Astrophysics Research at the University of Leicester
Lead Research Organisation:
University of Leicester
Department Name: Physics and Astronomy
Abstract
We will deliver world-class research programmes in astrophysics through the exploitation of data from space missions and ground based telescopes, as well as the development of new theories and the numerical simulation of processes in these areas. We will also develop new instrumental techniques and detectors for future missions and telescopes. The research programme is based mainly around two research groups, with some participation by three others. These groups conduct their own research projects but also have a strong ethos of collaboration on topics of mutual interest.
Our research seeks to understand basic processes in our own and other galaxies, addressing questions of great interest to the wider public. We will search for new planets orbiting nearby stars which may mimic the planets that are present in our own solar system or possibly be very different, such as hot Neptunes, or Super Earths.
We will investigate some of the most extreme environments in our Universe by high energy astrophysics research focusing on extreme phenomena ranging from Galactic black hole binaries, through to active galactic nuclei and gamma-ray bursts. These studies will include the feedback processes that link black holes to the evolution of their host galaxies.
We will maintain and enhance a programme in stellar astronomy with emphasis on the astrophysics of white dwarf stars. We will be using high performance computers to simulate these systems theoretically. This in turn will help our observations and vice versa. Through these simulations we will build theories and models of how these extreme systems behave. We will use these simulations to try to understand the `dark' matter which constitutes much of the material
content of the Universe. We will use laboratory experimentation to develop new ways to observe these phenomena, building new instruments for the next generation of space missions.
This work also offers spin-off activities which often drive progress in areas far removed from astrophysics. Our department has an active programme of engagement with the wider community, particularly school age children, who are thrilled to hear about research in the Department. We will maintain a strong commitment to knowledge transfer for academic beneficiaries.
Our research seeks to understand basic processes in our own and other galaxies, addressing questions of great interest to the wider public. We will search for new planets orbiting nearby stars which may mimic the planets that are present in our own solar system or possibly be very different, such as hot Neptunes, or Super Earths.
We will investigate some of the most extreme environments in our Universe by high energy astrophysics research focusing on extreme phenomena ranging from Galactic black hole binaries, through to active galactic nuclei and gamma-ray bursts. These studies will include the feedback processes that link black holes to the evolution of their host galaxies.
We will maintain and enhance a programme in stellar astronomy with emphasis on the astrophysics of white dwarf stars. We will be using high performance computers to simulate these systems theoretically. This in turn will help our observations and vice versa. Through these simulations we will build theories and models of how these extreme systems behave. We will use these simulations to try to understand the `dark' matter which constitutes much of the material
content of the Universe. We will use laboratory experimentation to develop new ways to observe these phenomena, building new instruments for the next generation of space missions.
This work also offers spin-off activities which often drive progress in areas far removed from astrophysics. Our department has an active programme of engagement with the wider community, particularly school age children, who are thrilled to hear about research in the Department. We will maintain a strong commitment to knowledge transfer for academic beneficiaries.
Planned Impact
The applicants offer a diverse skill set that constitute a valuable resource to the private and public sectors. We have extensive experience and expertise in e.g. data analysis and handling, spacecraft and mission management, algorithm design, software engineering and high performance computing. Exploitation of this expertise is supported at all levels within the University. The Department of Physics and Astronomy is committed to
promoting and maximising the impact of our research. The College of Science and Engineering plays a leading role in the Enterprise Agenda for the University and offers dedicated enterprise officers and impact enhancing resources. Further support is provided by the University's Enterprise and Business Development Office, which works with academics and external stakeholders to create maximum impact in the local, provide national, and international community. This structure (i) delivers enterprising impact through the alignment of our research with major global and industrial challenges, (ii) identifies and addresses the opportunities to play a positive role in the economic development of our region and the UK, (iii) utilises research and related activities to develop skills and capability within a broad spectrum of the public and private sectors, (iv) provides expert advice and
guidance to industry and policy makers, (v) ensures that its intellectual property is effectively transferred and disseminated, and (vi) contributes to the wider cultural benefit of society through an enterprising and engaging outreach programme.
