DiRAC-3 Operations - 2022-23 extension - Cambridge

Lead Research Organisation: University of Cambridge
Department Name: Institute of Astronomy

Abstract

This grant is a costed 12-month extension of the grant "DiRAC-3 Operations 2019-2022 - Cambridge [2020-06 resubmission]", (STFC reference: ST/V002635/1).

Publications

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Dobbs C (2022) The formation of massive stellar clusters in converging galactic flows with photoionization in Monthly Notices of the Royal Astronomical Society

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Drach V (2022) Singlet channel scattering in a composite Higgs model on the lattice in The European Physical Journal C

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Elbakyan V (2023) Episodic accretion and mergers during growth of massive protostars in Monthly Notices of the Royal Astronomical Society

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Elbers W (2022) Higher order initial conditions with massive neutrinos in Monthly Notices of the Royal Astronomical Society

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Evans T (2022) Observing EAGLE galaxies with JWST : predictions for Milky Way progenitors and their building blocks in Monthly Notices of the Royal Astronomical Society

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Fancher J (2023) On the relative importance of shocks and self-gravity in modifying tidal disruption event debris streams in Monthly Notices of the Royal Astronomical Society

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Fenton A (2024) The 3D structure of disc-instability protoplanets in Astronomy & Astrophysics

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Flynn J (2023) Exclusive semileptonic B s ? K l ? decays on the lattice in Physical Review D

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Font A (2022) Quenching of satellite galaxies of Milky Way analogues: reconciling theory and observations 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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Forouhar Moreno V (2022) Galactic satellite systems in CDM, WDM and SIDM in Monthly Notices of the Royal Astronomical Society

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Gavardi A (2023) NNLO+PS W+W- production using jet veto resummation at NNLL' in Journal of High Energy Physics

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Genina A (2023) On the edge: the relation between stellar and dark matter haloes of Milky Way-mass galaxies in Monthly Notices of the Royal Astronomical Society

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Genina A (2022) Can tides explain the low dark matter density in Fornax? in Monthly Notices of the Royal Astronomical Society

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Ghosh S (2022) Age dissection of the vertical breathing motions in Gaia DR2: evidence for spiral driving in Monthly Notices of the Royal Astronomical Society

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Givans J (2022) Non-linearities in the Lyman-a forest and in its cross-correlation with dark matter halos in Journal of Cosmology and Astroparticle Physics

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Glowacki M (2022) ASymba: H i global profile asymmetries in the simba simulation 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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Gupta P (2022) A study of global magnetic helicity in self-consistent spherical dynamos in Geophysical & Astrophysical Fluid Dynamics

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Gómez J (2022) Halo merger tree comparison: impact on galaxy formation models in Monthly Notices of the Royal Astronomical Society

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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

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Hadzhiyska B (2023) The MillenniumTNG Project: refining the one-halo model of red and blue galaxies at different redshifts in Monthly Notices of the Royal Astronomical Society

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Haidar H (2022) The black hole population in low-mass galaxies in large-scale cosmological simulations 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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He Q (2022) Galaxy-galaxy strong lens perturbations: line-of-sight haloes versus lens subhaloes in Monthly Notices of the Royal Astronomical Society

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He Q (2022) A forward-modelling method to infer the dark matter particle mass from strong gravitational lenses in Monthly Notices of the Royal Astronomical Society

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Heinesen A (2022) A prediction for anisotropies in the nearby Hubble flow in Journal of Cosmology and Astroparticle Physics