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View article: The MUSE eXtremely Deep Field
The MUSE eXtremely Deep Field Open
Context. The hydrogen Lyman-alpha (Ly α ) line, the brightest rest-frame ultraviolet line of high-redshift galaxies, exhibits a large variety of shapes, which is due to factors at different scales, from the interstellar medium to the inter…
View article: The MUSE Extremely Deep Field: Classifying the Spectral Shapes of Lya Emitting Galaxies
The MUSE Extremely Deep Field: Classifying the Spectral Shapes of Lya Emitting Galaxies Open
The Hydrogen Lyman-alpha (Lya) line shows a large variety of shapes which is caused by factors at different scales, from the interstellar medium to the intergalactic medium. This work aims to provide a systematic inventory and classificati…
View article: The intrinsic distribution of Lyman-<i>α</i> halos
The intrinsic distribution of Lyman-<i>α</i> halos Open
The emission and escape of Lyman- α photons from star-forming galaxies is determined through complex interactions between the emitted photons and a galaxy’s interstellar and circumgalactic gas. This causes Lyman- α emitters (LAEs) to commo…
View article: The Intrinsic Distribution of Lyman-$α$ Halos
The Intrinsic Distribution of Lyman-$α$ Halos Open
The emission and escape of Lyman-$α$ photons from star-forming galaxies is determined through complex interactions between the emitted photons and a galaxy's interstellar and circumgalactic gas, causing Lyman-$α$ emitters (LAEs) to commonl…
View article: Median surface-brightness profiles of Lyman-<i>α</i> haloes in the MUSE Extremely Deep Field
Median surface-brightness profiles of Lyman-<i>α</i> haloes in the MUSE Extremely Deep Field Open
We present the median surface brightness profiles of diffuse Ly α haloes (LAHs) around star-forming galaxies by stacking 155 spectroscopically confirmed Ly α emitters (LAEs) at 3 < z < 4 in the MUSE Extremely Deep Field (MXDF) with a media…
View article: Lyman continuum leaker candidates at <i>z</i> ∼ 3–4 in the HDUV based on a spectroscopic sample of MUSE LAEs
Lyman continuum leaker candidates at <i>z</i> ∼ 3–4 in the HDUV based on a spectroscopic sample of MUSE LAEs Open
Context. In recent years, a number of Lyman continuum (LyC) leaker candidates have been found at intermediate redshifts, providing insight into how the Universe was reionised at early cosmic times. There are now around 100 known LyC leaker…
View article: Lyman Continuum Leaker Candidates at $z\sim3-4$ in the HDUV Based on a Spectroscopic Sample of MUSE LAEs
Lyman Continuum Leaker Candidates at $z\sim3-4$ in the HDUV Based on a Spectroscopic Sample of MUSE LAEs Open
In recent years, a number of Lyman continuum (LyC) leaker candidates at intermediate redshifts have been found, providing insight into how the Universe was reionised at early cosmic times. Here we identify new LyC leaker candidates at $z\a…
View article: JWST/NIRSpec Measurements of Extremely Low Metallicities in High Equivalent Width Lyα Emitters
JWST/NIRSpec Measurements of Extremely Low Metallicities in High Equivalent Width Lyα Emitters Open
Deep Very Large Telescope/MUSE optical integral field spectroscopy has recently revealed an abundant population of ultra-faint galaxies ( M UV ≈ −15; 0.01 L ⋆ ) at z = 2.9−6.7 due to their strong Ly α emission with no detectable continuum.…
View article: JWST/NIRSpec Measurements of Extremely Low Metallicities in High Equivalent Width Lyman-$α$ Emitters
JWST/NIRSpec Measurements of Extremely Low Metallicities in High Equivalent Width Lyman-$α$ Emitters Open
Deep VLT/MUSE optical integral field spectroscopy has recently revealed an abundant population of ultra-faint galaxies ($M_{UV} \approx -15$; 0.01 $L_{\star}$) at $z=$2.9$-$6.7 due to their strong Lyman-$α$ emission with no detectable cont…
View article: The MUSE<i>Hubble</i>Ultra Deep Field surveys: Data release II
The MUSE<i>Hubble</i>Ultra Deep Field surveys: Data release II Open
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 content, amazing depth, wide spectral range, and excellent spatial…
View article: The MUSE Hubble Ultra Deep Field surveys: Data release II
The MUSE Hubble Ultra Deep Field surveys: Data release II Open
We present the second data release of the MUSE Hubble UDF surveys, which includes the deepest spectroscopic survey ever performed. The MUSE data, with their 3D content, amazing depth, wide spectral range, and excellent spatial and medium s…
View article: The Lensed Lyman-Alpha MUSE Arcs Sample (LLAMAS)
The Lensed Lyman-Alpha MUSE Arcs Sample (LLAMAS) Open
Aims. We present the Lensed Lyman-Alpha MUSE Arcs Sample (LLAMAS) selected from MUSE and HST observations of 17 lensing clusters. The sample consists of 603 continuum-faint (−23 < M UV < −14) lensed Lyman- α emitters (producing 959 images)…
View article: The MUSE eXtremely Deep Field: Individual detections of Ly<i>α</i> haloes around rest-frame UV-selected galaxies at <i>z</i> ≃ 2.9–4.4
The MUSE eXtremely Deep Field: Individual detections of Ly<i>α</i> haloes around rest-frame UV-selected galaxies at <i>z</i> ≃ 2.9–4.4 Open
Hydrogen Ly α haloes (LAHs) are commonly used as a tracer of the circumgalactic medium (CGM) at high redshifts. In this work, we aim to explore the existence of Ly α haloes around individual UV-selected galaxies, rather than around Ly α em…
View article: Equivalent widths of Lyman <i>α</i> emitters in MUSE-Wide and MUSE-Deep
Equivalent widths of Lyman <i>α</i> emitters in MUSE-Wide and MUSE-Deep Open
Context. The hydrogen Lyman α line is often the only measurable feature in optical spectra of high-redshift galaxies. Its shape and strength are influenced by radiative transfer processes and the properties of the underlying stellar popula…
View article: The MUSE eXtremely Deep Field: Individual detections of Lyα haloes around rest-frame UV-selected galaxies at z~2.9-4.4
The MUSE eXtremely Deep Field: Individual detections of Lyα haloes around rest-frame UV-selected galaxies at z~2.9-4.4 Open
Hydrogen Ly$α$ haloes (LAHs) are commonly used as a tracer of the circumgalactic medium (CGM) at high redshifts. In this work, we aim to explore the existence of Ly$α$ haloes around individual UV-selected galaxies, rather than around Ly$α$…