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
Schwinn J
(2018)
Uncovering substructure with wavelets:proof of concept using Abell 2744
in Monthly Notices of the Royal Astronomical Society
Schreyer E
(2024)
Using helium 10 830 Å transits to constrain planetary magnetic fields
in Monthly Notices of the Royal Astronomical Society
Schreyer E
(2024)
Using Ly a transits to constrain models of atmospheric escape
in Monthly Notices of the Royal Astronomical Society
Scholtz J
(2018)
Identifying the subtle signatures of feedback from distant AGN using ALMA observations and the EAGLE hydrodynamical simulations
in Monthly Notices of the Royal Astronomical Society
Scholtz J
(2023)
GN-z11: The environment of an AGN at $z=$10.603
Scholtz J
(2024)
GN-z11: The environment of an active galactic nucleus at z = 10.603 New insights into the most distant Ly a detection
in Astronomy & Astrophysics
Schoettler C
(2024)
The effect of dynamical interactions in stellar birth environments on the orbits of young close-in planetary systems
in Monthly Notices of the Royal Astronomical Society
Schirra A
(2021)
Bringing faint active galactic nuclei (AGNs) to light: a view from large-scale cosmological simulations
in Monthly Notices of the Royal Astronomical Society
Schaye J
(2023)
The FLAMINGO project: cosmological hydrodynamical simulations for large-scale structure and galaxy cluster surveys
in Monthly Notices of the Royal Astronomical Society
Schaller M
(2024)
Swift : a modern highly parallel gravity and smoothed particle hydrodynamics solver for astrophysical and cosmological applications
in Monthly Notices of the Royal Astronomical Society
Schaller M
(2023)
On the anisotropic distribution of clusters in the local Universe
Schaller M
(2024)
On the anisotropic distribution of clusters in the local Universe
in Monthly Notices of the Royal Astronomical Society: Letters
Sawala T
(2023)
Distinct distributions of elliptical and disk galaxies across the Local Supercluster as a ?CDM prediction
in Nature Astronomy
Sawala T
(2022)
The SIBELIUS Project: E Pluribus Unum
in Monthly Notices of the Royal Astronomical Society
Sawala T
(2021)
Setting the stage: structures from Gaussian random fields
in Monthly Notices of the Royal Astronomical Society
Sawala T
(2023)
The Timeless Timing Argument and the Mass of the Local Group
Sawala T
(2021)
The SIBELIUS Project: E Pluribus Unum
Sawala T
(2023)
The timeless timing argument and the total mass of the Local Group
in Monthly Notices of the Royal Astronomical Society: Letters
Satyavolu S
(2023)
The need for obscured supermassive black hole growth to explain quasar proximity zones in the epoch of reionization
in Monthly Notices of the Royal Astronomical Society
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)
Satellite mass functions and the faint end of the galaxy mass-halo mass relation in LCDM
in Monthly Notices of the Royal Astronomical Society
Santos-Santos I
(2021)
Magellanic satellites in ?CDM cosmological hydrodynamical simulations of the Local Group
in Monthly Notices of the Royal Astronomical Society
Santos-Santos I
(2021)
Magellanic satellites in ?CDM cosmological hydrodynamical simulations of the Local Group
in Monthly Notices of the Royal Astronomical Society
Santos-Santos I
(2021)
Satellite mass functions and the faint end of the galaxy mass-halo mass relation in LCDM
Santos-Santos I
(2022)
The Tucana dwarf spheroidal: a distant backsplash galaxy of M31?
Santos-Santos I
(2019)
Baryonic clues to the puzzling diversity of dwarf galaxy rotation curves
Santos-Santos I
(2020)
Baryonic clues to the puzzling diversity of dwarf galaxy rotation curves
in Monthly Notices of the Royal Astronomical Society
Santos-Santos I
(2024)
Anisotropies in the spatial distribution and kinematics of dwarf galaxies in the Local Group and beyond
in Monthly Notices of the Royal Astronomical Society
Sante A
(2024)
Applying machine learning to Galactic Archaeology: how well can we recover the origin of stars in Milky Way-like galaxies?
in Monthly Notices of the Royal Astronomical Society
Sanati M
(2024)
Dwarf galaxies as a probe of a primordially magnetized Universe
in Astronomy & Astrophysics
Sana T
(2023)
Plasma sheath around sunlit moon: monotonic and non-monotonic structures
in Monthly Notices of the Royal Astronomical Society
Saló LA
(2022)
Well-Posedness of the Four-Derivative Scalar-Tensor Theory of Gravity in Singularity Avoiding Coordinates.
in Physical review letters
Salcido J
(2020)
How feedback shapes galaxies: an analytic model
in Monthly Notices of the Royal Astronomical Society
Salcido J
(2019)
How feedback shapes galaxies: an analytic model
Salcido J
(2023)
SP(k) - a hydrodynamical simulation-based model for the impact of baryon physics on the non-linear matter power spectrum
in Monthly Notices of the Royal Astronomical Society
Saavedra-Bastidas J
(2024)
Gravitational collapse at low to moderate Mach numbers: The relationship between star formation efficiency and the fraction of mass in the massive object
in Astronomy & Astrophysics
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
Ruiz-Macias O
(2021)
Characterizing the target selection pipeline for the Dark Energy Spectroscopic Instrument Bright Galaxy Survey
in Monthly Notices of the Royal Astronomical Society
Ruiz-Bonilla S
(2021)
The effect of pre-impact spin on the Moon-forming collision
in Monthly Notices of the Royal Astronomical Society
Ruan C
(2024)
An emulator-based halo model in modified gravity - I. The halo concentration-mass relation and density profile
in Monthly Notices of the Royal Astronomical Society
Ruan C
(2024)
An emulator-based halo model in modified gravity - I. The halo concentration-mass relation and density profile
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 |