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20042009
most citedEfficient Simulations of Early Structure Formation and Reionization

454 citations · 1.1k across the 9 of their papers we have counts for

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astro-ph2008261 cited

Fluctuations in the High-Redshift Lyman-Werner Background: Close Halo Pairs as the Origin of Supermassive Black Holes

Mark Dijkstra, Zoltan Haiman, Andrei Mesinger +1

The earliest generation of stars and black holes must have established an early 'Lyman-Werner' background (LWB) at high redshift, prior to the epoch of reionization. Because of the…

astro-ph200849 cited

The ionizing background at the end of overlap

Steven Furlanetto, Andrei Mesinger

One of the most sought-after signatures of reionization is a rapid increase in the ionizing background (usually measured through the Lyman-alpha optical depth toward distant quasar…

astro-ph200885 cited

UV Radiative Feedback During the Advanced Stages of Reionization

Andrei Mesinger, Mark Dijkstra

The ionizing ultraviolet background (UVB) during reionization can suppress the gas content of low-mass galaxies, even those capable of efficient atomic cooling, and thus lead to an…

astro-ph200784 cited

Lyman-alpha Damping Wing Constraints on Inhomogeneous Reionization

Andrei Mesinger, Steven Furlanetto

One well-known way to constrain the hydrogen neutral fraction, x_H, of the high-redshift intergalactic medium (IGM) is through the shape of the red damping wing of the Lya absorpti…

astro-ph200797 cited

Lyman-alpha Emitters During the Early Stages of Reionization

Andrei Mesinger, Steven Furlanetto

We investigate the potential of exploiting Lya Emitters (LAEs) to constrain the volume-weighted mean neutral hydrogen fraction of the IGM, x_H, at high redshifts (specifically z~9)…

astro-ph2007454 cited

Efficient Simulations of Early Structure Formation and Reionization

Andrei Mesinger, Steven Furlanetto

We present a method to construct semi-numerical ``simulations'', which can efficiently generate realizations of halo distributions and ionization maps at high redshifts. Our proced…