DiRAC-3 Operations 2023-26 - UCL - Additional Grant

Lead Research Organisation: UNIVERSITY COLLEGE LONDON
Department Name: Physics and Astronomy

Abstract

This JeS form is a resubmission of part of the UCL DiRAC Operations grant request containing only the DI posts which have been approved for funding at 100% by STFC.

Publications

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Kannan R (2023) The MillenniumTNG project: the galaxy population at z = 8 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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Altamura E (2023) EAGLE-like simulation models do not solve the entropy core problem in groups and clusters of galaxies in Monthly Notices of the Royal Astronomical Society

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Chen C (2023) Can a binary star host three giant circumbinary planets? in Monthly Notices of the Royal Astronomical Society

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Trotta D (2023) Three-dimensional modelling of the shock-turbulence interaction in Monthly Notices of the Royal Astronomical Society

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Braspenning J (2023) Sensitivity of non-radiative cloud-wind interactions to the hydrodynamic solver in Monthly Notices of the Royal Astronomical Society

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Czakon M (2023) Infrared-safe flavoured anti-kT jets in Journal of High Energy Physics

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Pfeffer J (2023) Globular cluster metallicity distributions in the E-MOSAICS simulations in Monthly Notices of the Royal Astronomical Society

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Mak M (2023) 3D Simulations of the Archean Earth Including Photochemical Haze Profiles in Journal of Geophysical Research: Atmospheres

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Hernández-Aguayo C (2023) The MillenniumTNG Project: high-precision predictions for matter clustering and halo statistics in Monthly Notices of the Royal Astronomical Society

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Yankelevich V (2023) The halo bispectrum as a sensitive probe of massive neutrinos and baryon physics in Monthly Notices of the Royal Astronomical Society

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Morello G (2023) Spitzer thermal phase curve of WASP-121 b in Astronomy & Astrophysics

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Deason A (2023) Unravelling the mass spectrum of destroyed dwarf galaxies with the metallicity distribution function in Monthly Notices of the Royal Astronomical Society