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
Santos-Santos I
(2024)
Anisotropies in the spatial distribution and kinematics of dwarf galaxies in the Local Group and beyond
in Monthly Notices of the Royal Astronomical Society
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
Saló L
(2024)
GRFolres: A code for modified gravity simulations in strong gravity
in Journal of Open Source Software
| 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 |