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
Stafford S
(2020)
Exploring extensions to the standard cosmological model and the impact of baryons on small scales
in Monthly Notices of the Royal Astronomical Society
Porth L
(2021)
Fast estimation of aperture-mass statistics - II. Detectability of higher order statistics in current and future surveys
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
Newton O
(2018)
The total satellite population of the Milky Way
in Monthly Notices of the Royal Astronomical Society
Tescari E
(2018)
The SAMI Galaxy Survey: understanding observations of large-scale outflows at low redshift with EAGLE simulations
in Monthly Notices of the Royal Astronomical Society
Appleby S
(2021)
The low-redshift circumgalactic medium in simba
in Monthly Notices of the Royal Astronomical Society
Teyssier R
(2020)
The loss of the intracluster medium in globular clusters
in Monthly Notices of the Royal Astronomical Society
Orkney M
(2021)
EDGE: two routes to dark matter core formation in ultra-faint dwarfs
in Monthly Notices of the Royal Astronomical Society
Davis T
(2019)
Evolution of the cold gas properties of simulated post-starburst galaxies
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
Šoltinskí T
(2021)
The detectability of strong 21 centimetre forest absorbers from the diffuse intergalactic medium in late reionisation models
in Monthly Notices of the Royal Astronomical Society
Deason A
(2022)
Dwarf stellar haloes: a powerful probe of small-scale galaxy formation and the nature of dark matter
in Monthly Notices of the Royal Astronomical Society
De Beer S
(2023)
Resolving the physics of quasar Ly a nebulae (RePhyNe): I. Constraining quasar host halo masses through circumgalactic medium kinematics
in Monthly Notices of the Royal Astronomical Society
Robertson A
(2023)
Why weak lensing cluster shapes are insensitive to self-interacting dark matter
in Monthly Notices of the Royal Astronomical Society
Garzilli A
(2021)
How to constrain warm dark matter with the Lyman-a forest
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
Bilimogga P
(2022)
Using eagle simulations to study the effect of observational constraints on the determination of H i asymmetries in galaxies
in Monthly Notices of the Royal Astronomical Society
Mayes R
(2021)
Contribution of stripped nuclei to the ultracompact dwarf galaxy population in the Virgo cluster
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
Baraffe I
(2023)
A study of convective core overshooting as a function of stellar mass based on two-dimensional hydrodynamical simulations
in Monthly Notices of the Royal Astronomical Society
Hafen Z
(2024)
The Halo21 absorption modelling challenge: lessons from 'observing' synthetic circumgalactic absorption spectra
in Monthly Notices of the Royal Astronomical Society
Deason A
(2023)
Unravelling the mass spectrum of destroyed dwarf galaxies with the metallicity distribution function
in Monthly Notices of the Royal Astronomical Society
Yurchenko S
(2024)
ExoMol line lists - LIV. Empirical line lists for AlH and AlD and experimental emission spectroscopy of AlD in A1? ( v = 0, 1, 2)
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
Baxter E
(2021)
The correlation of high-redshift galaxies with the thermal Sunyaev-Zel'dovich effect traces reionization
in Monthly Notices of the Royal Astronomical Society
Mackereth J
(2018)
The origin of diverse a-element abundances in galaxy discs
in Monthly Notices of the Royal Astronomical Society
Mitchell M
(2021)
A general framework to test gravity using galaxy clusters III: observable-mass scaling relations in f ( R ) gravity
in Monthly Notices of the Royal Astronomical Society
Suarez T
(2021)
Modelling intergalactic low ionization metal absorption line systems near the epoch of reionization
in Monthly Notices of the Royal Astronomical Society
Farahi A
(2018)
Localized massive halo properties in bahamas and MACSIS simulations: scalings, lognormality, and covariance
in Monthly Notices of the Royal Astronomical Society
Hillier A
(2023)
The role of cooling induced by mixing in the mass and energy cycles of the solar atmosphere
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
Jahns-Schindler J
(2023)
How limiting is optical follow-up for fast radio burst applications? Forecasts for radio and optical surveys
in Monthly Notices of the Royal Astronomical Society
Hou J
(2021)
How well is angular momentum accretion modelled in semi-analytic galaxy formation models?
in Monthly Notices of the Royal Astronomical Society
Elbers W
(2023)
Persistent topology of the reionization bubble network - II. Evolution and classification
in Monthly Notices of the Royal Astronomical Society
Shao S
(2019)
Evolution of galactic planes of satellites in the eagle simulation
in Monthly Notices of the Royal Astronomical Society
Orkney M
(2023)
Exploring the diversity and similarity of radially anisotropic Milky Way-like stellar haloes: implications for disrupted dwarf galaxy searches
in Monthly Notices of the Royal Astronomical Society
Mastromarino C
(2023)
Properties and observables of massive galaxies in self-interacting dark matter cosmologies
in Monthly Notices of the Royal Astronomical Society
Pichon C
(2020)
And yet it flips: connecting galactic spin and the cosmic web
in Monthly Notices of the Royal Astronomical Society
Desmond H
(2023)
On the functional form of the radial acceleration relation
in Monthly Notices of the Royal Astronomical Society
Gonzalez-Perez V
(2020)
Do model emission line galaxies live in filaments at z ~ 1?
in Monthly Notices of the Royal Astronomical Society
Šoltinský T
(2023)
Probing quasar lifetimes with proximate 21-centimetre absorption in the diffuse intergalactic medium at redshifts z = 6
in Monthly Notices of the Royal Astronomical Society
Santos-Santos I
(2023)
The Tucana dwarf spheroidal: a distant backsplash galaxy of M31?
in Monthly Notices of the Royal Astronomical Society
Becker G
(2021)
The mean free path of ionizing photons at 5 < z < 6: evidence for rapid evolution near reionization
in Monthly Notices of the Royal Astronomical Society
Cuesta-Lazaro C
(2020)
Towards a non-Gaussian model of redshift space distortions
in Monthly Notices of the Royal Astronomical Society
Hadzhiyska B
(2023)
The MillenniumTNG Project: an improved two-halo model for the galaxy-halo connection of red and blue galaxies
in Monthly Notices of the Royal Astronomical Society
Delgado A
(2023)
The MillenniumTNG project: intrinsic alignments of galaxies and haloes
in Monthly Notices of the Royal Astronomical Society
Koudmani S
(2022)
Two can play at that game: constraining the role of supernova and AGN feedback in dwarf galaxies with cosmological zoom-in simulations
in Monthly Notices of the Royal Astronomical Society
Borrow J
(2020)
Cosmological baryon transfer in the simba simulations
in Monthly Notices of the Royal Astronomical Society
Gaikwad P
(2023)
Measuring the photoionization rate, neutral fraction, and mean free path of H i ionizing photons at 4.9 = z = 6.0 from a large sample of XShooter and ESI spectra
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
| 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 |