3 papers
astro-ph.GA2025
From simulations to observations. Methodology and data release of mock TNG50 galaxies at 0.3 < z < 0.7 for WEAVE-StePS
A. Ikhsanova, L. Costantin, A. Pizzella +17
The new generation of optical spectrographs (i.e., WEAVE, 4MOST, DESI, and WST) offer unprecedented opportunities for statistically studying the star formation histories of galaxie…
astro-ph.GA2025
The COSMOS Wall at z ~ 0.73: Quiescent galaxies and their evolution in different environments
F. R. Ditrani, M. Longhetti, A. Iovino +12
The evolution of quiescent galaxies is driven by numerous physical processes, often considered to be related to their stellar mass and environment over cosmic time. Tracing their s…
astro-ph.GA2025
The COSMOS Wall at z0.73: star-forming galaxies and their evolution in different environments
S. Zhou, A. Iovino, M. Longhetti +11
We present a study of the evolution of star-forming galaxies within the so-called Wall structure at z0.73 in the field of the COSMOS survey. We use a sample of star-forming g…