Astronomy at Durham 2020-2023
Lead Research Organisation:
Durham University
Department Name: Physics
Abstract
Astronomy can capture the public imagination to a greater extent than almost any other branch of science. It is accessible to anyone who gazes up into the night sky to look at the Moon, the planets, stars, and nearby galaxies. Our understanding of the universe has developed rapidly over the past several decades. On the basis of the standard cosmological model we live in a universe where at least two thirds of the mass energy is in the form of dark energy which causes the Universe to expand at an ever increasing rate. About a quarter of the mass energy is in the form of dark matter, most probably a new weakly interacting elementary particle yet to be detected on Earth (and hence of great interest to particle physicists). The remaining five percent of the mass energy is in the form of ordinary, or baryonic, matter of which only about a tenth is in stars and planets such as the Earth, and the rest resides mostly as gas in between galaxies.
Our programme combines cutting-edge theoretical and observational research with innovative instrumentation development to understand the universe in which we inhabit. We blend theoretical research on the earliest phases of the Universe with theoretical and observational projects to determine the formation and evolution of black holes, galaxies, and the larger-scale structures in which they reside. We confront the predictions from our models with our latest observational results, while actively exploiting innovative instrumentation developments pursued in Durham. We will explore astrophysical clues to the identity of the dark matter and the nature of the dark energy, focus on the evolution of galaxies back to the earliest times in the Universe and the influence on which the larger-scale environment has had on their properties. We will investigate the formation and evolution of black holes and their role in determining the structure and properties of galaxies and their larger scale structures, using the latest instruments on ground-based observatories and Earth-orbiting satellites.
Our programme combines cutting-edge theoretical and observational research with innovative instrumentation development to understand the universe in which we inhabit. We blend theoretical research on the earliest phases of the Universe with theoretical and observational projects to determine the formation and evolution of black holes, galaxies, and the larger-scale structures in which they reside. We confront the predictions from our models with our latest observational results, while actively exploiting innovative instrumentation developments pursued in Durham. We will explore astrophysical clues to the identity of the dark matter and the nature of the dark energy, focus on the evolution of galaxies back to the earliest times in the Universe and the influence on which the larger-scale environment has had on their properties. We will investigate the formation and evolution of black holes and their role in determining the structure and properties of galaxies and their larger scale structures, using the latest instruments on ground-based observatories and Earth-orbiting satellites.
Planned Impact
We have a strong track record of public engagement. What started out as a Physics-centric outreach initiative over a decade ago has become a University wide activity. It has led to the creation of the highly successful Celebrate Science festival in Durham, which attracts ~7,000 people each year. This year we are aiming to quantify the impact of our outreach by sending out carefully designed questionnaires to the local schools attending the Durham University Schools' Science Festival, which attracts over 850 pupils annually. This will allow us to develop our outreach activities into an impact case study for the upcoming REF exercise, combining the six Royal Society Summer Science exhibitions that we have been involved in between 2002-2016. We aim to submit a new proposal for Summer Science 2020 or 2021 to refresh our outreach materials. Building on the Cosmic Architecture and Cosmoscope installations we built for Durham's Lumiere festival in 2017, we plan to include one or more of these in the "greatest hits" version of Lumiere in 2019, the tenth anniversary of the first event, after which we will develop new exhibits for Lumiere 2021.
Our Knowledge Exchange (KE) programme builds upon the strong industry links within all three of the astronomy groups at Durham, and has been expanded in recent years with the establishment of the Durham Data Intensive Science CDT. We will continue to exploit the opportunities afforded by the CDT for placements and team projects with local SMEs and wider UK industries. We will also use these opportunities to build the visibility of our wider research knowledge and skills to industry.
We are expanding our capabilities in precision diamond machining via infrastructure investments from the University and elsewhere, and will seek to develop their economic impact via applications into the STFC FOF and IPS programmes. Our expertise in adaptive optics is recognised worldwide and we will continue develop its international impact with joint programmes in China, Turkey & Thailand. Our work on novel detectors (MKIDs) will naturally support wider European initiatives such as the ATTRACT project.
