output
19942026
most citedLOFAR: The LOw-Frequency ARray

2.7k citations

583 papers

astro-ph.GA2026

First statistical constraints on galactic scale outflows properties traced by their extended Mg II emission with MUSE

Ismael Pessa, Lutz Wisotzki, Tanya Urrutia +7

Galaxies evolve within vast gaseous halos that fuel star formation and carry signatures of feedback-driven outflows. Deep integral field data have enabled the study of MgII halos,…

astro-ph.GA2026★ 1 cited

ARCHITECTS I: Impact of subgrid physics on the simulated properties of the circumgalactic medium

Maxime Rey, Jérémy Blaizot, Taysun Kimm +2

Galaxy evolution is shaped by star formation and stellar feedback at scales unresolved by current high-resolution cosmological simulations. Precise subgrid models are thus necessar…

astro-ph.GA2025

KURVS: chemical properties from multiple strong line calibrations for star-forming galaxies at

Zefeng Li, Ugnė Dudzevičiūtė, Annagrazia Puglisi +13

Gas-phase oxygen abundance (metallicity) properties can be constrained through emission line analyses, and are of great importance to investigate galaxy evolution histories. We pre…

astro-ph.GA2025★ 1 cited

On the Dusty Proximate Damped Lyman-α System toward Q2310-3358 at z = 2.40

S. Han, J. -K. Krogager, C. Ledoux +6

Quasar absorption systems not only affect the way quasars are selected, but also serve as key probes of galaxies, providing insight into their chemical evolution and interstellar m…

astro-ph.IM2025★ 1 cited

Stellar halo subtraction alternative for accreting companions' characterization with integral field spectroscopy: Analytical and on-sky demonstration on the PDS70, HTLup, and YSES1 systems

R. Julo, M. Bonnefoy, F. Chatelain +5

Context. Medium-resolution IFS, such as MUSE at the VLT, are equipped to detect the emission lines of faint accreting companions when associated with dedicated stellar halo subtrac…

astro-ph.GA2025★ 5 cited

Targeting cluster galaxies for the 4MOST CHANCES Low-z sub-survey with photometric redshifts

Hugo Méndez-Hernández, Ciria Lima-Dias, Antonela Monachesi +54

The evolution of galaxies is shaped by both internal processes and their external environments. Galaxy clusters and their surroundings provide ideal laboratories to study these eff…