activity
20242026
collaborators

6 papers

astro-ph.GA2026

The multiple coherence scales of C IV at cosmic noon

H. Cortés-Muñoz, S. Lopez, N. Tejos +6

The spatial and kinematic structure of the circumgalactic medium (CGM) remains poorly constrained observationally. In this article we compute the clustering of CIV absorption syste…

astro-ph.CO2026

One H2 molecule per ten million H-atoms reveals sub-pc scale cold overdensities at z~4

P. Noterdaeme, S. Balashev, T. Berg +11

We present the detection and analysis of H2 absorption at z = 4.24 towards the bright quasar J0007-5705, observed with the Very Large Telescope as part of the ESPRESSO QUasar Absor…

astro-ph.GA2025

From the Intergalactic to the Interstellar Scales -- EQUALS: a High-resolution Legacy Survey of Gas in the Distant Universe Using ESPRESSO

Trystyn Berg, Valentina D'Odorico, Elisa Boera +14

Understanding how the Universe evolved from diffuse primordial gas into the rich cosmic web we observe today is one of the great challenges of modern astrophysics. Quasar absorptio…

astro-ph.GA2025

Quasar radiation transforms the gas in a merging companion galaxy

Sergei Balashev, Pasquier Noterdaeme, Neeraj Gupta +7

Quasars, powered by gas accretion onto supermassive black holes, rank among the most energetic objects of the Universe. While they are thought to be ignited by galaxy mergers and a…

astro-ph.GA2025

Exploring quasar evolution with proximate molecular absorbers: Insights from the kinematics of highly ionized nitrogen

R. Cuellar, P. Noterdaeme, S. Balashev +3

We investigate the presence and kinematics of NV absorption proximate to high redshift quasars selected upon the presence of strong and HI absorption at the quasar redshift…

astro-ph.GA2024

Transverse clues on the kpc-scale structure of the circumgalactic medium as traced by C IV absorption

S. Lopez, A. Afruni, D. Zamora +13

We present VLT/MUSE integral-field spectroscopy () of four giant gravitational arcs exhibiting strong C IV absorption at 8 intervening redshifts, $z_{abs}\approx 2…