The long term impact strategy has four elements:
(1) to support and develop the skills and experience of the applicants;
(2) to ensure that links with public and private sector industries are developed, cultivated and maximised;
(3) to disseminate knowledge, skills and expterise to the benefit of the local, national and international business and civic communities;
(4) to sustain and develop our successful outreach programme with particular emphasis on enhancing our efforts to develop valid outcome measures.
promoting and maximising the impact of our research. The College of Science and Engineering plays a leading role in the Enterprise Agenda for the University and offers dedicated enterprise officers and impact enhancing resources. Further support is provided by the University's Enterprise and Business Development Office, which works with academics and external stakeholders to create maximum impact in the local, provide national, and international community. This structure (i) delivers enterprising impact through the alignment of our research with major global and industrial challenges, (ii) identifies and addresses the opportunities to play a positive role in the economic development of our region and the UK, (iii) utilises research and related activities to develop skills and capability within a broad spectrum of the public and private sectors, (iv) provides expert advice and
guidance to industry and policy makers, (v) ensures that its intellectual property is effectively transferred and disseminated, and (vi) contributes to the wider cultural benefit of society through an enterprising and engaging outreach programme.
The long term impact strategy has four elements:
(1) to support and develop the skills and experience of the applicants;
(2) to ensure that links with public and private sector industries are developed, cultivated and maximised;
(3) to disseminate knowledge, skills and expterise to the benefit of the local, national and international business and civic communities;
(4) to sustain and develop our successful outreach programme with particular emphasis on enhancing our efforts to develop valid outcome measures.
Organisations
Publications
Bainbridge Matthew B.
(2017)
Probing the Gravitational Dependence of the Fine-Structure Constant from Observations of White Dwarf Stars
in ArXiv e-prints
Mink S
(2017)
Electromagnetic Signals Following Stellar-mass Black Hole Mergers
in The Astrophysical Journal Letters
Amaral-Rogers A
(2017)
The pulse luminosity function of Swift gamma-ray bursts
in Monthly Notices of the Royal Astronomical Society
Gualandris A
(2017)
Collisionless loss-cone refilling: there is no final parsec problem
in Monthly Notices of the Royal Astronomical Society
Covino S
(2017)
The unpolarized macronova associated with the gravitational wave event GW 170817
in Nature Astronomy
Pei L
(2017)
Space Telescope and Optical Reverberation Mapping Project. V. Optical Spectroscopic Campaign and Emission-line Analysis for NGC 5548
in The Astrophysical Journal
Dehnen W
(2017)
Towards time symmetric N-body integration
in Monthly Notices of the Royal Astronomical Society
Abbott B
(2017)
Multi-messenger Observations of a Binary Neutron Star Merger
in The Astrophysical Journal
LIGO Scientific Collaboration And The Virgo Collaboration
(2017)
A gravitational-wave standard siren measurement of the Hubble constant.
in Nature
Alexander K
(2017)
A Reverse Shock and Unusual Radio Properties in GRB 160625B
in The Astrophysical Journal
Stratta G.
(2017)
THESEUS: a key space mission for Multi-Messenger Astrophysics
in ArXiv e-prints
Evans PA
(2017)
Swift and NuSTAR observations of GW170817: Detection of a blue kilonova.
in Science (New York, N.Y.)
