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
Jackson T
(2020)
The star formation properties of the observed and simulated AGN Universe: BAT versus EAGLE
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
Ploeckinger S
(2020)
Radiative cooling rates, ion fractions, molecule abundances, and line emissivities including self-shielding and both local and metagalactic radiation fields
in Monthly Notices of the Royal Astronomical Society
Gómez J
(2022)
Halo merger tree comparison: impact on galaxy formation models
in Monthly Notices of the Royal Astronomical Society
Vera-Casanova A
(2022)
Linking the brightest stellar streams with the accretion history of Milky Way like galaxies
in Monthly Notices of the Royal Astronomical Society
Tress R
(2020)
Simulations of the Milky Way's central molecular zone - I. Gas dynamics
in Monthly Notices of the Royal Astronomical Society
Jennings F
(2023)
Halo scaling relations and hydrostatic mass bias in the simba simulation from realistic mock X-ray catalogues
in Monthly Notices of the Royal Astronomical Society
Pichon C
(2020)
Why do extremely massive disc galaxies exist today?
in Monthly Notices of the Royal Astronomical Society
Reina-Campos M
(2023)
Constraining the shape of dark matter haloes with globular clusters and diffuse stellar light in the E-MOSAICS simulations
in Monthly Notices of the Royal Astronomical Society
Ilee J
(2020)
Observing protoplanetary discs with the Square Kilometre Array - I. Characterizing pebble substructure caused by forming planets
in Monthly Notices of the Royal Astronomical Society
De Beer S
(2023)
Resolving the physics of quasar Ly a nebulae (RePhyNe): I. Constraining quasar host halo masses through circumgalactic medium kinematics
in Monthly Notices of the Royal Astronomical Society
Elvis M
(2020)
Q wind code release: a non-hydrodynamical approach to modelling line-driven winds in active galactic nuclei
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
Simpson C
(2020)
The milky way total mass profile as inferred from Gaia DR2
in Monthly Notices of the Royal Astronomical Society
De Ceuster F
(2023)
Radiative transfer as a Bayesian linear regression problem
in Monthly Notices of the Royal Astronomical Society
Srisawat C
(2020)
MEGA: Merger graphs of structure formation
in Monthly Notices of the Royal Astronomical Society
Eke V
(2020)
Understanding the large inferred Einstein radii of observed low-mass galaxy clusters
in Monthly Notices of the Royal Astronomical Society
Vidal J
(2020)
Efficiency of tidal dissipation in slowly rotating fully convective stars or planets
in Monthly Notices of the Royal Astronomical Society
Sawala T
(2023)
The Local Group's mass: probably no more than the sum of its parts
in Monthly Notices of the Royal Astronomical Society
Betts J
(2023)
Machine learning and structure formation in modified gravity
in Monthly Notices of the Royal Astronomical Society
Chaikin E
(2023)
A thermal-kinetic subgrid model for supernova feedback in simulations of galaxy formation
in Monthly Notices of the Royal Astronomical Society
Lamberts A
(2022)
Constraining blazar heating with the 2 ? z ? 3 Lyman-a forest
in Monthly Notices of the Royal Astronomical Society
Appleby S
(2023)
Mapping circumgalactic medium observations to theory using machine learning
in Monthly Notices of the Royal Astronomical Society
Van Daalen M
(2020)
Exploring the effects of galaxy formation on matter clustering through a library of simulation power spectra
in Monthly Notices of the Royal Astronomical Society
Kruijssen J
(2020)
Kraken reveals itself - the merger history of the Milky Way reconstructed with the E-MOSAICS simulations
in Monthly Notices of the Royal Astronomical Society