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
Prole L
(2023)
From dark matter halos to pre-stellar cores: high resolution follow-up of cosmological Lyman-Werner simulations
in Monthly Notices of the Royal Astronomical Society
Yang T
(2024)
Feedback-driven anisotropy in the circumgalactic medium for quenching galaxies in the simba simulations
in Monthly Notices of the Royal Astronomical Society
Camps P
(2022)
High-resolution synthetic UV-submm images for Milky Way-mass simulated galaxies from the ARTEMIS project
in Monthly Notices of the Royal Astronomical Society
Pakmor R
(2023)
The MillenniumTNG Project: the hydrodynamical full physics simulation and a first look at its galaxy clusters
in Monthly Notices of the Royal Astronomical Society
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
Merrow A
(2024)
Did the Gaia Enceladus/Sausage merger form the Milky Way's bar?
in Monthly Notices of the Royal Astronomical Society
Yurchenko S
(2024)
ExoMol line lists-LIX. High-temperature line list for N2O
in Monthly Notices of the Royal Astronomical Society
Choustikov N
(2024)
The great escape: understanding the connection between Ly a emission and LyC escape in simulated JWST analogues
in Monthly Notices of the Royal Astronomical Society
Tress R
(2020)
Simulations of the star-forming molecular gas in an interacting M51-like galaxy
in Monthly Notices of the Royal Astronomical Society
Forouhar Moreno V
(2022)
Baryon-driven decontraction in Milky Way-mass haloes
in Monthly Notices of the Royal Astronomical Society
Fattahi A
(2020)
A tale of two populations: surviving and destroyed dwarf galaxies and the build-up of the Milky Way's stellar halo
in Monthly Notices of the Royal Astronomical Society
Davies C
(2022)
Cosmological forecasts with the clustering of weak lensing peaks
in Monthly Notices of the Royal Astronomical Society
Ziampras A
(2025)
Dusty substructures induced by planets in ALMA discs: how dust growth and dynamics changes the picture
in Monthly Notices of the Royal Astronomical Society
Pereira-Wilson M
(2023)
The cosmic UV background and the beginning and end of star formation in simulated field dwarf galaxies
in Monthly Notices of the Royal Astronomical Society
Xu W
(2020)
Galaxy properties in the cosmic web of EAGLE simulation
in Monthly Notices of the Royal Astronomical Society
Baugh C
(2022)
Modelling emission lines in star-forming galaxies
in Monthly Notices of the Royal Astronomical Society
Zarrouk P
(2022)
Preliminary clustering properties of the DESI BGS bright targets using DR9 Legacy Imaging Surveys
in Monthly Notices of the Royal Astronomical Society
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
Bose S
(2023)
The MillenniumTNG Project: the large-scale clustering of galaxies
in Monthly Notices of the Royal Astronomical Society
Nealon R
(2020)
Spirals, shadows & precession in HD 100453 - II. The hidden companion
in Monthly Notices of the Royal Astronomical Society
Kukstas E
(2023)
GOGREEN: A critical assessment of environmental trends in cosmological hydrodynamical simulations at z ˜ 1
in Monthly Notices of the Royal Astronomical Society
Qiao L
(2022)
The evolution of protoplanetary discs in star formation and feedback simulations
in Monthly Notices of the Royal Astronomical Society
Young A
(2024)
Introducing two improved methods for approximating radiative cooling in hydrodynamical simulations of accretion discs
in Monthly Notices of the Royal Astronomical Society
Brooks R
(2023)
The north-south asymmetry of the ALFALFA H i velocity width function
in Monthly Notices of the Royal Astronomical Society
Turpin G
(2024)
Orbital evolution of close binary systems: comparing viscous and wind-driven circumbinary disc models
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 |