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
Jennings F
(2023)
Halo scaling relations and hydrostatic mass bias in the simba simulation from realistic mock X-ray catalogues
in Monthly Notices of the Royal Astronomical Society
Han J
(2018)
hbt+: an improved code for finding subhaloes and building merger trees in cosmological simulations
in Monthly Notices of the Royal Astronomical Society
Daley-Yates S
(2023)
Heating and cooling in stellar coronae: coronal rain on a young Sun
in Monthly Notices of the Royal Astronomical Society
Collins C
(2023)
Helium as a signature of the double detonation in Type Ia supernovae
in Monthly Notices of the Royal Astronomical Society
Martinez-Delgado D
(2021)
Hidden depths in the local Universe: The Stellar Stream Legacy Survey
Martínez-Delgado D
(2023)
Hidden depths in the local Universe: The Stellar Stream Legacy Survey
in Astronomy & Astrophysics
Leo M
(2019)
High-redshift test of gravity using enhanced growth of small structures probed by the neutral hydrogen distribution
in Physical Review D
Camps P
(2022)
High-resolution synthetic UV-submm images for Milky Way-mass simulated galaxies from the ARTEMIS project
in Monthly Notices of the Royal Astronomical Society
Elbers W
(2022)
Higher order initial conditions with massive neutrinos
in Monthly Notices of the Royal Astronomical Society
Elbers W
(2022)
Higher-order initial conditions with massive neutrinos
Sorini D
(2022)
How baryons affect haloes and large-scale structure: a unified picture from the Simba simulation
in Monthly Notices of the Royal Astronomical Society
Salcido J
(2019)
How feedback shapes galaxies: an analytic model
Salcido J
(2020)
How feedback shapes galaxies: an analytic model
in Monthly Notices of the Royal Astronomical Society
Mitchell P
(2022)
How gas flows shape the stellar-halo mass relation in the eagle simulation
in Monthly Notices of the Royal Astronomical Society
Ho S
(2021)
How Identifying Circumgalactic Gas by Line-of-sight Velocity instead of the Location in 3D Space Affects O vi Measurements
in The Astrophysical Journal
Jahns-Schindler J
(2023)
How limiting is optical follow-up for fast radio burst applications? Forecasts for radio and optical surveys
in Monthly Notices of the Royal Astronomical Society
Garzilli A
(2021)
How to constrain warm dark matter with the Lyman-a forest
in Monthly Notices of the Royal Astronomical Society
Ahad S
(2023)
How to interpret measurements of diffuse light in stacked observations of groups and clusters of galaxies
in Monthly Notices of the Royal Astronomical Society
Hou J
(2021)
How well is angular momentum accretion modelled in semi-analytic galaxy formation models?
in Monthly Notices of the Royal Astronomical Society
Pagano P
(2020)
Hydrogen non-equilibrium ionisation effects in coronal mass ejections
in Astronomy & Astrophysics
Bosman S
(2022)
Hydrogen reionization ends by z = 5.3: Lyman-a optical depth measured by the XQR-30 sample
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
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
Kegerreis J
(2022)
Immediate Origin of the Moon as a Post-impact Satellite
in The Astrophysical Journal Letters
Kegerreis J
(2022)
Immediate origin of the Moon as a post-impact satellite
Chakraborty B
(2021)
Improved V c s determination using precise lattice QCD form factors for D ? K l ?
in Physical Review D
Antolin P
(2018)
In Situ Generation of Transverse Magnetohydrodynamic Waves from Colliding Flows in the Solar Corona
in The Astrophysical Journal Letters
Trujillo-Gomez S
(2023)
In situ or accreted? Using deep learning to infer the origin of extragalactic globular clusters from observables
in Monthly Notices of the Royal Astronomical Society
Borrow J
(2021)
Inconsistencies arising from the coupling of galaxy formation sub-grid models to pressure-smoothed particle hydrodynamics
in Monthly Notices of the Royal Astronomical Society
Falck B
(2021)
Indra: a public computationally accessible suite of cosmological N -body simulations
in Monthly Notices of the Royal Astronomical Society
Poole-McKenzie R
(2020)
Informing dark matter direct detection limits with the ARTEMIS simulations
in Journal of Cosmology and Astroparticle Physics
Poole-McKenzie R
(2020)
Informing dark matter direct detection limits with the ARTEMIS simulations
Civiš S
(2023)
Infrared Spectra of Small Radicals for Exoplanetary Spectroscopy: OH, NH, CN and CH: The State of Current Knowledge.
in Molecules (Basel, Switzerland)
Czakon M
(2023)
Infrared-safe flavoured anti-kT jets
in Journal of High Energy Physics
Xia Q
(2020)
Intergalactic filaments spin
Xia Q
(2021)
Intergalactic filaments spin
in Monthly Notices of the Royal Astronomical Society
Ratnasingam R
(2023)
Internal gravity waves in massive stars II. Frequency analysis across stellar mass
in Astronomy & Astrophysics
Katz H
(2017)
Interpreting ALMA observations of the ISM during the epoch of reionization
in Monthly Notices of the Royal Astronomical Society
Vizgan D
(2022)
Investigating the [C ii]-to-H i Conversion Factor and the H i Gas Budget of Galaxies at z ˜ 6 with Hydrodynamic Simulations
in The Astrophysical Journal Letters
| 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 |