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
Bevins H
(2025)
On the accuracy of posterior recovery with neural network emulators
in Monthly Notices of the Royal Astronomical Society
Khan N
(2024)
Particle initialization effects on Lyman-a forest statistics in cosmological SPH simulations
in Monthly Notices of the Royal Astronomical Society
Jahns-Schindler J
(2023)
How limiting is optical follow-up for fast radio burst applications? Forecasts for radio and optical surveys
in Monthly Notices of the Royal Astronomical Society
Madar M
(2024)
Predictions for the abundance and clustering of H a emitting galaxies
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
Pakmor R
(2025)
Auriga Superstars : Improving the resolution and fidelity of stellar dynamics in cosmological galaxy simulations
in Monthly Notices of the Royal Astronomical Society
Morison A
(2024)
Effects of stratification on overshooting and waves atop the convective core of M? main-sequence stars
in Monthly Notices of the Royal Astronomical Society
Lance S
(2024)
Viscous dissipation and dynamics in simulations of rotating, stratified plane-layer convection
in Monthly Notices of the Royal Astronomical Society
Wan J
(2025)
Decoding the variability in the star formation histories of z ~ 0.8 galaxies
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
Petrovic H
(2024)
Material transport in protoplanetary discs with massive embedded planets
in Monthly Notices of the Royal Astronomical Society
Herrington N
(2024)
Magnetic fields in star-forming environments: how does field strength affect gas on spiral arm and cloud scales?
in Monthly Notices of the Royal Astronomical Society
Huško F
(2024)
Winds versus jets: a comparison between black hole feedback modes in simulations of idealized galaxy groups and clusters
in Monthly Notices of the Royal Astronomical Society
Witten C
(2025)
Rising from the ashes: evidence of old stellar populations and rejuvenation events in the very early Universe
in Monthly Notices of the Royal Astronomical Society
Barrera M
(2023)
The MillenniumTNG Project: semi-analytic galaxy formation models on the past lightcone
in Monthly Notices of the Royal Astronomical Society
Jun R
(2025)
Scatter in the star formation rate-halo mass relation: secondary bias and its impact on line-intensity mapping
in Monthly Notices of the Royal Astronomical Society
Ibrahim D
(2024)
The impact of supernova feedback on the mass-metallicity relations
in Monthly Notices of the Royal Astronomical Society
Raste J
(2024)
The 21-cm bispectrum from neutral hydrogen islands at z < 6
in Monthly Notices of the Royal Astronomical Society
Joshi-Hartley T
(2025)
Heat transport and dissipation in 2.5D rotating internally heated and cooled convection
in Monthly Notices of the Royal Astronomical Society
Štofanová L
(2024)
Prospects for detecting the circum- and intergalactic medium in X-ray absorption using the extended intracluster medium as a backlight
in Monthly Notices of the Royal Astronomical Society
Orkney M
(2023)
EDGE: the shape of dark matter haloes in the faintest galaxies
in Monthly Notices of the Royal Astronomical Society
Carrillo A
(2024)
Can we really pick and choose? Benchmarking various selections of Gaia Enceladus/Sausage stars in observations with simulations
in Monthly Notices of the Royal Astronomical Society
Hou J
(2025)
A random walk model for the evolution of the halo spin vector
in Monthly Notices of the Royal Astronomical Society
Jun R
(2025)
The power spectrum of galaxies from large to small scales: a line-intensity mapping perspective
in Monthly Notices of the Royal Astronomical Society
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