DiRAC Bridging Grant 2019 - Cambridge
Lead Research Organisation:
University of Cambridge
Department Name: Institute of Astronomy
Abstract
Abstracts are not currently available in GtR for all funded research. This is normally because the abstract was not required at the time of proposal submission, but may be because it included sensitive information such as personal details.
Organisations
Publications
Wilkins S
(2023)
First light and reionization epoch simulations (FLARES) XI: [O iii ] emitting galaxies at 5 < z < 10
in Monthly Notices of the Royal Astronomical Society
Griffin A
(2020)
AGNs at the cosmic dawn: predictions for future surveys from a ?CDM cosmological model
in Monthly Notices of the Royal Astronomical Society
Theuns T
(2021)
Connecting cosmological accretion to strong Ly a absorbers
in Monthly Notices of the Royal Astronomical Society
Frenk C
(2020)
The little things matter: relating the abundance of ultrafaint satellites to the hosts' assembly history
in Monthly Notices of the Royal Astronomical Society
Bahé Y
(2021)
Strongly lensed cluster substructures are not in tension with ?CDM
in Monthly Notices of the Royal Astronomical Society
Stafford S
(2021)
Testing extensions to ?CDM on small scales with forthcoming cosmic shear surveys
in Monthly Notices of the Royal Astronomical Society
Lovell C
(2022)
An orientation bias in observations of submillimetre galaxies
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
Mitchell M
(2022)
A general framework to test gravity using galaxy clusters - VI. Realistic galaxy formation simulations to study clusters in modified gravity
in Monthly Notices of the Royal Astronomical Society
Dutta R
(2020)
MUSE Analysis of Gas around Galaxies (MAGG) - II: metal-enriched halo gas around z ~ 1 galaxies
in Monthly Notices of the Royal Astronomical Society
Ganeshaiah Veena P
(2021)
Cosmic Ballet III: Halo spin evolution in the cosmic web
in Monthly Notices of the Royal Astronomical Society
McAlpine S
(2019)
The nature of submillimetre and highly star-forming galaxies in the EAGLE simulation
in Monthly Notices of the Royal Astronomical Society
Wurster J
(2019)
Disc formation and fragmentation using radiative non-ideal magnetohydrodynamics
in Monthly Notices of the Royal Astronomical Society
Irodotou D
(2022)
The effects of AGN feedback on the structural and dynamical properties of Milky Way-mass galaxies in cosmological simulations
in Monthly Notices of the Royal Astronomical Society
Robertson A
(2020)
Mapping dark matter and finding filaments: calibration of lensing analysis techniques on simulated data
in Monthly Notices of the Royal Astronomical Society
Vijayan A
(2022)
First Light And Reionisation Epoch Simulations (FLARES) - III. The properties of massive dusty galaxies at cosmic dawn
in Monthly Notices of the Royal Astronomical Society
Riley A
(2019)
The velocity anisotropy of the Milky Way satellite system
in Monthly Notices of the Royal Astronomical Society
Robson D
(2023)
Redshift evolution of galaxy group X-ray properties in the Simba simulations
in Monthly Notices of the Royal Astronomical Society
Pfeffer J
(2020)
Predicting accreted satellite galaxy masses and accretion redshifts based on globular cluster orbits in the E-MOSAICS simulations
in Monthly Notices of the Royal Astronomical Society
Reeves A
(2023)
Constraining quenching time-scales in galaxy clusters by forward-modelling stellar ages and quiescent fractions in projected phase space
in Monthly Notices of the Royal Astronomical Society
Altamura E
(2023)
Galaxy cluster rotation revealed in the MACSIS simulations with the kinetic Sunyaev-Zeldovich effect
in Monthly Notices of the Royal Astronomical Society
Altamura E
(2023)
EAGLE-like simulation models do not solve the entropy core problem in groups and clusters of galaxies
in Monthly Notices of the Royal Astronomical Society
Acuto A
(2021)
The BAHAMAS project: evaluating the accuracy of the halo model in predicting the non-linear matter power spectrum
in Monthly Notices of the Royal Astronomical Society
Borukhovetskaya A
(2022)
The tidal evolution of the Fornax dwarf spheroidal and its globular clusters
in Monthly Notices of the Royal Astronomical Society
Kong S
(2022)
Filament formation via collision-induced magnetic reconnection - formation of a star cluster
in Monthly Notices of the Royal Astronomical Society
Dobbs C
(2019)
Comparing the properties of GMCs in M33 from simulations and observations
in Monthly Notices of the Royal Astronomical Society
McAlpine S
(2020)
Galaxy mergers in eagle do not induce a significant amount of black hole growth yet do increase the rate of luminous AGN
in Monthly Notices of the Royal Astronomical Society
Elbers W
(2021)
An optimal non-linear method for simulating relic neutrinos
in Monthly Notices of the Royal Astronomical Society
Ballabio G
(2021)
HD 143006: circumbinary planet or misaligned disc?
