Matthieu Schaller

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University Lecturer - Tenure Track

Leiden University

Netherlands

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About

Matthieu Schaller is a University Lecturer on Tenure Track at Leiden University in the Netherlands. His research focuses on cosmology and galaxy formation, with recent publications addressing topics such as the properties of halo masses, the assessment of subhalo finders in simulations, and radiative cooling models. He is actively involved in advancing the understanding of galaxy quenching mechanisms and baryonic effects on the matter power spectrum.

Recent Grants

Grant: Close

Evaluating the effect of baryons on cosmological probes with next-generation simulations

Open Date: 2018-01-01

Close Date: 2021-12-01

Grant: Close

Continuation of the IPCC at Durham around the SWIFT code

Open Date: 2015-10-01

Close Date: 2017-09-01

Grant: Close

Creation of the IPCC at Durham around the SWIFT code

Open Date: 2015-10-01

Close Date: 2017-09-01

Articles (20)

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2022

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2022

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2022

Collaborators (16)

Joop Schaye

Leiden University

NETHERLANDS

Matthieu Schaller

Research Interests

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About

Recent Grants

Articles (20)

Mass Proxy Quality of Massive Halo Properties in the IllustrisTNG and FLAMINGO Simulations: I. Hot Gas

Assessing subhalo finders in cosmological hydrodynamical simulations

hybrid-chimes: a model for radiative cooling and the abundances of ions and molecules in simulations of galaxy formation

Cosmological feedback from a halo assembly perspective

In-situ vs. ex-situ drivers of galaxy quenching: critical black hole mass and main sequence universality in the FLAMINGO simulation

Map-level baryonification: unified treatment of weak lensing two-point and higher-order statistics

SOAP: A Python Package for Calculating the Properties of Galaxies and Halos Formed in Cosmological Simulations

Entropy plateaus can emerge from gas replacement at a characteristic halo mass in simulated groups and clusters of galaxies

Kinematic dynamos and resolution limits for smoothed particle magnetohydrodynamics

An analytic redshift-independent formulation of baryonic effects on the matter power spectrum

The FLAMINGO project: cosmological hydrodynamical simulations for large-scale structure and galaxy cluster surveys

Hydrodynamic simulations of the disc of gas around supermassive black holes (HDGAS) – I. Molecular gas dynamics

A thermal–kinetic subgrid model for supernova feedback in simulations of galaxy formation

Sensitivity of non-radiative cloud–wind interactions to the hydrodynamic solver

EAGLE-like simulation models do not solve the entropy core problem in groups and clusters of galaxies

Spin-driven jet feedback in idealized simulations of galaxy groups and clusters

A common origin for the fundamental plane of quiescent and star-forming galaxies in the EAGLE simulations

A sparse regression approach for populating dark matter haloes and subhaloes with galaxies

TangoSIDM: tantalizing models of self-interacting dark matter

The importance of black hole repositioning for galaxy formation simulations

Collaborators (16)

Joop Schaye

Alejandro Benítez-Llambay

Scott Dodelson

John Helly

Edoardo Altamura

Scott Kay

Sandro Tacchella

Sylvia Ploeckinger

Camila A Correa

Cedric Lacey

Jaime Salcido

Miguel Icaza-Lizaola

Robert McGibbon

Oliver Hahn

Folkert S J Nobels

Filip Huško

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