Bayliss D
(2017)
NGTS-1b: A hot Jupiter transiting an M-dwarf
Heintz K
(2017)
Steep extinction towards GRB 140506A reconciled from host galaxy observations: Evidence that steep reddening laws are local
in Astronomy & Astrophysics
Tanvir N
(2017)
The Emergence of a Lanthanide-rich Kilonova Following the Merger of Two Neutron Stars
in The Astrophysical Journal
Christensen L
(2017)
Solving the conundrum of intervening strong Mg II absorbers towards gamma-ray bursts and quasars
in Astronomy & Astrophysics
Nayakshin S
(2017)
Dawes Review 7: The Tidal Downsizing Hypothesis of Planet Formation
in Publications of the Astronomical Society of Australia
Gilbertson Christian
(2017)
A Study of the Gamma-Ray Burst Fundamental Plane
in American Astronomical Society Meeting Abstracts #229
Edelson R.
(2017)
VizieR Online Data Catalog: X-ray/UV Swift monitoring of NGC 4151 (Edelson+, 2017)
in VizieR Online Data Catalog
McCormac J
(2017)
The Next Generation Transit Survey-Prototyping Phase
in Publications of the Astronomical Society of the Pacific
Stelzer B
(2017)
X-ray orbital modulation of a white dwarf accreting from an L dwarf The system SDSS J121209.31+013627.7
in Astronomy & Astrophysics
Braker I. P.
(2017)
Photometric Variability and Spectroscopic Characterisation of White Dwarfs in Kepler 2 Fields
in 20th European White Dwarf Workshop
Lyman J
(2017)
The host galaxies and explosion sites of long-duration gamma ray bursts: Hubble Space Telescope near-infrared imaging
in Monthly Notices of the Royal Astronomical Society
Diakogiannis F
(2017)
A novel JEAnS analysis of the Fornax dwarf using evolutionary algorithms: mass follows light with signs of an off-centre merger
in Monthly Notices of the Royal Astronomical Society
Gillon M
(2017)
Seven temperate terrestrial planets around the nearby ultracool dwarf star TRAPPIST-1.
in Nature
Dehnen W
(2017)
Towards time symmetric N-body integration
Cherenkov Telescope Array Consortium The
(2017)
Science with the Cherenkov Telescope Array
in arXiv e-prints
Perley D
(2017)
Late-time VLA reobservations rule out ULIRG-like host galaxies for most pre- Swift long-duration gamma-ray bursts
in Monthly Notices of the Royal Astronomical Society
Kacharov N
(2017)
Prolate rotation and metallicity gradient in the transforming dwarf galaxy Phoenix
in Monthly Notices of the Royal Astronomical Society
CTA Consortium The
(2017)
Prospects for CTA observations of the young SNR RX J1713.7-3946
in ArXiv e-prints
Starkey D
(2017)
SPACE TELESCOPE AND OPTICAL REVERBERATION MAPPING PROJECT.VI. REVERBERATING DISK MODELS FOR NGC 5548
in The Astrophysical Journal
Brown G
(2017)
Late-time observations of the relativistic tidal disruption flare candidate Swift J1112.2-8238
in Monthly Notices of the Royal Astronomical Society
Nayakshin Sergei
(2016)
A desert of gas giant planets beyond tens of au
in arXiv e-prints
Zubovas K
(2016)
The small observed scale of AGN-driven outflows, and inside-out disc quenching
in Monthly Notices of the Royal Astronomical Society
Evans P
(2016)
Swift follow-up of gravitational wave triggers: results from the first aLIGO run and optimization for the future
in Monthly Notices of the Royal Astronomical Society
Perley D
(2016)
THE SWIFT GAMMA-RAY BURST HOST GALAXY LEGACY SURVEY. I. SAMPLE SELECTION AND REDSHIFT DISTRIBUTION
in The Astrophysical Journal
CTA Consortium The
(2016)
Contributions of the Cherenkov Telescope Array (CTA) to the 6th International Symposium on High-Energy Gamma-Ray Astronomy (Gamma 2016)
in arXiv e-prints
Middleton M
(2016)
Geometrical beaming of stellar mass ULXs
in Monthly Notices of the Royal Astronomical Society: Letters
