Lancaster University Observational Astrophysics 2021-2024

Lead Research Organisation: Lancaster University
Department Name: Physics

Abstract

The work proposed here tackles some of the most important open questions in astrophysics, broadly centred on understanding the formation and evolution of galaxies and the properties of the Universe itself. It is closely linked with the STFC Science Roadmap challenges pertaining to the roles and nature of dark matter and dark energy, the formation of the first stars and galaxies in the Universe and the still unsolved key question of how galaxies evolve. In order to address such fundamental questions, we use complementary approaches. We will use new telescopes that are now coming on line to find and study Type Ia supernovae. These will be used as distance indicators across time to study the evolution of the universe itself and to better understand what is causing the expansion of the universe to accelerate. New telescope data will also be used to discover twinkling supermassive black holes hidden in the centres of thousands of galaxies. We will compare these black holes with data from their much more luminous siblings - quasars - which have grown rapidly in galaxies similar to our own. By studying the full population we will advance our understanding of how these black holes grow and influence the galaxies which host them. We will unveil the physical mechanisms behind the production and escape of high energy photons through galactic labyrinths, near and far, and unveil which sources caused the last major phase transition in the Universe. With artificial intelligence techniques, we will discover thousands of new clusters of galaxies, which will be used to understand how galaxies evolve in dense environments and the nature of dark matter itself. We will find new types of galaxies and use them to understand what controls the growth of galaxies in the distant Universe.

Our research involves making state-of-the-art observations using the world's most powerful and advanced telescopes such as the Hubble Space Telescope and facilities run by the European Southern Observatory including ALMA (the Atacama Large Millimeter Array) and the VLT (Very Large Telescope). We will also begin to use new facilities including the 4-m Multi-Object Spectroscopic Telescope (4MOST), the Rubin Observatory's Legacy Survey of Space and Time (LSST), and in space the James Webb Space Telescope (JWST) and the European Space Agency's Euclid mission.

We will bring our state-of-the art research to a wide audience by creating inspiring new shows for our portable inflatable planetarium, the LUniverse. These new shows will explain our group's current research projects to a general audience and will be shown at outreach events and in schools around the North-West.

Planned Impact

The beneficiaries of this research are primarily academics interested in the important areas of STFC Science Challenges as described in the STFC Science Roadmap, particularly understanding how galaxies like our own Milky Way formed and evolved, improving the precision of SN Ia measurements to better understand the roles of dark matter and dark energy, understanding the distribution of dark matter, understanding the role of supermassive black holes in galaxy evolution, and illuminating physical processes in the early universe. The impact of this research will be disseminated in the form of open-access publications in peer-reviewed journals, and talks at national and international conferences. The methods and techniques developed are also expected to generate significant wider interest in disciplines such as particle physics, medical imaging and earth observation, and there is potential for commercial impact for the computer vision and time-series analysis techniques described in the projects.

The research also has important economic and societal impacts. Research in astronomy addresses some of the most fundamental questions about our origins and the Universe around us. The excitement it generates inspires young people to enter science and research. All members of the Astrophysics group give regular public lectures and also engage the public in a variety of ways, including media interviews with wide reach and activities with more direct 2-way engagement such as citizen science projects and participatory events at music festivals where underserved audiences are located. During the grant period these activities will directly incorporate the research results of this project. Engagement with authentic cutting-edge research, including citizen science, is effective at inspiring the public and can lead to independent science learning.

The group is also involved in the Physics department's schools outreach program, working with the department's Schools outreach Officer. The Department of Physics offers day-long "Cosmology and Astrophysics Masterclasses" and residential work experience and courses throughout the year. The new Observational Astrophysics group at Lancaster is augmenting the provision of such Masterclasses and is also contributing significantly to the department's outreach work via its planetarium programme, LUniverse. The planetarium is expected to reach tens of thousands of members of the public via direct, immersive, participatory engagement during the grant period. Its audience includes members of the public of all ages, with a particular focus on schools engagement and engagement with underserved audiences. This grant will enable LUniverse to incorporate the proposed projects' research directly into planetarium shows, significantly increasing the direct public impact of the research in this proposal.

