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
Ludlow A
(2016)
Einasto Profiles and the Dark Matter Power Spectrum
in Monthly Notices of the Royal Astronomical Society: Letters
Mateu C
(2017)
Predictions for the detection of tidal streams with Gaia using great-circle methods
in Monthly Notices of the Royal Astronomical Society
Shi D
(2017)
Environmental screening of dark matter haloes in f ( R ) gravity
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
Correa C
(2017)
The relation between galaxy morphology and colour in the EAGLE simulation
in Monthly Notices of the Royal Astronomical Society: Letters
Tramonte D
(2017)
Testing the conditional mass function of dark matter haloes against numerical N-body simulations
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
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
Wang M
(2017)
Tidal features of classical Milky Way satellites in a ? cold dark matter universe
in Monthly Notices of the Royal Astronomical Society
Peñarrubia J
(2017)
What galaxy masses perturb the local cosmic expansion?
in Monthly Notices of the Royal Astronomical Society
Oman K
(2017)
The "Building Blocks" of Stellar Halos
in Galaxies
Desmond H
(2017)
On the galaxy-halo connection in the EAGLE simulation
in Monthly Notices of the Royal Astronomical Society: Letters
Katz H
(2017)
Interpreting ALMA observations of the ISM during the epoch of reionization
in Monthly Notices of the Royal Astronomical Society
Syntelis P
(2017)
Recurrent CME-like Eruptions in Emerging Flux Regions. I. On the Mechanism of Eruptions
in The Astrophysical Journal
Schönrich R
(2017)
Assessing distances and consistency of kinematics in Gaia/TGAS
in Monthly Notices of the Royal Astronomical Society
Turner M
(2017)
A comparison of observed and simulated absorption from H i , C iv , and Si iv around z ˜ 2 star-forming galaxies suggests redshift-space distortions are due to inflows
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
Ashworth G
(2017)
Exploring the IMF of star clusters: a joint SLUG and LEGUS effort
in Monthly Notices of the Royal Astronomical Society
Wang W
(2017)
What to expect from dynamical modelling of galactic haloes
in Monthly Notices of the Royal Astronomical Society
Gonzalez-Perez V
(2017)
The host dark matter haloes of [O II] emitters at 0.5 < z < 1.5
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
Cristini A
(2017)
The First 3D Simulations of Carbon Burning in a Massive Star
in Proceedings of the International Astronomical Union
Bourne M
(2017)
AGN jet feedback on a moving mesh: cocoon inflation, gas flows and turbulence
in Monthly Notices of the Royal Astronomical Society
Pagano P
(2017)
Contribution of mode-coupling and phase-mixing of Alfvén waves to coronal heating
in Astronomy & Astrophysics
Barnes D
(2017)
The Cluster-EAGLE project: global properties of simulated clusters with resolved galaxies
in Monthly Notices of the Royal Astronomical Society
Müller B
(2017)
Supernova simulations from a 3D progenitor model - Impact of perturbations and evolution of explosion properties
in Monthly Notices of the Royal Astronomical Society
Aumer M
(2017)
The structural evolution of galaxies with both thin and thick discs
in Monthly Notices of the Royal Astronomical Society
Llinares C
(2017)
Weighted density fields as improved probes of modified gravity models
in Monthly Notices of the Royal Astronomical Society: Letters
Peters A
(2018)
Supercluster simulations: impact of baryons on the matter power spectrum and weak lensing forecasts for Super-CLASS
in Monthly Notices of the Royal Astronomical Society
Goldstraw E
(2018)
Comparison of methods for modelling coronal magnetic fields
in Astronomy & Astrophysics
Smith M
(2018)
Supernova feedback in numerical simulations of galaxy formation: separating physics from numerics
in Monthly Notices of the Royal Astronomical Society
Kegerreis J
(2018)
Consequences of Giant Impacts on Early Uranus for Rotation, Internal Structure, Debris, and Atmospheric Erosion
in The Astrophysical Journal
Ashworth G
(2018)
Theoretical predictions for IMF diagnostics in UV spectroscopy of star clusters
in Monthly Notices of the Royal Astronomical Society
Navarro J
(2018)
The innate origin of radial and vertical gradients in a simulated galaxy disc
in Monthly Notices of the Royal Astronomical Society
Henden N
(2018)
The FABLE simulations: a feedback model for galaxies, groups, and clusters
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
Camps P
(2018)
Data Release of UV to Submillimeter Broadband Fluxes for Simulated Galaxies from the EAGLE Project
in The Astrophysical Journal Supplement Series
Sharma M
(2018)
CEMPlifying reionization
in Monthly Notices of the Royal Astronomical Society
Wang W
(2018)
What to expect from dynamical modelling of galactic haloes - II. The spherical Jeans equation
in Monthly Notices of the Royal Astronomical Society
Ploeckinger S
(2018)
Tidal dwarf galaxies in cosmological simulations
in Monthly Notices of the Royal Astronomical Society
Antolin P
(2018)
In Situ Generation of Transverse Magnetohydrodynamic Waves from Colliding Flows in the Solar Corona
in The Astrophysical Journal Letters
Barber C
(2018)
Calibrated, cosmological hydrodynamical simulations with variable IMFs I: Method and effect on global galaxy scaling relations
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
Correa C
(2018)
The impact of feedback and the hot halo on the rates of gas accretion on to galaxies
in Monthly Notices of the Royal Astronomical Society
Mao T
(2018)
Resolution of the apparent discrepancy between the number of massive subhaloes in Abell 2744 and ?CDM
in Monthly Notices of the Royal Astronomical Society: Letters
Leo M
(2018)
Nonlinear growth of structure in cosmologies with damped matter fluctuations
in Journal of Cosmology and Astroparticle Physics
Grand R
(2018)
Aurigaia: mock Gaia DR2 stellar catalogues from the auriga cosmological simulations
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
Barnes L
(2018)
Galaxy formation efficiency and the multiverse explanation of the cosmological constant with EAGLE simulations
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 |