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
Threlfall J
(2020)
How Is Helicity (and Twist) Partitioned in Magnetohydrodynamic Simulations of Reconnecting Magnetic Flux Tubes?
in The Astrophysical Journal
Thomas N
(2022)
The environments of the radio galaxy population in simba
in Monthly Notices of the Royal Astronomical Society
Theuns T
(2020)
Correlations between mass, stellar kinematics, and gas metallicity in eagle galaxies
in Monthly Notices of the Royal Astronomical Society: Letters
Stiskalek R
(2022)
The scatter in the galaxy-halo connection: a machine learning analysis
in Monthly Notices of the Royal Astronomical Society
Stickle A
(2022)
Effects of Impact and Target Parameters on the Results of a Kinetic Impactor: Predictions for the Double Asteroid Redirection Test (DART) Mission
in The Planetary Science Journal
Stevenson P
(2020)
A time-dependent Hartree-Fock study of triple-alpha dynamics
in SciPost Physics Proceedings
Stevenson P
(2020)
Internuclear potentials from the Sky3D code
in IOP SciNotes
Stevenson P
(2022)
Mean-field simulations of Es-254 + Ca-48 heavy-ion reactions
in Frontiers in Physics
Steele T
(2021)
Precise calibration of the one-loop bispectrum in the effective field theory of large scale structure
in Physical Review D
Stafford S
(2020)
Exploring extensions to the standard cosmological model and the impact of baryons on small scales
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
Sormani M
(2020)
Simulations of the Milky Way's Central Molecular Zone - II. Star formation
in Monthly Notices of the Royal Astronomical Society
Sorini D
(2020)
simba: the average properties of the circumgalactic medium of 2 = z = 3 quasars are determined primarily by stellar feedback
in Monthly Notices of the Royal Astronomical Society
Sorini D
(2022)
How baryons affect haloes and large-scale structure: a unified picture from the Simba simulation
in Monthly Notices of the Royal Astronomical Society
Soler J
(2020)
The history of dynamics and stellar feedback revealed by the H I filamentary structure in the disk of the Milky Way
in Astronomy & Astrophysics
Soler J
(2022)
The Galactic dynamics revealed by the filamentary structure in atomic hydrogen emission
in Astronomy & Astrophysics
Smith G
(2020)
The distribution of dark matter and gas spanning 6 Mpc around the post-merger galaxy cluster MS 0451-03
in Monthly Notices of the Royal Astronomical Society
Smith A
(2022)
A light-cone catalogue from the Millennium-XXL simulation: improved spatial interpolation and colour distributions for the DESI BGS
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
Skullerud J
(2022)
Hadrons at high temperature: An update from the FASTSUM collaboration
in EPJ Web of Conferences
Sirks E
(2022)
The effects of self-interacting dark matter on the stripping of galaxies that fall into clusters
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
Shao S
(2021)
The twisted dark matter halo of the Milky Way
in Monthly Notices of the Royal Astronomical Society
Sergeev D
(2020)
Atmospheric Convection Plays a Key Role in the Climate of Tidally Locked Terrestrial Exoplanets: Insights from High-resolution Simulations
in The Astrophysical Journal
Sedda M
(2020)
The missing link in gravitational-wave astronomy: discoveries waiting in the decihertz range
in Classical and Quantum Gravity