activity
20092026
most citedAn 800-million-solar-mass black hole in a significantly neutral Universe at redshift 7.5

1.1k citations · 7.2k across the 104 of their papers we have counts for

collaborators

106 papers

astro-ph.CO2026

A Robust Estimator for the Lyman- Forest 1D Power Spectrum at High Redshift

Molly Wolfson, Joseph F. Hennawi, Frederick B. Davies +1

The Lyman- (Ly) forest flux power spectrum is sensitive to a range of astrophysical and cosmological effects, including the thermal state of and large-scale fluctuatio…

astro-ph.GA2025

The Light Echo of a High-Redshift Quasar mapped with Lyman- Tomography

Anna-Christina Eilers, Minghao Yue, Jorryt Matthee +11

Ultra-violet (UV) radiation from accreting black holes ionizes the intergalactic gas around early quasars, carving out highly ionized bubbles in their surroundings. Any changes in…

astro-ph.CO2025

First constraints on the local ionization topology in front of two quasars at z ~ 7.5

Timo Kist, Joseph F. Hennawi, Frederick B. Davies +10

Thus far, Lyman- damping wings towards quasars have been used to probe the \textit{global} ionization state of the foreground intergalactic medium (IGM). A new parameterization…

astro-ph.CO2025

Inferring local quasar IGM damping wing constraints

Timo Kist, Joseph F. Hennawi, Frederick B. Davies

Lyman- damping wings towards quasars are a highly sensitive probe of the neutral hydrogen (HI) content in the foreground intergalactic medium (IGM), not only constraining the gl…

astro-ph.GA2025★ 4 cited

Quasar lifetime measurements from extended Ly nebulae at

Dominika Ďurovčíková, Anna-Christina Eilers, Romain A. Meyer +7

The existence of billion-solar-mass black holes hosted in luminous quasars within the first gigayear of cosmic history poses a challenge to our understanding of supermassive black…

astro-ph.CO2025★ 1 cited

A local, topology-independent parameterization of quasar IGM damping wings

Timo Kist, Joseph F. Hennawi, Frederick B. Davies

Lyman- damping wings towards quasars provide a unique probe of reionization because their strength correlates strongly with the global volume-averaged neutral hydrogen (HI) frac…

astro-ph.CO2024★ 1 cited

Quantifying the Precision of IGM Damping Wing Measurements Towards Quasars

Timo Kist, Joseph F. Hennawi, Frederick B. Davies

We investigate the precision with which the Lyman- damping wing signature imprinted on the spectra of high-redshift quasars (QSOs) by the foreground neutral intergalactic medium…

astro-ph.CO2024★ 3 cited

Precisely Measuring the Cosmic Reionization History from IGM Damping Wings Towards Quasars

Joseph F. Hennawi, Timo Kist, Frederick B. Davies +1

We introduce a new approach for analyzing the IGM damping wings imprinted on the proximity zones of quasars in the epoch of reionization (EoR). Whereas past work has typically forg…

astro-ph.GA2024★ 1 cited

A Spatially Resolved [CII] Survey of 31 Massive Galaxies Hosting Luminous Quasars

Feige Wang, Jinyi Yang, Xiaohui Fan +15

The [CII] 158 m emission line and the underlying far-infrared (FIR) dust continuum are important tracers for studying star formation and kinematic properties of early galaxies.…

astro-ph.GA2024

A Massive Protocluster Anchored by a Luminous Quasar at

Feige Wang, Jinyi Yang, Joseph F. Hennawi +13

Protoclusters, the progenitors of galaxy clusters, trace large scale structures in the early Universe and are important to our understanding of structure formation and galaxy evolu…

astro-ph.GA2024

Recognizing Blazars Using Radio Morphology from the VLA Sky Survey

Zhang-Liang Xie, Eduardo Banados, Silvia Belladitta +4

Blazars are radio-loud Active Galactic Nuclei (AGN) whose jets have a very small angle to our line of sight. Observationally, the radio emission are mostly compact or a compact-cor…

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★ 2 cited

Signatures of Small-scale Structure of the Pre-reionization Intergalactic Medium in Quasar Proximity Zones

