activity
20102026
most citedNew Constraints on the free-streaming of warm dark matter from intermediate and small scale Lyman- forest data

540 citations · 5.3k across the 112 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

46 papers · 1 filter

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

Detecting the IGM metal enrichment with the 2-point correlation function of the flux. Application to the UVES deep spectrum

Simona Di Stefano, Valentina D'Odorico, Guido Cupani +5

The distribution and the abundance of metals in the intergalactic medium (IGM) have strong implications on galaxy formation and evolution models. The ionic transitions of heavy ele…

astro-ph.GA2025★ 1 cited

The clustering of C IV and Si IV at the end of reionisation: A perspective from the E-XQR-30 survey

Louise Welsh, Valentina D'Odorico, Fabio Fontanot +14

We aim to study the clustering of metal absorption lines and the structures that they arise in as a function of cosmic time. We focus on C IV and Si IV absorption features that are…

astro-ph.GA2025★ 2 cited

Multi-phase investigation of outflows in the circumgalactic and interstellar media of luminous quasars at z~5

Matilde Brazzini, Valentina D'Odorico, Manuela Bischetti +4

Aims. Outflows from active galactic nuclei are invoked as the principal feedback process regulating the co-evolution of supermassive black holes and their host galaxies. Because of…

astro-ph.GA2024

Isotopic abundance of carbon in the DLA towards QSO B1331+170

Dinko Milaković, John K. Webb, Paolo Molaro +19

Chemical evolution models predict a gradual build-up of C in the universe, based on empirical nuclear reaction rates and assumptions on the properties of stellar populations…

astro-ph.GA2024★ 18 cited

Evidence of Pop~III stars' chemical signature in neutral gas at z~6. A study based on the E-XQR-30 spectroscopic sample

Alessio Sodini, Valentina D'Odorico, Stefania Salvadori +16

This study explores the metal enrichment signatures attributed to the first generation of stars (PopIII) in the Universe, focusing on the E-XQR-30 sample. We aim to identify traces…