Finally, our broader research programme underpins the research and development of a cohort of postgraduate students at Durham, providing them with training in specific and transferable skills which is being accelerated by our CDTs. Former students have taken jobs in a range of industries from computer gaming to finance and genetics. Physics students at Durham benefit through their participation in our research work via their 4th year MPhys projects. Our technical training of these post/undergraduate students provides a pool of talented, skilled candidates to the UK economy which will continue throughout the period of our Consolidated Grant proposal. We will continue to add industrial partners to the CDT in Data Intensive Science to offer new placement opportunities for PhD students and for students on our new MSc course in Scientific Computing and Data Analysis.
Our Knowledge Exchange (KE) programme builds upon the strong industry links within all three of the astronomy groups at Durham, and has been expanded in recent years with the establishment of the Durham Data Intensive Science CDT. We will continue to exploit the opportunities afforded by the CDT for placements and team projects with local SMEs and wider UK industries. We will also use these opportunities to build the visibility of our wider research knowledge and skills to industry.
We are expanding our capabilities in precision diamond machining via infrastructure investments from the University and elsewhere, and will seek to develop their economic impact via applications into the STFC FOF and IPS programmes. Our expertise in adaptive optics is recognised worldwide and we will continue develop its international impact with joint programmes in China, Turkey & Thailand. Our work on novel detectors (MKIDs) will naturally support wider European initiatives such as the ATTRACT project.
Finally, our broader research programme underpins the research and development of a cohort of postgraduate students at Durham, providing them with training in specific and transferable skills which is being accelerated by our CDTs. Former students have taken jobs in a range of industries from computer gaming to finance and genetics. Physics students at Durham benefit through their participation in our research work via their 4th year MPhys projects. Our technical training of these post/undergraduate students provides a pool of talented, skilled candidates to the UK economy which will continue throughout the period of our Consolidated Grant proposal. We will continue to add industrial partners to the CDT in Data Intensive Science to offer new placement opportunities for PhD students and for students on our new MSc course in Scientific Computing and Data Analysis.
Publications
Trapp C
(2022)
Gas infall and radial transport in cosmological simulations of milky way-mass discs
in Monthly Notices of the Royal Astronomical Society
Mitchell M
(2021)
The impact of modified gravity on the Sunyaev-Zeldovich effect
in Monthly Notices of the Royal Astronomical Society
Gillman S
(2022)
The resolved chemical abundance properties within the interstellar medium of star-forming galaxies at z ˜ 1.5
in Monthly Notices of the Royal Astronomical Society
Cuesta-Lazaro C
(2023)
Galaxy clustering from the bottom up: a streaming model emulator I
in Monthly Notices of the Royal Astronomical Society
Koprowski M
(2020)
An ALMA survey of the SCUBA-2 cosmology legacy survey UKIDSS/UDS field: Dust attenuation in high-redshift Lyman-break galaxies
in Monthly Notices of the Royal Astronomical Society
Gillman S
(2020)
The Evolution of Gas-Phase Metallicity and Resolved Abundances in Star-forming Galaxies at z ˜ 0.6 - 1.8
in Monthly Notices of the Royal Astronomical Society
Ristea A
(2024)
The Tully-Fisher relation from SDSS-MaNGA: physical causes of scatter and variation at different radii
in Monthly Notices of the Royal Astronomical Society
Wang Y
(2020)
Iterative removal of redshift-space distortions from galaxy clustering
in Monthly Notices of the Royal Astronomical Society
Salcido J
(2020)
How feedback shapes galaxies: an analytic model
in Monthly Notices of the Royal Astronomical Society
