DiRAC 2.5y Bridging Funding - UCL
Lead Research Organisation:
UNIVERSITY COLLEGE LONDON
Department Name: Physics and Astronomy
Abstract
Abstracts are not currently available in GtR for all funded research. This is normally because the abstract was not required at the time of proposal submission, but may be because it included sensitive information such as personal details.
Organisations
Publications
Becker G
(2024)
Damping wing absorption associated with a giant Ly a trough at z < 6: direct evidence for late-ending reionization
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
Dutta R
(2020)
MUSE Analysis of Gas around Galaxies (MAGG) - II: metal-enriched halo gas around z ~ 1 galaxies
in Monthly Notices of the Royal Astronomical Society
Thomas N
(2021)
The radio galaxy population in the simba simulations
in Monthly Notices of the Royal Astronomical Society
Owens A
(2024)
ExoMol line lists - LI. Molecular line lists for lithium hydroxide (LiOH)
in Monthly Notices of the Royal Astronomical Society
Smith G
(2020)
The distribution of dark matter and gas spanning 6 Mpc around the post-merger galaxy cluster MS 0451-03
in Monthly Notices of the Royal Astronomical Society
Deason A
(2023)
Unravelling the mass spectrum of destroyed dwarf galaxies with the metallicity distribution function
in Monthly Notices of the Royal Astronomical Society
Appleby S
(2021)
The low-redshift circumgalactic medium in simba
in Monthly Notices of the Royal Astronomical Society
Bate M
(2023)
The statistical properties of stars at redshift, z = 5, compared with the present epoch
in Monthly Notices of the Royal Astronomical Society
Šoltinský T
(2023)
Probing quasar lifetimes with proximate 21-centimetre absorption in the diffuse intergalactic medium at redshifts z = 6
in Monthly Notices of the Royal Astronomical Society
Lovell M
(2019)
The signal of decaying dark matter with hydrodynamical simulations
in Monthly Notices of the Royal Astronomical Society
Young A
(2021)
Chemical signatures of a warped protoplanetary disc
in Monthly Notices of the Royal Astronomical Society
Becker G
(2021)
The mean free path of ionizing photons at 5 < z < 6: evidence for rapid evolution near reionization
in Monthly Notices of the Royal Astronomical Society
Porth L
(2020)
Fast estimation of aperture mass statistics - I. Aperture mass variance and an application to the CFHTLenS data
in Monthly Notices of the Royal Astronomical Society
Henriques B
(2020)
L-GALAXIES 2020: Spatially resolved cold gas phases, star formation, and chemical enrichment in galactic discs
in Monthly Notices of the Royal Astronomical Society
Ruiz-Bonilla S
(2022)
Dealing with density discontinuities in planetary SPH simulations
in Monthly Notices of the Royal Astronomical Society
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
Jankovic M
(2019)
Observing substructure in circumstellar discs around massive young stellar objects
in Monthly Notices of the Royal Astronomical Society
Collins C
(2024)
Towards inferring the geometry of kilonovae
in Monthly Notices of the Royal Astronomical Society
Thomas N
(2019)
Black hole - Galaxy correlations in simba
in Monthly Notices of the Royal Astronomical Society
Pontzen A
(2021)
EDGE: a new approach to suppressing numerical diffusion in adaptive mesh simulations of galaxy formation
in Monthly Notices of the Royal Astronomical Society
Griffin A
(2020)
AGNs at the cosmic dawn: predictions for future surveys from a ?CDM cosmological model
in Monthly Notices of the Royal Astronomical Society
Nobels F
(2022)
The interplay between AGN feedback and precipitation of the intracluster medium in simulations of galaxy groups and clusters
in Monthly Notices of the Royal Astronomical Society
Jauzac M
(2019)
The core of the massive cluster merger MACS J0417.5-1154 as seen by VLT/MUSE
in Monthly Notices of the Royal Astronomical Society
Gratton S
(2020)
Understanding parameter differences between analyses employing nested data subsets
in Monthly Notices of the Royal Astronomical Society
Reina-Campos M
(2022)
Radial distributions of globular clusters trace their host dark matter halo: insights from the E-MOSAICS simulations
in Monthly Notices of the Royal Astronomical Society
Vijayan A
(2024)
