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
Thomas N
(2022)
The environments of the radio galaxy population in simba.
in Monthly notices of the Royal Astronomical Society
Thomas P
(2023)
First light and reionization epoch simulations ( Flares ) X: environmental galaxy bias and survey variance at high redshift
in Monthly Notices of the Royal Astronomical Society
Thompson J
(2024)
Phenomenological gravitational-wave model for precessing black-hole binaries with higher multipoles and asymmetries
in Physical Review D
Thompson O
(2024)
Predictions for CO emission and the CO-to-H2 conversion factor in galaxy simulations with non-equilibrium chemistry
in Monthly Notices of the Royal Astronomical Society
Threlfall J
(2020)
How Is Helicity (and Twist) Partitioned in Magnetohydrodynamic Simulations of Reconnecting Magnetic Flux Tubes?
in The Astrophysical Journal
Tillman M
(2023)
Efficient Long-range Active Galactic Nuclei (AGNs) Feedback Affects the Low-redshift Lya Forest
in The Astrophysical Journal Letters
Tinoco-Arenas A
(2022)
Parametric Study of Magnetosheath Jets in 2D Local Hybrid Simulations
in Frontiers in Astronomy and Space Sciences
Tissera P
(2022)
The evolution of the oxygen abundance gradients in star-forming galaxies in the eagle simulations
in Monthly Notices of the Royal Astronomical Society
Tobias S
(2020)
Angular momentum transport, layering, and zonal jet formation by the GSF instability: non-linear simulations at a general latitude
in Monthly Notices of the Royal Astronomical Society
Towler I
(2023)
Gas clumping and its effect on hydrostatic bias in the MACSIS simulations
in Monthly Notices of the Royal Astronomical Society
Towler I
(2024)
Inferring the dark matter splashback radius from cluster gas and observable profiles in the FLAMINGO simulations
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
Trayford J
(2020)
Massive low-surface-brightness galaxies in the eagle simulation
in Monthly Notices of the Royal Astronomical Society
Tress R
(2020)
Simulations of the star-forming molecular gas in an interacting M51-like galaxy
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
Tripathi B
(2024)
Predicting the Slowing of Stellar Differential Rotation by Instability-driven Turbulence
in The Astrophysical Journal
Trotta D
(2022)
On the Transmission of Turbulent Structures across the Earth's Bow Shock
in The Astrophysical Journal
Trotta D
(2023)
Irregular Proton Injection to High Energies at Interplanetary Shocks
in The Astrophysical Journal Letters
Trotta D
(2020)
Fast Acceleration of Transrelativistic Electrons in Astrophysical Turbulence
in The Astrophysical Journal
Trotta D
(2022)
Single-spacecraft techniques for shock parameters estimation: A systematic approach
in Frontiers in Astronomy and Space Sciences
Trotta D
(2023)
Three-dimensional modelling of the shock-turbulence interaction
in Monthly Notices of the Royal Astronomical Society
Trujillo-Gomez S
(2023)
In situ or accreted? Using deep learning to infer the origin of extragalactic globular clusters from observables
in Monthly Notices of the Royal Astronomical Society
Trusov S
(2024)
The two-point correlation function covariance with fewer mocks
in Monthly Notices of the Royal Astronomical Society
Tsang Y
(2020)
Characterising Jupiter's dynamo radius using its magnetic energy spectrum
in Earth and Planetary Science Letters
Tsang Y
(2024)
Scaling of the geomagnetic secular variation timescale
in Geophysical Journal International
Turpin G
(2024)
Orbital evolution of close binary systems: comparing viscous and wind-driven circumbinary disc models
in Monthly Notices of the Royal Astronomical Society
Upadhye A
(2024)
Non-linear CMB lensing with neutrinos and baryons: FLAMINGO simulations versus fast approximations
in Monthly Notices of the Royal Astronomical Society
Vandenbroucke B
(2020)
CMACIONIZE 2.0: a novel task-based approach to Monte Carlo radiation transfer
in Astronomy & Astrophysics
Vandenbroucke B
(2020)
Infrared luminosity functions and dust mass functions in the EAGLE simulation
in Monthly Notices of the Royal Astronomical Society
Vanon R
(2023)
Three-dimensional Simulations of Massive Stars. II. Age Dependence
in The Astrophysical Journal
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
Varghese A
(2024)
Effect of Rotation on Wave Mixing in Intermediate-mass Stars
in The Astrophysical Journal
Varghese A
(2023)
Chemical Mixing Induced by Internal Gravity Waves in Intermediate-mass Stars
in The Astrophysical Journal
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
Vidal J
(2020)
Turbulent Viscosity Acting on the Equilibrium Tidal Flow in Convective Stars
in The Astrophysical Journal Letters
Vidal J
(2020)
Efficiency of tidal dissipation in slowly rotating fully convective stars or planets
in Monthly Notices of the Royal Astronomical Society
Vijayan A
(2024)
First Light And Reionisation Epoch Simulations (FLARES) - XII: The consequences of star-dust geometry on galaxies in the EoR
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
Vizgan D
(2022)
Investigating the [C ii]-to-H i Conversion Factor and the H i Gas Budget of Galaxies at z ˜ 6 with Hydrodynamic Simulations
in The Astrophysical Journal Letters
Vlaykov D
(2022)
Impact of radial truncation on global 2D hydrodynamic simulations for a Sun-like model
in Monthly Notices of the Royal Astronomical Society
Vorabbi M
(2024)
Microscopic optical potentials for medium-mass isotopes derived at the first order of Watson multiple-scattering theory
in Physical Review C
Wakita S
(2022)
Effect of Impact Velocity and Angle on Deformational Heating and Postimpact Temperature
in Journal of Geophysical Research: Planets
Wang C
(2023)
Ghostly Galaxies: Accretion-dominated Stellar Systems in Low-mass Dark Matter Halos
in The Astrophysical Journal
Wang J
(2020)
Universal structure of dark matter haloes over a mass range of 20 orders of magnitude
in Nature
Wang Y
(2020)
Iterative removal of redshift-space distortions from galaxy clustering
in Monthly Notices of the Royal Astronomical Society
Waterfall C
(2022)
Modeling the Transport of Relativistic Solar Protons along a Heliospheric Current Sheet during Historic GLE Events
in The Astrophysical Journal
Welsh L
(2024)
A survey of extremely metal-poor gas at cosmic noon Evidence of elevated [O/Fe]
in Astronomy & Astrophysics
Welsh L
(2022)
Oxygen-enhanced Extremely Metal-poor Damped Lya Systems: A Signpost of the First Stars?
in The Astrophysical Journal
White S
(2020)
The globular cluster system of the Auriga simulations
in Monthly Notices of the Royal Astronomical Society
Whitworth D
(2022)
Is the molecular KS relationship universal down to low metallicities?
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 |