Understanding the properties of dust attenuation curves in galaxies and the physical
mechanisms that shape them are among the fundamental questions of extragalactic …

I present a comprehensive review of the evolution of galaxy structure in the Universe from
the first galaxies currently observable at z∼ 6 down to galaxies observable in the local …

We introduce serra, a suite of zoom-in high-resolution (, at z= 7.7) cosmological simulations
including non-equilibrium chemistry and on-the-fly radiative transfer. The outputs are post …

▪ Abstract Observations of star formation rates (SFRs) in galaxies provide vital clues to the
physical nature of the Hubble sequence and are key probes of the evolutionary histories of …

Young massive clusters (YMCs) are dense aggregates of young stars that form the
fundamental building blocks of galaxies. Several examples exist in the Milky Way Galaxy …

▪ Abstract At luminosities above 1011, infrared galaxies become the dominant population of
extragalactic objects in the local Universe (z≲ 0.3), being more numerous than optically …

We present a new model for computing the effects of dust on the integrated spectral
properties of galaxies, based on an idealized description of the main features of the …

We present new calibrations of far-ultraviolet (FUV) attenuation as derived from the total
infrared to FUV luminosity ratio (IRX) and the FUV–near-UV (NUV) color. We find that the …

▪ Abstract Galactic winds are the primary mechanism by which energy and metals are
recycled in galaxies and are deposited into the intergalactic medium. New observations are …

We refine a technique to measure the absorption-corrected ultraviolet (UV) luminosity of
starburst galaxies using rest-frame UV quantities alone and apply it to Lyman-limit U …