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
Wijers N
(2020)
The warm-hot circumgalactic medium around EAGLE-simulation galaxies and its detection prospects with X-ray and UV line absorption
in Monthly Notices of the Royal Astronomical Society
Montargès M
(2023)
The VLT/SPHERE view of the ATOMIUM cool evolved star sample I. Overview: Sample characterization through polarization analysis
in Astronomy & Astrophysics
Dong-Páez C
(2024)
The Uchuu-SDSS galaxy light-cones: a clustering, redshift space distortion and baryonic acoustic oscillation study
in Monthly Notices of the Royal Astronomical Society
Dong-Páez C
(2024)
The Uchuu-SDSS galaxy light-cones: a clustering, redshift space distortion and baryonic acoustic oscillation study
in Monthly Notices of the Royal Astronomical Society
Ereza J
(2024)
The Uchuu - glam BOSS and eBOSS LRG lightcones: exploring clustering and covariance errors
in Monthly Notices of the Royal Astronomical Society
Trusov S
(2024)
The two-point correlation function covariance with fewer mocks
in Monthly Notices of the Royal Astronomical Society
Read P
(2020)
The turbulent dynamics of Jupiter's and Saturn's weather layers: order out of chaos?
in Geoscience Letters
Santos-Santos I
(2023)
The Tucana dwarf spheroidal: a distant backsplash galaxy of M31?
in Monthly Notices of the Royal Astronomical Society
Santos-Santos I
(2022)
The Tucana dwarf spheroidal: a distant backsplash galaxy of M31?
Newton O
(2018)
The total satellite population of the Milky Way
in Monthly Notices of the Royal Astronomical Society
Sawala T
(2023)
The timeless timing argument and the total mass of the Local Group
in Monthly Notices of the Royal Astronomical Society: Letters
Sawala T
(2023)
The Timeless Timing Argument and the Mass of the Local Group
Zhang M
(2025)
The Three Hundred project: The relationship between the shock and splashback radii of simulated galaxy clusters
in Publications of the Astronomical Society of Australia
Benitez-Llambay A
(2021)
The Tail of Late-forming Dwarf Galaxies in ?CDM
in The Astrophysical Journal Letters
Shao S
(2021)
The survival of globular clusters in a cuspy Fornax
in Monthly Notices of the Royal Astronomical Society
Robertson A
(2021)
The surprising accuracy of isothermal Jeans modelling of self-interacting dark matter density profiles
in Monthly Notices of the Royal Astronomical Society
Aumer M
(2017)
The structural evolution of galaxies with both thin and thick discs
in Monthly Notices of the Royal Astronomical Society
Welsh L
(2021)
The stochastic enrichment of Population II stars
in Monthly Notices of the Royal Astronomical Society
Ahad S
(2021)
The stellar mass function and evolution of the density profile of galaxy clusters from the Hydrangea simulations at 0 < z < 1.5
in Monthly Notices of the Royal Astronomical Society
Ahad S
(2021)
The stellar mass function and evolution of the density profile of galaxy clusters from the Hydrangea simulations at 0 < z < 1.5
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
Katz H
(2023)
The SPHINX Public Data Release: Forward Modelling High-Redshift JWST Observations with Cosmological Radiation Hydrodynamics Simulations
in The Open Journal of Astrophysics
Katsianis A
(2021)
The specific star formation rate function at different mass scales and quenching: a comparison between cosmological models and SDSS
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
Lovell M
(2021)
The spatial distribution of Milky Way satellites, gaps in streams, and the nature of dark matter
in Monthly Notices of the Royal Astronomical Society
Lovell M
(2021)
The spatial distribution of Milky Way satellites, gaps in streams, and the nature of dark matter
in Monthly Notices of the Royal Astronomical Society
Sawala T
(2022)
The SIBELIUS Project: E Pluribus Unum
in Monthly Notices of the Royal Astronomical Society
Sawala T
(2021)
The SIBELIUS Project: E Pluribus Unum
Puchwein E
(2023)
The Sherwood-Relics simulations: overview and impact of patchy reionization and pressure smoothing on the intergalactic medium
in Monthly Notices of the Royal Astronomical Society
Dethero M
(2024)
The shape of convection in 2D and 3D global simulations of stellar interiors
in Astronomy & Astrophysics
Davies C
(2019)
The self-similarity of weak lensing peaks
in Monthly Notices of the Royal Astronomical Society
Davies C
(2019)
The self similarity of weak lensing peaks
Paillas E
(2019)
The Santiago-Harvard-Edinburgh-Durham void comparison II: unveiling the Vainshtein screening using weak lensing
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
Tescari E
(2018)
The SAMI Galaxy Survey: understanding observations of large-scale outflows at low redshift with EAGLE simulations
in Monthly Notices of the Royal Astronomical Society
Herrington N
(2023)
The role of previous generations of stars in triggering star formation and driving gas dynamics
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
Beckett A
(2021)
The relationship between gas and galaxies at z < 1 using the Q0107 quasar triplet
in Monthly Notices of the Royal Astronomical Society
Beckett A
(2021)
The relationship between gas and galaxies at z < 1 using the Q0107 quasar triplet
in Monthly Notices of the Royal Astronomical Society
Beckett, Alexander
(2021)
The relationship between gas and galaxies at z < 1 using the Q0107 quasar triplet
| 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 |