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most citedThe Atlas3D project -- I. A volume-limited sample of 260 nearby early-type galaxies: science goals and selection criteria

1.1k citations · 19k across the 166 of their papers we have counts for

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astro-ph.GA2022★ 1 cited

Linking the Internal Properties of Infant Globular Clusters to their Formation Environments

Frederika Phipps, Sadegh Khochfar, Anna Lisa Varri +1

We investigate the formation of infant globular cluster (GC) candidates in high-resolution cosmological simulations from the First Billion Years (FiBY) project. By analysing the ev…

astro-ph.GA2022★ 6 cited

FOREVER22: the first bright galaxies with population III stars at redshifts and comparisons with JWST data

Hidenobu Yajima, Makito Abe, Hajime Fukushima +5

We study the formation of the first galaxies in overdense regions modelled by the FORmation and EVolution of galaxies in Extremely overdense Regions motivated by SSA22 (FOREVER22)…

astro-ph.HE2022★ 13 cited

Role of magnetic fields in the formation of direct collapse black holes

Muhammad A. Latif, Dominik R. G. Schleicher, Sadegh Khochfar

Direct collapse black holes (DCBHs) are the leading candidates for the origin of the first supermassive black holes. However, the role of magnetic fields during their formation is…

astro-ph.CO2022

The fate of baryons in counterfactual universes

Boon Kiat Oh, John A. Peacock, Sadegh Khochfar +1

We present results from nine simulations that compare the standard Cold Dark Matter cosmology (CDM) with counterfactual universes, for approximately using t…

astro-ph.GA2022★ 98 cited

Turbulent Cold Flows Gave Birth to the First Quasars

Muhammad A. Latif, Daniel J. Whalen, Sadegh Khochfar +2

How quasars powered by supermassive black holes (SMBHs) formed less than a billion years after the Big Bang is still one of the outstanding problems in astrophysics 20 years after…

astro-ph.IM2022★ 2 cited

A New Residual Distribution Hydrodynamics Solver for Astrophysical Simulations

Ben Morton, Sadegh Khochfar, Zhenyu Wu

Many astrophysical systems can only be accurately modelled when the behaviour of their baryonic gas components is well understood. The residual distribution (RD) family of partial…