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
Semenov M
(2021)
Rovibronic spectroscopy of PN from first principles.
in Physical chemistry chemical physics : PCCP
Seeyave L
(2023)
First light and reionization epoch simulations (FLARES) X iii : the lyman-continuum emission of high-redshift galaxies
in Monthly Notices of the Royal Astronomical Society
Scott L
(2021)
Convective core entrainment in 1D main-sequence stellar models
in Monthly Notices of the Royal Astronomical Society
Schönrich R
(2017)
Assessing distances and consistency of kinematics in Gaia/TGAS
in Monthly Notices of the Royal Astronomical Society
Schönrich R
(2018)
Warp, waves, and wrinkles in the Milky Way
in Monthly Notices of the Royal Astronomical Society
Schwinn J
(2018)
Uncovering substructure with wavelets:proof of concept using Abell 2744
in Monthly Notices of the Royal Astronomical Society
Scholtz J
(2023)
GN-z11: The environment of an AGN at $z=$10.603
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
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)
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
(2021)
Setting the stage: structures from Gaussian random fields
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
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
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
(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
(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
(2020)
Baryonic clues to the puzzling diversity of dwarf galaxy rotation curves
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 |