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.

Publications

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Kelly A (2022) Apostle-Auriga: effects of different subgrid models on the baryon cycle around Milky Way-mass galaxies in Monthly Notices of the Royal Astronomical Society

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Glowacki M (2021) The redshift evolution of the baryonic Tully-Fisher relation in SIMBA in Monthly Notices of the Royal Astronomical Society

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Gu Q (2022) The spatial distribution of satellites in galaxy clusters in Monthly Notices of the Royal Astronomical Society

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Hou J (2018) A new gas cooling model for semi-analytic galaxy formation models in Monthly Notices of the Royal Astronomical Society

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Appleby S (2021) The low-redshift circumgalactic medium in simba in Monthly Notices of the Royal Astronomical Society

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Regan J (2018) Fragmentation inside atomic cooling haloes exposed to Lyman-Werner radiation in Monthly Notices of the Royal Astronomical Society

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McAlpine S (2018) The rapid growth phase of supermassive black holes in Monthly Notices of the Royal Astronomical Society

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Harnois-Déraps J (2023) mglens : Modified gravity weak lensing simulations for emulation-based cosmological inference in Monthly Notices of the Royal Astronomical Society

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Forouhar Moreno V (2022) Baryon-driven decontraction in Milky Way-mass haloes in Monthly Notices of the Royal Astronomical Society

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Manera M (2021) Obtaining nonlinear galaxy bias constraints from galaxy-lensing phase differences in Monthly Notices of the Royal Astronomical Society

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Chaikin E (2022) Simulations of 60Fe entrained in ejecta from a near-Earth supernova: effects of observer motion in Monthly Notices of the Royal Astronomical Society

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Gonzalez-Perez V (2020) Do model emission line galaxies live in filaments at z ~ 1? in Monthly Notices of the Royal Astronomical Society

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Hernández-Aguayo C (2019) Large-scale redshift space distortions in modified gravity theories in Monthly Notices of the Royal Astronomical Society

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Icaza-Lizaola M (2023) A sparse regression approach for populating dark matter haloes and subhaloes with galaxies in Monthly Notices of the Royal Astronomical Society

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Lovell M (2021) The spatial distribution of Milky Way satellites, gaps in streams, and the nature of dark matter in Monthly Notices of the Royal Astronomical Society

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Tress R (2020) Simulations of the star-forming molecular gas in an interacting M51-like galaxy 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