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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Priestley F (2023) NEATH - II. N2H+ as a tracer of imminent star formation in quiescent high-density gas in Monthly Notices of the Royal Astronomical Society

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Priestley F (2020) Dust masses and grain size distributions of a sample of Galactic pulsar wind nebulae in Monthly Notices of the Royal Astronomical Society

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Priestley F (2023) Non-Equilibrium Abundances Treated Holistically (NEATH): the molecular composition of star-forming clouds in Monthly Notices of the Royal Astronomical Society

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Priestley F (2020) Constraining early-time dust formation in core-collapse supernovae in Monthly Notices of the Royal Astronomical Society

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Priestley F (2022) The origin of a universal filament width in molecular clouds in Monthly Notices of the Royal Astronomical Society

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Priestley F (2022) Properties of shocked dust grains in supernova remnants in Monthly Notices of the Royal Astronomical Society

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Priestley F (2019) Erratum: Modelling the ArH+ emission from the Crab Nebula in Monthly Notices of the Royal Astronomical Society

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Priestley F (2023) Do simulated molecular clouds look like real ones? in Monthly Notices of the Royal Astronomical Society

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Priestley F (2020) The apparent anticorrelation between the mass opacity of interstellar dust and the surface density of interstellar gas in Monthly Notices of the Royal Astronomical Society: Letters

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Priestley F (2021) The efficiency of grain growth in the diffuse interstellar medium in Monthly Notices of the Royal Astronomical Society

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Priestley F (2022) The initial magnetic criticality of pre-stellar cores in Monthly Notices of the Royal Astronomical Society

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Priestley F (2021) Molecular line signatures of cloud-cloud collisions in Monthly Notices of the Royal Astronomical Society

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Priestley F. D. (2019) Revisiting the Crab Nebula's dust and synchrotron radiation from the infrared to radio domain in Supernova Remnants: An Odyssey in Space after Stellar Death II

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Prole L (2022) Primordial magnetic fields in Population III star formation: a magnetized resolution study in Monthly Notices of the Royal Astronomical Society

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Prole Lewis R. (2023) Heavy Black Hole Seed Formation in High-z Atomic Cooling Halos in arXiv e-prints

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Pursiainen M. (2023) Polarimetry of Hydrogen-Poor Superluminous Supernovae in arXiv e-prints

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

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Raghunathan S (2019) Detection of CMB-Cluster Lensing using Polarization Data from SPTpol. in Physical review letters

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Rho J (2023) Far-infrared polarization of the supernova remnant Cassiopeia A with SOFIA HAWC + in Monthly Notices of the Royal Astronomical Society

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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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Roberts I (2023) VERTICO VI. Cold-gas asymmetries in Virgo cluster galaxies in Astronomy & Astrophysics

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Rodighiero G (2019) Active Galactic Nuclei in Dusty Starbursts at z = 2: Feedback Still to Kick in in The Astrophysical Journal Letters

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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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Rohde P (2019) Evolution of Hubble wedges in episodic protostellar outflows in Monthly Notices of the Royal Astronomical Society

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Rohde P (2022) Protostellar outflows: a window to the past in Monthly Notices of the Royal Astronomical Society

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Rowe S (2022) The MUSCAT Readout Electronics Backend: Design and Pre-deployment Performance in Journal of Low Temperature Physics