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
Pallero D
(2024)
Galaxy evolution in modified gravity simulations: using galaxy properties to constrain our gravitational model
in Monthly Notices of the Royal Astronomical Society
Parrott W
(2023)
B ? K and D ? K form factors from fully relativistic lattice QCD
in Physical Review D
Parrott W
(2023)
Standard Model predictions for B ? K l + l - , B ? K l 1 - l 2 + and B ? K ? ? ¯ using form factors from N f = 2 + 1 + 1 lattice QCD
in Physical Review D
Penzlin A
(2024)
Viscous circumbinary protoplanetary discs - I. Structure of the inner cavity
in Monthly Notices of the Royal Astronomical Society
Pereira-Wilson M
(2023)
The cosmic UV background and the beginning and end of star formation in simulated field dwarf galaxies
in Monthly Notices of the Royal Astronomical Society
Petrovic H
(2024)
Material transport in protoplanetary discs with massive embedded planets
in Monthly Notices of the Royal Astronomical Society
Pfeffer J
(2023)
Globular cluster metallicity distributions in the E-MOSAICS simulations
in Monthly Notices of the Royal Astronomical Society
Pfeffer J
(2024)
Origin of the correlation between stellar kinematics and globular cluster system richness in ultradiffuse galaxies
in Monthly Notices of the Royal Astronomical Society
Pizzati E
(2024)
A unified model for the clustering of quasars and galaxies at z ˜ 6
in Monthly Notices of the Royal Astronomical Society
Pizzati E
(2024)
Revisiting the extreme clustering of z ˜ 4 quasars with large volume cosmological simulations
in Monthly Notices of the Royal Astronomical Society
Ploeckinger S
(2024)
Resolution criteria to avoid artificial clumping in Lagrangian hydrodynamic simulations with a multiphase interstellar medium
in Monthly Notices of the Royal Astronomical Society
Pollin J
(2024)
On the fate of the secondary white dwarf in double-degenerate double-detonation Type Ia supernovae - II. 3D synthetic observables
in Monthly Notices of the Royal Astronomical Society
Prathaban M
(2024)
Costless correction of chain based nested sampling parameter estimation in gravitational wave data and beyond
in Monthly Notices of the Royal Astronomical Society
Prole L
(2024)
Population III star formation: multiple gas phases prevent the use of an equation of state at high densities
in The Open Journal of Astrophysics
Prole L
(2024)
Heavy black hole seed formation in high- z atomic cooling halos
in Astronomy & Astrophysics
Puchwein E
(2023)
The Sherwood-Relics simulations: overview and impact of patchy reionization and pressure smoothing on the intergalactic medium
in Monthly Notices of the Royal Astronomical Society
Qu F
(2024)
The Atacama Cosmology Telescope: A Measurement of the DR6 CMB Lensing Power Spectrum and Its Implications for Structure Growth
in The Astrophysical Journal
Raste J
(2024)
The 21-cm bispectrum from neutral hydrogen islands at z < 6
in Monthly Notices of the Royal Astronomical Society
Ratnasingam R
(2024)
On the Geometry of the Near-core Magnetic Field in Massive Stars
in The Astrophysical Journal Letters
Ratnasingam R
(2023)
Internal gravity waves in massive stars II. Frequency analysis across stellar mass
in Astronomy & Astrophysics
Reeves A
(2023)
Constraining quenching time-scales in galaxy clusters by forward-modelling stellar ages and quiescent fractions in projected phase space
in Monthly Notices of the Royal Astronomical Society
Regos E
(2024)
Percolation Statistics in the MillenniumTNG Simulations
in The Astrophysical Journal
Reina-Campos M
(2023)
Constraining the shape of dark matter haloes with globular clusters and diffuse stellar light in the E-MOSAICS simulations
in Monthly Notices of the Royal Astronomical Society
Rey M
(2024)
Boosting galactic outflows with enhanced resolution
in Monthly Notices of the Royal Astronomical Society
Rizzuti F
(2024)
Stellar Evolution and Convection in 3D Hydrodynamic Simulations of a Complete Burning Phase
in Galaxies
Rizzuti F
(2024)
Shell mergers in the late stages of massive star evolution: new insight from 3D hydrodynamic simulations
in Monthly Notices of the Royal Astronomical Society
Robinson A
(2024)
Introducing cuDisc : a 2D code for protoplanetary disc structure and evolution calculations
in Monthly Notices of the Royal Astronomical Society
Robinson A
(2025)
The effect of radiation pressure on the dispersal of photoevaporating discs
in Monthly Notices of the Royal Astronomical Society
Rodríguez Montero F
(2024)
The impact of cosmic rays on the interstellar medium and galactic outflows of Milky Way analogues
in Monthly Notices of the Royal Astronomical Society
Rogers J
(2024)
Under the light of a new star: evolution of planetary atmospheres through protoplanetary disc dispersal and boil-off
in Monthly Notices of the Royal Astronomical Society
Roper F
(2023)
The diversity of rotation curves of simulated galaxies with cusps and cores
in Monthly Notices of the Royal Astronomical Society
Roper W
(2023)
First light and reionization epoch simulations (FLARES) IX: the physical mechanisms driving compact galaxy formation and evolution
in Monthly Notices of the Royal Astronomical Society
Rosca-Mead R
(2023)
Stochastic gravitational wave background from supernovae in massive scalar-tensor gravity
in Physical Review D
Roth A
(2024)
Hot Jupiter diversity and the onset of TiO/VO revealed by a large grid of non-grey global circulation models
in Monthly Notices of the Royal Astronomical Society
Rowther S
(2024)
The role of drag and gravity on dust concentration in a gravitationally unstable disc
in Monthly Notices of the Royal Astronomical Society
Rowther S
(2024)
Short-lived gravitational instability in isolated irradiated discs
in Monthly Notices of the Royal Astronomical Society
Ruan C
(2024)
An emulator-based halo model in modified gravity - I. The halo concentration-mass relation and density profile
in Monthly Notices of the Royal Astronomical Society
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
Saha B
(2024)
Quantifying the impact of AGN feedback on the large-scale matter distribution using two- and three-point statistics
in Monthly Notices of the Royal Astronomical Society
Salcido J
(2023)
SP(k) - a hydrodynamical simulation-based model for the impact of baryon physics on the non-linear matter power spectrum
in Monthly Notices of the Royal Astronomical Society
Saló L
(2024)
GRFolres: A code for modified gravity simulations in strong gravity
in Journal of Open Source Software
Sana T
(2023)
Plasma sheath around sunlit moon: monotonic and non-monotonic structures
in Monthly Notices of the Royal Astronomical Society
Sanati M
(2024)
Dwarf galaxies as a probe of a primordially magnetized Universe
in Astronomy & Astrophysics
Sante A
(2024)
Applying machine learning to Galactic Archaeology: how well can we recover the origin of stars in Milky Way-like galaxies?
in Monthly Notices of the Royal Astronomical Society
Santos-Santos I
(2023)
The Tucana dwarf spheroidal: a distant backsplash galaxy of M31?
in Monthly Notices of the Royal Astronomical Society
Santos-Santos I
(2024)
Anisotropies in the spatial distribution and kinematics of dwarf galaxies in the Local Group and beyond
in Monthly Notices of the Royal Astronomical Society
Satyavolu S
(2024)
Robustness of direct measurements of the mean free path of ionizing photons in the epoch of reionization
in Monthly Notices of the Royal Astronomical Society
Satyavolu S
(2023)
The need for obscured supermassive black hole growth to explain quasar proximity zones in the epoch of reionization
in Monthly Notices of the Royal Astronomical Society