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
Li Y
(2022)
Non-linear reconstruction of features in the primordial power spectrum from large-scale structure
in Monthly Notices of the Royal Astronomical Society
Lindert J
(2023)
Precise predictions for V + 2 jet backgrounds in searches for invisible Higgs decays
in Journal of High Energy Physics
Lovell C
(2022)
A machine learning approach to mapping baryons on to dark matter haloes using the eagle and C-EAGLE simulations
in Monthly Notices of the Royal Astronomical Society
Lovell C
(2023)
First light and reionisation epoch simulations (FLARES) - VIII. The emergence of passive galaxies at z = 5
in Monthly Notices of the Royal Astronomical Society
Lovell C
(2022)
An orientation bias in observations of submillimetre galaxies
in Monthly Notices of the Royal Astronomical Society
Macpherson H
(2023)
Cosmological distances with general-relativistic ray tracing: framework and comparison to cosmographic predictions
in Journal of Cosmology and Astroparticle Physics
Mak M
(2023)
3D Simulations of the Archean Earth Including Photochemical Haze Profiles
in Journal of Geophysical Research: Atmospheres
Malbrunot-Ettenauer S
(2022)
Nuclear Charge Radii of the Nickel Isotopes ^{58-68,70}Ni.
in Physical review letters
Mann A
(2022)
TESS Hunt for Young and Maturing Exoplanets (THYME). VI. An 11 Myr Giant Planet Transiting a Very-low-mass Star in Lower Centaurus Crux
in The Astronomical Journal
Mason S
(2022)
Magnetoconvection in a rotating spherical shell in the presence of a uniform axial magnetic field
in Geophysical & Astrophysical Fluid Dynamics
McAlpine S
(2022)
SIBELIUS-DARK: a galaxy catalogue of the local volume from a constrained realization simulation
in Monthly Notices of the Royal Astronomical Society
McCarthy I
(2023)
The FLAMINGO project: revisiting the S 8 tension and the role of baryonic physics
in Monthly Notices of the Royal Astronomical Society
Mitchell M
(2022)
A general framework to test gravity using galaxy clusters - VI. Realistic galaxy formation simulations to study clusters in modified gravity
in Monthly Notices of the Royal Astronomical Society
Mitchell P
(2022)
Baryonic mass budgets for haloes in the eagle simulation, including ejected and prevented gas
in Monthly Notices of the Royal Astronomical Society
Mitchell P
(2022)
How gas flows shape the stellar-halo mass relation in the eagle simulation
in Monthly Notices of the Royal Astronomical Society
Montargès M
(2023)
The VLT/SPHERE view of the ATOMIUM cool evolved star sample I. Overview: Sample characterization through polarization analysis
in Astronomy & Astrophysics
Mosbech M
(2023)
Gravitational-wave event rates as a new probe for dark matter microphysics
in Physical Review D
Murtas G
(2022)
Collisional ionization and recombination effects on coalescence instability in chromospheric partially ionized plasmas
in Physics of Plasmas
Negri A
(2022)
The luminosity of cluster galaxies in the Cluster-EAGLE simulations
in Monthly Notices of the Royal Astronomical Society
Nelson R
(2023)
Gas accretion onto Jupiter mass planets in discs with laminar accretion flows
in Astronomy & Astrophysics
Nixon C
(2022)
Stellar Revival and Repeated Flares in Deeply Plunging Tidal Disruption Events
in The Astrophysical Journal Letters
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
Orkney M
(2022)
EDGE: the puzzling ellipticity of Eridanus II's star cluster and its implications for dark matter at the heart of an ultra-faint dwarf
in Monthly Notices of the Royal Astronomical Society
Orkney M
(2023)
EDGE: the shape of dark matter haloes in the faintest galaxies
in Monthly Notices of the Royal Astronomical Society