DiRAC-3 Operations 2019-2022 - Cambridge [2020-06 resubmission]
Lead Research Organisation:
University of Cambridge
Department Name: Institute of Astronomy
Abstract
DiRAC-3 Operations 2019-2022 resubmission; This is an administrative resubmission to replace ST/S003800/1 which has already been peer-reviewed.
Organisations
Publications
Lee J
(2022)
Simulating Jellyfish Galaxies: A Case Study for a Gas-rich Dwarf Galaxy
in The Astrophysical Journal
Lee J
(2020)
Dual Effects of Ram Pressure on Star Formation in Multiphase Disk Galaxies with Strong Stellar Feedback
in The Astrophysical Journal
Leo M
(2020)
Constraining structure formation using EDGES
in Journal of Cosmology and Astroparticle Physics
Le Saux A
(2023)
Two-dimensional simulations of internal gravity waves in a 5 M? zero-age-main-sequence model
in Monthly Notices of the Royal Astronomical Society
Li B
(2020)
Measuring the baryon acoustic oscillation peak position with different galaxy selections
in Monthly Notices of the Royal Astronomical Society
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
Lim S
(2024)
The FLAMINGO simulation view of cluster progenitors observed in the epoch of reionization with JWST
in Monthly Notices of the Royal Astronomical Society
Lindert J
(2024)
Logarithmic EW corrections at one-loop
in The European Physical Journal C
Lindert J
(2023)
Precise predictions for V + 2 jet backgrounds in searches for invisible Higgs decays
in Journal of High Energy Physics
Linh B
(2021)
Investigation of the ground-state spin inversion in the neutron-rich Cl 47 , 49 isotopes
in Physical Review C
Linh B
(2024)
Onset of collectivity for argon isotopes close to N = 32
in Physical Review C
Liow K
(2020)
The role of collision speed, cloud density, and turbulence in the formation of young massive clusters via cloud-cloud collisions
in Monthly Notices of the Royal Astronomical Society
Liu Y
(2024)
The mass accretion history of dark matter haloes down to Earth mass
in Monthly Notices of the Royal Astronomical Society
Lofthouse E
(2020)
MUSE Analysis of Gas around Galaxies (MAGG) - I: Survey design and the environment of a near pristine gas cloud at z ˜ 3.5
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
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)
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 M
(2020)
Toward a General Parameterization of the Warm Dark Matter Halo Mass Function
in The Astrophysical Journal
Lovell M
(2020)
Local group star formation in warm and self-interacting dark matter cosmologies
in Monthly Notices of the Royal Astronomical Society
Lower S
(2020)
How Well Can We Measure the Stellar Mass of a Galaxy: The Impact of the Assumed Star Formation History Model in SED Fitting
in The Astrophysical Journal
Lynas-Gray A
(2024)
ExoMol line lists - LXII. Ro-vibrational energy levels and line strengths for the propadienediylidene (C3) in its ground electronic state
in Monthly Notices of the Royal Astronomical Society
Maccagni F
(2024)
MHONGOOSE discovery of a gas-rich low surface brightness galaxy in the Dorado group
in Astronomy & Astrophysics
Macpherson H
(2023)
Cosmological distances with general-relativistic ray tracing: framework and comparison to cosmographic predictions
in Journal of Cosmology and Astroparticle Physics
Macpherson H
(2024)
The Impact of Anisotropic Sky Sampling on the Hubble Constant in Numerical Relativity
in The Astrophysical Journal
Madar M
(2024)
Predictions for the abundance and clustering of H a emitting galaxies
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 our results |
| Sectors | Aerospace Defence and Marine Digital/Communication/Information Technologies (including Software) Education |