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
Negri A
(2022)
The luminosity of cluster galaxies in the Cluster-EAGLE simulations
in Monthly Notices of the Royal Astronomical Society
Katsianis A
(2021)
The specific star formation rate function at different mass scales and quenching: a comparison between cosmological models and SDSS
in Monthly Notices of the Royal Astronomical Society
Smith G
(2020)
The distribution of dark matter and gas spanning 6 Mpc around the post-merger galaxy cluster MS 0451-03
in Monthly Notices of the Royal Astronomical Society
Wang D
(2023)
Star formation concentration as a tracer of environmental quenching in action: a study of the eagle and c-eagle simulations
in Monthly Notices of the Royal Astronomical Society
Decataldo D
(2020)
Shaping the structure of a GMC with radiation and winds
in Monthly Notices of the Royal Astronomical Society
Wilkins S
(2022)
First Light and Reionisation Epoch Simulations (FLARES) - VI. The colour evolution of galaxies z = 5-15
in Monthly Notices of the Royal Astronomical Society
Newton O
(2018)
The total satellite population of the Milky Way
in Monthly Notices of the Royal Astronomical Society
Lovell C
(2023)
First light and reionisation epoch simulations (FLARES) - VIII. The emergence of passive galaxies at z = 5
in Monthly Notices of the Royal Astronomical Society
Davies C
(2019)
The self-similarity of weak lensing peaks
in Monthly Notices of the Royal Astronomical Society
Mitchell P
(2020)
Galactic inflow and wind recycling rates in the eagle simulations
in Monthly Notices of the Royal Astronomical Society
Sorini D
(2020)
simba: the average properties of the circumgalactic medium of 2 = z = 3 quasars are determined primarily by stellar feedback
in Monthly Notices of the Royal Astronomical Society
Kugel R
(2023)
FLAMINGO: calibrating large cosmological hydrodynamical simulations with machine learning.
in Monthly notices of the Royal Astronomical Society
Keating L
(2020)
Constraining the second half of reionization with the Ly ß forest
in Monthly Notices of the Royal Astronomical Society
Cai Y
(2017)
Gravitational redshift and asymmetric redshift-space distortions for stacked clusters
in Monthly Notices of the Royal Astronomical Society
Zarrouk P
(2021)
Baryon acoustic oscillations in the projected cross-correlation function between the eBOSS DR16 quasars and photometric galaxies from the DESI Legacy Imaging Surveys
in Monthly Notices of the Royal Astronomical Society
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
Forouhar Moreno V
(2022)
Galactic satellite systems in CDM, WDM and SIDM
in Monthly Notices of the Royal Astronomical Society
Bennett J
(2024)
The growth of the gargantuan black holes powering high-redshift quasars and their impact on the formation of early galaxies and protoclusters
in Monthly Notices of the Royal Astronomical Society
Hughes M
(2021)
What to expect when using globular clusters as tracers of the total mass distribution in Milky Way-mass galaxies
in Monthly Notices of the Royal Astronomical Society
Aumer M
(2017)
Migration and kinematics in growing disc galaxies with thin and thick discs
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
Pontzen A
(2021)
EDGE: a new approach to suppressing numerical diffusion in adaptive mesh simulations of galaxy formation
in Monthly Notices of the Royal Astronomical Society
Haworth T
(2021)
Warm millimetre dust in protoplanetary discs near massive stars
in Monthly Notices of the Royal Astronomical Society
Sharma M
(2018)
CEMPlifying reionization
in Monthly Notices of the Royal Astronomical Society
Zheng Y
(2022)
Rapidly quenched galaxies in the Simba cosmological simulation and observations
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 |