Frederick B. Davies, Joseph F. Hennawi

The small-scale structure of baryons in the intergalactic medium is intimately linked to their past thermal history. Prior to the K photoheating during the epoch of r…

astro-ph.GA2023★ 4 cited

Possible Contamination of the Intergalactic Medium Damping Wing in ULAS J1342+0928 by Proximate Damped Ly Absorption

Frederick B. Davies, Eduardo Bañados, Joseph F. Hennawi +1

The red damping wing from neutral hydrogen in the intergalactic medium is a smoking-gun signal of ongoing reionization. One potential contaminant of the intergalactic damping wing…

astro-ph.CO2023★ 1 cited

The impact of varying inhomogeneous reionization histories on metrics of Ly opacity

Caitlin C. Doughty, Joseph F. Hennawi, Jose Oñorbe +2

The epoch of hydrogen reionization is complete by , but its progression at higher redshifts is uncertain. Measurements of Ly forest opacity show large scatter at , sug…

astro-ph.GA2023★ 4 cited

Searching for the Imprints of AGN Feedback on the Lyman Alpha Forest Around Luminous Red Galaxies

Vikram Khaire, Teng Hu, Joseph F. Hennawi +3

We explore the potential of using the low-redshift Lyman- (Ly) forest surrounding luminous red galaxies (LRGs) as a tool to constrain active galactic nuclei (AGN) feedback mo…

astro-ph.CO2023★ 4 cited

Forecasting constraints on the high-z IGM thermal state from the Lyman- forest flux auto-correlation function

Molly Wolfson, Joseph F. Hennawi, Frederick B. Davies +2

The auto-correlation function of the Lyman- (Ly) forest flux from high-z quasars can statistically probe all scales of the intergalactic medium (IGM) just after the epoch of…

astro-ph.CO2023

Measurements of the Lyman- forest flux auto-correlation functions from the extended XQR-30 data set

Molly Wolfson, Joseph F. Hennawi, Sarah E. I. Bosman +14

Recently, the Lyman- (Ly) forest flux auto-correlation function has been shown to be sensitive to the mean free path of hydrogen-ionizing photons, , for simul…

astro-ph.CO2023★ 3 cited

The Impact of the WHIM on the IGM Thermal State Determined from the Low- Lyman- Forest

Teng Hu, Vikram Khaire, Joseph F. Hennawi +4

At , shock heating caused by large-scale velocity flows and possibly violent feedback from galaxy formation, converts a significant fraction of the cool gas ($T\sim 1…

astro-ph.GA2023★ 1 cited

The relationship between IGM Lyman-alpha opacity and galaxy density near the end of reionization

Holly M. Christenson, George D. Becker, Anson D'Aloisio +6

Observed scatter in the Lyman-alpha opacity of quasar sightlines at has motivated measurements of the correlation between Ly opacity and galaxy density, as models that pre…

astro-ph.CO2023★ 1 cited

First measurement of the Mg II forest correlation function in the Epoch of Reionization

Suk Sien Tie, Joseph F. Hennawi, Feige Wang +5

In the process of producing the roughly three ionizing photons per atom required to reionize the IGM, the same massive stars explode and eject metals into their surroundings. While…

astro-ph.CO2023★ 2 cited

Probing Ultra-late Reionization: Direct Measurements of the Mean Free Path over

Yongda Zhu, George D. Becker, Holly M. Christenson +22

The mean free path of ionizing photons, , is a critical parameter for modeling the intergalactic medium (IGM) both during and after reionization. We present direct mea…

astro-ph.GA2023★ 80 cited

XQR-30: the ultimate XSHOOTER quasar sample at the reionization epoch

Valentina D'Odorico, E. Banados, G. D. Becker +46

The final phase of the reionization process can be probed by rest-frame UV absorption spectra of quasars at z>6, shedding light on the properties of the diffuse intergalactic mediu…

astro-ph.CO2023★ 9 cited

Can the Low Redshift Lyman Alpha Forest Constrain AGN Feedback Models?

Vikram Khaire, Teng Hu, Joseph F. Hennawi +2

We investigate the potential of low-redshift Lyman alpha (Ly) forest for constraining active galactic nuclei (AGN) feedback models by analyzing the Illustris and IllustrisTNG si…