DiRAC-3 Operations 2023-26 - UCL - Additional Grant
Lead Research Organisation:
UNIVERSITY COLLEGE LONDON
Department Name: Physics and Astronomy
Abstract
This JeS form is a resubmission of part of the UCL DiRAC Operations grant request containing only the DI posts which have been approved for funding at 100% by STFC.
Organisations
People |
ORCID iD |
| Clare Jenner (Principal Investigator) |
Publications
Trotta D
(2023)
Three-dimensional modelling of the shock-turbulence interaction
in Monthly Notices of the Royal Astronomical Society
Trotta D
(2023)
Irregular Proton Injection to High Energies at Interplanetary Shocks
in The Astrophysical Journal Letters
Tripathi B
(2024)
Predicting the Slowing of Stellar Differential Rotation by Instability-driven Turbulence
in The Astrophysical Journal
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
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
Thompson J
(2024)
Phenomenological gravitational-wave model for precessing black-hole binaries with higher multipoles and asymmetries
in Physical Review D
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
Theuns T
(2024)
A halo model for cosmological Lyman-limit systems
in Monthly Notices of the Royal Astronomical Society
Teodoro L
(2023)
A Recent Impact Origin of Saturn's Rings and Mid-sized Moons
in The Astrophysical Journal
Teed R
(2023)
Solenoidal force balances in numerical dynamos
in Journal of Fluid Mechanics
Talbot R
(2024)
Simulations of spin-driven AGN jets in gas-rich galaxy mergers
in Monthly Notices of the Royal Astronomical Society
Tahseen T
(2024)
Enhancing 3D planetary atmosphere simulations with a surrogate radiative transfer model
in Monthly Notices of the Royal Astronomical Society
Stiskalek R
(2024)
Evaluating the variance of individual halo properties in constrained cosmological simulations
in Monthly Notices of the Royal Astronomical Society
Sorini D
(2024)
The impact of feedback on the evolution of gas density profiles from galaxies to clusters: a universal fitting formula from the Simba suite of simulations
in The Open Journal of Astrophysics
Somogyi W
(2024)
An ab initio spectroscopic model of the molecular oxygen atmospheric and infrared bands
in Physical Chemistry Chemical Physics
Snow B
(2024)
Kelvin-Helmholtz-induced mixing in multi-fluid partially ionized plasmas
in Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences
Smail R
(2023)
Constraining beyond the standard model nucleon isovector charges
in Physical Review D
Sirks E
(2024)
Hydrodynamical simulations of merging galaxy clusters: giant dark matter particle colliders, powered by gravity
in Monthly Notices of the Royal Astronomical Society
Sifón C
(2024)
The history and mass content of cluster galaxies in the EAGLE simulation
in Astronomy & Astrophysics
Shingles L
(2023)
Self-consistent 3D Radiative Transfer for Kilonovae: Directional Spectra from Merger Simulations
in The Astrophysical Journal Letters
Sherletov A
(2023)
Lattice Studies of 3D Maximally Supersymmetric Yang-Mills
Sergeev D
(2024)
The Impact of the Explicit Representation of Convection on the Climate of a Tidally Locked Planet in Global Stretched-mesh Simulations
in The Astrophysical Journal
Sergeev D
(2023)
Simulations of idealised 3D atmospheric flows on terrestrial planets using LFRic-Atmosphere
in Geoscientific Model Development
Sellek A
(2024)
Modeling JWST MIRI-MRS Observations of T Cha: Mid-IR Noble Gas Emission Tracing a Dense Disk Wind
in The Astronomical Journal
Sellek A
(2024)
Photoevaporation of protoplanetary discs with PLUTO+PRIZMO I. Lower X-ray-driven mass-loss rates due to enhanced cooling
in Astronomy & Astrophysics
Seeyave L
(2023)
First light and reionization epoch simulations (FLARES) X iii : the lyman-continuum emission of high-redshift galaxies
in Monthly Notices of the Royal Astronomical Society
Schreyer E
(2024)
Using Ly a transits to constrain models of atmospheric escape
in Monthly Notices of the Royal Astronomical Society
Schreyer E
(2024)
Using helium 10 830 Å transits to constrain planetary magnetic fields
in Monthly Notices of the Royal Astronomical Society
Scholtz J
(2024)
GN-z11: The environment of an active galactic nucleus at z = 10.603 New insights into the most distant Ly a detection
in Astronomy & Astrophysics
Schoettler C
(2024)
The effect of dynamical interactions in stellar birth environments on the orbits of young close-in planetary systems
in Monthly Notices of the Royal Astronomical Society
Schaye J
(2023)
The FLAMINGO project: cosmological hydrodynamical simulations for large-scale structure and galaxy cluster surveys
in Monthly Notices of the Royal Astronomical Society
Scharré L
(2024)
The effects of stellar and AGN feedback on the cosmic star formation history in the simba simulations
in Monthly Notices of the Royal Astronomical Society
Schaller M
(2024)
On the anisotropic distribution of clusters in the local Universe
in Monthly Notices of the Royal Astronomical Society: Letters
Schaller M
(2024)
Swift : a modern highly parallel gravity and smoothed particle hydrodynamics solver for astrophysical and cosmological applications
in Monthly Notices of the Royal Astronomical Society
Scardoni C
(2024)
Seeing the Unseen: A Method to Detect Unresolved Rings in Protoplanetary Disks
in The Astrophysical Journal
Sawala T
(2023)
Distinct distributions of elliptical and disk galaxies across the Local Supercluster as a ?CDM prediction
in Nature Astronomy
Sawala T
(2023)
The timeless timing argument and the total mass of the Local Group
in Monthly Notices of the Royal Astronomical Society: Letters
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
Satyavolu S
(2024)
Robustness of direct measurements of the mean free path of ionizing photons in the epoch of reionization
in Monthly Notices of the Royal Astronomical Society
Satyavolu S
(2023)
The need for obscured supermassive black hole growth to explain quasar proximity zones in the epoch of reionization
in Monthly Notices of the Royal Astronomical Society
Santos-Santos I
(2023)
The Tucana dwarf spheroidal: a distant backsplash galaxy of M31?
in Monthly Notices of the Royal Astronomical Society
Santos-Santos I
(2024)
Anisotropies in the spatial distribution and kinematics of dwarf galaxies in the Local Group and beyond
in Monthly Notices of the Royal Astronomical Society
Sante A
(2024)
Applying machine learning to Galactic Archaeology: how well can we recover the origin of stars in Milky Way-like galaxies?
in Monthly Notices of the Royal Astronomical Society
Sanati M
(2024)
Dwarf galaxies as a probe of a primordially magnetized Universe
in Astronomy & Astrophysics
Sana T
(2023)
Plasma sheath around sunlit moon: monotonic and non-monotonic structures
in Monthly Notices of the Royal Astronomical Society
Saló L
(2024)
GRFolres: A code for modified gravity simulations in strong gravity
in Journal of Open Source Software
Salcido J
(2023)
SP(k) - a hydrodynamical simulation-based model for the impact of baryon physics on the non-linear matter power spectrum
in Monthly Notices of the Royal Astronomical Society