Stuart Sim

The Queen's University Belfast

United Kingdom

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Articles (30)

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Collaborators (17)

William Bate

University of Hertfordshire

UNITED KINGDOM

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Leo Mulholland

Queen's University Belfast

UNITED KINGDOM

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Ivo Seitenzahl

Senior Lecturer

UNSW Sydney

AUSTRALIA

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Christian Knigge

University of Southampton

UNITED KINGDOM

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XINYUE SHENG

Queen's University Belfast

UNITED KINGDOM

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Shubham Srivastav

The Queen's University Belfast

UNITED KINGDOM

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Wolfgang Kerzendorf

Assistant Professor

Michigan State University

UNITED STATES

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Ashley Ruiter

ARC Future Fellow and Senior Lecturer

University of New South Wales Canberra at ADFA

AUSTRALIA

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Catherine Ramsbottom

Queen's University Belfast

IRELAND

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Seppo Mattila

Professor of Astronomy

University of Turku

FINLAND

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Keiichi Maeda

教授 / Professor

Kyoto University

JAPAN

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David Young

The Queen's University Belfast

UNITED KINGDOM

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David Jess

Reader

The Queen's University Belfast

UNITED KINGDOM

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Cosimo Inserra

College Dean of Equality, Diversity and Inclusivity

Cardiff University

UNITED KINGDOM

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Christine Collins

Trinity College Dublin

IRELAND

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Bernhard Mueller

Associate Professor

MONASH UNIVERSITY

AUSTRALIA

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Ruediger Pakmor

Max-Planck-Institut für Astronomie

GERMANY

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Stuart Sim

Research Interests

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Articles (30)

On the use of the Axelrod formula for thermal electron collisions in astrophysical modelling

NLTE spectral modelling for a carbon-oxygen and helium white dwarf merger as a Ca-rich transient candidate

A diagnostic kit for optical emission lines shaped by accretion disc winds

Effect of Positronium on the γ-Ray Spectra and Energy Deposition in Type Ia Supernovae

Monte Carlo radiation hydrodynamic simulations of line-driven disc winds: relaxing the isothermal approximation

Erratum: “Self-consistent 3D Radiative Transfer for Kilonovae: Directional Spectra from Merger Simulations” (2023, ApJL, 954, L41)

Calcium in a supernova remnant as a fingerprint of a sub-Chandrasekhar-mass explosion

Electron-impact excitation of zirconium i–iii in support of neutron star merger diagnostics

The asymmetry of white dwarf double detonations and the observed scatter around the Phillips relation

Exploring the range of impacts of helium in the spectra of double detonation models for Type Ia supernovae

On the fate of the secondary white dwarf in double-degenerate double-detonation Type Ia supernovae – II. 3D synthetic observables

New radiative and collisional atomic data for Sr ii and Y ii with application to Kilonova modelling

Type Ia supernova explosion models are inherently multidimensional

Including a luminous central remnant in radiative transfer simulations for Type Iax supernovae

Modelling the spectra of the kilonova AT2017gfo – II. Beyond the photospheric epochs

Towards inferring the geometry of kilonovae

Self-consistent 3D Radiative Transfer for Kilonovae: Directional Spectra from Merger Simulations

Photometry and spectroscopy of the Type Icn supernova 2021ckj

State-of-the-art simulations of line-driven accretion disc winds: realistic radiation hydrodynamics leads to weaker outflows

Synthetic light curves and spectra from a self-consistent 2D simulation of an ultra-strippped supernova

SN 2022jli: A Type Ic Supernova with Periodic Modulation of Its Light Curve and an Unusually Long Rise

Unprecedented Early Flux Excess in the Hybrid 02es-like Type Ia Supernova 2022ywc Indicates Interaction with Circumstellar Material

Models of pulsationally assisted gravitationally confined detonations with different ignition conditions

Type Iax supernovae from deflagrations in Chandrasekhar mass white dwarfs

Metallicity-dependent nucleosynthetic yields of Type Ia supernovae originating from double detonations of sub-MCh white dwarfs

Double detonations of sub-MCh CO white dwarfs: variations in Type Ia supernovae due to different core and He shell masses

HOLISMOKES: III. Achromatic phase of strongly lensed Type Ia supernovae

The Lowest of the Low: Discovery of SN 2019gsc and the Nature of Faint Iax Supernovae

Thermal and radiation driving can produce observable disc winds in hard-state X-ray binaries

Thermal and radiation driving can produce observable disc winds in hard-state X-ray binaries

Collaborators (17)

William Bate

Leo Mulholland

Ivo Seitenzahl

Christian Knigge

XINYUE SHENG

Shubham Srivastav

Wolfgang Kerzendorf

Ashley Ruiter

Catherine Ramsbottom

Seppo Mattila

Keiichi Maeda

David Young

David Jess

Cosimo Inserra

Christine Collins

Bernhard Mueller

Ruediger Pakmor

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