activity
20122026
most citedDamping Wing-Like Features in the Stacked Ly Forest: Potential Neutral Hydrogen Islands at

52 citations · 149 across the 20 of their papers we have counts for

collaborators

20 papers

astro-ph.GA2026

Probing Direct Contributions of Galaxies and AGN to Cosmic Reionization in a Quasar Field J0226+0302 with JWST NIRCam and NIRSpec

Xiangyu Jin, Jinyi Yang, Feige Wang +19

We present JWST Cycle 2 NIRCam and NIRSpec observations in a quasar field J0226+0302 at z=6.5412 to probe the direct connections between the intergalactic medium (IGM), galaxies, a…

astro-ph.GA2026★ 1 cited

E-XQR-30: Evidence for an Increase in the Ionization State of Metal Absorbers from z~6 to z~2

Stephanie Rowlands, R. L. Davies, E. Ryan-Weber +15

We investigate the evolution of the ionization state of metal-enriched gas in and around galaxies near the epoch of reionization using a sample of 488 metal absorption systems at 4…

astro-ph.CO2025★ 7 cited

Updated dark pixel fraction constraints on reionization's end from the Lyman-series forests of XQR-30

Frederick B. Davies, Sarah E. I. Bosman, Valentina D'Odorico +16

The fraction of "dark pixels" in the Ly and other Lyman-series forests at provides a powerful constraint on the end of the reionization process. Any spectral region…

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★ 3 cited

Ly Emission from [OIII] Emitters Near Reionization: The role of environment in galaxy Ly detection

Seyedazim Hashemi, George D. Becker, Yongda Zhu +1

Using galaxy Ly emission to probe reionization relies on establishing baseline expectations for its detectability in the absence of attenuation by neutral gas in the IGM. Toward…

astro-ph.GA2025★ 4 cited

An extremely metal-poor Lyman emitter candidate at revealed through absorption spectroscopy

Dominika Ďurovčíková, Anna-Christina Eilers, Robert A. Simcoe +10

We report the discovery of a Lyman emitter (LAE) candidate in the immediate foreground of the quasar PSO J158-14 at at a projected distance $\sim29\ {\rm p…

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.GA2025★ 4 cited

JWST ASPIRE: How Did Galaxies Complete Reionization? Evidence for Excess IGM Transmission around Emitters during Reionization

Koki Kakiichi, Xiangyu Jin, Feige Wang +23

The spatial correlation between galaxies and the Ly forest provides insights into how galaxies reionized the Universe. Here, we present initial results on the spatial cross-corr…

astro-ph.CO2025

How probable is the Lyman- damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600?

Fiona Sawyer, James S. Bolton, George D. Becker +5

The shape of the Ly- transmission in the near zone of the redshift quasar ULAS J01480600 (hereafter J0148) is consistent with a damping wing arising from an extend…

astro-ph.CO2024★ 2 cited

Percent-level timing of reionization: self-consistent, implicit-likelihood inference from XQR-30+ Ly forest data

Yuxiang Qin, Andrei Mesinger, David Prelogović +13

The Lyman alpha (Lya) forest in the spectra of z>5 quasars provides a powerful probe of the late stages of the Epoch of Reionization (EoR). With the recent advent of exquisite data…

astro-ph.CO2024★ 1 cited

A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): JWST Supports Earlier Reionization around [OIII] Emitters

Xiangyu Jin, Jinyi Yang, Xiaohui Fan +22

Understanding when and how reionization happened is crucial for studying the early structure formation and the properties of first galaxies in the Universe. At , the observe…

astro-ph.GA2024

No Redshift Evolution in the Fe II/Mg II Flux Ratios of Quasars across Cosmic Time

Danyang Jiang, Masafusa Onoue, Linhua Jiang +13

The Fe II/Mg II emission line flux ratio in quasar spectra serves as a proxy for the relative Fe to alpha-element abundances in the broad line regions of quasars. Due to the expect…

astro-ph.CO2024★ 52 cited

Damping Wing-Like Features in the Stacked Ly Forest: Potential Neutral Hydrogen Islands at

Yongda Zhu, George D. Becker, Sarah E. I. Bosman +28

Recent quasar absorption line observations suggest that reionization may end as late as . As a means to search for large neutral hydrogen islands at , we revisi…

astro-ph.CO2024★ 3 cited

Damping wing absorption associated with a giant Ly trough at : direct evidence for late-ending reionization

George D. Becker, James S. Bolton, Yongda Zhu +1

Multiple observations now suggest that the hydrogen reionization may have ended well below redshift six. While there has previously been no conclusive proof of extended neutral isl…

astro-ph.CO2024

IGM damping wing constraints on the tail end of reionisation from the enlarged XQR-30 sample

Bradley Greig, Andrei Mesinger, Eduardo Bañados +16

The attenuation of Ly photons by neutral hydrogen in the intergalactic medium (IGM) at continues to be a powerful probe for studying the epoch of reionisation. Given…

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…

astro-ph.GA2024★ 15 cited

Chemical Diagnostics to Unveil Environments Enriched by First Stars

Irene Vanni, Stefania Salvadori, Valentina D'Odorico +2

Unveiling the chemical fingerprints of the first (Pop III) stars is crucial for indirectly studying their properties and probing their massive nature. In particular, very massive P…

astro-ph.CO2023

Constraints on the Evolution of the Ionizing Background and Ionizing Photon Mean Free Path at the End of Reionization

Frederick B. Davies, Sarah E. I. Bosman, Prakash Gaikwad +16

The variations in Ly forest opacity observed at between lines of sight to different background quasars are too strong to be caused by fluctuations in the density field a…

astro-ph.CO2023★ 1 cited

The effect of reionization on direct measurements of the mean free path

Joshua T. Roth, Anson D'Aloisio, Christopher Cain +3

Recent measurements of the ionizing photon mean free path (MFP) based on composite quasar spectra may point to reionization ending at . These measurements are challenging beca…

astro-ph.CO2012★ 35 cited

Thermal constraints on the reionisation of hydrogen by population-II stellar sources

Sudhir Raskutti, James S. Bolton, J. Stuart B. Wyithe +1

Measurements of the intergalactic medium (IGM) temperature provide a potentially powerful constraint on the reionisation history due to the thermal imprint left by the photo-ionisa…