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
Bate M
(2023)
The statistical properties of stars at redshift, z = 5, compared with the present epoch
in Monthly Notices of the Royal Astronomical Society
Trotta D
(2023)
Three-dimensional modelling of the shock-turbulence interaction
in Monthly Notices of the Royal Astronomical Society
Callingham T
(2022)
The chemo-dynamical groups of Galactic globular clusters
in Monthly Notices of the Royal Astronomical Society
Genina A
(2020)
To ß or not to ß: can higher order Jeans analysis break the mass-anisotropy degeneracy in simulated dwarfs?
in Monthly Notices of the Royal Astronomical Society
Grove C
(2022)
The DESI N -body simulation project - I. Testing the robustness of simulations for the DESI dark time survey
in Monthly Notices of the Royal Astronomical Society
Qiao L
(2022)
The evolution of protoplanetary discs in star formation and feedback simulations
in Monthly Notices of the Royal Astronomical Society
Genina A
(2022)
Can tides explain the low dark matter density in Fornax?
in Monthly Notices of the Royal Astronomical Society
Gonzalez-Perez V
(2020)
Do model emission line galaxies live in filaments at z ~ 1?
in Monthly Notices of the Royal Astronomical Society
Santos-Santos I
(2022)
Satellite mass functions and the faint end of the galaxy mass-halo mass relation in LCDM
in Monthly Notices of the Royal Astronomical Society
Hughes M
(2022)
The physics governing the upper truncation mass of the globular cluster mass function
in Monthly Notices of the Royal Astronomical Society
Pakmor R
(2023)
The MillenniumTNG Project: the hydrodynamical full physics simulation and a first look at its galaxy clusters
in Monthly Notices of the Royal Astronomical Society
Chaikin E
(2022)
The importance of the way in which supernova energy is distributed around young stellar populations in simulations of galaxies
in Monthly Notices of the Royal Astronomical Society
Wilkins S
(2023)
First Light And Reionization Epoch Simulations (FLARES) VII: The star formation and metal enrichment histories of galaxies in the early Universe
in Monthly Notices of the Royal Astronomical Society
Bending T
(2022)
Supernovae and photoionizing feedback in spiral arm molecular clouds
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
Smith A
(2022)
Solving small-scale clustering problems in approximate light-cone mocks
in Monthly Notices of the Royal Astronomical Society
Zhang H
(2022)
Spherical accretion of collisional gas in modified gravity I: self-similar solutions and a new cosmological hydrodynamical code
in Monthly Notices of the Royal Astronomical Society
Vandenbroucke B
(2020)
Infrared luminosity functions and dust mass functions in the EAGLE simulation
in Monthly Notices of the Royal Astronomical Society
Kukstas E
(2020)
Environment from cross-correlations: connecting hot gas and the quenching of galaxies
in Monthly Notices of the Royal Astronomical Society
Richings A
(2022)
The effects of local stellar radiation and dust depletion on non-equilibrium interstellar chemistry
in Monthly Notices of the Royal Astronomical Society
Dalla Vecchia C
(2020)
Constraining the inner density slope of massive galaxy clusters
in Monthly Notices of the Royal Astronomical Society
Ramírez-Galeano L
(2022)
Why most molecular clouds are gravitationally dominated
in Monthly Notices of the Royal Astronomical Society
Icaza-Lizaola M
(2023)
A sparse regression approach for populating dark matter haloes and subhaloes with galaxies
in Monthly Notices of the Royal Astronomical Society
Trayford J
(2020)
Fade to grey: systematic variation of galaxy attenuation curves with galaxy properties in the eagle simulations
in Monthly Notices of the Royal Astronomical Society
He J
(2020)
Modelling the tightest relation between galaxy properties and dark matter halo properties from hydrodynamical simulations of galaxy formation
in Monthly Notices of the Royal Astronomical Society