DiRAC-3 Operations - 2022-23 extension - Cambridge
Lead Research Organisation:
University of Cambridge
Department Name: Institute of Astronomy
Abstract
This grant is a costed 12-month extension of the grant "DiRAC-3 Operations 2019-2022 - Cambridge [2020-06 resubmission]", (STFC reference: ST/V002635/1).
Organisations
Publications
Hellinger P
(2022)
Ion-scale Transition of Plasma Turbulence: Pressure-Strain Effect
in The Astrophysical Journal
Hermansson-Truedsson N
(2022)
Isospin-breaking corrections to light leptonic decays in lattice QCD+QED at the physical point
Hernández-Aguayo C
(2023)
The MillenniumTNG Project: high-precision predictions for matter clustering and halo statistics
in Monthly Notices of the Royal Astronomical Society
Hernández-Aguayo C
(2022)
Fast full N-body simulations of generic modified gravity: derivative coupling models
in Journal of Cosmology and Astroparticle Physics
Herrington N
(2023)
The role of previous generations of stars in triggering star formation and driving gas dynamics
in Monthly Notices of the Royal Astronomical Society
Heyl J
(2023)
Data quality and autism: Issues and potential impacts
in International Journal of Medical Informatics
Hill A
(2022)
Intrinsic alignments of the extended radio continuum emission of galaxies in the EAGLE simulations
in Monthly Notices of the Royal Astronomical Society
Hillier A
(2023)
The role of cooling induced by mixing in the mass and energy cycles of the solar atmosphere
in Monthly Notices of the Royal Astronomical Society
Hough R
(2023)
SIMBA - C : an updated chemical enrichment model for galactic chemical evolution in the SIMBA simulation
in Monthly Notices of the Royal Astronomical Society
Huang J
(2023)
Global 3D Radiation Magnetohydrodynamic Simulations of Accretion onto a Stellar-mass Black Hole at Sub- and Near-critical Accretion Rates
in The Astrophysical Journal
Hughes M
(2022)
The physics governing the upper truncation mass of the globular cluster mass function
in Monthly Notices of the Royal Astronomical Society
Hutchinson A
(2022)
Energetic proton back-precipitation onto the solar atmosphere in relation to long-duration gamma-ray flares
in Astronomy & Astrophysics
Hutchinson A
(2023)
Modelling shock-like injections of solar energetic particles with 3D test particle simulations
in Astronomy & Astrophysics
Hutchinson A
(2023)
Impact of corotation on gradual solar energetic particle event intensity profiles
in Astronomy & Astrophysics
Hutt M
(2022)
The effect of local Universe constraints on halo abundance and clustering
in Monthly Notices of the Royal Astronomical Society
Huško F
(2023)
The buildup of galaxies and their spheroids: The contributions of mergers, disc instabilities, and star formation
in Monthly Notices of the Royal Astronomical Society
Huško F
(2022)
Spin-driven jet feedback in idealized simulations of galaxy groups and clusters
in Monthly Notices of the Royal Astronomical Society
Huško F
(2022)
Statistics of galaxy mergers: bridging the gap between theory and observation
in Monthly Notices of the Royal Astronomical Society
Huško F
(2023)
Active galactic nuclei jets simulated with smoothed particle hydrodynamics
in Monthly Notices of the Royal Astronomical Society
Huško F
(2023)
The complex interplay of AGN jet-inflated bubbles and the intracluster medium
in Monthly Notices of the Royal Astronomical Society
Icaza-Lizaola M
(2023)
A sparse regression approach for populating dark matter haloes and subhaloes with galaxies
in Monthly Notices of the Royal Astronomical Society
Igoshev A
(2023)
Three-dimensional magnetothermal evolution of off-centred dipole magnetic field configurations in neutron stars
in Monthly Notices of the Royal Astronomical Society
Irodotou D
(2022)
The effects of AGN feedback on the structural and dynamical properties of Milky Way-mass galaxies in cosmological simulations
in Monthly Notices of the Royal Astronomical Society
Jahns-Schindler J
(2023)
How limiting is optical follow-up for fast radio burst applications? Forecasts for radio and optical surveys
in Monthly Notices of the Royal Astronomical Society