activity
20072021
most citedConditions for Reionizing the Universe with A Low Galaxy Ionizing Photon Escape Fraction

339 citations · 419 across the 6 of their papers we have counts for

collaborators

16 papers

astro-ph.CO202141 cited

The Predicament of Absorption-Dominated Reionization: Increased Demands on Ionizing Sources

Frederick B. Davies, Sarah E. I. Bosman, Steven R. Furlanetto +2

The reionization epoch concludes when ionizing photons reach every corner of the Universe. Reionization has generally been assumed to be limited primarily by the rate at which gala…

astro-ph.CO2021

A short mean free path at favors late and rapid reionization by faint galaxies

Christopher Cain, Anson D'Aloisio, Nakul Gangolli +1

Recent measurements of the ionizing photon mean free path () at suggest that the IGM was rapidly evolving at those times. We use radiative transfer s…

astro-ph.CO2021

The mean free path of ionizing photons at 5 < z < 6: evidence for rapid evolution near reionization

George D. Becker, Anson D'Aloisio, Holly M. Christenson +3

The mean free path of ionizing photons, , is a key factor in the photoionization of the intergalactic medium (IGM). At , however, may be sho…

astro-ph.CO202019 cited

Constraining Reionization in Progress at z=5.7 with Lyman- Emitters: Voids, Peaks, and Cosmic Variance

Nakul Gangolli, Anson D'Aloisio, Fahad Nasir +1

A number of independent observations suggest that the intergalactic medium was significantly neutral at and that reionization was, perhaps, still in progress at . The…

astro-ph.CO2020

A Model-Insensitive Baryon Acoustic Oscillation Feature in the 21 cm Signal from Reionization

Christopher Cain, Anson D'Aloisio, Vid Iršič +2

We examine the impact of baryon-dark matter relative velocities on intergalactic small-scale structure and the 21 cm signal during reionization. Streaming velocities reduced clumpi…

astro-ph.CO2020

Hydrodynamic Response of the Intergalactic Medium to Reionization

Anson D'Aloisio, Matthew McQuinn, Hy Trac +2

The intergalactic medium is expected to clump on scales down to M before the onset of reionization. The impact of these small-scale structures on reionization…