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
Christiansen J
(2020)
Jet feedback and the photon underproduction crisis in simba
in Monthly Notices of the Royal Astronomical Society
Maunder T
(2024)
Synthetic light curves and spectra from a self-consistent 2D simulation of an ultra-strippped supernova
in Monthly Notices of the Royal Astronomical Society
Bahé Y
(2021)
Strongly lensed cluster substructures are not in tension with ?CDM
in Monthly Notices of the Royal Astronomical Society
Elliott E
(2021)
Efficient exploration and calibration of a semi-analytical model of galaxy formation with deep learning
in Monthly Notices of the Royal Astronomical Society
Fumagalli M
(2017)
Witnessing galaxy assembly in an extended z˜3 structure
in Monthly Notices of the Royal Astronomical Society
Koudmani S
(2021)
A little FABLE: exploring AGN feedback in dwarf galaxies with cosmological simulations
in Monthly Notices of the Royal Astronomical Society
Barnes D
(2021)
Characterizing hydrostatic mass bias with mock-X
in Monthly Notices of the Royal Astronomical Society
Pizzati E
(2024)
Revisiting the extreme clustering of z ˜ 4 quasars with large volume cosmological simulations
in Monthly Notices of the Royal Astronomical Society
Nobels F
(2022)
The interplay between AGN feedback and precipitation of the intracluster medium in simulations of galaxy groups and clusters
in Monthly Notices of the Royal Astronomical Society
Bourne M
(2019)
AGN jet feedback on a moving mesh: lobe energetics and X-ray properties in a realistic cluster environment
in Monthly Notices of the Royal Astronomical Society
Lacerna I
(2018)
Galactic conformity measured in semi-analytic models
in Monthly Notices of the Royal Astronomical Society
Sullivan D
(2018)
Using artificial neural networks to constrain the halo baryon fraction during reionization
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
Mitchell P
(2020)
Galactic outflow rates in the EAGLE simulations
in Monthly Notices of the Royal Astronomical Society
Acuto A
(2021)
The BAHAMAS project: evaluating the accuracy of the halo model in predicting the non-linear matter power spectrum
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
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
Lovell C
(2021)
Reproducing submillimetre galaxy number counts with cosmological hydrodynamic simulations
in Monthly Notices of the Royal Astronomical Society
Brooks R
(2023)
The north-south asymmetry of the ALFALFA H i velocity width function
in Monthly Notices of the Royal Astronomical Society
Cowley W
(2017)
Blending bias impacts the host halo masses derived from a cross-correlation analysis of bright submillimetre galaxies
in Monthly Notices of the Royal Astronomical Society
Šoltinský T
(2023)
Probing quasar lifetimes with proximate 21-centimetre absorption in the diffuse intergalactic medium at redshifts z = 6
in Monthly Notices of the Royal Astronomical Society
Vijayan A
(2024)
First Light And Reionisation Epoch Simulations (FLARES) - XII: The consequences of star-dust geometry on galaxies in the EoR
in Monthly Notices of the Royal Astronomical Society
Cataneo M
(2022)
The matter density PDF for modified gravity and dark energy with Large Deviations Theory
in Monthly Notices of the Royal Astronomical Society
DeGraf C
(2021)
Morphological evolution of supermassive black hole merger hosts and multimessenger signatures
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
| 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 |