Downing E
(2023)
The many reasons that the rotation curves of low-mass galaxies can fail as tracers of their matter distributions
in Monthly Notices of the Royal Astronomical Society
Richard-Laferrière A
(2020)
On the relation between mini-halos and AGN feedback in clusters of galaxies
in Monthly Notices of the Royal Astronomical Society
Cooke R
(2020)
The ACCELERATION programme: I. Cosmology with the redshift drift
in Monthly Notices of the Royal Astronomical Society
Mitchell M
(2021)
A general framework to test gravity using galaxy clusters III: observable-mass scaling relations in f ( R ) gravity
in Monthly Notices of the Royal Astronomical Society
Sykes C
(2020)
Determining the primordial helium abundance and UV background using fluorescent emission in star-free dark matter haloes
in Monthly Notices of the Royal Astronomical Society
Dhillon V
(2021)
HiPERCAM: a quintuple-beam, high-speed optical imager on the 10.4-m Gran Telescopio Canarias
in Monthly Notices of the Royal Astronomical Society
Ansarinejad B
(2023)
VST ATLAS galaxy cluster catalogue I: cluster detection and mass calibration
in Monthly Notices of the Royal Astronomical Society
Muxlow T
(2020)
The e-MERGE Survey (e-MERLIN Galaxy Evolution Survey): overview and survey description
in Monthly Notices of the Royal Astronomical Society
Zarrouk P
(2022)
Preliminary clustering properties of the DESI BGS bright targets using DR9 Legacy Imaging Surveys
in Monthly Notices of the Royal Astronomical Society
Sharma M
(2019)
The I?ea model of feedback-regulated galaxy formation
in Monthly Notices of the Royal Astronomical Society
Smith R
(2021)
A fully-spectroscopic triple-source-plane lens: the Jackpot completed
in Monthly Notices of the Royal Astronomical Society
Lagattuta D
(2023)
RXJ0437+00: constraining dark matter with exotic gravitational lenses
in Monthly Notices of the Royal Astronomical Society
Deason A
(2023)
Unravelling the mass spectrum of destroyed dwarf galaxies with the metallicity distribution function
in Monthly Notices of the Royal Astronomical Society
Huško F
(2022)
Spin-driven jet feedback in idealized simulations of galaxy groups and clusters
in Monthly Notices of the Royal Astronomical Society
Chan T
(2024)
The impact and response of mini-haloes and the interhalo medium on cosmic reionization
in Monthly Notices of the Royal Astronomical Society
Laidlaw D
(2019)
Automated wind velocity profiling from adaptive optics telemetry
in Monthly Notices of the Royal Astronomical Society
Kugel R
(2023)
FLAMINGO: calibrating large cosmological hydrodynamical simulations with machine learning
in Monthly Notices of the Royal Astronomical Society
Acharyya A
(2021)
Locating the gamma-ray emission region in the brightest Fermi -LAT flat-spectrum radio quasars
in Monthly Notices of the Royal Astronomical Society
Muxlow T
(2020)
The e-MERGE Survey (e-MERLIN Galaxy Evolution Survey): overview and survey description
in Monthly Notices of the Royal Astronomical Society
Dalla Vecchia C
(2020)
Constraining the inner density slope of massive galaxy clusters
in Monthly Notices of the Royal Astronomical Society
Fossati M
(2021)
MUSE analysis of gas around galaxies (MAGG) - III. The gas and galaxy environment of z = 3-4.5 quasars
in Monthly Notices of the Royal Astronomical Society
Walton D
(2022)
A multimission catalogue of ultraluminous X-ray source candidates
in Monthly Notices of the Royal Astronomical Society
Amorisco N
(2022)
Halo concentration strengthens dark matter constraints in galaxy-galaxy strong lensing analyses
in Monthly Notices of the Royal Astronomical Society
Gonzalez-Perez V
(2020)
Multiwavelength consensus of large-scale linear bias
in Monthly Notices of the Royal Astronomical Society
Simpson C
(2020)
The milky way total mass profile as inferred from Gaia DR2
in Monthly Notices of the Royal Astronomical Society
Alston W
(2021)
Quasi-periodic dipping in the ultraluminous X-ray source, NGC 247 ULX-1
in Monthly Notices of the Royal Astronomical Society
Hernández-Aguayo C
(2021)
Building a digital twin of a luminous red galaxy spectroscopic survey: galaxy properties and clustering covariance
in Monthly Notices of the Royal Astronomical Society
