A Programme of Technology, Astrophysics and Cosmology in Cardiff 2019-22

Lead Research Organisation: CARDIFF UNIVERSITY
Department Name: School of Physics and Astronomy

Abstract

We propose a programme of Astrophysics, Cosmology and Technology development for Astrophysics and Cosmology, to investigate star and planet formation in our own and other galaxies, how galaxies form and evolve and the signals from the very early Universe embedded in the polarisation properties of the Cosmic Microwave background. This programme will combine observational data from world-class ground and space-based observatories, as well as theoretical modelling and simulations of the processes that result in the Universe we observe around us. We will also continue to develop the world's most sensitive detectors for very long infrared wavelengths, along with associated optical components utilising 'metamaterials' the class of materials designed and manufactured by human beings to have the properties best suited to their task, rather than relying on naturally occurring minerals and plastics. Both of these areas of technology development potentially have wide applications outside of Astronomy, in areas such as security scanners and bio-medical imaging for example.

Planned Impact

The technology programme proposed here will have extensive impact outside of astronomy. Firstly in other academic subject areas such as Earth-observing where the technology is used to look downwards or sideways through the atmosphere rather than upwards, but also in bio-medical imaging, where the Far-infrared wavelength range has many spectral features, and is currently being used in collaboration with the School of Optometry in Cardiff to assess corneal damage, for example. Secondly we also plan to exploit the technology commercially, through the spinout company QMCI (www.terahertz.co.uk) which operates from within the School, with broad applications from fast plasma diagnostic systems in use in Fusion experiments, through laboratory spectroscopy across a wide range of chemistry and materials applications, and the new spinout Sequestym, for security cameras. We also plan a very strong Outreach programme across both the technology developments and the observational and theoretical astrophysics and cosmology programme, following on from the skills developed during the very successful Herschel/Planck outreach programme, with web-based and standard media information releases, but also tied in with Open days, school visits, and going out into schools and colleges to give presentations and host workshops

Publications

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Rigby A (2021) GASTON: Galactic Star Formation with NIKA2 - evidence for the mass growth of star-forming clumps in Monthly Notices of the Royal Astronomical Society

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Seth Anil C. (2021) Revealing Low Luminosity Active Galactic Nuclei (ReveaLLAGN) in JWST Proposal. Cycle 1

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Rohde P (2021) The impact of episodic outflow feedback on stellar multiplicity and the star formation efficiency in Monthly Notices of the Royal Astronomical Society

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Inserra C (2021) The first Hubble diagram and cosmological constraints using superluminous supernovae in Monthly Notices of the Royal Astronomical Society

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Priestley F (2021) Revisiting the dust destruction efficiency of supernovae in Monthly Notices of the Royal Astronomical Society

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Eden D (2021) Characteristic scale of star formation - I. Clump formation efficiency on local scales in Monthly Notices of the Royal Astronomical Society

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Xie J (2021) Studying infall in infrared dark clouds with multiple HCO + transitions in Research in Astronomy and Astrophysics

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Anderson M (2021) An ALMA study of hub-filament systems - I. On the clump mass concentration within the most massive cores in Monthly Notices of the Royal Astronomical Society

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Wünsch R (2021) Tree-based solvers for adaptive mesh refinement code flash - II: radiation transport module TreeRay in Monthly Notices of the Royal Astronomical Society

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North E (2021) WISDOM project - VIII. Multiscale feedback cycles in the brightest cluster galaxy NGC 0708 in Monthly Notices of the Royal Astronomical Society

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Young L (2021) The Evolution of NGC 7465 as Revealed by Its Molecular Gas Properties in The Astrophysical Journal

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Schuller F (2021) The SEDIGISM survey: First Data Release and overview of the Galactic structure in Monthly Notices of the Royal Astronomical Society

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Perley D (2021) Real-time discovery of AT2020xnd: a fast, luminous ultraviolet transient with minimal radioactive ejecta in Monthly Notices of the Royal Astronomical Society

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Urquhart J (2021) SEDIGISM-ATLASGAL: dense gas fraction and star formation efficiency across the Galactic disc in Monthly Notices of the Royal Astronomical Society

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Whitworth A (2021) Ionizing feedback from an O star formed in a filament in Monthly Notices of the Royal Astronomical Society

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Hilton M (2021) The Atacama Cosmology Telescope: A Catalog of >4000 Sunyaev-Zel'dovich Galaxy Clusters in The Astrophysical Journal Supplement Series

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Zabel N (2021) AlFoCS  + F3D - II. Unexpectedly low gas-to-dust ratios in the Fornax galaxy cluster in Monthly Notices of the Royal Astronomical Society

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Whitworth A (2021) A systematic bias in fitting the surface-density profiles of interstellar filaments in Monthly Notices of the Royal Astronomical Society

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Nightingale J (2021) PyAutoLens: Open-Source Strong Gravitational Lensing in Journal of Open Source Software

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Izquierdo A (2021) The Cloud Factory II: gravoturbulent kinematics of resolved molecular clouds in a galactic potential in Monthly Notices of the Royal Astronomical Society

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Duarte-Cabral A (2021) The SEDIGISM survey: molecular clouds in the inner Galaxy in Monthly Notices of the Royal Astronomical Society

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Querejeta M (2021) ALMA resolves giant molecular clouds in a tidal dwarf galaxy in Astronomy & Astrophysics

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Mallaby-Kay M (2021) The Atacama Cosmology Telescope: Summary of DR4 and DR5 Data Products and Data Access in The Astrophysical Journal Supplement Series

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Han D (2021) The Atacama Cosmology Telescope: delensed power spectra and parameters in Journal of Cosmology and Astroparticle Physics

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Barna B (2021) SN 2019muj - a well-observed Type Iax supernova that bridges the luminosity gap of the class in Monthly Notices of the Royal Astronomical Society