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
De Ceuster F
(2023)
Radiative transfer as a Bayesian linear regression problem
in Monthly Notices of the Royal Astronomical Society
Dhandha J
(2024)
Decaying turbulence in molecular clouds: how does it affect filament networks and star formation?
in Monthly Notices of the Royal Astronomical Society
Dimmock A
(2023)
Backstreaming ions at a high Mach number interplanetary shock Solar Orbiter measurements during the nominal mission phase
in Astronomy & Astrophysics
Dome T
(2025)
Increased burstiness at high redshift in multiphysics models combining supernova feedback, radiative transfer, and cosmic rays
in Monthly Notices of the Royal Astronomical Society
Doneva D
(2023)
Testing the limits of scalar-Gauss-Bonnet gravity through nonlinear evolutions of spin-induced scalarization
in Physical Review D
Dong-Páez C
(2024)
The Uchuu-SDSS galaxy light-cones: a clustering, redshift space distortion and baryonic acoustic oscillation study
in Monthly Notices of the Royal Astronomical Society
Downing E
(2023)
The many reasons that the rotation curves of low-mass galaxies can fail as tracers of their matter distributions
in Monthly Notices of the Royal Astronomical Society
Drew A
(2024)
Axion string source modeling
in Physical Review D
Dudek J
(2024)
Coupled-channel J - - meson resonances from lattice QCD
in Physical Review D
Duguid C
(2024)
Shear-driven magnetic buoyancy in the solar tachocline: dependence of the mean electromotive force on diffusivity and latitude
in Monthly Notices of the Royal Astronomical Society
Durán-Camacho E
(2024)
Self-consistent modelling of the Milky Way structure using live potentials
in Monthly Notices of the Royal Astronomical Society
Dutta R
(2024)
Metal line emission around z < 1 galaxies
in Astronomy & Astrophysics
Edwards B
(2023)
Exploring the Ability of Hubble Space Telescope WFC3 G141 to Uncover Trends in Populations of Exoplanet Atmospheres through a Homogeneous Transmission Survey of 70 Gaseous Planets
in The Astrophysical Journal Supplement Series
Edwards B
(2024)
Measuring Tracers of Planet Formation in the Atmosphere of WASP-77A b: Substellar O/H and C/H Ratios, with a Stellar C/O Ratio and a Potentially Superstellar Ti/H Ratio
in The Astrophysical Journal Letters
Edwards B
(2023)
Characterizing a World Within the Hot-Neptune Desert: Transit Observations of LTT 9779 b with the Hubble Space Telescope/WFC3
in The Astronomical Journal
Eilers A
(2024)
EIGER. VI. The Correlation Function, Host Halo Mass, and Duty Cycle of Luminous Quasars at z ? 6
in The Astrophysical Journal
Elbakyan V
(2023)
Episodic accretion and mergers during growth of massive protostars
in Monthly Notices of the Royal Astronomical Society
Elley M
(2025)
Robustness of inflation to kinetic inhomogeneities
in Journal of Cosmology and Astroparticle Physics
Elsender D
(2024)
An implicit algorithm for simulating the dynamics of small dust grains with smoothed particle hydrodynamics
in Monthly Notices of the Royal Astronomical Society
Ereza J
(2024)
The Uchuu - glam BOSS and eBOSS LRG lightcones: exploring clustering and covariance errors
in Monthly Notices of the Royal Astronomical Society
Etherington A
(2024)
Strong gravitational lensing's 'external shear' is not shear
in Monthly Notices of the Royal Astronomical Society
Etherington A
(2023)
Beyond the bulge-halo conspiracy? Density profiles of early-type galaxies from extended-source strong lensing
in Monthly Notices of the Royal Astronomical Society
Evstafyeva T
(2024)
Gravitational-Wave Data Analysis with High-Precision Numerical Relativity Simulations of Boson Star Mergers.
in Physical review letters
Evstafyeva T
(2023)
Boson stars in massless and massive scalar-tensor gravity
in Physical Review D