activity
20152026
most citedModels of the Thermal Evolution of the Intergalactic Medium After Reionization

97 citations · 350 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2026

OCEANS of Absorption: High-resolution NIRSpec Spectroscopy Reveals Diverse Balmer-line Absorption in Little Red Dots

Kelcey Davis, Madisyn Brooks, Raymond C. Simons +24

The ``Little Red Dots' (LRDs) that appeared in JWST deep field images have been the subject of significant study since their discovery. In this work, we present high-resolution fol…

astro-ph.GA2026

Extreme Emission Line Galaxies in CEERS Are Powered by Star Formation, not AGN

Kelcey Davis, Madisyn Brooks, Jonathan R. Trump +28

We present a spectroscopic study of photometrically identified extreme emission-line galaxies (EELGs) with observed-frame equivalent widths (EWs) >5000 A of either H alpha or H bet…

astro-ph.GA2025★ 2 cited

Population III star formation near high-redshift active galactic nuclei

Ethan M. Fisk, Madeline A. Marshall, Phoebe R. Upton Sanderbeck +1

Using cosmological radiation-hydrodynamical simulations, we study the effect of accreting supermassive black holes (SMBHs) on nearby dark-matter (DM) haloes in the very early unive…

astro-ph.GA2023

An Estimate of the Impact of Reionization on Supermassive Black Hole Growth

Phoebe R. Upton Sanderbeck, Jarrett L. Johnson, Madeline A. Marshall

The supermassive black holes (SMBHs) that power active galactic nuclei found at were formed during the epoch of reionization. Because reionization is an inhomogeneous proce…

astro-ph.GA2022

A Simple Condition for Sustained Super-Eddington Black Hole Growth

Jarrett Lawrence Johnson, Phoebe R. Upton Sanderbeck

One of the most pressing questions in cosmology is how the black holes (BHs) powering quasars at high redshift grow to supermassive scales within a billion years of the Big Bang. H…

astro-ph.CO2020★ 38 cited

Inhomogeneous HeII reionization in Hydrodynamic Simulations

Phoebe Upton Sanderbeck, Simeon Bird

The reionization of the second electron of helium shapes the physical state of intergalactic gas at redshifts between 2 < z < 5. Because performing full in situ radiative transfer…

astro-ph.CO2017★ 30 cited

The Sources of Extreme Ultraviolet and Soft X-ray Backgrounds

Phoebe R. Upton Sanderbeck, Matthew McQuinn, Anson D'Aloisio +1

Radiation in the extreme ultraviolet (EUV) and soft X-ray holds clues to the location of the missing baryons, the energetics in stellar feedback processes, and the cosmic enrichmen…

astro-ph.CO2016★ 87 cited

On the Contribution of Active Galactic Nuclei to the High-Redshift Metagalactic Ionizing Background

Anson D'Aloisio, Phoebe R. Upton Sanderbeck, Matthew McQuinn +2

Motivated by the claimed detection of a large population of faint active galactic nuclei (AGN) at high redshift, recent studies have proposed models in which AGN contribute signifi…

astro-ph.CO2015★ 97 cited

Models of the Thermal Evolution of the Intergalactic Medium After Reionization

Phoebe R. Upton Sanderbeck, Anson D'Aloisio, Matthew J. McQuinn

Recent years have brought more precise temperature measurements of the low-density intergalactic medium (IGM). These new measurements constrain the processes that heated the IGM, s…

astro-ph.CO2015★ 96 cited

On the intergalactic temperature-density relation

Matthew McQuinn, Phoebe R. Upton Sanderbeck

Cosmological simulations of the low-density intergalactic medium exhibit a strikingly tight power-law relation between temperature and density that holds over two decades in densit…