Hydrogen Lyman-α (Lyα) emission has been one of the major observational probes for the
high-redshift Universe since the first discoveries of high-z Lyα-emitting galaxies in the late …

The Atacama Large Millimetre/submillimetre Array (ALMA) is currently in the process of
transforming our view of star-forming galaxies in the distant (z≳ 1) universe. Before ALMA …

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 …

We present the PHANGS-MUSE survey, a programme that uses the MUSE integral field
spectrograph at the ESO VLT to map 19 massive (9.4< log (M⋆/M⊙)< 11.0) nearby (D≲ 20 …

The processing of raw data from modern astronomical instruments is often carried out
nowadays using dedicated software, known as pipelines, largely run in automated …

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 study the ionizing photon production efficiency at the end of the Epoch of Reionization
(z∼ 5.4− 6.6) for a sample of 30 Ly α emitters. This is a crucial quantity to infer the ionizing …

The ionizing photon escape fraction [Lyman continuum (LyC) f esc] of star-forming galaxies
is the single greatest unknown in the reionization budget. Stochastic sightline effects prohibit …

We make use of sensitive (9.3 μJy beam− 1 rms) 1.2 mm continuum observations from the
Atacama Large Millimeter/submillimeter Array (ALMA) Spectroscopic Survey in the Hubble …

Lyα emission from galaxies can be utilized to characterize the ionization state in the
intergalactic medium (IGM). We report our search for Lyα emission at z> 7 using a …