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
Katsianis A
(2020)
The high-redshift SFR-M* relation is sensitive to the employed star formation rate and stellar mass indicators: towards addressing the tension between observations and simulations
in Monthly Notices of the Royal Astronomical Society
Gómez-Guijarro C
(2020)
How primordial magnetic fields shrink galaxies
in Monthly Notices of the Royal Astronomical Society
Can K
(2020)
Lattice QCD evaluation of the Compton amplitude employing the Feynman-Hellmann theorem
in Physical Review D
Brown S
(2020)
Connecting the structure of dark matter haloes to the primordial power spectrum
in Monthly Notices of the Royal Astronomical Society
Pfeffer J
(2020)
Predicting accreted satellite galaxy masses and accretion redshifts based on globular cluster orbits in the E-MOSAICS simulations
in Monthly Notices of the Royal Astronomical Society
Salvioni G
(2020)
Model nuclear energy density functionals derived from ab initio calculations
in Journal of Physics G: Nuclear and Particle Physics
Hall C
(2020)
Predicting the Kinematic Evidence of Gravitational Instability
in The Astrophysical Journal
Wurster J
(2020)
Non-ideal magnetohydrodynamics versus turbulence II: Which is the dominant process in stellar core formation?
in Monthly Notices of the Royal Astronomical Society
He J
(2020)
Modelling the tightest relation between galaxy properties and dark matter halo properties from hydrodynamical simulations of galaxy formation
in Monthly Notices of the Royal Astronomical Society