Publications

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Carrick J (2021) Optimizing a magnitude-limited spectroscopic training sample for photometric classification of supernovae in Monthly Notices of the Royal Astronomical Society

 
Description 4MOST Consortium 
Organisation Leibniz Association
Department Leibniz Institute for Astrophysics Potsdam
Country Germany 
Sector Academic/University 
PI Contribution The consortium consists of 17 full members and 9 minor participants, some contributing to the hardware development, others to the software development, and almost all to the science case development. My collaboration (TiDES) has contributed financially towards the construction of the 4MOST instrument. We also contribute scientific planning effort.
Collaborator Contribution Other institutions contribute financially as well as technically in the design and construction of the instrument. Other institutions also contribute to the scientific planning.
Impact publications listed in appropriate grant report.
Start Year 2015
 
Description Euclid Consortium 
Organisation Autonomous University of Barcelona (UAB)
Country Spain 
Sector Academic/University 
PI Contribution Euclid is a planned ESA mission that will be launched in 2022 and will survey the sky with the main goals of measuring the cosmological parameters of the universe. From the ESA web site: "Nearly 1000 scientists from 100 institutes form the Euclid Consortium building the instruments and participating in the scientific harvest of the mission. The Euclid Consortium comprises scientists from 13 European countries: Austria, Denmark, France, Finland, Germany, Italy, Netherlands, Norway, Spain, Switzerland, Portugal, Romania and the UK. It also includes a US NASA team of scientists." Prof. Hook and Prof. Miller are members of the Euclid consortium. Prof Hook is one of two UK representatives on the Euclid Consortium Board. She work on aspects of the survey design connected to discovery and study of astrophysical transients.
Collaborator Contribution The partners are involved in design of the mission and the survey, and planning the science program that it will carry out after launch. Some partners are involved in construction of instruments that will fly on the mission.
Impact There have been many publications from the Euclid consortium as a whole. There are also outreach activities connected to the mission.
Start Year 2010
 
Description Euclid Consortium 
Organisation National Aeronautics and Space Administration (NASA)
Department Jet Propulsion Laboratory
Country United States 
Sector Public 
PI Contribution Euclid is a planned ESA mission that will be launched in 2022 and will survey the sky with the main goals of measuring the cosmological parameters of the universe. From the ESA web site: "Nearly 1000 scientists from 100 institutes form the Euclid Consortium building the instruments and participating in the scientific harvest of the mission. The Euclid Consortium comprises scientists from 13 European countries: Austria, Denmark, France, Finland, Germany, Italy, Netherlands, Norway, Spain, Switzerland, Portugal, Romania and the UK. It also includes a US NASA team of scientists." Prof. Hook and Prof. Miller are members of the Euclid consortium. Prof Hook is one of two UK representatives on the Euclid Consortium Board. She work on aspects of the survey design connected to discovery and study of astrophysical transients.
Collaborator Contribution The partners are involved in design of the mission and the survey, and planning the science program that it will carry out after launch. Some partners are involved in construction of instruments that will fly on the mission.
Impact There have been many publications from the Euclid consortium as a whole. There are also outreach activities connected to the mission.
Start Year 2010
 
Description Euclid Consortium 
Organisation Paris Institute of Astrophysics
Country France 
Sector Academic/University 
PI Contribution Euclid is a planned ESA mission that will be launched in 2022 and will survey the sky with the main goals of measuring the cosmological parameters of the universe. From the ESA web site: "Nearly 1000 scientists from 100 institutes form the Euclid Consortium building the instruments and participating in the scientific harvest of the mission. The Euclid Consortium comprises scientists from 13 European countries: Austria, Denmark, France, Finland, Germany, Italy, Netherlands, Norway, Spain, Switzerland, Portugal, Romania and the UK. It also includes a US NASA team of scientists." Prof. Hook and Prof. Miller are members of the Euclid consortium. Prof Hook is one of two UK representatives on the Euclid Consortium Board. She work on aspects of the survey design connected to discovery and study of astrophysical transients.
Collaborator Contribution The partners are involved in design of the mission and the survey, and planning the science program that it will carry out after launch. Some partners are involved in construction of instruments that will fly on the mission.
Impact There have been many publications from the Euclid consortium as a whole. There are also outreach activities connected to the mission.
Start Year 2010
 
