DiRAC-3 Operations - 2022-23 extension - Leicester
Lead Research Organisation:
University of Leicester
Department Name: Physics and Astronomy
Abstract
This grant is a costed 12-month extension of the grant "DiRAC-3 Operations", (STFC reference: ST/V002384/1).
Organisations
People |
ORCID iD |
| Mark Wilkinson (Principal Investigator) |
Publications
Flynn J
(2023)
Exclusive semileptonic B s ? K l ? decays on the lattice
in Physical Review D
Font A
(2022)
Quenching of satellite galaxies of Milky Way analogues: reconciling theory and observations
in Monthly Notices of the Royal Astronomical Society
Forouhar Moreno V
(2022)
Galactic satellite systems in CDM, WDM and SIDM
in Monthly Notices of the Royal Astronomical Society
Forouhar Moreno V
(2022)
Baryon-driven decontraction in Milky Way-mass haloes
in Monthly Notices of the Royal Astronomical Society
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
Franci L
(2022)
Anisotropic Electron Heating in Turbulence-driven Magnetic Reconnection in the Near-Sun Solar Wind
in The Astrophysical Journal
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
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
Genina A
(2022)
Can tides explain the low dark matter density in Fornax?
in Monthly Notices of the Royal Astronomical Society
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
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
Ghosh S
(2022)
Age dissection of the vertical breathing motions in Gaia DR2: evidence for spiral driving
in Monthly Notices of the Royal Astronomical Society
Givans J
(2022)
Non-linearities in the Lyman-a forest and in its cross-correlation with dark matter halos
in Journal of Cosmology and Astroparticle Physics
Glasscock K
(2024)
Statistical estimation of full-sky radio maps from 21 cm array visibility data using Gaussian constrained realizations
in RAS Techniques and Instruments
Glowacki M
(2022)
ASymba: H i global profile asymmetries in the simba simulation
in Monthly Notices of the Royal Astronomical Society
Grand R
(2024)
Overview and public data release of the augmented Auriga Project: cosmological simulations of dwarf and Milky Way-mass galaxies
in Monthly Notices of the Royal Astronomical Society
Grove C
(2022)
The DESI N -body simulation project - I. Testing the robustness of simulations for the DESI dark time survey
in Monthly Notices of the Royal Astronomical Society
Gu Q
(2022)
The spatial distribution of satellites in galaxy clusters
in Monthly Notices of the Royal Astronomical Society