activity
20162023
most citedImprints of temperature fluctuations on the Lyman- forest: a view from radiation-hydrodynamic simulations of reionization

47 citations · 289 across the 13 of their papers we have counts for

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Showing astro-ph.COShow all

5 papers · 1 filter

astro-ph.CO2022★ 1 cited

Non-parametric Lagrangian biasing from the insights of neural nets

Xiaohan Wu, Julian B. Munoz, Daniel J. Eisenstein

We present a Lagrangian model of galaxy clustering bias in which we train a neural net using the local properties of the smoothed initial density field to predict the late-time mas…

astro-ph.CO2021★ 4 cited

A fully Lagrangian, non-parametric bias model for dark-matter halos

Xiaohan Wu, Julian B. Munoz, Daniel Eisenstein

We present a non-parametric Lagrangian biasing model and fit the ratio of the halo and mass densities at the field level using the mass-weighted halo field in the AbacusSummit simu…

astro-ph.CO2021★ 12 cited

The high-redshift tail of stellar reionization in LCDM is beyond the reach of the low- CMB

Xiaohan Wu, Matthew McQuinn, Daniel Eisenstein +1

The first generation (Pop-III) stars can ionize 1-10% of the universe by , when the metal-enriched (Pop-II) stars may contribute negligibly to the ionization. This low ioniza…

astro-ph.CO2020★ 16 cited

On the accuracy of common moment-based radiative transfer methods for simulating reionization

Xiaohan Wu, Matthew McQuinn, Daniel Eisenstein

Cosmological simulations of reionization often treat radiative transfer by solving for the monopole and dipoles of the intensity field and by making ansatz for the quadrupole momen…

astro-ph.CO2019★ 47 cited

Imprints of temperature fluctuations on the Lyman- forest: a view from radiation-hydrodynamic simulations of reionization

Xiaohan Wu, Matthew McQuinn, Rahul Kannan +5

Reionization leads to large spatial fluctuations in the intergalactic temperature that can persist well after its completion. We study the imprints of such fluctuations on the $z\s…