Description Euclid UK 
Organisation Durham University
Country United Kingdom 
Sector Academic/University 
PI Contribution Planning and developing algorithms for "Time Domain" studies and (in the implementation phase) Weak Lensing within the Euclid Ground Segment
Collaborator Contribution Planning and developing algorithms for other aspects of the Euclid ground segment including weak lensing, galaxy clustering and galaxy photometric redshifts
Impact Internal reports
Start Year 2010
 
Description Euclid UK 
Organisation Open University
Country United Kingdom 
Sector Academic/University 
PI Contribution Planning and developing algorithms for "Time Domain" studies and (in the implementation phase) Weak Lensing within the Euclid Ground Segment
Collaborator Contribution Planning and developing algorithms for other aspects of the Euclid ground segment including weak lensing, galaxy clustering and galaxy photometric redshifts
Impact Internal reports
Start Year 2010
 
Description Euclid UK 
Organisation University College London
Department Department of Space and Climate Physics (MSSL)
Country United Kingdom 
Sector Academic/University 
PI Contribution Planning and developing algorithms for "Time Domain" studies and (in the implementation phase) Weak Lensing within the Euclid Ground Segment
Collaborator Contribution Planning and developing algorithms for other aspects of the Euclid ground segment including weak lensing, galaxy clustering and galaxy photometric redshifts
Impact Internal reports
Start Year 2010
 
Description Euclid UK 
Organisation University of Edinburgh
Country United Kingdom 
Sector Academic/University 
PI Contribution Planning and developing algorithms for "Time Domain" studies and (in the implementation phase) Weak Lensing within the Euclid Ground Segment
Collaborator Contribution Planning and developing algorithms for other aspects of the Euclid ground segment including weak lensing, galaxy clustering and galaxy photometric redshifts
Impact Internal reports
Start Year 2010
 
Description Euclid UK 
Organisation University of Portsmouth
Department Institute of Cosmology and Gravitation (ICG)
Country United Kingdom 
Sector Academic/University 
PI Contribution Planning and developing algorithms for "Time Domain" studies and (in the implementation phase) Weak Lensing within the Euclid Ground Segment
Collaborator Contribution Planning and developing algorithms for other aspects of the Euclid ground segment including weak lensing, galaxy clustering and galaxy photometric redshifts
Impact Internal reports
Start Year 2010
 
Description LSST Dark Energy Science Collaboration 
Organisation University of Chicago
Country United States 
Sector Academic/University 
PI Contribution Planning survey strategies for the future Large Synoptic Survey Telescope (LSST) surveys via simulations and calculations. Also developing follow-up strategies for LSST transients, for the purposes of Dark Energy science in particular. Testing transient classification software under various assumptions for training samples.
Collaborator Contribution Simulations of the LSST data, planning of survey strategies, software for classification of transients. Partners have also help review papers prior to submission to journals.
Impact Papers (non-refereed) that have resulted include: Enhancing LSST Science with Euclid Synergy (2019), a white paper by the Tri-Agency Working Group (TAG), P. Capak et al. The LSST Dark Energy Science Collaboration (DESC) Science Requirements Document (2018), The LSST Dark Energy Science Collaboration; Mandelbaum, R. et al. Optimizing the LSST Observing Strategy for Dark Energy Science: DESC Recommendations for the Wide-Fast-Deep Survey (2018) Lochner M. et al Optimizing the LSST Observing Strategy for Dark Energy Science: DESC Recommendations for the Deep Drilling Fields and other Special Programs (2018), Scolnic, D. et al
Start Year 2015
 
