DiRAC-2.5 - the pathway to DiRAC Phase 3
Lead Research Organisation:
Durham University
Department Name: Physics
Abstract
We request funding to relocate the Blue Wonder HPC cluster and associated storage, currently at the Hartree Centre at Daresbury, to Durham, together with installation and hardware maintenance costs. This move would enable DiRAC to expand the current DiRAC-2 Data centric service, managed by Durham, by a factor of two in both computing power and data storage capacity. The new service would be called the DiRAC-2.5 Data Centric service.
Planned Impact
DiRAC would seek to continue to engage with industry at various levels, from the
provision of computing cycles for industrial applications to the
exchange of technical knowledge and shared training programmes. The
facility will serve to train young scientists in the most advanced
techniques for supercomputing. These have extensive applications beyond
academia, for example in industry and finance. Finally, output from Dirac-based
projects will be used for science outreach activities.
provision of computing cycles for industrial applications to the
exchange of technical knowledge and shared training programmes. The
facility will serve to train young scientists in the most advanced
techniques for supercomputing. These have extensive applications beyond
academia, for example in industry and finance. Finally, output from Dirac-based
projects will be used for science outreach activities.
Organisations
Publications
Tam S
(2020)
Mapping dark matter and finding filaments: calibration of lensing analysis techniques on simulated data
in Monthly Notices of the Royal Astronomical Society
Katz H
(2023)
Two modes of LyC escape from bursty star formation: implications for [C ii ] deficits and the sources of reionization
in Monthly Notices of the Royal Astronomical Society
Icaza-Lizaola M
(2021)
A sparse regression approach to modelling the relation between galaxy stellar masses and their host haloes
in Monthly Notices of the Royal Astronomical Society
Hernández-Aguayo C
(2021)
Building a digital twin of a luminous red galaxy spectroscopic survey: galaxy properties and clustering covariance
in Monthly Notices of the Royal Astronomical Society
Goater A
(2024)
EDGE: The direct link between mass growth history and the extended stellar haloes of the faintest dwarf galaxies
in Monthly Notices of the Royal Astronomical Society
Glowacki M
(2022)
ASymba: H i global profile asymmetries in the simba simulation
in Monthly Notices of the Royal Astronomical Society
Icaza-Lizaola M
(2021)
A sparse regression approach to modelling the relation between galaxy stellar masses and their host haloes
in Monthly Notices of the Royal Astronomical Society
Grand R
(2024)
Overview and public data release of the augmented Auriga Project: cosmological simulations of dwarf and Milky Way-mass galaxies
in Monthly Notices of the Royal Astronomical Society
Bennett J
(2024)
The growth of the gargantuan black holes powering high-redshift quasars and their impact on the formation of early galaxies and protoclusters
in Monthly Notices of the Royal Astronomical Society
McCarthy I
(2023)
The FLAMINGO project: revisiting the S 8 tension and the role of baryonic physics
in Monthly Notices of the Royal Astronomical Society
Robson D
(2023)
Redshift evolution of galaxy group X-ray properties in the Simba simulations
in Monthly Notices of the Royal Astronomical Society
Ansarinejad B
(2023)
VST ATLAS galaxy cluster catalogue I: cluster detection and mass calibration
in Monthly Notices of the Royal Astronomical Society
Fattahi A
(2019)
The origin of galactic metal-rich stellar halo components with highly eccentric orbits
in Monthly Notices of the Royal Astronomical Society
Regan J
(2018)
Rise of the first supermassive stars
in Monthly Notices of the Royal Astronomical Society
Costa T
(2018)
Quenching star formation with quasar outflows launched by trapped IR radiation
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
Mastromarino C
(2023)
Properties and observables of massive galaxies in self-interacting dark matter cosmologies
in Monthly Notices of the Royal Astronomical Society
Hillier A
(2023)
The role of cooling induced by mixing in the mass and energy cycles of the solar atmosphere
in Monthly Notices of the Royal Astronomical Society
Ho C
(2024)
Shallower radius valley around low-mass hosts: evidence for icy planets, collisions, or high-energy radiation scatter
in Monthly Notices of the Royal Astronomical Society
Fumagalli M
(2020)
Detecting neutral hydrogen at z ? 3 in large spectroscopic surveys of quasars
in Monthly Notices of the Royal Astronomical Society
Farahi A
(2018)
Localized massive halo properties in bahamas and MACSIS simulations: scalings, lognormality, and covariance
in Monthly Notices of the Royal Astronomical Society
