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 …

We describe JWST/NIRSpec prism measurements of Ly α emission in z≳ 5 galaxies. We
identify Ly α detections in 10 out of 69 galaxies with robust rest-optical emission-line redshift …

We use MUSE spectroscopic observations of the dwarf spheroidal galaxy Leo T between
470 and 935 nm to search for radiative decays of axion like particles (ALPs). Under the …

Context. A census of faint and tiny star forming complexes at high redshift is key to improving
our understanding of reionizing sources, galaxy growth, and the formation of globular …

Using the exquisite data from the MUSE eXtremely Deep Field (MXDF), we report the
discovery of an Mg II emission nebula with an area above a 2σ significance level of 1000 …

An important limitation of standard multiple testing procedures is that the null distribution
should be known. Here, we consider a null distribution-free approach for multiple testing in …

We study the stellar population properties of 182 spectroscopically confirmed (MUSE/VLT)
Lyα emitters (LAEs) and 450 photometrically selected Lyman-break galaxies (LBGs) at z …

We report the discovery of diffuse extended Lyα emission from redshift 3.1 to 4.5, tracing
cosmic web filaments on scales of 2.5− 4 cMpc. These structures have been observed in …

Rest-frame ultraviolet (UV) emission lines probe electron densities, gas-phase abundances,
metallicities, and ionization parameters of the emitting star-forming galaxies and their …

We investigate the dependence of Lyα emitter (LAE) clustering on Lyα luminosity and
connect the clustering properties of≈ L⋆ LAEs with those of much fainter ones, namely,≈ …