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
Gómez J
(2025)
The Three Hundred Project: A fast semi-analytic model emulator of hydrodynamical galaxy cluster simulations
in Astronomy & Astrophysics
Broxterman J
(2025)
Matter power spectrum reconstruction with KiDS-Legacy: Improved internal ?CDM consistency and preference for strong baryonic feedback
in Astronomy & Astrophysics
Herle A
(2025)
Unbiased estimates of the shapes of haloes using the positions of satellite galaxies
in Astronomy & Astrophysics
Morello G
(2023)
Spitzer thermal phase curve of WASP-121 b
in Astronomy & Astrophysics
Prole L
(2024)
Heavy black hole seed formation in high- z atomic cooling halos
in Astronomy & Astrophysics
Contreras S
(2024)
Validating the clustering predictions of empirical models with the FLAMINGO simulations
in Astronomy & Astrophysics
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
Callingham T
(2025)
Group accretion in Milky Way-like stellar haloes
in Astronomy & Astrophysics
Kimmig L
(2025)
Intra-cluster light as a dynamical clock for galaxy clusters: Insights from the MAGNETICUM, IllustrisTNG, Hydrangea, and Horizon-AGN simulations
in Astronomy & Astrophysics
Ratnasingam R
(2023)
Internal gravity waves in massive stars II. Frequency analysis across stellar mass
in Astronomy & Astrophysics
Saavedra-Bastidas J
(2024)
Gravitational collapse at low to moderate Mach numbers: The relationship between star formation efficiency and the fraction of mass in the massive object
in Astronomy & Astrophysics
Punyasheel P
(2025)
First Light And Reionisation Epoch Simulations (FLARES) XVI. Size evolution of massive dusty galaxies at cosmic dawn from the ultraviolet to infrared
in Astronomy & Astrophysics
Mercier W
(2024)
The COSMOS-Web ring: In-depth characterization of an Einstein ring lensing system at z ~ 2
in Astronomy & Astrophysics
Kumar A
(2025)
Modeling submillimeter galaxies in cosmological simulations: Contribution to the cosmic star formation density and predictions for future surveys
in Astronomy & Astrophysics
Dethero M
(2024)
The shape of convection in 2D and 3D global simulations of stellar interiors
in Astronomy & Astrophysics
Welsh L
(2024)
A survey of extremely metal-poor gas at cosmic noon Evidence of elevated [O/Fe]
in Astronomy & Astrophysics
Nowak M
(2024)
The orbit of HD 142527 B is too compact to explain many of the disc features
in Astronomy & Astrophysics
Bernet M
(2025)
Dark matter spiral arms in Milky Way-like halos
in Astronomy & Astrophysics
Sanati M
(2024)
Dwarf galaxies as a probe of a primordially magnetized Universe
in Astronomy & Astrophysics
Fenton A
(2024)
The 3D structure of disc-instability protoplanets
in Astronomy & Astrophysics
Júlio M
(2025)
The radial acceleration relation at the EDGE of galaxy formation Testing its universality in low-mass dwarf galaxies
in Astronomy & Astrophysics
Miró-Carretero J
(2025)
Extragalactic stellar tidal streams: Observations meet simulation
in Astronomy & Astrophysics
Bahé Y
(2025)
Galaxies in the simulated cosmic web I. Filament identification and properties
in Astronomy & Astrophysics
Dutta R
(2024)
Metal line emission around z < 1 galaxies
in Astronomy & Astrophysics
Maccagni F
(2024)
MHONGOOSE discovery of a gas-rich low surface brightness galaxy in the Dorado group
in Astronomy & Astrophysics
Scholtz J
(2025)
JADES: A large population of obscured, narrow-line active galactic nuclei at high redshift
in Astronomy & Astrophysics
Dimmock A
(2023)
Backstreaming ions at a high Mach number interplanetary shock Solar Orbiter measurements during the nominal mission phase
in Astronomy & Astrophysics
Stuck M
(2025)
Convective shells in the interior of Cepheid variable stars: Overshooting models based on hydrodynamic simulations
in Astronomy & Astrophysics
Sifón C
(2024)
The history and mass content of cluster galaxies in the EAGLE simulation
in Astronomy & Astrophysics
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
He Y
(2025)
Characterising galaxy cluster scaling relations as cosmic isotropy tracers using FLAMINGO simulations
in Astronomy & Astrophysics
Laitinen T
(2023)
Solar energetic particle event onsets at different heliolongitudes: The effect of turbulence in Parker spiral geometry
in Astronomy & Astrophysics
Scardoni C
(2025)
Eccentric disks as a gateway to giant planet outward migration
in Astronomy & Astrophysics
Mombarg J
(2025)
Calibrating chemical mixing induced by internal gravity waves based on hydrodynamical simulations The chemical evolution of OB-type stars
in Astronomy & Astrophysics
Changeat Q
(2025)
Cloud and haze parameterization in atmospheric retrievals: Insights from Titan's Cassini data and JWST observations of hot Jupiters
in Astronomy & Astrophysics
Vecchi F
(2025)
Impact of line of sight structure on weak lensing observables of galaxy clusters
in Astronomy & Astrophysics
Fontanot F
(2025)
Galaxy assembly and evolution in the P-Millennium simulation: Galaxy clustering
in Astronomy & Astrophysics
Montargès M
(2023)
The VLT/SPHERE view of the ATOMIUM cool evolved star sample I. Overview: Sample characterization through polarization analysis
in Astronomy & Astrophysics
Galbiati M
(2024)
MUSE Analysis of Gas around Galaxies (MAGG) VI. The cool and enriched gas environment of z ? 3 Ly a emitters
in Astronomy & Astrophysics
Ni S
(2025)
Effect of liquid droplets on premixed laminar acetone flames
in Applications in Energy and Combustion Science
Advincula XR
(2025)
Protons Accumulate at the Graphene-Water Interface.
in ACS nano
Peng B
(2025)
Electronic Structure of Fullerene Nanoribbons.
in ACS nano