activity
20042026
most cited21cmFAST: A Fast, Semi-Numerical Simulation of the High-Redshift 21-cm Signal

778 citations · 12.9k across the 191 of their papers we have counts for

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Showing 2016Show all

10 papers · 1 filter

astro-ph.CO2016★ 10 cited

Upper Limits on the 21 cm Power Spectrum at z = 5.9 from Quasar Absorption Line Spectroscopy

Jonathan C. Pober, Bradley Greig, Andrei Mesinger

We present upper limits on the 21 cm power spectrum at calculated from the model-independent limit on the neutral fraction of the intergalactic medium of $x_{\rm H{\small…

astro-ph.GA2016★ 26 cited

Dark-ages reionization and galaxy formation simulation--VII. The sizes of high-redshift galaxies

Chuanwu Liu, Simon J. Mutch, Gregory B. Poole +5

We investigate high-redshift galaxy sizes using a semi-analytic model constructed for the Dark-ages Reionization And Galaxy-formation Observables from Numerical Simulation project.…

astro-ph.IM2016★ 657 cited

Hydrogen Epoch of Reionization Array (HERA)

David R. DeBoer, Aaron R. Parsons, James E. Aguirre +51

The Hydrogen Epoch of Reionization Array (HERA) is a staged experiment to measure 21 cm emission from the primordial intergalactic medium (IGM) throughout cosmic reionization ($z=6…

astro-ph.CO2016★ 159 cited

Are we witnessing the epoch of reionisation at from the spectrum of J1120+0641?

Bradley Greig, Andrei Mesinger, Zoltán Haiman +1

We quantify the presence of Lyα damping wing absorption from a partially-neutral intergalactic medium (IGM) in the spectrum of the QSO, ULASJ1120+0641. Using a Bayesian fr…

astro-ph.CO2016★ 110 cited

First Limits on the 21 cm Power Spectrum during the Epoch of X-ray heating

A. Ewall-Wice, Joshua S. Dillon, J. N. Hewitt +62

We present first results from radio observations with the Murchison Widefield Array seeking to constrain the power spectrum of 21 cm brightness temperature fluctuations between the…

astro-ph.GA2016★ 117 cited

Lyα emission line reconstruction for high- QSOs

Bradley Greig, Andrei Mesinger, Ian D. McGreer +2

We introduce an intrinsic Lyα emission line profile reconstruction method for high- quasars (QSOs). This approach utilises a covariance matrix of emission line properties obtain…