📣 Help Shape the Future of UKRI's Gateway to Research (GtR)

We're improving UKRI's Gateway to Research and are seeking your input! If you would be interested in being interviewed about the improvements we're making and to have your say about how we can make GtR more user-friendly, impactful, and effective for the Research and Innovation community, please email gateway@ukri.org.

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.

Publications

10 25 50
publication icon
Trayford J (2020) Fade to grey: systematic variation of galaxy attenuation curves with galaxy properties in the eagle simulations in Monthly Notices of the Royal Astronomical Society

publication icon
Chen C (2023) Can a binary star host three giant circumbinary planets? in Monthly Notices of the Royal Astronomical Society

publication icon
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

publication icon
Agertz O (2020) EDGE: the mass-metallicity relation as a critical test of galaxy formation physics in Monthly Notices of the Royal Astronomical Society

publication icon
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

publication icon
Robson D (2023) Redshift evolution of galaxy group X-ray properties in the Simba simulations in Monthly Notices of the Royal Astronomical Society

publication icon
Soussana A (2020) The impact of AGN feedback on galaxy intrinsic alignments in the Horizon simulations in Monthly Notices of the Royal Astronomical Society

publication icon
Grove C (2022) The DESI N -body simulation project - I. Testing the robustness of simulations for the DESI dark time survey in Monthly Notices of the Royal Astronomical Society

publication icon
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

publication icon
Oppenheimer B (2020) Feedback from supermassive black holes transforms centrals into passive galaxies by ejecting circumgalactic gas 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