DiRAC 2.5 Operations Bridging 2019 - Leicester
Lead Research Organisation:
University of Leicester
Department Name: Physics and Astronomy
Abstract
This is a request for bridging funds to support the operation of the DiRAC HPC Facility at the University of Leicester while the peer review of the 2019-2022 operations budget is completed.
Planned Impact
This is a request for bridging funds to support the operation of the DiRAC HPC Facility at the University of Leicester while the peer review of the 2019-2022 operations budget is completed.
Organisations
Publications
Lim S
(2024)
The FLAMINGO simulation view of cluster progenitors observed in the epoch of reionization with JWST
in Monthly Notices of the Royal Astronomical Society
Langleben J
(2019)
ExoMol line list - XXXIV. A rovibrational line list for phosphinidene (PH) in its $X\, {}^3\Sigma ^-$ and $a\, {}^1\Delta$ electronic states
in Monthly Notices of the Royal Astronomical Society
De Beer S
(2023)
Resolving the physics of quasar Ly a nebulae (RePhyNe): I. Constraining quasar host halo masses through circumgalactic medium kinematics
in Monthly Notices of the Royal Astronomical Society
Bower R
(2020)
Numerical convergence of hydrodynamical simulations of galaxy formation: the abundance and internal structure of galaxies and their cold dark matter haloes
in Monthly Notices of the Royal Astronomical Society
Evans T
(2022)
Observing EAGLE galaxies with JWST : predictions for Milky Way progenitors and their building blocks
in Monthly Notices of the Royal Astronomical Society
Gómez J
(2022)
Halo merger tree comparison: impact on galaxy formation models
in Monthly Notices of the Royal Astronomical Society
Solar M
(2020)
Azimuthal variations of oxygen abundance profiles in star-forming regions of disc galaxies in EAGLE simulations
in Monthly Notices of the Royal Astronomical Society
Sirks E
(2022)
The effects of self-interacting dark matter on the stripping of galaxies that fall into clusters
in Monthly Notices of the Royal Astronomical Society
Satyavolu S
(2024)
Robustness of direct measurements of the mean free path of ionizing photons in the epoch of reionization
in Monthly Notices of the Royal Astronomical Society
Trayford J
(2019)
Resolved galaxy scaling relations in the eagle simulation: star formation, metallicity, and stellar mass on kpc scales
in Monthly Notices of the Royal Astronomical Society
McCarthy I
(2020)
The imprint of dark subhaloes on the circumgalactic medium
in Monthly Notices of the Royal Astronomical Society
Pallero D
(2024)
Galaxy evolution in modified gravity simulations: using galaxy properties to constrain our gravitational model
in Monthly Notices of the Royal Astronomical Society
Baes M
(2019)
The cosmic spectral energy distribution in the EAGLE simulation
in Monthly Notices of the Royal Astronomical Society
Sharma M
(2019)
The I?ea model of feedback-regulated galaxy formation
in Monthly Notices of the Royal Astronomical Society
Rizzuti F
(2022)
Realistic 3D hydrodynamics simulations find significant turbulent entrainment in massive stars
in Monthly Notices of the Royal Astronomical Society
Borrow J
(2022)
Sphenix : smoothed particle hydrodynamics for the next generation of galaxy formation simulations
in Monthly Notices of the Royal Astronomical Society
Grove C
(2022)
The DESI N -body simulation project - I. Testing the robustness of simulations for the DESI dark time survey
in Monthly Notices of the Royal Astronomical Society
Vera-Casanova A
(2022)
Linking the brightest stellar streams with the accretion history of Milky Way like galaxies
in Monthly Notices of the Royal Astronomical Society
Amvrosiadis A
(2025)
The onset of bar formation in a massive galaxy at z ~ 3.8
in Monthly Notices of the Royal Astronomical Society
Pearce F
(2020)
Hydrostatic mass estimates of massive galaxy clusters: a study with varying hydrodynamics flavours and non-thermal pressure support
in Monthly Notices of the Royal Astronomical Society
Harvey D
(2019)
Observable tests of self-interacting dark matter in galaxy clusters: BCG wobbles in a constant density core
in Monthly Notices of the Royal Astronomical Society
Brown S
(2024)
ARTEMIS emulator: exploring the effect of cosmology and galaxy formation physics on Milky Way-mass haloes and their satellites
in Monthly Notices of the Royal Astronomical Society
Nobels F
(2022)
The interplay between AGN feedback and precipitation of the intracluster medium in simulations of galaxy groups and clusters
in Monthly Notices of the Royal Astronomical Society
Wijers N
(2022)
The warm-hot circumgalactic medium around EAGLE-simulation galaxies and its detection prospects with X-ray-line emission
in Monthly Notices of the Royal Astronomical Society
Chachan Y
(2019)
Dust accretion in binary systems: implications for planets and transition discs
in Monthly Notices of the Royal Astronomical Society
Mitchell P
(2020)
Galactic outflow rates in the EAGLE simulations
in Monthly Notices of the Royal Astronomical Society
Davey J
(2025)
The effect of spectroscopic binning on atmospheric retrievals
in Monthly Notices of the Royal Astronomical Society
Cooke R
(2020)
The ACCELERATION programme: I. Cosmology with the redshift drift
in Monthly Notices of the Royal Astronomical Society
Gu Q
(2022)
The spatial distribution of satellites in galaxy clusters
in Monthly Notices of the Royal Astronomical Society
Vandenbroucke B
(2020)
Infrared luminosity functions and dust mass functions in the EAGLE simulation
in Monthly Notices of the Royal Astronomical Society
Comerford T
(2019)
Bondi-Hoyle-Lyttleton accretion by binary stars
in Monthly Notices of the Royal Astronomical Society
Oleskiewicz P
(2019)
The connection between halo concentrations and assembly histories: a probe of gravity?
