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
Li B
(2018)
Galaxy-galaxy weak gravitational lensing in f(R) gravity
in Monthly Notices of the Royal Astronomical Society
Roper W
(2022)
First Light And Reionisation Epoch Simulations ( flares ) - IV. The size evolution of galaxies at z = 5
in Monthly Notices of the Royal Astronomical Society
Zarrouk P
(2022)
Preliminary clustering properties of the DESI BGS bright targets using DR9 Legacy Imaging Surveys
in Monthly Notices of the Royal Astronomical Society
Negri A
(2022)
The luminosity of cluster galaxies in the Cluster-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
Errani R
(2021)
The asymptotic tidal remnants of cold dark matter subhaloes
in Monthly Notices of the Royal Astronomical Society
Katz H
(2018)
A Census of the LyC photons that form the UV background during reionization
in Monthly Notices of the Royal Astronomical Society
Errani R
(2022)
Structure and kinematics of tidally limited satellite galaxies in LCDM
in Monthly Notices of the Royal Astronomical Society
Regan J
(2018)
Rise of the first supermassive stars
in Monthly Notices of the Royal Astronomical Society
Pearce F
(2021)
Redshift evolution of the hot intracluster gas metallicity in the C-EAGLE cluster simulations
in Monthly Notices of the Royal Astronomical Society
Dillamore A
(2022)
Merger-induced galaxy transformations in the artemis simulations
in Monthly Notices of the Royal Astronomical Society
Ruiz-Macias O
(2021)
Characterizing the target selection pipeline for the Dark Energy Spectroscopic Instrument Bright Galaxy Survey
in Monthly Notices of the Royal Astronomical Society
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
Wu X
(2020)
Photometric properties of reionization-epoch galaxies in the simba simulations
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
Sormani M
(2019)
The geometry of the gas surrounding the Central Molecular Zone: on the origin of localized molecular clouds with extreme velocity dispersions
in Monthly Notices of the Royal Astronomical Society
Appleby S
(2023)
Mapping circumgalactic medium observations to theory using machine learning
in Monthly Notices of the Royal Astronomical Society
Smith A
(2022)
Solving small-scale clustering problems in approximate light-cone mocks
in Monthly Notices of the Royal Astronomical Society
Velliscig M
(2017)
Galaxy-galaxy lensing in EAGLE: comparison with data from 180 deg2 of the KiDS and GAMA surveys
in Monthly Notices of the Royal Astronomical Society
Müller B
(2018)
Multidimensional simulations of ultrastripped supernovae to shock breakout
in Monthly Notices of the Royal Astronomical Society
McNally C
(2018)
Low-mass planet migration in magnetically torqued dead zones - II. Flow-locked and runaway migration, and a torque prescription
in Monthly Notices of the Royal Astronomical Society
Armitage T
(2018)
The Cluster-EAGLE project: velocity bias and the velocity dispersion-mass relation of cluster galaxies
in Monthly Notices of the Royal Astronomical Society
Cautun M
(2018)
The Santiago-Harvard-Edinburgh-Durham void comparison - I. SHEDding light on chameleon gravity tests
in Monthly Notices of the Royal Astronomical Society
Ramírez-Galeano L
(2022)
Why most molecular clouds are gravitationally dominated
in Monthly Notices of the Royal Astronomical Society
Meru F
(2019)
Is the ring inside or outside the planet?: the effect of planet migration on dust rings
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 |