Cenko S
(2016)
AN ULTRAVIOLET SPECTRUM OF THE TIDAL DISRUPTION FLARE ASASSN-14li
in The Astrophysical Journal Letters
Nixon C
(2016)
Astrophysical Black Holes
Angus C
(2016)
A Hubble Space Telescope survey of the host galaxies of Superluminous Supernovae
in Monthly Notices of the Royal Astronomical Society
Pounds K
(2016)
Imprints of a high-velocity wind on the soft X-ray spectrum of PG1211+143
in Monthly Notices of the Royal Astronomical Society
MacLeod C
(2016)
A systematic search for changing-look quasars in SDSS
in Monthly Notices of the Royal Astronomical Society
Abbott B
(2016)
SUPPLEMENT: "LOCALIZATION AND BROADBAND FOLLOW-UP OF THE GRAVITATIONAL-WAVE TRANSIENT GW150914" (2016, ApJL, 826, L13)
in The Astrophysical Journal Supplement Series
Evans P
(2016)
Swift follow-up of the Gravitational Wave source GW150914
in Monthly Notices of the Royal Astronomical Society: Letters
King A
(2016)
ULXs: Neutron stars versus black holes
in Monthly Notices of the Royal Astronomical Society: Letters
Fausnaugh M
(2016)
SPACE TELESCOPE AND OPTICAL REVERBERATION MAPPING PROJECT. III. OPTICAL CONTINUUM EMISSION AND BROADBAND TIME DELAYS IN NGC 5548
in The Astrophysical Journal
Abbott B
(2016)
LOCALIZATION AND BROADBAND FOLLOW-UP OF THE GRAVITATIONAL-WAVE TRANSIENT GW150914
in The Astrophysical Journal Letters
Reeves J
(2016)
DISCOVERY OF BROAD SOFT X-RAY ABSORPTION LINES FROM THE QUASAR WIND IN PDS 456
in The Astrophysical Journal
Williams JO
(2016)
Towards a Graphene-Based Low Intensity Photon Counting Photodetector.
in Sensors (Basel, Switzerland)
Description | Further progress in a variety of fields of astrophysics. |
Exploitation Route | Further research in various areas of astrophysics. |
Sectors | Education |
Description | Royal Society Research Grant |
Amount | £13,055 (GBP) |
Funding ID | RG170230 |
Organisation | The Royal Society |
Sector | Charity/Non Profit |
Country | United Kingdom |
Start | 10/2017 |
End | 10/2018 |
Description | Creativity and Curiosity - Art meets astronomy |
Form Of Engagement Activity | A formal working group, expert panel or dialogue |
Part Of Official Scheme? | No |
Geographic Reach | International |
Primary Audience | Public/other audiences |
Results and Impact | The project started as a discussion between artists and astronomers to stimulate new art and engage with new audiences. Events have included exhibitions of the artworks and associated discussion events across the county and abroad. |
Year(s) Of Engagement Activity | 2017 |
URL | https://www.creativityandcuriosity.com |
Description | US NSF announcement of discovery of first gravitational wave source with electromagnetic counterpart - Oct 2017 |
Form Of Engagement Activity | A press release, press conference or response to a media enquiry/interview |
Part Of Official Scheme? | No |
Geographic Reach | International |
Primary Audience | Media (as a channel to the public) |
Results and Impact | US National Science Foundation press release. |
Year(s) Of Engagement Activity | 2017 |
URL | https://www.ligo.caltech.edu/page/press-release-gw170817 |
Description | Various school visits, astronomical society lectures |
Form Of Engagement Activity | A talk or presentation |
Part Of Official Scheme? | No |
Geographic Reach | National |
Primary Audience | Schools |
Results and Impact | Many presentations, 100s of students, excellent questions and discussion. Audience figures are totals for activities during each year. Improvements in interest in applying for science degrees |
Year(s) Of Engagement Activity | 2006,2007,2008,2009,2010,2011,2012,2013,2014,2015,2016,2017,2018,2019,2020,2021 |