activity
20082021
most citedThe DESI Experiment Part I: Science,Targeting, and Survey Design

1.3k citations · 2.8k across the 23 of their papers we have counts for

collaborators
Showing astro-ph.COShow all

12 papers · 1 filter

astro-ph.CO2021★ 9 cited

Improving IGM temperature constraints using wavelet analysis on high-redshift quasars

Molly Wolfson, Joseph F. Hennawi, Frederick B. Davies +3

The thermal state of the intergalactic medium (IGM) contains vital information about the epoch of reionization, one of the most transformative yet poorly understood periods in the…

astro-ph.CO2021★ 14 cited

HyPhy: Deep Generative Conditional Posterior Mapping of Hydrodynamical Physics

Benjamin Horowitz, Max Dornfest, Zarija Lukić +1

Generating large volume hydrodynamical simulations for cosmological observables is a computationally demanding task necessary for next generation observations. In this work, we con…

astro-ph.CO2021★ 15 cited

Fast, high-fidelity Lyman forests with convolutional neural networks

Peter Harrington, Mustafa Mustafa, Max Dornfest +2

Full-physics cosmological simulations are powerful tools for studying the formation and evolution of structure in the universe but require extreme computational resources. Here, we…

astro-ph.CO2018★ 45 cited

The Power Spectrum of the Lyman- Forest at z < 0.5

Vikram Khaire, Michael Walther, Joseph F. Hennawi +6

We present new measurements of the flux power-spectrum P(k) of the HI Lyman- forest spanning scales k ~ 0.001-0.1 s/km. These results were derived from 65 far ultraviole…

astro-ph.CO2018★ 168 cited

New Constraints on IGM Thermal Evolution from the Lyα Forest Power Spectrum

Michael Walther, Jose Oñorbe, Joseph F. Hennawi +1

We determine the thermal evolution of the intergalactic medium (IGM) over of cosmic time by comparing measurements of the Lyα forest power spectrum t…

astro-ph.CO2018★ 313 cited

Quantitative Constraints on the Reionization History from the IGM Damping Wing Signature in Two Quasars at z > 7

Frederick B. Davies, Joseph F. Hennawi, Eduardo Bañados +10

During reionization, neutral hydrogen in the intergalactic medium (IGM) imprints a damping wing absorption feature on the spectrum of high-redshift quasars. A detection of this sig…

astro-ph.CO2017★ 36 cited

A Detection of ~2.3 Cosmic Voids from 3D Lyman- Forest Tomography in the COSMOS Field

Alex Krolewski, Khee-Gan Lee, Martin White +10

We present the most distant detection of cosmic voids () and the first detection of three-dimensional voids in the Lyman- forest. We used a 3D tomographic map of the…

astro-ph.CO2017★ 54 cited

A New Method to Measure the Post-Reionization Ionizing Background from the Joint Distribution of Lyman- and Lyman- Forest Transmission

Frederick B. Davies, Joseph F. Hennawi, Anna-Christina Eilers +1

The amplitude of the ionizing background that pervades the intergalactic medium (IGM) at the end of the epoch of reionization provides a valuable constraint on the emissivity of th…

astro-ph.CO2016★ 106 cited

Self-Consistent Modeling of Reionization in Cosmological Hydrodynamical Simulations

Jose Oñorbe, Joseph F Hennawi, Zarija Lukić

The ultraviolet background (UVB) emitted by quasars and galaxies governs the ionization and thermal state of the intergalactic medium (IGM), regulates the formation of high-redshif…

astro-ph.CO2016★ 35 cited

Modeling the Lyman-alpha Forest in Collisionless Simulations

Daniele Sorini, José Oñorbe, Zarija Lukić +1

Cosmological hydrodynamic simulations can accurately predict the properties of the intergalactic medium (IGM), but only under the condition of retaining high spatial resolution nec…

astro-ph.CO2010★ 187 cited

Mass Function Predictions Beyond LCDM

Suman Bhattacharya, Katrin Heitmann, Martin White +3

The mass distribution of halos, as specified by the halo mass function, is a key input for several cosmological probes. The sizes of -body simulations are now such that, for the…

astro-ph.CO2010★ 21 cited

Galaxy Clusters as a probe of early dark energy

Ujjaini Alam, Zarija Lukić, Suman Bhattacharya

We study a class of early dark energy (EDE) models, in which, unlike in standard dark energy models, a substantial amount of dark energy exists in the matter-dominated era. We self…