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
Fenton A
(2024)
The 3D structure of disc-instability protoplanets
in Astronomy & Astrophysics
Štofanová L
(2024)
Prospects for detecting the circum- and intergalactic medium in X-ray absorption using the extended intracluster medium as a backlight
in Monthly Notices of the Royal Astronomical Society
Aurrekoetxea J
(2024)
Revisiting the Cosmic String Origin of GW190521
in Physical Review Letters
Rey M
(2024)
Boosting galactic outflows with enhanced resolution
in Monthly Notices of the Royal Astronomical Society
Xiao M
(2024)
Accelerated formation of ultra-massive galaxies in the first billion years.
in Nature
Varghese A
(2024)
Effect of Rotation on Wave Mixing in Intermediate-mass Stars
in The Astrophysical Journal
Broxterman J
(2024)
The FLAMINGO project: baryonic impact on weak gravitational lensing convergence peak counts
in Monthly Notices of the Royal Astronomical Society
Schreyer E
(2024)
Using Ly a transits to constrain models of atmospheric escape
in Monthly Notices of the Royal Astronomical Society
Martin-Alvarez S
(2024)
Extragalactic Magnetism with SOFIA (SALSA Legacy Program). VII. A Tomographic View of Far-infrared and Radio Polarimetric Observations through MHD Simulations of Galaxies
in The Astrophysical Journal
Chung-Jukko L
(2024)
Multimessenger signals from compact axion star mergers
in Physical Review D
Lim S
(2024)
The FLAMINGO simulation view of cluster progenitors observed in the epoch of reionization with JWST
in Monthly Notices of the Royal Astronomical Society
Ziampras A
(2024)
Migration of low-mass planets in inviscid discs: the effect of radiation transport on the dynamical corotation torque
in Monthly Notices of the Royal Astronomical Society
Sante A
(2024)
Applying machine learning to Galactic Archaeology: how well can we recover the origin of stars in Milky Way-like galaxies?
in Monthly Notices of the Royal Astronomical Society
Bowesman C
(2024)
ExoMol line lists - LV: hyperfine-resolved molecular line list for vanadium monoxide (51V16O)
in Monthly Notices of the Royal Astronomical Society
Nasir F
(2024)
Deep learning the intergalactic medium using Lyman-alpha forest at 4 = z = 5
in Monthly Notices of the Royal Astronomical Society
Prole L
(2024)
Heavy black hole seed formation in high- z atomic cooling halos
in Astronomy & Astrophysics
Rowther S
(2024)
The role of drag and gravity on dust concentration in a gravitationally unstable disc
in Monthly Notices of the Royal Astronomical Society
Durán-Camacho E
(2024)
Self-consistent modelling of the Milky Way structure using live potentials
in Monthly Notices of the Royal Astronomical Society
Arvizu A
(2024)
Modeling the 3-point correlation function of projected scalar fields on the sphere
in Journal of Cosmology and Astroparticle Physics
Murtas G
(2024)
Kink Instability of Flux Ropes in Partially Ionized Plasmas
in The Astrophysical Journal
Zamyatina M
(2024)
Quenching-driven equatorial depletion and limb asymmetries in hot Jupiter atmospheres: WASP-96b example
in Monthly Notices of the Royal Astronomical Society
Brough S
(2024)
Preparing for low surface brightness science with the Vera C. Rubin Observatory: a comparison of observable and simulated intracluster light fractions
in Monthly Notices of the Royal Astronomical Society
Bennett E
(2024)
Lattice investigations of the chimera baryon spectrum in the S p ( 4 ) gauge theory
in Physical Review D
Lindert J
(2024)
Logarithmic EW corrections at one-loop
in The European Physical Journal C
Welsh L
(2024)
A survey of extremely metal-poor gas at cosmic noon Evidence of elevated [O/Fe]
in Astronomy & Astrophysics
Boyle P
(2024)
Kaon mixing beyond the standard model with physical masses
in Physical Review D
Lynas-Gray A
(2024)
ExoMol line lists - LXII. Ro-vibrational energy levels and line strengths for the propadienediylidene (C3) in its ground electronic state
in Monthly Notices of the Royal Astronomical Society
Pallero D
(2024)
Galaxy evolution in modified gravity simulations: using galaxy properties to constrain our gravitational model
in Monthly Notices of the Royal Astronomical Society
Ziampras A
(2024)
Buoyancy torques prevent low-mass planets from stalling in low-turbulence radiative discs
in Monthly Notices of the Royal Astronomical Society
Dai Z
(2024)
Physics-informed neural networks in the recreation of hydrodynamic simulations from dark matter
in Monthly Notices of the Royal Astronomical Society
Ibrahim D
(2024)
The impact of supernova feedback on the mass-metallicity relations
in Monthly Notices of the Royal Astronomical Society
Hoy C
(2024)
bilby in space: Bayesian inference for transient gravitational-wave signals observed with LISA
in Monthly Notices of the Royal Astronomical Society
Huško F
(2024)
Winds versus jets: a comparison between black hole feedback modes in simulations of idealized galaxy groups and clusters
in Monthly Notices of the Royal Astronomical Society
Pfeffer J
(2024)
Origin of the correlation between stellar kinematics and globular cluster system richness in ultradiffuse galaxies
in Monthly Notices of the Royal Astronomical Society
Kugel R
(2024)
The FLAMINGO project: a comparison of galaxy cluster samples selected on mass, X-ray luminosity, Compton-Y parameter, or galaxy richness
in Monthly Notices of the Royal Astronomical Society
Bennett E
(2024)
Singlets in gauge theories with fundamental matter
in Physical Review D
Nowak M
(2024)
The orbit of HD 142527 B is too compact to explain many of the disc features
in Astronomy & Astrophysics
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
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
| 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 |