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
Correa C
(2017)
The relation between galaxy morphology and colour in the EAGLE simulation
in Monthly Notices of the Royal Astronomical Society: Letters
Henden N
(2019)
The redshift evolution of X-ray and Sunyaev-Zel'dovich scaling relations in the fable simulations
in Monthly Notices of the Royal Astronomical Society
Glowacki M
(2021)
The redshift evolution of the baryonic Tully-Fisher relation in SIMBA
in Monthly Notices of the Royal Astronomical Society
Glowacki M
(2021)
The redshift evolution of the baryonic Tully-Fisher relation in SIMBA
in Monthly Notices of the Royal Astronomical Society
Glowacki M
(2020)
The redshift evolution of the baryonic Tully-Fisher relation in Simba
McAlpine S
(2018)
The rapid growth phase of supermassive black holes
in Monthly Notices of the Royal Astronomical Society
Thomas N
(2021)
The radio galaxy population in the simba simulations
in Monthly Notices of the Royal Astronomical Society
Thomas N
(2020)
The Radio Galaxy Population in the SIMBA SImulations
Thomas N
(2021)
The radio galaxy population in the simba simulations
in Monthly Notices of the Royal Astronomical Society
Bose S
(2023)
The progenitor galaxies of stellar haloes as 'failed' Milky Ways
in Monthly Notices of the Royal Astronomical Society
Herzog G
(2023)
The present-day gas content of simulated field dwarf galaxies
in Monthly Notices of the Royal Astronomical Society
Herzog G
(2022)
The present-day gas content of simulated field dwarf galaxies
Appleby S
(2022)
The Physical Nature of Circumgalactic Medium Absorbers in Simba
Appleby S
(2023)
The physical nature of circumgalactic medium absorbers in Simba
in Monthly Notices of the Royal Astronomical Society
Appleby S
(2023)
The physical nature of circumgalactic medium absorbers in Simba
in Monthly Notices of the Royal Astronomical Society
Manzoni G
(2024)
The PAU Survey: a new constraint on galaxy formation models using the observed colour redshift relation
in Monthly Notices of the Royal Astronomical Society
Martin-Alvarez S
(2023)
The Pandora project - I. The impact of radiation, magnetic fields, and cosmic rays on the baryonic and dark matter properties of dwarf galaxies
in Monthly Notices of the Royal Astronomical Society
Kelly A
(2021)
The origin of X-ray coronae around simulated disc galaxies
in Monthly Notices of the Royal Astronomical Society
Kelly A
(2021)
The origin of X-ray coronae around simulated disc galaxies
in Monthly Notices of the Royal Astronomical Society
Kelly A
(2020)
The origin of X-ray coronae around simulated disc galaxies
Correa C
(2019)
The origin of the red-sequence galaxy population in the EAGLE simulation
in Monthly Notices of the Royal Astronomical Society
Keating L
(2024)
The origin of the characteristic shape and scatter of intergalactic damping wings during reionization
in Monthly Notices of the Royal Astronomical Society: Letters
Cui W
(2021)
The origin of galaxy colour bimodality in the scatter of the stellar-to-halo mass relation
in Nature Astronomy
Fattahi A
(2019)
The origin of galactic metal-rich stellar halo components with highly eccentric orbits
in Monthly Notices of the Royal Astronomical Society
Kobayashi C
(2020)
The Origin of Elements from Carbon to Uranium
in The Astrophysical Journal
Mackereth J
(2018)
The origin of diverse a-element abundances in galaxy discs
in Monthly Notices of the Royal Astronomical Society
Zenocratti L
(2022)
The origin of correlations between mass, metallicity, and morphology in galaxies from the eagle simulation
in Monthly Notices of the Royal Astronomical Society
Nowak M
(2024)
The orbit of HD 142527 B is too compact to explain many of the disc features
in Astronomy & Astrophysics
Brooks R
(2023)
The north-south asymmetry of the ALFALFA H i velocity width function
in Monthly Notices of the Royal Astronomical Society
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
Hill A
(2021)
The morphology of star-forming gas and its alignment with galaxies and dark matter haloes in the EAGLE simulations
in Monthly Notices of the Royal Astronomical Society
Tanaka M
(2018)
The Missing Satellite Problem Outside of the Local Group. I. Pilot Observation
in The Astrophysical Journal
Bose S
(2023)
The MillenniumTNG Project: the large-scale clustering of galaxies
in Monthly Notices of the Royal Astronomical Society
Ferlito F
(2023)
The MillenniumTNG Project: the impact of baryons and massive neutrinos on high-resolution weak gravitational lensing convergence maps
in Monthly Notices of the Royal Astronomical Society
Pakmor R
(2023)
The MillenniumTNG Project: the hydrodynamical full physics simulation and a first look at its galaxy clusters
in Monthly Notices of the Royal Astronomical Society
Kannan R
(2023)
The MillenniumTNG project: the galaxy population at z = 8
in Monthly Notices of the Royal Astronomical Society
Kannan R
(2022)
The MillenniumTNG Project: The galaxy population at $z\geq 8$
Barrera M
(2023)
The MillenniumTNG Project: semi-analytic galaxy formation models on the past lightcone
in Monthly Notices of the Royal Astronomical Society
Hadzhiyska B
(2023)
The MillenniumTNG Project: refining the one-halo model of red and blue galaxies at different redshifts
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 |