in Monthly Notices of the Royal Astronomical Society
Clarke C
(2020)
Forbidden line diagnostics of photoevaporative disc winds
in Monthly Notices of the Royal Astronomical Society
Ruan C
(2022)
Towards an accurate model of small-scale redshift-space distortions in modified gravity
in Monthly Notices of the Royal Astronomical Society
Dobbs C
(2021)
The properties of clusters, and the orientation of magnetic fields relative to filaments, in magnetohydrodynamic simulations of colliding clouds
in Monthly Notices of the Royal Astronomical Society
Du Buisson L
(2020)
Cosmic rates of black hole mergers and pair-instability supernovae from chemically homogeneous binary evolution
in Monthly Notices of the Royal Astronomical Society
Georgy C
(2024)
3D simulations of a neon burning convective shell in a massive star
in Monthly Notices of the Royal Astronomical Society
Sharma M
(2019)
The I?ea model of feedback-regulated galaxy formation
in Monthly Notices of the Royal Astronomical Society
Jauzac M
(2019)
The core of the massive cluster merger MACS J0417.5-1154 as seen by VLT/MUSE
in Monthly Notices of the Royal Astronomical Society
Brown S
(2022)
Towards a universal model for the density profiles of dark matter haloes
in Monthly Notices of the Royal Astronomical Society
Pfeifer S
(2020)
The bahamas project: effects of a running scalar spectral index on large-scale structure
in Monthly Notices of the Royal Astronomical Society
Battino U
(2019)
NuGrid stellar data set - III. Updated low-mass AGB models and s-process nucleosynthesis with metallicities Z= 0.01, Z = 0.02, and Z = 0.03
in Monthly Notices of the Royal Astronomical Society
Armijo J
(2022)
Making use of sub-resolution haloes in N -body simulations
in Monthly Notices of the Royal Astronomical Society: Letters
Schaller M
(2024)
On the anisotropic distribution of clusters in the local Universe
in Monthly Notices of the Royal Astronomical Society: Letters
Tröster T
(2019)
Painting with baryons: augmenting N -body simulations with gas using deep generative models
in Monthly Notices of the Royal Astronomical Society: Letters
Zenocratti L
(2020)
Correlations between mass, stellar kinematics, and gas metallicity in eagle galaxies
in Monthly Notices of the Royal Astronomical Society: Letters
Khachaturyants T
(2022)
The pattern speeds of vertical breathing waves
in Monthly Notices of the Royal Astronomical Society: Letters
Kulkarni G
(2019)
Large Ly a opacity fluctuations and low CMB t in models of late reionization with large islands of neutral hydrogen extending to z < 5.5
in Monthly Notices of the Royal Astronomical Society: Letters
McNally C
(2019)
Multiplanet systems in inviscid discs can avoid forming resonant chains
in Monthly Notices of the Royal Astronomical Society: Letters
Simpson C
(2019)
Simulating cosmological substructure in the solar neighbourhood
in Monthly Notices of the Royal Astronomical Society: Letters
| Description | Many new discoveries about the formation and evolution of galaxies, star formation, planet formation have been made possible by the award. |
| Exploitation Route | Many international collaborative projects are supported by the HPC resources provided by DiRAC. |
| Sectors | Aerospace Defence and Marine Creative Economy Digital/Communication/Information Technologies (including Software) Education Manufacturing including Industrial Biotechology Retail Other |
| URL | http://www.dirac.ac.uk |