Jin C
(2023)
The extreme super-eddington NLS1 RX J0134.2-4258 - II. A weak-line Seyfert linking to the weak-line quasar
in Monthly Notices of the Royal Astronomical Society
Eltvedt A
(2023)
The VST ATLAS quasar survey I: Catalogue of photometrically selected quasar candidates
in Monthly Notices of the Royal Astronomical Society
Cochrane R
(2021)
Resolving a dusty, star-forming SHiZELS galaxy at z = 2.2 with HST , ALMA, and SINFONI on kiloparsec scales
in Monthly Notices of the Royal Astronomical Society
Ferland G
(2020)
State-of-the-art AGN SEDs for photoionization models: BLR predictions confront the observations
in Monthly Notices of the Royal Astronomical Society
Macfarlane C
(2021)
The radio loudness of SDSS quasars from the LOFAR Two-metre Sky Survey: ubiquitous jet activity and constraints on star formation
in Monthly Notices of the Royal Astronomical Society
Shanks T
(2021)
The nature of sub-millimetre galaxies I: a comparison of AGN and star-forming galaxy SED fits
in Monthly Notices of the Royal Astronomical Society
Nomura M
(2020)
Line-driven disc wind in near-Eddington active galactic nuclei: decrease of mass accretion rate due to powerful outflow
in Monthly Notices of the Royal Astronomical Society
Jarvis M
(2021)
The quasar feedback survey: discovering hidden Radio-AGN and their connection to the host galaxy ionized gas
in Monthly Notices of the Royal Astronomical Society
Gonzalez-Perez V
(2020)
Do model emission line galaxies live in filaments at z ~ 1?
in Monthly Notices of the Royal Astronomical Society
He Q
(2023)
Testing strong lensing subhalo detection with a cosmological simulation
in Monthly Notices of the Royal Astronomical Society
Kawamura T
(2023)
The origin of long soft lags and the nature of the hard-intermediate state in black hole binaries
in Monthly Notices of the Royal Astronomical Society
Delhaize J
(2021)
MIGHTEE: are giant radio galaxies more common than we thought?
in Monthly Notices of the Royal Astronomical Society
Li Y
(2022)
Non-linear reconstruction of features in the primordial power spectrum from large-scale structure
in Monthly Notices of the Royal Astronomical Society
Anshul P
(2021)
Pair lines of sight observations of multiphase gas bearing O vi in a galaxy environment
in Monthly Notices of the Royal Astronomical Society
Description | Data Intensive Science Translation Fellow |
Amount | £276,889 (GBP) |
Funding ID | ST/R005516/1 |
Organisation | Science and Technologies Facilities Council (STFC) |
Sector | Public |
Country | United Kingdom |
Start | 07/2018 |
End | 06/2021 |
Description | Dirac-3 Operations 2019-2022- Durham |
Amount | £2,232,863 (GBP) |
Funding ID | ST/S003908/1 |
Organisation | Science and Technologies Facilities Council (STFC) |
Sector | Public |
Country | United Kingdom |
Start | 10/2019 |
End | 03/2020 |
Description | Dirac-3 Operations 2019-2022- Durham |
Amount | £1,748,945 (GBP) |
Funding ID | ST/V002376/1 |
Organisation | Science and Technologies Facilities Council (STFC) |
Sector | Public |
Country | United Kingdom |
Start | 10/2019 |
End | 03/2023 |
Description | Durham Astronomy Consolidated Grant 2017-2020 |
Amount | £5,911,198 (GBP) |
Funding ID | ST/P000541/1 |
Organisation | Science and Technologies Facilities Council (STFC) |
Sector | Public |
Country | United Kingdom |
Start | 04/2017 |
End | 03/2021 |
Description | STFC Durham Physics 2017 DTP |
Amount | £735,070 (GBP) |
Funding ID | ST/R504725/1 |
Organisation | Science and Technologies Facilities Council (STFC) |
Sector | Public |
Country | United Kingdom |
Start | 09/2017 |
End | 09/2021 |
Description | Using Cosmic Beasts to Uncover the Nature of Dark Matter |
Amount | £743,842 (GBP) |
Funding ID | MR/S017216/1 |
Organisation | Medical Research Council (MRC) |
Sector | Public |
Country | United Kingdom |
Start | 05/2019 |
End | 04/2023 |
Description | Your Place in the Universe |
Amount | £14,484 (GBP) |
Funding ID | ST/T00567X/1 |
Organisation | Science and Technologies Facilities Council (STFC) |
Sector | Public |
Country | United Kingdom |
Start | 08/2020 |
End | 03/2022 |
Description | Zooming in on feedback in active galaxies: the first high-resolution radio survey |
