It remains a major challenge to derive a theory of cloud-scale (pc) star formation and
feedback, describing how galaxies convert gas into stars as a function of the galactic …

The onset of the JWST-era provides a much-improved opportunity to characterize the
resolved structure of early star-forming systems. Previous Spitzer observations of z≳ 6 …

Understanding the variability of galaxy star formation histories (SFHs) across a range of time-
scales provides insight into the underlying physical processes that regulate star formation …

We study the physical properties (size, stellar mass, luminosity, and star formation rate) and
scaling relations for a sample of 166 star-forming clumps with redshift z∼ 2–6.2. They are …

We investigate the strongly lensed (μ≃× 10− 100) Lyman continuum (LyC) galaxy, dubbed
Sunburst, at z= 2.37, taking advantage of a new accurate model of the lens. A …

We study the dynamics of cold molecular gas in two main-sequence galaxies at cosmic
noon (zC-488879 at z≃ 1.47 and zC-400569 at z≃ 2.24) using new high-resolution ALMA …

We investigate the blue and optical rest-frame sizes (λ≃ 2300–4000 Å) of three compact star-
forming regions in a galaxy at z= 4 strongly lensed (× 30,× 45, and× 100) by the Hubble …

ABSTRACT A key uncertainty in galaxy evolution is the physics regulating star formation,
ranging from small-scale processes related to the life-cycle of molecular clouds within …

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 …

High-resolution imaging of galaxies in rest-frame UV has revealed the existence of giant star-
forming clumps prevalent in high-redshift galaxies. Studying these substructures provides …