Description LSST Dark Energy Science Collaboration 
Organisation University of Clermont Auvergne
Country France 
Sector Academic/University 
PI Contribution Planning survey strategies for the future Large Synoptic Survey Telescope (LSST) surveys via simulations and calculations. Also developing follow-up strategies for LSST transients, for the purposes of Dark Energy science in particular. Testing transient classification software under various assumptions for training samples.
Collaborator Contribution Simulations of the LSST data, planning of survey strategies, software for classification of transients. Partners have also help review papers prior to submission to journals.
Impact Papers (non-refereed) that have resulted include: Enhancing LSST Science with Euclid Synergy (2019), a white paper by the Tri-Agency Working Group (TAG), P. Capak et al. The LSST Dark Energy Science Collaboration (DESC) Science Requirements Document (2018), The LSST Dark Energy Science Collaboration; Mandelbaum, R. et al. Optimizing the LSST Observing Strategy for Dark Energy Science: DESC Recommendations for the Wide-Fast-Deep Survey (2018) Lochner M. et al Optimizing the LSST Observing Strategy for Dark Energy Science: DESC Recommendations for the Deep Drilling Fields and other Special Programs (2018), Scolnic, D. et al
Start Year 2015
 
Description LSST Dark Energy Science Collaboration 
Organisation University of Illinois at Urbana-Champaign
Country United States 
Sector Academic/University 
PI Contribution Planning survey strategies for the future Large Synoptic Survey Telescope (LSST) surveys via simulations and calculations. Also developing follow-up strategies for LSST transients, for the purposes of Dark Energy science in particular. Testing transient classification software under various assumptions for training samples.
Collaborator Contribution Simulations of the LSST data, planning of survey strategies, software for classification of transients. Partners have also help review papers prior to submission to journals.
Impact Papers (non-refereed) that have resulted include: Enhancing LSST Science with Euclid Synergy (2019), a white paper by the Tri-Agency Working Group (TAG), P. Capak et al. The LSST Dark Energy Science Collaboration (DESC) Science Requirements Document (2018), The LSST Dark Energy Science Collaboration; Mandelbaum, R. et al. Optimizing the LSST Observing Strategy for Dark Energy Science: DESC Recommendations for the Wide-Fast-Deep Survey (2018) Lochner M. et al Optimizing the LSST Observing Strategy for Dark Energy Science: DESC Recommendations for the Deep Drilling Fields and other Special Programs (2018), Scolnic, D. et al
Start Year 2015
 
Description LSST Dark Energy Science Collaboration 
Organisation University of Toronto
Country Canada 
Sector Academic/University 
PI Contribution Planning survey strategies for the future Large Synoptic Survey Telescope (LSST) surveys via simulations and calculations. Also developing follow-up strategies for LSST transients, for the purposes of Dark Energy science in particular. Testing transient classification software under various assumptions for training samples.
Collaborator Contribution Simulations of the LSST data, planning of survey strategies, software for classification of transients. Partners have also help review papers prior to submission to journals.
Impact Papers (non-refereed) that have resulted include: Enhancing LSST Science with Euclid Synergy (2019), a white paper by the Tri-Agency Working Group (TAG), P. Capak et al. The LSST Dark Energy Science Collaboration (DESC) Science Requirements Document (2018), The LSST Dark Energy Science Collaboration; Mandelbaum, R. et al. Optimizing the LSST Observing Strategy for Dark Energy Science: DESC Recommendations for the Wide-Fast-Deep Survey (2018) Lochner M. et al Optimizing the LSST Observing Strategy for Dark Energy Science: DESC Recommendations for the Deep Drilling Fields and other Special Programs (2018), Scolnic, D. et al
Start Year 2015
 
Description Manchester Lit and Phil Society 
Form Of Engagement Activity A talk or presentation
Part Of Official Scheme? No
Geographic Reach Regional
Primary Audience Public/other audiences
Results and Impact This was a talk to a joint audience of the Institute of Physics and the Manchester Literary and Philosophical Society (with a history dating back to 1781). The event took place during the Covid-19 pandemic and has held online. The subject of the talk was the discovery of the accelerating expansion of the universe and the quest to understand the nature of Dark Energy.
Year(s) Of Engagement Activity 2021