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
Tress R
(2020)
Simulations of the star-forming molecular gas in an interacting M51-like galaxy
in Monthly Notices of the Royal Astronomical Society
Tress R
(2020)
Simulations of the Milky Way's central molecular zone - I. Gas dynamics
in Monthly Notices of the Royal Astronomical Society
Trujillo-Gomez S
(2021)
The kinematics of globular cluster populations in the E-MOSAICS simulations and their implications for the assembly history of the Milky Way
in Monthly Notices of the Royal Astronomical Society
Tröster T
(2019)
Painting with baryons: augmenting N-body simulations with gas using deep generative models
in Monthly Notices of the Royal Astronomical Society: Letters
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
Upadhyay A
(2021)
Star formation histories of Coma cluster galaxies matched to simulated orbits hint at quenching around first pericenter
in Astronomy & Astrophysics
Vandenbroucke B
(2020)
CMACIONIZE 2.0: a novel task-based approach to Monte Carlo radiation transfer
in Astronomy & Astrophysics
Vandenbroucke B
(2021)
Polarised emission from aligned dust grains in nearby galaxies: Predictions from the Auriga simulations
in Astronomy & Astrophysics
Van Daalen M
(2020)
Exploring the effects of galaxy formation on matter clustering through a library of simulation power spectra
in Monthly Notices of the Royal Astronomical Society
Van der Werf P
(2020)
An ALMA survey of the SCUBA-2 CLS UDS field: physical properties of 707 sub-millimetre galaxies
in Monthly Notices of the Royal Astronomical Society
Van Loon M
(2021)
Explaining the scatter in the galaxy mass-metallicity relation with gas flows
in Monthly Notices of the Royal Astronomical Society
Van Son L
(2019)
Galaxies with monstrous black holes in galaxy cluster environments
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
Veresvarska M
(2023)
Outer disc edge: properties of low-frequency aperiodic variability in ultracompact interacting binaries
in Monthly Notices of the Royal Astronomical Society
Vernon I
(2022)
Bayesian emulation and history matching of JUNE.
in Philosophical transactions. Series A, Mathematical, physical, and engineering sciences
Vidal J
(2020)
Efficiency of tidal dissipation in slowly rotating fully convective stars or planets
in Monthly Notices of the Royal Astronomical Society
Vijayan A
(2022)
First Light And Reionisation Epoch Simulations (FLARES) - III. The properties of massive dusty galaxies at cosmic dawn
in Monthly Notices of the Royal Astronomical Society
Vijayan A
(2020)
First Light And Reionisation Epoch Simulations (FLARES) II: The Photometric Properties of High-Redshift Galaxies
in Monthly Notices of the Royal Astronomical Society
Vincenzo F
(2018)
On the [a/Fe]-[Fe/H] relations in early-type galaxies
in Monthly Notices of the Royal Astronomical Society: Letters
Vizgan D
(2022)
Tracing Molecular Gas Mass in z ? 6 Galaxies with [C ii]
in The Astrophysical Journal
Vizgan D
(2022)
Investigating the [C ii]-to-H i Conversion Factor and the H i Gas Budget of Galaxies at z ˜ 6 with Hydrodynamic Simulations
in The Astrophysical Journal Letters
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
Wang E
(2019)
The impact of black hole seeding in cosmological simulations
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
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
Wang W
(2017)
What to expect from dynamical modelling of galactic haloes
in Monthly Notices of the Royal Astronomical Society
Wang Z
(2022)
Superradiance in massive vector fields with spatially varying mass
in Physical Review D
Wareing C
(2018)
A new mechanical stellar wind feedback model for the Rosette Nebula
in Monthly Notices of the Royal Astronomical Society
Weinberger L
(2018)
Lyman-a emitters gone missing: the different evolution of the bright and faint populations
in Monthly Notices of the Royal Astronomical Society
Welsh L
(2021)
The stochastic enrichment of Population II stars
in Monthly Notices of the Royal Astronomical Society
Wijers N
(2019)
The abundance and physical properties of O vii and O viii X-ray absorption systems in the EAGLE simulations
in Monthly Notices of the Royal Astronomical Society
Wijers N
(2022)
The warm-hot circumgalactic medium around EAGLE-simulation galaxies and its detection prospects with X-ray-line emission
in Monthly Notices of the Royal Astronomical Society
Wijers N
(2020)
The warm-hot circumgalactic medium around EAGLE-simulation galaxies and its detection prospects with X-ray and UV line absorption
in Monthly Notices of the Royal Astronomical Society
Wilkins S
(2023)
First Light And Reionization Epoch Simulations (FLARES) VII: The star formation and metal enrichment histories of galaxies in the early Universe
in Monthly Notices of the Royal Astronomical Society
Wilkins S
(2023)
First light and reionization epoch simulations (FLARES) XI: [O iii ] emitting galaxies at 5 < z < 10
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
Wilkins S
(2023)
First light and reionization epoch simulations (FLARES) V: the redshift frontier
in Monthly Notices of the Royal Astronomical Society
Williams C
(2021)
ALMA Measures Rapidly Depleted Molecular Gas Reservoirs in Massive Quiescent Galaxies at z ~ 1.5
in The Astrophysical Journal
Witstok J
(2021)
Prospects for observing the low-density cosmic web in Lyman- a emission
in Astronomy & Astrophysics
Wu X
(2020)
Photometric properties of reionization-epoch galaxies in the simba simulations
in Monthly Notices of the Royal Astronomical Society
Xia Q
(2021)
Intergalactic filaments spin
in Monthly Notices of the Royal Astronomical Society
Yachmenev A
(2021)
Electric quadrupole transitions in carbon dioxide.
in The Journal of chemical physics
Yang T
(2022)
Understanding the relation between thermal Sunyaev-Zeldovich decrement and halo mass using the simba and TNG simulations
in Monthly Notices of the Royal Astronomical Society
Yankelevich V
(2023)
The halo bispectrum as a sensitive probe of massive neutrinos and baryon physics
in Monthly Notices of the Royal Astronomical Society
Yardley S
(2021)
Simulating the Coronal Evolution of Bipolar Active Regions to Investigate the Formation of Flux Ropes
in Solar Physics
Young A
(2021)
Chemical signatures of a warped protoplanetary disc
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
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
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
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| Sectors | Digital/Communication/Information Technologies (including Software),Education |
| URL | https://dirac.ac.uk |