in Monthly Notices of the Royal Astronomical Society
Mahmoud R
(2019)
Reverberation reveals the truncated disc in the hard state of GX 339-4
in Monthly Notices of the Royal Astronomical Society
Deason A
(2021)
The mass of the Milky Way out to 100 kpc using halo stars
in Monthly Notices of the Royal Astronomical Society
Pettini M
(2020)
A bound on the 12C/13C ratio in near-pristine gas with ESPRESSO
in Monthly Notices of the Royal Astronomical Society
Deason A
(2022)
Dwarf stellar haloes: a powerful probe of small-scale galaxy formation and the nature of dark matter
in Monthly Notices of the Royal Astronomical Society
Humphries J
(2019)
Constraining the initial planetary population in the gravitational instability model
in Monthly Notices of the Royal Astronomical Society
Katsianis A
(2020)
The high-redshift SFR-M* relation is sensitive to the employed star formation rate and stellar mass indicators: towards addressing the tension between observations and simulations
in Monthly Notices of the Royal Astronomical Society
Deason A
(2019)
The local high-velocity tail and the Galactic escape speed
in Monthly Notices of the Royal Astronomical Society
Navarro J
(2019)
Baryon-induced dark matter cores in the eagle simulations
in Monthly Notices of the Royal Astronomical Society
Lovell M
(2019)
The signal of decaying dark matter with hydrodynamical simulations
in Monthly Notices of the Royal Astronomical Society
Braspenning J
(2023)
Sensitivity of non-radiative cloud-wind interactions to the hydrodynamic solver
in Monthly Notices of the Royal Astronomical Society
Pfeffer J
(2023)
Globular cluster metallicity distributions in the E-MOSAICS simulations
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
Wijers N
(2020)
The warm-hot circumgalactic medium around EAGLE-simulation galaxies and its detection prospects with X-ray and UV line absorption
in Monthly Notices of the Royal Astronomical Society
Evans T
(2020)
How unusual is the Milky Way's assembly history?
in Monthly Notices of the Royal Astronomical Society
Cuesta-Lazaro C
(2020)
Towards a non-Gaussian model of redshift space distortions
in Monthly Notices of the Royal Astronomical Society
Nobels F
(2022)
The interplay between AGN feedback and precipitation of the intracluster medium in simulations of galaxy groups and clusters
in Monthly Notices of the Royal Astronomical Society
Lovell M
(2021)
The spatial distribution of Milky Way satellites, gaps in streams, and the nature of dark matter
in Monthly Notices of the Royal Astronomical Society
Hughes M
(2021)
What to expect when using globular clusters as tracers of the total mass distribution in Milky Way-mass galaxies
in Monthly Notices of the Royal Astronomical Society
Christiansen J
(2020)
Jet feedback and the photon underproduction crisis in simba
in Monthly Notices of the Royal Astronomical Society
Ragusa E
(2020)
The evolution of large cavities and disc eccentricity in circumbinary discs
in Monthly Notices of the Royal Astronomical Society
Sormani M
(2020)
Simulations of the Milky Way's Central Molecular Zone - II. Star formation
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 the HPC resources provided by DiRAC. |
| Sectors | Aerospace, Defence and Marine,Creative Economy,Digital/Communication/Information Technologies (including Software),Education,Healthcare |