papers

Publications (33)

astro-ph.IM2024

SWIFT: A modern highly-parallel gravity and smoothed particle hydrodynamics solver for astrophysical and cosmological applications

Matthieu Schaller, Josh Borrow, Peter W. Draper +24

Numerical simulations have become one of the key tools used by theorists in all the fields of astrophysics and cosmology. The development of modern tools that target the largest ex…

astro-ph.GA2017

The link between galaxy and black hole growth in the EAGLE simulation

Stuart McAlpine, Richard G. Bower, Chris M. Harrison +4

We investigate the connection between the star formation rate (SFR) of galaxies and their central black hole accretion rate (BHAR) using the EAGLE cosmological hydrodynamical simul…

astro-ph.GA2022

SIBELIUS-DARK: a galaxy catalogue of the Local Volume from a constrained realisation simulation

Stuart McAlpine, John C. Helly, Matthieu Schaller +7

We present SIBELIUS-DARK, a constrained realisation simulation of the local volume to a distance of 200~Mpc from the Milky Way. SIBELIUS-DARK is the first study of the \textit{Simu…

astro-ph.GA2021

Supermassive black holes in cosmological simulations I: M_BH-M_star relation and black hole mass function

Melanie Habouzit, Yuan Li, Rachel S. Somerville +15

The past decade has seen significant progress in understanding galaxy formation and evolution using large-scale cosmological simulations. While these simulations produce galaxies i…

astro-ph.GA2020

Galaxy mergers in EAGLE do not induce a significant amount of black hole growth yet do increase the rate of luminous AGN

Stuart McAlpine, Chris M. Harrison, David J. Rosario +4

We investigate the connection between galaxy--galaxy mergers and enhanced black hole (BH) growth using the cosmological hydrodynamical EAGLE simulation. We do this via three method…

astro-ph.GA2019

The nature of sub-millimeter and highly star-forming galaxies in the EAGLE simulation

Stuart McAlpine, Ian Smail, Richard G. Bower +7

We exploit EAGLE, a cosmological hydrodynamical simulation, to reproduce the selection of the observed sub-millimeter (submm) galaxy population by selecting the model galaxies at $…

astro-ph.GA2018

The abundances and properties of Dual AGN and their host galaxies in the EAGLE simulations

Yetli Rosas-Guevara, Richard Bower, Stuart McAlpine +2

We look into the abundance of Dual AGN in the largest hydrodynamical simulation from the EAGLE project. We define a Dual AGN as two active black holes (BHs) with a separation below…

astro-ph.GA2018

The rapid growth phase of supermassive black holes

Stuart McAlpine, Richard G. Bower, David J. Rosario +3

We investigate the rapid growth phase of supermassive black holes (BHs) within the hydrodynamical cosmological \eagle simulation. This non-linear phase of BH growth occurs within $…

astro-ph.CO2026

The Manticore-Local Cluster Catalogue: A Posterior Map of Massive Structures in the Nearby Universe

Stuart McAlpine

We present a publicly available catalogue of massive structures in the nearby Universe, constructed from the Manticore-Local posterior ensemble, a Bayesian field-level reconstructi…

astro-ph.CO2020

Setting the Stage: Structures from Gaussian Random Fields

Till Sawala, Adrian Jenkins, Stuart McAlpine +4

We study structure formation in a set of cosmological simulations to uncover the scales in the initial density field that gave rise to the formation of present-day structures. Our…

astro-ph.GA2016

The EAGLE simulations of galaxy formation: public release of halo and galaxy catalogues

Stuart McAlpine, John C. Helly, Matthieu Schaller +16

We present the public data release of halo and galaxy catalogues extracted from the EAGLE suite of cosmological hydrodynamical simulations of galaxy formation. These simulations we…

astro-ph.CO2026

Learning the Universe: Constrained simulations of the Coma galaxy cluster -- I. Radial X-ray and Compton-y signatures

Ulrich P. Steinwandel, Stuart McAlpine, Richard Stiskalek +7

We present a suite of 50 high-fidelity simulations of Coma cluster analogues constructed from BORG/MANTICORE constrained initial conditions and evolved with the IllustrisTNG galaxy…

astro-ph.CO2025

The Manticore Project I: a digital twin of our cosmic neighbourhood from Bayesian field-level analysis

Stuart McAlpine, Jens Jasche, Metin Ata +4

We present the first results from the Manticore project, dubbed Manticore-Local, a suite of Bayesian constrained simulations of the nearby Universe, generated by fitting a physical…

astro-ph.CO2026

Revisiting the Great Attractor: The Local Group's streamline trajectory, cosmic velocity and dynamical fate

Richard Stiskalek, Harry Desmond, Stuart McAlpine +3

We revisit the Great Attractor using the Manticore-Local suite of digital twins of the nearby Universe. The Great Attractor concept has been proposed as an answer to three distinct…

astro-ph.GA2019

The gas fractions of dark matter haloes hosting simulated galaxies are governed by the feedback history of their black holes

Jonathan J. Davies, Robert A. Crain, Ian G. McCarthy +4

We examine the origin of scatter in the relationship between the gas fraction and mass of dark matter haloes hosting present-day central galaxies in the EAGLE simula…

astro-ph.CO2021

The SIBELIUS Project: E Pluribus Unum

Till Sawala, Stuart McAlpine, Jens Jasche +4

We introduce "Simulations Beyond The Local Universe" (SIBELIUS) that connect the Local Group to its cosmic environment. We show that introducing hierarchical small-scale perturbati…

astro-ph.GA2016

Supermassive black holes in the EAGLE Universe. Revealing the observables of their growth

