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
Organisations
Publications
Simpson J
(2020)
An ALMA survey of the brightest sub-millimetre sources in the SCUBA-2-COSMOS field
in Monthly Notices of the Royal Astronomical Society
Shitvov A
(2020)
Reflective Toraldo pupil for high-resolution millimeter-wave astronomy.
in Applied optics
Shirley R
(2021)
HELP: the Herschel Extragalactic Legacy Project
in Monthly Notices of the Royal Astronomical Society
Shimajiri Y.
(2023)
Witnessing the fragmentation of a filament into prestellar cores in Orion B/NGC 2024
in arXiv e-prints
Shimajiri Y
(2020)
The accretion history of high-mass stars: an ArTéMiS pilot study of infrared dark clouds
in Monthly Notices of the Royal Astronomical Society
Shelest A
(2020)
From spirals to lenticulars: Evidence from the rotation curves and mass models of three early-type galaxies
in Astronomy & Astrophysics
Shariff J
(2019)
Submillimeter Polarization Spectrum of the Carina Nebula
in The Astrophysical Journal
Seth Anil C.
(2021)
Revealing Low Luminosity Active Galactic Nuclei (ReveaLLAGN)
in JWST Proposal. Cycle 1
Schuller F.
(2023)
VizieR Online Data Catalog: The SEDIGISM survey: First Data Release (Schuller+, 2021)
in VizieR Online Data Catalog
Schuller F
(2021)
The SEDIGISM survey: First Data Release and overview of the Galactic structure
in Monthly Notices of the Royal Astronomical Society
Schuller F
(2021)
Probing the structure of a massive filament: ArTéMiS 350 and 450 µm mapping of the integral-shaped filament in Orion A
in Astronomy & Astrophysics
Schombert J
(2020)
Using the Baryonic Tully-Fisher Relation to Measure H o
in The Astronomical Journal
Schisano E
(2020)
The Hi-GAL catalogue of dusty filamentary structures in the Galactic plane
in Monthly Notices of the Royal Astronomical Society
Schillaci A.
(2020)
Design and performance of the first BICEP Array receiver
in arXiv e-prints
Schillaci A
(2020)
Design and Performance of the First BICEP Array Receiver
in Journal of Low Temperature Physics
Schaan E
(2021)
Atacama Cosmology Telescope: Combined kinematic and thermal Sunyaev-Zel'dovich measurements from BOSS CMASS and LOWZ halos
in Physical Review D
Sayre J. T.
(2019)
Measurements of B-mode Polarization of the Cosmic Microwave Background from 500 Square Degrees of SPTpol Data
in arXiv e-prints
Sayre J
(2020)
Measurements of B -mode polarization of the cosmic microwave background from 500 square degrees of SPTpol data
in Physical Review D
Sarzi M
(2019)
WISDOM project - IV. A molecular gas dynamical measurement of the supermassive black hole mass in NGC 524
in Monthly Notices of the Royal Astronomical Society
Sarkar Subhajit
(2019)
Detection of Earth-like atmospheres by transit spectroscopy: exploring instrumental parameters for optimal yield
in EPSC-DPS Joint Meeting 2019
Sansom A
(2019)
ALMA observations of massive molecular gas reservoirs in dusty early-type galaxies
in Monthly Notices of the Royal Astronomical Society