Amount | £992,150 (GBP) |
Funding ID | MR/T042842/1 |
Organisation | Medical Research Council (MRC) |
Sector | Public |
Country | United Kingdom |
Start | 10/2020 |
End | 09/2024 |
Description | LOFAR radio telescope |
Organisation | LOFAR |
Country | Netherlands |
Sector | Academic/University |
PI Contribution | Development of the processing and reduction of international long-baseline array data |
Collaborator Contribution | Priority access to the LOFAR radio data |
Impact | Publications on the long-baseline LOFAR results will be coming out very soon |
Start Year | 2019 |
Description | SKA radio telescope |
Organisation | SKA Square Kilometre Array |
Country | United Kingdom |
Sector | Charity/Non Profit |
PI Contribution | Scientific and technical development through membership of the SKA science committee and member of very long baseline interferometry and extragalactic continuum working groups. |
Collaborator Contribution | Scientific planning and development. |
Impact | none |
Start Year | 2019 |
Description | Astronomical society talks (~5/year) |
Form Of Engagement Activity | A talk or presentation |
Part Of Official Scheme? | No |
Geographic Reach | Regional |
Primary Audience | Public/other audiences |
Results and Impact | Giving presentations on specialist topics to astronomical societies: typically about 5/year. |
Year(s) Of Engagement Activity | 2017,2018,2019,2020,2021,2022 |
Description | Celebrate Science Festival |
Form Of Engagement Activity | Participation in an activity, workshop or similar |
Part Of Official Scheme? | No |
Geographic Reach | Regional |
Primary Audience | Public/other audiences |
Results and Impact | Celebrate Science is an annual Durham University science festival. It runs for approximately 3 days and attracts about 7000 visitors, many of them school children and their parents: it is scheduled for a half-term week. Each year ~30 members of the astronomy group participate to the Celebrate Science festival. They engage with visitors through exhibits including many created in the astronomy group such as our "Galaxy Maker" and "Gravitational Lens" simulators. Unfortunately, Celebrate Science was cancelled in 2020 due to the covid pandemic and was on line in 2021. |
Year(s) Of Engagement Activity | 2017,2018,2019,2022 |
URL | https://www.dur.ac.uk/celebrate.science/ |
Description | General public talks including Pint of Science |
Form Of Engagement Activity | A talk or presentation |
Part Of Official Scheme? | No |
Geographic Reach | Regional |
Primary Audience | Public/other audiences |
Results and Impact | Presenting and discussing ideas in astronomy and cosmology to the general public including the popular "Pint of Science" series of talks organised in a local pubs. Typically about 10 talks/year. |
Year(s) Of Engagement Activity | 2017,2018,2019,2020,2021,2022 |
Description | Royal Society Summer Science Exhibition 2020 |
Form Of Engagement Activity | Participation in an activity, workshop or similar |
Part Of Official Scheme? | No |
Geographic Reach | National |
Primary Audience | Public/other audiences |
Results and Impact | The Summer Science Exhibition is run by the Royal Society and is held in London. Over 14,000 members of the public including 2000 school children visit the Summer Science Exhibition each year. Many more are engaged through media coverage on TV and online. Exhibiting at the Royal Society not only engages the school children and the general public in STEM subjects, it also has the potential to influence policy makers and to engage potential funders. We estimate we had direct contact with over 3000 visitors for our astronomy and cosmology exhibits. |
Year(s) Of Engagement Activity | 2020,2022 |
Description | School visits to enthuse students about STEM subjects (~10/year) |
Form Of Engagement Activity | A talk or presentation |
Part Of Official Scheme? | No |
Geographic Reach | Regional |
Primary Audience | Schools |
Results and Impact | School visits to discuss astronomy to enthuse them in STEM-related subjects. Typically ~10 visits per year. |
Year(s) Of Engagement Activity | 2017,2018,2019,2020,2021,2022 |