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.
Organisations
Publications
Owen J
(2020)
Massive discs around low-mass stars
in Monthly Notices of the Royal Astronomical Society
Huško F
(2023)
The buildup of galaxies and their spheroids: The contributions of mergers, disc instabilities, and star formation
in Monthly Notices of the Royal Astronomical Society
Le Saux A
(2023)
Two-dimensional simulations of internal gravity waves in a 5 M? zero-age-main-sequence model
in Monthly Notices of the Royal Astronomical Society
Amorisco N
(2022)
Halo concentration strengthens dark matter constraints in galaxy-galaxy strong lensing analyses
in Monthly Notices of the Royal Astronomical Society
Burba J
(2024)
Sensitivity of Bayesian 21 cm power spectrum estimation to foreground model errors
in Monthly Notices of the Royal Astronomical Society
Goyal J
(2020)
A library of self-consistent simulated exoplanet atmospheres
in Monthly Notices of the Royal Astronomical Society
Prole L
(2022)
Primordial magnetic fields in Population III star formation: a magnetized resolution study
in Monthly Notices of the Royal Astronomical Society
Hassan S
(2020)
Testing galaxy formation simulations with damped Lyman-a abundance and metallicity evolution
in Monthly Notices of the Royal Astronomical Society
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
Bending T
(2022)
Supernovae and photoionizing feedback in spiral arm molecular clouds
in Monthly Notices of the Royal Astronomical Society
Young A
(2023)
On the conditions for warping and breaking protoplanetary discs
in Monthly Notices of the Royal Astronomical Society
Coleman G
(2024)
Photoevaporation obfuscates the distinction between wind and viscous angular momentum transport in protoplanetary discs
in Monthly Notices of the Royal Astronomical Society
Yankelevich V
(2023)
The halo bispectrum as a sensitive probe of massive neutrinos and baryon physics
in Monthly Notices of the Royal Astronomical Society
Upadhye A
(2024)
Non-linear CMB lensing with neutrinos and baryons: FLAMINGO simulations versus fast approximations
in Monthly Notices of the Royal Astronomical Society
Herrington N
(2024)
Magnetic fields in star-forming environments: how does field strength affect gas on spiral arm and cloud scales?
in Monthly Notices of the Royal Astronomical Society
Zheng H
(2024)
The influence of baryons on low-mass haloes
in Monthly Notices of the Royal Astronomical Society
Izquierdo A
(2021)
The Cloud Factory II: gravoturbulent kinematics of resolved molecular clouds in a galactic potential
in Monthly Notices of the Royal Astronomical Society
Sirks E
(2024)
Hydrodynamical simulations of merging galaxy clusters: giant dark matter particle colliders, powered by gravity
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
Sorini D
(2020)
simba: the average properties of the circumgalactic medium of 2 = z = 3 quasars are determined primarily by stellar feedback
in Monthly Notices of the Royal Astronomical Society
Campos Estrada B
(2024)
On the likely magnesium-iron silicate dusty tails of catastrophically evaporating rocky planets
in Monthly Notices of the Royal Astronomical Society
He J
(2020)
Modelling the tightest relation between galaxy properties and dark matter halo properties from hydrodynamical simulations of galaxy formation
in Monthly Notices of the Royal Astronomical Society
Davé R
(2020)
Galaxy cold gas contents in modern cosmological hydrodynamic simulations
in Monthly Notices of the Royal Astronomical Society
Kugel R
(2023)
FLAMINGO: calibrating large cosmological hydrodynamical simulations with machine learning.
in Monthly notices of the Royal Astronomical Society
Nobels F
(2024)
Tests of subgrid models for star formation using simulations of isolated disc galaxies
in Monthly Notices of the Royal Astronomical Society
| Description | Many new discoveries about the formation and evolution of galaxies, star formation, planet formation and particle physics theory have been made possible by the award. |
| Exploitation Route | Many international collaborative projects are supported by our results |
| Sectors | Aerospace Defence and Marine Digital/Communication/Information Technologies (including Software) Education |