Yetli Rosas-Guevara, Richard G. Bower, Joop Schaye +5

We investigate the evolution of supermassive black holes in the `Evolution and Assembly of GaLaxies and their Environments' (EAGLE) cosmological hydrodynamic simulations. The large…

astro-ph.GA2016

Music from the heavens - Gravitational waves from supermassive black hole mergers in the EAGLE simulations

Jaime Salcido, Richard G. Bower, Tom Theuns +5

We estimate the expected event rate of gravitational wave signals from mergers of supermassive black holes that could be resolved by a space-based interferometer, such as the Evolv…

astro-ph.GA2019

The aftermath of the Great Collision between our Galaxy and the Large Magellanic Cloud

Marius Cautun, Alis J. Deason, Carlos S. Frenk +1

The Milky Way (MW) offers a uniquely detailed view of galactic structure and is often regarded as a prototypical spiral galaxy. But recent observations indicate that the MW is atyp…

astro-ph.GA2017

Data release of UV to submm broadband fluxes for simulated galaxies from the EAGLE project

Peter Camps, Ana Trčka, James Trayford +6

We present dust-attenuated and dust emission fluxes for sufficiently resolved galaxies in the EAGLE suite of cosmological hydrodynamical simulations, calculated with the SKIRT radi…

astro-ph.GA2019

Evolution of the cold gas properties of simulated post-starburst galaxies

Timothy A. Davis, Freeke van de Voort, Kate Rowlands +3

Post-starburst galaxies are typically considered to be a transition population, en route to the red sequence after a recent quenching event. Despite this, recent observations have…

astro-ph.CO2025

A Bayesian catalog of 100 high-significance voids in the Local Universe

Rosa Malandrino, Guilhem Lavaux, Benjamin D. Wandelt +2

While cosmic voids are now recognized as a valuable cosmological probe, identifying them in a galaxy catalog is challenging for multiple reasons: observational effects such as hole…

astro-ph.GA2023

Modelling the accretion and feedback of supermassive black hole binaries in gas-rich galaxy mergers

Shihong Liao, Peter H. Johansson, Matias Mannerkoski +6

We introduce a new model for the accretion and feedback of supermassive black hole (SMBH) binaries to the KETJU code, which enables us to resolve the evolution of SMBH binaries dow…

astro-ph.CO2026

The Manticore Project II: Bayesian digital twins of cosmic structure across the SDSS and BOSS volumes

Stuart McAlpine, Jens Jasche, Guilhem Lavaux +2

We present Manticore-Deep, a high-resolution Bayesian field-level reconstruction of cosmic large-scale structure over a comoving volume of to $z\approx…

astro-ph.CO2026

Reconstructing the largest scales of the Universe with field-level inference applied to the Quaia Quasar Catalogue

Adam Andrews, Arthur Loureiro, Jens Jasche +3

The recently released Quaia quasar catalogue, with its broad redshift range and all-sky coverage, enables unprecedented three-dimensional reconstructions of matter across cosmic ti…

astro-ph.CO2026

Illuminating the Local Universe: Large-Scale Structure from ZTF Type Ia Supernovae

Antoine Gilles Lordet, Ariel Goobar, Jens Jasche +12

Within the volume-limited subsample at of the Zwicky Transient Facility (ZTF) DR2 sample, we confirm a statistically significant excess of Type Ia supernovae (SNe Ia) at $…

astro-ph.GA2020

Interacting galaxies in the IllustrisTNG simulations -- I: Triggered star formation in a cosmological context

David R. Patton, Kieran D. Wilson, Colin J. Metrow +7

We use the IllustrisTNG cosmological hydrodynamical simulations to investigate how the specific star formation rates (sSFRs) of massive galaxies depend on…

astro-ph.GA2021

Supermassive black holes in cosmological simulations II: the AGN population and predictions for upcoming X-ray missions

Melanie Habouzit, Rachel S. Somerville, Yuan Li +13

In large-scale hydrodynamical cosmological simulations, the fate of massive galaxies is mainly dictated by the modeling of feedback from active galactic nuclei (AGN). The amount of…

astro-ph.GA2022

The Milky Way's plane of satellites: consistent with CDM

Till Sawala, Marius Cautun, Carlos S. Frenk +7

The "plane of satellites problem" describes the arrangement of the Milky Way's 11 brightest satellite galaxies in a remarkably thin plane, possibly supported by rotation. This is i…

astro-ph.GA2016

The dark nemesis of galaxy formation: why hot haloes trigger black hole growth and bring star formation to an end

Richard Bower, Joop Schaye, Carlos S. Frenk +4

Galaxies fall into two clearly distinct types: `blue-sequence' galaxies that are rapidly forming young stars, and `red-sequence' galaxies in which star formation has almost complet…

astro-ph.CO2026

Two per cent measurement of from Cepheids alone

Richard Stiskalek, Harry Desmond, Eleni Tsaprazi +4

One of the most pressing problems in current cosmology is the cause of the Hubble tension. We revisit a two-rung distance ladder, composed only of Cepheid periods and magnitudes, a…

astro-ph.GA2020

The Star-Formation Properties of the Observed and Simulated AGN Universe: BAT vs EAGLE

Thomas M. Jackson, D. J. Rosario, D. M. Alexander +3

In this paper we present data from 72 low redshift, hard X-ray selected AGN taken from the {\it Swift}-BAT 58 month catalogue. We utilise spectral energy distribution fitting to th…

astro-ph.GA2016

A chronicle of galaxy mass assembly in the EAGLE simulation

Yan Qu, John C. Helly, Richard G. Bower +8

We analyse the mass assembly of central galaxies in the EAGLE hydrodynamical simulations. We build merger trees to connect galaxies to their progenitors at different redshifts and…