DiRAC-3 Operations 2019-2022 - Cambridge [2020-06 resubmission]

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

Abstract

DiRAC-3 Operations 2019-2022 resubmission; This is an administrative resubmission to replace ST/S003800/1 which has already been peer-reviewed.

Publications

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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

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Borrow J (2023) The impact of stochastic modelling on the predictive power of galaxy formation simulations in Monthly Notices of the Royal Astronomical Society

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Trujillo-Gomez S (2023) In situ or accreted? Using deep learning to infer the origin of extragalactic globular clusters from observables in Monthly Notices of the Royal Astronomical Society

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Dobbs C (2022) The formation of clusters and OB associations in different density spiral arm environments in Monthly Notices of the Royal Astronomical Society

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Ballabio G (2023) [O i ] 6300 Å emission as a probe of external photoevaporation of protoplanetary discs in Monthly Notices of the Royal Astronomical Society

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Lee E (2022) A multisimulation study of relativistic SZ temperature scalings in galaxy clusters and groups in Monthly Notices of the Royal Astronomical Society

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Davé R (2020) Galaxy cold gas contents in modern cosmological hydrodynamic simulations in Monthly Notices of the Royal Astronomical Society

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Whitworth D (2022) Is the molecular KS relationship universal down to low metallicities? in Monthly Notices of the Royal Astronomical Society

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Wilson B (2022) A measurement of the Ly ß forest power spectrum and its cross with the Ly a forest in X-Shooter XQ-100 in Monthly Notices of the Royal Astronomical Society

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Robson D (2023) Redshift evolution of galaxy group X-ray properties in the Simba simulations in Monthly Notices of the Royal Astronomical Society

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Li B (2020) Measuring the baryon acoustic oscillation peak position with different galaxy selections 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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Wurster J (2021) Do we need non-ideal magnetohydrodynamic to model protostellar discs? in Monthly Notices of the Royal Astronomical Society

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Young A (2022) Characteristics of small protoplanetary disc warps in kinematic observations in Monthly Notices of the Royal Astronomical Society

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Cataneo M (2022) The matter density PDF for modified gravity and dark energy with Large Deviations Theory in Monthly Notices of the Royal Astronomical Society

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Kong S (2022) Filament formation via collision-induced magnetic reconnection - formation of a star cluster in Monthly Notices of the Royal Astronomical Society

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Prgomet M (2022) EDGE: The sensitivity of ultra-faint dwarfs to a metallicity-dependent initial mass function in Monthly Notices of the Royal Astronomical Society

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Amorisco N (2022) Halo concentration strengthens dark matter constraints in galaxy-galaxy strong lensing analyses in Monthly Notices of the Royal Astronomical Society

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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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Davies C (2022) Cosmological forecasts with the clustering of weak lensing peaks 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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Oppenheimer B (2020) Feedback from supermassive black holes transforms centrals into passive galaxies by ejecting circumgalactic gas 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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Falle S (2020) Thermal instability revisited in Monthly Notices of the Royal Astronomical Society

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Brown S (2022) Towards a universal model for the density profiles of dark matter haloes in Monthly Notices of the Royal Astronomical Society

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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

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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

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Ali A (2023) Star cluster formation and feedback in different environments of a Milky Way-like galaxy in Monthly Notices of the Royal Astronomical Society

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Rey M (2022) EDGE: What shapes the relationship between H i and stellar observables in faint dwarf galaxies? in Monthly Notices of the Royal Astronomical Society

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Lovell C (2023) First light and reionisation epoch simulations (FLARES) - VIII. The emergence of passive galaxies at z = 5 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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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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Anderson S (2022) The secular growth of bars revealed by flat (peak + shoulders) density profiles in Monthly Notices of the Royal Astronomical Society

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Huško F (2022) Spin-driven jet feedback in idealized simulations of galaxy groups and clusters in Monthly Notices of the Royal Astronomical Society

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Borukhovetskaya A (2022) The tidal evolution of the Fornax dwarf spheroidal and its globular clusters in Monthly Notices of the Royal Astronomical Society

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Conaboy L (2023) Relative baryon-dark matter velocities in cosmological zoom simulations in Monthly Notices of the Royal Astronomical Society

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Negri A (2022) The luminosity of cluster galaxies in the Cluster-EAGLE simulations in Monthly Notices of the Royal Astronomical Society

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Rosenberg E (2022) CMB power spectra and cosmological parameters from Planck PR4 with CamSpec in Monthly Notices of the Royal Astronomical Society

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Cuesta-Lazaro C (2020) Towards a non-Gaussian model of redshift space distortions in Monthly Notices of the Royal Astronomical Society