activity
20042023
most citedGalaxy Clusters around radio-loud AGN at 1.3 < z < 3.2 as seen by Spitzer

236 citations · 4.1k across the 75 of their papers we have counts for

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Showing astro-ph.COShow all

26 papers · 1 filter

astro-ph.CO2022★ 10 cited

Probing quasar lifetimes with proximate -centimetre absorption in the diffuse intergalactic medium at redshifts

Tomáš Šoltinský, James S. Bolton, Margherita Molaro +5

Enhanced ionizing radiation in close proximity to redshift quasars creates short windows of intergalactic Ly transmission blueward of the quasar Ly emission line…

astro-ph.CO2021★ 8 cited

Searching for the shadows of giants II: the effect of local ionisation on the Lyman- absorption signatures of protoclusters at redshift

Joel S. A. Miller, James S. Bolton, Nina Hatch

Local variations in the intergalactic medium (IGM) neutral hydrogen fraction will affect the Ly- absorption signature of protoclusters identified in tomographic surveys. Using t…

astro-ph.CO2021★ 18 cited

The detectability of strong 21 centimetre forest absorbers from the diffuse intergalactic medium in late reionisation models

Tomáš Šoltinský, James S. Bolton, Nina Hatch +6

A late end to reionisation at redshift is consistent with observed spatial variations in the Ly forest transmission and the deficit of Ly emitting galaxies arou…

astro-ph.CO2019★ 13 cited

Searching for the shadows of giants: characterising protoclusters with line of sight Lyman-α absorption

Joel S. A. Miller, James S. Bolton, Nina Hatch

We use state of the art hydrodyamical simulations from the Sherwood, EAGLE and Illustris projects to examine the signature of protoclusters obs…

astro-ph.CO2015★ 196 cited

What are Protoclusters? -- Defining High Redshift Galaxy Clusters and Protoclusters

Stuart I. Muldrew, Nina A. Hatch, Elizabeth A. Cooke

We explore the structures of protoclusters and their relationship with high redshift clusters using the Millennium Simulation combined with a semi-analytic model. We find that prot…

astro-ph.CO2014★ 80 cited

The Galaxy Cluster Mid-Infrared Luminosity Function at 1.3<z<3.2

Dominika Wylezalek, Joël Vernet, Carlos De Breuck +8

We present 4.5 μm luminosity functions for galaxies identified in 178 candidate galaxy clusters at 1.3 < z < 3.2. The clusters were identified as Spitzer/IRAC color-selected overde…