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
Evstafyeva T
(2024)
Gravitational-Wave Data Analysis with High-Precision Numerical Relativity Simulations of Boson Star Mergers.
in Physical review letters
Fancher J
(2023)
On the relative importance of shocks and self-gravity in modifying tidal disruption event debris streams
in Monthly Notices of the Royal Astronomical Society
Farren G
(2024)
The Atacama Cosmology Telescope: Cosmology from Cross-correlations of unWISE Galaxies and ACT DR6 CMB Lensing
in The Astrophysical Journal
Feng J
(2024)
On the evolution of the observed mass-to-length relationship for star-forming filaments
in Monthly Notices of the Royal Astronomical Society
Fenton A
(2024)
The 3D structure of disc-instability protoplanets
in Astronomy & Astrophysics
Ferlito F
(2023)
The MillenniumTNG Project: the impact of baryons and massive neutrinos on high-resolution weak gravitational lensing convergence maps
in Monthly Notices of the Royal Astronomical Society
Ferlito F
(2024)
Ray-tracing versus Born approximation in full-sky weak lensing simulations of the MillenniumTNG project
in Monthly Notices of the Royal Astronomical Society
Feron J
(2024)
The Lyman-limit photon mean free path at the end of late reionization in the Sherwood-Relics simulations
in Monthly Notices of the Royal Astronomical Society
Figueras P
(2023)
Endpoint of the Gregory-Laflamme instability of black strings revisited
in Physical Review D
Flynn J
(2023)
Exclusive semileptonic B s ? K l ? decays on the lattice
in Physical Review D
Forrest B
(2024)
MAGAZ3NE: Massive, Extremely Dusty Galaxies at z ~ 2 Lead to Photometric Overestimation of Number Densities of the Most Massive Galaxies at 3 < z < 4*
in The Astrophysical Journal
Forzano N
(2023)
Lattice studies of Sp(2N) gauge theories using GRID
Fu B
(2024)
Testing realistic SO(10) SUSY GUTs with proton decay and gravitational waves
in Physical Review D
Gaikwad P
(2023)
Measuring the photoionization rate, neutral fraction, and mean free path of H i ionizing photons at 4.9 = z = 6.0 from a large sample of XShooter and ESI spectra
in Monthly Notices of the Royal Astronomical Society
Gaire B
(2024)
Maintaining spherical polarization in solar wind plasma
in Nature Astronomy
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
Garg P
(2024)
Theoretical Strong-line Metallicity Diagnostics for the JWST Era
in The Astrophysical Journal
Garron N
(2023)
Nonperturbative renormalization with interpolating momentum schemes
in Physical Review D
Garver B
(2023)
Exploring the Evolution of Massive Clumps in Simulations That Reproduce the Observed Milky Way a-element Abundance Bimodality
in The Astrophysical Journal
Gavardi A
(2023)
NNLO+PS W+W- production using jet veto resummation at NNLL'
in Journal of High Energy Physics
Gayer L
(2025)
Highly excited B, Bs and Bc meson spectroscopy from lattice QCD
in Journal of High Energy Physics
Genina A
(2023)
On the edge: the relation between stellar and dark matter haloes of Milky Way-mass galaxies
in Monthly Notices of the Royal Astronomical Society
Georgy C
(2024)
3D simulations of a neon burning convective shell in a massive star
in Monthly Notices of the Royal Astronomical Society
Gessey-Jones T
(2024)
Fully Bayesian forecasts with evidence networks
in Physical Review D
Ghosh S
(2024)
First frequency-domain phenomenological model of the multipole asymmetry in gravitational-wave signals from binary-black-hole coalescence
in Physical Review D