First Light And Reionisation Epoch Simulations (FLARES) - XII: The consequences of star-dust geometry on galaxies in the EoR
in Monthly Notices of the Royal Astronomical Society
Mitchell P
(2020)
Galactic outflow rates in the EAGLE simulations
in Monthly Notices of the Royal Astronomical Society
Shingles L
(2020)
Monte Carlo radiative transfer for the nebular phase of Type Ia supernovae
in Monthly Notices of the Royal Astronomical Society
Dobbs C
(2021)
The properties of clusters, and the orientation of magnetic fields relative to filaments, in magnetohydrodynamic simulations of colliding clouds
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
Stiskalek R
(2024)
Evaluating the variance of individual halo properties in constrained cosmological simulations
in Monthly Notices of the Royal Astronomical Society
Kirchschlager F
(2024)
From total destruction to complete survival: dust processing at different evolutionary stages in the supernova remnant Cassiopeia A
in Monthly Notices of the Royal Astronomical Society
Kruijssen J
(2020)
Kraken reveals itself - the merger history of the Milky Way reconstructed with the E-MOSAICS simulations
in Monthly Notices of the Royal Astronomical Society
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
Smith R
(2020)
The Cloud Factory I: Generating resolved filamentary molecular clouds from galactic-scale forces
in Monthly Notices of the Royal Astronomical Society
Seeyave L
(2023)
First light and reionization epoch simulations (FLARES) X iii : the lyman-continuum emission of high-redshift galaxies
in Monthly Notices of the Royal Astronomical Society
Humphries J
(2019)
On the origin of wide-orbit ALMA planets: giant protoplanets disrupted by their cores
in Monthly Notices of the Royal Astronomical Society
Thomas P
(2023)
First light and reionization epoch simulations ( Flares ) X: environmental galaxy bias and survey variance at high redshift
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
Altamura E
(2023)
EAGLE-like simulation models do not solve the entropy core problem in groups and clusters of galaxies
in Monthly Notices of the Royal Astronomical Society
Santos-Santos I
(2022)
Satellite mass functions and the faint end of the galaxy mass-halo mass relation in LCDM
in Monthly Notices of the Royal Astronomical Society
Rizzuti F
(2022)
Realistic 3D hydrodynamics simulations find significant turbulent entrainment in massive stars
in Monthly Notices of the Royal Astronomical Society
Tissera P
(2022)
The evolution of the oxygen abundance gradients in star-forming galaxies in the eagle simulations
in Monthly Notices of the Royal Astronomical Society
Katz H
(2023)
Two modes of LyC escape from bursty star formation: implications for [C ii ] deficits and the sources of reionization
in Monthly Notices of the Royal Astronomical Society
Deason A
(2019)
The local high-velocity tail and the Galactic escape speed
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
Smith A
(2019)
Correcting for fibre assignment incompleteness in the DESI Bright Galaxy Survey
in Monthly Notices of the Royal Astronomical Society
Chen C
(2023)
Can a binary star host three giant circumbinary planets?
in Monthly Notices of the Royal Astronomical Society
Porth L
(2021)
Fast estimation of aperture-mass statistics - II. Detectability of higher order statistics in current and future surveys
in Monthly Notices of the Royal Astronomical Society
| Description | Many new discoveries about the formation and evolution of galaxies, star formation, planet formation and particle physics theory have been made possible by the award |
| Exploitation Route | Many international collaborative projects are supported by the HPC resources provided by DiRAC |
| Sectors | Aerospace Defence and Marine Creative Economy Digital/Communication/Information Technologies (including Software) Education Healthcare |
| URL | http://www.dirac.ac.uk |
| Description | any new discoveries about the formation and evolution of galaxies, star formation, planet formation and particle physics theory have been made possible by the award. |
| Sector | Aerospace, Defence and Marine,Creative Economy,Digital/Communication/Information Technologies (including Software),Education,Healthcare |