A Programme of Technology, Astrophysics and Cosmology in Cardiff, 2022-2025
Lead Research Organisation:
CARDIFF UNIVERSITY
Department Name: School of Physics and Astronomy
Abstract
Astronomers try to answer a wide range of questions, from fundamental ones, such as how stars and galaxies are formed and questions about the structure and evolution of the universe itself, to more detailed questions about the physical and chemical processes occurring in astronomical objects. A powerful way of trying to answer some of the most important ones is to make observations in the submillimetre waveband, one of the newest branches of astronomy. The births of stars and galaxies, for example, occur in huge clouds of gas and dust, and the dust - tiny solid fragments in interstellar space - hides the births from traditional optical telescopes like the Hubble Space Telescope. With submillimetre telescopes, however, it is possible to observe radiation from the dust itself, allowing astronomers to observe the very earliest stages in the lives of stars and galaxies. Submillimetre astronomy is one of our specialities in Cardiff, with our group containing both astronomers that use submillimetre telescopes but also scientists that build novel cameras and other devices that work in this waveband - technology that also has many uses outside astronomy. In this proposal we ask for funds from the UK taxpayer to support our research. Much of this research involves using or building submillimetre instruments, but some of the projects we propose will use telescopes in other wavebands or use powerful computers to simulate the processes involved in the birth of a star or the formation of a galaxy. The questions we will try to answer include many of the most important ones. One of the surprising things about planets like ours is that they exist at all, because centimetre-sized solid chunks around a star are likely to be destroyed before they coalesce to form bigger chunks and eventually planets. We will use radio observations to search for chunks of this size in the disks of dust around newly formed stars, with the aim of understanding how small rocky planets like our own were formed, and in another project we will use a new balloon observatory to study the other end of the planetary spectrum - the giant 'hot Jupiters' that have been discovered around nearby stars. We propose several projects to investigate the formation of stars, both the stars that are forming around us today and a special population of stars with very few heavy elements that astronomers think formed just after the Big Bang, using a mixture of observations and computer simulations. We propose two project that will study supernovae, the titanic explosions that occur when a massive star collapses at the end of its life. One project will investigate the formation of dust grains and molecular gas within a supernova explosion, the other the recently discovered superluminous supernovae, up to 100 times more luminous than the standard kind. Again using a mixture of observations and computer simulations, we propose several projects to study galaxies, including a study of the Andromeda Galaxy, the nearest big galaxy, an investigation of the super-massive black holes at the centres of nearby galaxies, a computer simulation of the gas flows around a galaxy, and a project to find more examples of very distant galaxies, which we are seeing only shortly after the Big Bang and that are being highly magnified by the gravity of close galaxies. More examples of these highly magnified galaxies is important because the magnification means that we can study the way galaxies are formed in great detail. We also propose two technical projects, one to develop kinetic inductance detectors, a kind of detector that our group largely discovered and which makes possible revolutionary new instruments, and one to develop further 'meta-materials', a kind of material that makes possible novel components for instruments, such as flat lenses, and which our group has used to make the filters for all submillimetre telescopes, on the ground and in space, over the last 30 years.
Organisations
Publications
Zsíros S
(2024)
Serendipitous detection of the dusty Type IIL SN 1980K with JWST /MIRI
in Monthly Notices of the Royal Astronomical Society
Zabel N
(2022)
VERTICO II: How H i-identified Environmental Mechanisms Affect the Molecular Gas in Cluster Galaxies
in The Astrophysical Journal
Zabel N
(2023)
Erratum: "VERTICO II: How H i-identified Environmental Mechanisms Affect the Molecular Gas in Cluster Galaxies" (2022, ApJ, 933, 10)
in The Astrophysical Journal
Young L
(2022)
Down but Not Out: Properties of the Molecular Gas in the Stripped Virgo Cluster Early-type Galaxy NGC 4526
in The Astrophysical Journal
Wolz K.
(2023)
The Simons Observatory: pipeline comparison and validation for large-scale B-modes
in arXiv e-prints
Wiseman P.
(2023)
Multiwavelength observations of the extraordinary accretion event AT2021lwx
in arXiv e-prints
Winkel Nico
(2022)
Tracing the onset of the AGN feeding-feedback cycle in the nearby NLS1 Mrk 1044
in American Astronomical Society Meeting #240
Winkel N
(2022)
The Close AGN Reference Survey (CARS) Tracing the circumnuclear star formation in the super-Eddington NLS1 Mrk 1044
in Astronomy & Astrophysics
Winkel N
(2023)
The Close AGN Reference Survey (CARS) A parsec-scale multi-phase outflow in the super-Eddington NLS1 Mrk 1044
in Astronomy & Astrophysics
Williams T
(2023)
WISDOM Project - XVII. Beam-by-beam properties of the molecular gas in early-type galaxies
in Monthly Notices of the Royal Astronomical Society
Whitworth A
(2022)
Ionizing feedback from an O star formed in a shock-compressed layer
in Monthly Notices of the Royal Astronomical Society
Wevers T
(2022)
An elliptical accretion disk following the tidal disruption event AT 2020zso
in Astronomy & Astrophysics
Wesson R.
(2022)
VizieR Online Data Catalog: Extreme abundance discrepancy factors in PNe (Wesson+, 2018)
in VizieR Online Data Catalog
Wesson R
(2023)
Evidence for late-time dust formation in the ejecta of supernova SN 1995N from emission-line asymmetries
in Monthly Notices of the Royal Astronomical Society
Wesson R
(2024)
JWST observations of the Ring Nebula (NGC 6720): I. Imaging of the rings, globules, and arcs
in Monthly Notices of the Royal Astronomical Society
Wells M
(2022)
ATLASGAL - star forming efficiencies and the Galactic star formation rate
in Monthly Notices of the Royal Astronomical Society
Watts Adam B.
(2023)
VERTICO V: The environmentally driven evolution of the inner cold gas discs of Virgo cluster galaxies
in arXiv e-prints
Watts A
(2023)
VERTICO V: The environmentally driven evolution of the inner cold gas discs of Virgo cluster galaxies
in Publications of the Astronomical Society of Australia
Ward B
(2024)
Little evolution of dust emissivity in bright infrared galaxies from 2 < z < 6
in Monthly Notices of the Royal Astronomical Society
Wang J
(2022)
Formation of the SDC13 Hub-filament System: A Cloud-Cloud Collision Imprinted on the Multiscale Magnetic Field
in The Astrophysical Journal
Villanueva V
(2022)
VERTICO. IV. Environmental Effects on the Gas Distribution and Star Formation Efficiency of Virgo Cluster Spirals
in The Astrophysical Journal
Vieira H
(2023)
Molecular clouds in M51 from high-resolution extinction mapping