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
Young A
(2024)
Introducing two improved methods for approximating radiative cooling in hydrodynamical simulations of accretion discs
in Monthly Notices of the Royal Astronomical Society
Braspenning J
(2024)
The FLAMINGO project: galaxy clusters in comparison to X-ray observations
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
Davey J
(2025)
The effect of spectroscopic binning on atmospheric retrievals
in Monthly Notices of the Royal Astronomical Society
Hafen Z
(2024)
The Halo21 absorption modelling challenge: lessons from 'observing' synthetic circumgalactic absorption spectra
in Monthly Notices of the Royal Astronomical Society
Harnois-Déraps J
(2023)
mglens : Modified gravity weak lensing simulations for emulation-based cosmological inference
in Monthly Notices of the Royal Astronomical Society
Martin-Alvarez S
(2023)
The Pandora project - I. The impact of radiation, magnetic fields, and cosmic rays on the baryonic and dark matter properties of dwarf galaxies
in Monthly Notices of the Royal Astronomical Society
Zerbo M
(2024)
Effective yields as tracers of feedback effects on metallicity scaling relations in the EAGLE cosmological simulations
in Monthly Notices of the Royal Astronomical Society
Kukstas E
(2023)
GOGREEN: A critical assessment of environmental trends in cosmological hydrodynamical simulations at z ˜ 1
in Monthly Notices of the Royal Astronomical Society
Nobels F
(2024)
Tests of subgrid models for star formation using simulations of isolated disc galaxies
in Monthly Notices of the Royal Astronomical Society