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
Scholtz J
(2024)
GN-z11: The environment of an active galactic nucleus at z = 10.603 New insights into the most distant Ly a detection
in Astronomy & Astrophysics
Forrest B
(2024)
MAGAZ3NE: Massive, Extremely Dusty Galaxies at z ~ 2 Lead to Photometric Overestimation of Number Densities of the Most Massive Galaxies at 3 < z < 4*
in The Astrophysical Journal
Feng J
(2024)
On the evolution of the observed mass-to-length relationship for star-forming filaments
in Monthly Notices of the Royal Astronomical Society
Callan F
(2024)
Including a luminous central remnant in radiative transfer simulations for Type Iax supernovae
in Monthly Notices of the Royal Astronomical Society
Del Debbio L
(2024)
Absorbing discretization effects with a massive renormalization scheme: The charm-quark mass
in Physical Review D
Rogers J
(2024)
Under the light of a new star: evolution of planetary atmospheres through protoplanetary disc dispersal and boil-off
in Monthly Notices of the Royal Astronomical Society
Sorini D
(2024)
The impact of feedback on the evolution of gas density profiles from galaxies to clusters: a universal fitting formula from the Simba suite of simulations
in The Open Journal of Astrophysics
Ahad S
(2024)
An environment-dependent halo mass function as a driver for the early quenching of z = 1.5 cluster galaxies
in Monthly Notices of the Royal Astronomical Society
Contreras S
(2024)
Validating the clustering predictions of empirical models with the FLAMINGO simulations
in Astronomy & Astrophysics
Satyavolu S
(2024)
Robustness of direct measurements of the mean free path of ionizing photons in the epoch of reionization
in Monthly Notices of the Royal Astronomical Society
Daley-Yates S
(2024)
Simulating stellar coronal rain and slingshot prominences
in Monthly Notices of the Royal Astronomical Society
Raste J
(2024)
The 21-cm bispectrum from neutral hydrogen islands at z < 6
in Monthly Notices of the Royal Astronomical Society
Delaney J
(2024)
Radiative transitions in charmonium from lattice QCD
in Journal of High Energy Physics
Brady R
(2024)
Numerical Equivalence of Diabatic and Adiabatic Representations in Diatomic Molecules
in Journal of Chemical Theory and Computation
Rizzuti F
(2024)
Shell mergers in the late stages of massive star evolution: new insight from 3D hydrodynamic simulations
in Monthly Notices of the Royal Astronomical Society
Cui W
(2024)
The HYENAS project: a prediction for the X-ray undetected galaxy groups
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
Merrow A
(2024)
Did the Gaia Enceladus/Sausage merger form the Milky Way's bar?
in Monthly Notices of the Royal Astronomical Society
Maccagni F
(2024)
MHONGOOSE discovery of a gas-rich low surface brightness galaxy in the Dorado group
in Astronomy & Astrophysics
Aurrekoetxea J
(2024)
Self-interacting scalar dark matter around binary black holes
in Physical Review D
Yurchenko S
(2024)
ExoMol line lists-LIX. High-temperature line list for N2O
in Monthly Notices of the Royal Astronomical Society
Regos E
(2024)
Percolation Statistics in the MillenniumTNG Simulations
in The Astrophysical Journal
Halim S
(2024)
Assessing the survival of carbonaceous chondrites impacting the lunar surface as a potential resource
in Planetary and Space Science
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
SalĆ³ L
(2024)
GRFolres: A code for modified gravity simulations in strong gravity
in Journal of Open Source Software
Worthy J
(2024)
Evaluation of the bilinear condensate of the planar Thirring model in the strongly coupled region
in International Journal of Modern Physics C
Garg P
(2024)
Theoretical Strong-line Metallicity Diagnostics for the JWST Era
in The Astrophysical Journal
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
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
Chadha-Day F
(2024)
ALP anarchy
in Journal of Cosmology and Astroparticle Physics
Burba J
(2024)
Sensitivity of Bayesian 21 cm power spectrum estimation to foreground model errors
in Monthly Notices of the Royal Astronomical Society
Kesri K
(2024)
Dependence of Spicule Properties on the Magnetic Field-Results from Magnetohydrodynamics Simulations
in The Astrophysical Journal
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
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
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
CamposĀ Estrada B
(2024)
On the likely magnesium-iron silicate dusty tails of catastrophically evaporating rocky planets
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
Aramburo-Garcia A
(2024)
Dark photon constraints from CMB temperature anisotropies
in Journal of Cosmology and Astroparticle Physics
Mills B
(2024)
Spectral Calculations of 3D Radiation Magnetohydrodynamic Simulations of Super-Eddington Accretion onto a Stellar-mass Black Hole
in The Astrophysical Journal
Madar M
(2024)
Predictions for the abundance and clustering of H a emitting galaxies
in Monthly Notices of the Royal Astronomical Society
Collier M
(2024)
Galaxy clustering in modified gravity from full-physics simulations - I. Two-point correlation functions
in Monthly Notices of the Royal Astronomical Society
Theuns T
(2024)
A halo model for cosmological Lyman-limit systems
in Monthly Notices of the Royal Astronomical Society
Kay S
(2024)
Relativistic SZ temperatures and hydrostatic mass bias for massive clusters in the FLAMINGO simulations
in Monthly Notices of the Royal Astronomical Society
Schaller M
(2024)
Swift : a modern highly parallel gravity and smoothed particle hydrodynamics solver for astrophysical and cosmological applications
in Monthly Notices of the Royal Astronomical Society
Zheng H
(2024)
The abundance of dark matter haloes down to Earth mass
in Monthly Notices of the Royal Astronomical Society
Jara-Ferreira F
(2024)
The metallicity gradients of star-forming regions store information of the assembly history of galaxies
in Monthly Notices of the Royal Astronomical Society
Wyper P
(2024)
A Model for Flux Rope Formation and Disconnection in Pseudostreamer Coronal Mass Ejections
in The Astrophysical Journal
Georgy C
(2024)
3D simulations of a neon burning convective shell in a massive star
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 |