Huško F
(2023)
The buildup of galaxies and their spheroids: The contributions of mergers, disc instabilities, and star formation
in Monthly Notices of the Royal Astronomical Society
Hassan S
(2020)
Testing galaxy formation simulations with damped Lyman-a abundance and metallicity evolution
in Monthly Notices of the Royal Astronomical Society
Hafen Z
(2024)
The Halo21 absorption modelling challenge: lessons from 'observing' synthetic circumgalactic absorption spectra
in Monthly Notices of the Royal Astronomical Society
Wilson B
(2022)
A measurement of the Ly ß forest power spectrum and its cross with the Ly a forest in X-Shooter XQ-100
in Monthly Notices of the Royal Astronomical Society
Kelly A
(2021)
The origin of X-ray coronae around simulated disc galaxies
in Monthly Notices of the Royal Astronomical Society
Davies C
(2019)
The self-similarity of weak lensing peaks
in Monthly Notices of the Royal Astronomical Society
Trotta D
(2023)
Three-dimensional modelling of the shock-turbulence interaction
in Monthly Notices of the Royal Astronomical Society
Teodoro L
(2019)
Planetary giant impacts: convergence of high-resolution simulations using efficient spherical initial conditions and swift
in Monthly Notices of the Royal Astronomical Society
Young A
(2022)
Characteristics of small protoplanetary disc warps in kinematic observations
in Monthly Notices of the Royal Astronomical Society
Jennings F
(2023)
Shattering and growth of cold clouds in galaxy clusters: the role of radiative cooling, magnetic fields, and thermal conduction
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
Ganeshaiah Veena P
(2019)
The Cosmic Ballet II: spin alignment of galaxies and haloes with large-scale filaments in the EAGLE simulation
in Monthly Notices of the Royal Astronomical Society
Armijo J
(2024)
A new test of gravity - II. Application of marked correlation functions to luminous red galaxy samples
in Monthly Notices of the Royal Astronomical Society
Mitchell P
(2018)
Comparing galaxy formation in semi-analytic models and hydrodynamical simulations
in Monthly Notices of the Royal Astronomical Society
Gonzalez-Perez V
(2017)
The host dark matter haloes of [O II] emitters at 0.5 < z < 1.5
in Monthly Notices of the Royal Astronomical Society
Richings A
(2022)
The effects of local stellar radiation and dust depletion on non-equilibrium interstellar chemistry
in Monthly Notices of the Royal Astronomical Society
Smith R
(2023)
On the distribution of the cold neutral medium in galaxy discs
in Monthly Notices of the Royal Astronomical Society
Font A
(2021)
Can cosmological simulations capture the diverse satellite populations of observed Milky Way analogues?
in Monthly Notices of the Royal Astronomical Society
Cowell J
(2023)
Potential signature of a quadrupolar hubble expansion in Pantheon+supernovae
in Monthly Notices of the Royal Astronomical Society
Ryczanowski D
(2020)
What does strong gravitational lensing? The mass and redshift distribution of high-magnification lenses
in Monthly Notices of the Royal Astronomical Society
Mukherjee S
(2018)
SEAGLE - I. A pipeline for simulating and modelling strong lenses from cosmological hydrodynamic simulations
in Monthly Notices of the Royal Astronomical Society
Bate M
(2023)
The statistical properties of stars at redshift, z = 5, compared with the present epoch
in Monthly Notices of the Royal Astronomical Society
Ahad S
(2024)
An environment-dependent halo mass function as a driver for the early quenching of z = 1.5 cluster galaxies
in Monthly Notices of the Royal Astronomical Society
Robson D
(2023)
Redshift evolution of galaxy group X-ray properties in the Simba simulations
in Monthly Notices of the Royal Astronomical Society
Errani R
(2021)
The asymptotic tidal remnants of cold dark matter subhaloes
in Monthly Notices of the Royal Astronomical Society
Barrera-Hinojosa C
(2022)
Looking for a twist: probing the cosmological gravitomagnetic effect via weak lensing-kSZ cross-correlations
in Monthly Notices of the Royal Astronomical Society
Roth A
(2024)
Hot Jupiter diversity and the onset of TiO/VO revealed by a large grid of non-grey global circulation models
in Monthly Notices of the Royal Astronomical Society
Štofanová L
(2024)
Prospects for detecting the circum- and intergalactic medium in X-ray absorption using the extended intracluster medium as a backlight
in Monthly Notices of the Royal Astronomical Society
Cautun M
(2018)
The Santiago-Harvard-Edinburgh-Durham void comparison - I. SHEDding light on chameleon gravity tests
in Monthly Notices of the Royal Astronomical Society
| Description | See Dirac annual report https://dirac.ac.uk |
| Exploitation Route | See Dirac annual report https://dirac.ac.uk |
| Sectors | Digital/Communication/Information Technologies (including Software) Education |
| URL | https://dirac.ac.uk |