
EK Lofthouse, M Fumagalli, M Fossati… - Monthly Notices of …, 2023 - academic.oup.com
We study the link between galaxies and H i-selected absorption systems at z∼ 3–4 in the
MUSE Analysis of Gas around Galaxies (MAGG) survey, an ESO large programme …
MUSE Analysis of Gas around Galaxies (MAGG) survey, an ESO large programme …
Metal line emission from galaxy haloes at z ≈ 1
We present a study of the metal-enriched halo gas, traced using Mg ii and [O ii] emission
lines, in two large, blind galaxy surveys–the MUSE (Multi Unit Spectroscopic Explorer) …
lines, in two large, blind galaxy surveys–the MUSE (Multi Unit Spectroscopic Explorer) …
MusE GAs FLOw and Wind (MEGAFLOW) VIII. Discovery of a Mgii emission halo probed by a quasar sightline
Using deep () VLT/MUSE data from the MEGAFLOW survey, we report the first detection of
extended emission from a galaxy's halo that is probed by a quasar sightline. The emission …
extended emission from a galaxy's halo that is probed by a quasar sightline. The emission …
A cosmic stream of atomic carbon gas connected to a massive radio galaxy at redshift 3.8
The growth of galaxies in the early Universe is driven by accretion of circum-and
intergalactic gas. Simulations have predicted that steady streams of cold gas penetrate the …
intergalactic gas. Simulations have predicted that steady streams of cold gas penetrate the …