Astrophysics Research at Liverpool John Moores University: Newly Appointed Academic Staff
Lead Research Organisation:
Liverpool John Moores University
Department Name: Astrophysics Research Institute
Abstract
This grant will allow six new academic staff, recently employed in the Astrophysics Research Institute, to carry out their World-leading research as they settle into their new academic environment in Liverpool. The areas of interest of these new staff broadly align with the existing scientific strengths of the ARI, namely: the origin of stars; the chemical composition of galaxies; observational and theoretical studies of the Milky Way; large cosmological hydrodynamical simulations of galaxy clusters; theoretical studies to determine the physical properties of supernovae.
Under the heading of the origin of stars, we will investigate how the initial masses of stars forming in the Galaxy change with environment. Observations of the gas in giant star-forming regions will be used to determine key physical properties on scales close to the size of individual stars.
We will carry out a major spectroscopic survey of nearly 1 million stars in the disc and bulge of the Milky Way. This major legacy survey (APOGEE) and its successor (APOGEE-2), partly supported by the Sloan Foundation, will have major impact on questions such as: the chemical composition of the disc and bulge regions of the galaxy; the origin of globular clusters and whether there is evidence for the very first generation (population III) stars. We will also carry out cosmological hydrodynamic simulations of the Milky Way on supercomputers to provide well-matched and high resolution predictions of the merger history of the galaxy to compare with the observations from the forthcoming Gaia satellite mission, which will provide a 3D map of the Milky Way.
Our extragalactic chemical composition work focuses on a new technique, using Red Supergiant Stars, to measure the element abundances in nearby galaxies. By examining physical relationships, such as the correlation between a galaxy's central mass and metallicity, or the abundance gradients within galaxies, we will make important insights into the processes of galaxy formation and evolution.
On the largest scales we will carry out cosmological simulations of galaxy clusters, including all known feedback mechanisms, in order to provide representative samples of mock clusters. Simulation results will be incorporated into real observations from on-going cluster surveys at different wavelengths (including the XMM-Cluster Survey, in which the ARI is heavily involved) in order to make unbiased estimates of the cosmological parameters and physical conditions in the clusters.
We will investigate the outburst properties of supernovae using data from large on-going transient surveys and explore the relationship between the properties of the SN and its progenitor, as well as searching for new types of transients. In particular we will examine a large population of type SN Ia supernovae and study "extreme" events which violate normal behaviour in order to improve their use as cosmological distance indicators.
All of our research uses the most advanced ground-based telescopes, satellites and data analysis techniques to carry out observations, including telescope time on newly commissioned facilities such as ALMA and the KMOS multi-object spectrograph on the VLT, along with space missions such as Gaia. The new staff lead programmes at the international level, which are also technically demanding and feed into the design and operation of the next generation of telescopes and their instruments, such as the E-ELT (EAGLE/EVE), Liverpool Telescope and WHT (WEAVE).
Under the heading of the origin of stars, we will investigate how the initial masses of stars forming in the Galaxy change with environment. Observations of the gas in giant star-forming regions will be used to determine key physical properties on scales close to the size of individual stars.
We will carry out a major spectroscopic survey of nearly 1 million stars in the disc and bulge of the Milky Way. This major legacy survey (APOGEE) and its successor (APOGEE-2), partly supported by the Sloan Foundation, will have major impact on questions such as: the chemical composition of the disc and bulge regions of the galaxy; the origin of globular clusters and whether there is evidence for the very first generation (population III) stars. We will also carry out cosmological hydrodynamic simulations of the Milky Way on supercomputers to provide well-matched and high resolution predictions of the merger history of the galaxy to compare with the observations from the forthcoming Gaia satellite mission, which will provide a 3D map of the Milky Way.
Our extragalactic chemical composition work focuses on a new technique, using Red Supergiant Stars, to measure the element abundances in nearby galaxies. By examining physical relationships, such as the correlation between a galaxy's central mass and metallicity, or the abundance gradients within galaxies, we will make important insights into the processes of galaxy formation and evolution.
On the largest scales we will carry out cosmological simulations of galaxy clusters, including all known feedback mechanisms, in order to provide representative samples of mock clusters. Simulation results will be incorporated into real observations from on-going cluster surveys at different wavelengths (including the XMM-Cluster Survey, in which the ARI is heavily involved) in order to make unbiased estimates of the cosmological parameters and physical conditions in the clusters.
We will investigate the outburst properties of supernovae using data from large on-going transient surveys and explore the relationship between the properties of the SN and its progenitor, as well as searching for new types of transients. In particular we will examine a large population of type SN Ia supernovae and study "extreme" events which violate normal behaviour in order to improve their use as cosmological distance indicators.
All of our research uses the most advanced ground-based telescopes, satellites and data analysis techniques to carry out observations, including telescope time on newly commissioned facilities such as ALMA and the KMOS multi-object spectrograph on the VLT, along with space missions such as Gaia. The new staff lead programmes at the international level, which are also technically demanding and feed into the design and operation of the next generation of telescopes and their instruments, such as the E-ELT (EAGLE/EVE), Liverpool Telescope and WHT (WEAVE).
Planned Impact
The major form of impact arising from additional funds to our current Consolidated Grant, will come from existing activities described in more detail in the Pathways to Impact document. These will benefit schools, amateur astronomers and the general public.
At a University level, the Research Support Office have recently launched the LJMU Research Café - a series of informal, cross-cutting research seminars which will be held monthly in one of the University's Learning Resource Centres. At each event four researchers will present their research to a mixed audience from across the University in a series of short presentations. Sessions will not be themed as the intention is to support a varied programme enabling the audience to engage with the rich variety of research which takes place across the University and for presenters to disseminate their research to a broader audience.
In addition, through activities initiated within the ARI, there will be other more traditional forms of public engagement growing from our research. In particular we would anticipate a number of talks, panel discussions and question-and-answer sessions relating to our research. These will vary with respect to audience: schools (from primary upwards), amateur astronomy societies, lecture societies, WI etc. We will also showcase the new research at events organised by the ARI (such as the annual Merseyside Astronomy Day) and, where appropriate, at the Spaceport visitor centre.
In all cases the benefits will be twofold. Obviously, an exposure to current research can stimulate inquiry and interest in any audience. However, a less obvious, but perhaps more important benefit is to use that stimulation to promote an appreciation of science as a whole. This is particularly important for engagement with schools where astronomy has a vital role to play in promoting science and other STEM subjects as potential careers.
In order to facilitate this, younger and less experienced researchers (especially PDRAs and PhD students) are encouraged to present their research to a variety of audiences, with training and support provided by the experienced Outreach team within the ARI.
We will also work with non-science organisations to find ways in which the research can be used to enhance their own work. This sort of impact is difficult to predict in advance, as it is usually opportunistic, but past examples in the ARI have involved work with arts organisations and artists (including musicians, theatre companies, street theatre performers, sculptors, photographers and writers) and organisations that promote access to education (such as Aim Higher).
At a University level, the Research Support Office have recently launched the LJMU Research Café - a series of informal, cross-cutting research seminars which will be held monthly in one of the University's Learning Resource Centres. At each event four researchers will present their research to a mixed audience from across the University in a series of short presentations. Sessions will not be themed as the intention is to support a varied programme enabling the audience to engage with the rich variety of research which takes place across the University and for presenters to disseminate their research to a broader audience.
In addition, through activities initiated within the ARI, there will be other more traditional forms of public engagement growing from our research. In particular we would anticipate a number of talks, panel discussions and question-and-answer sessions relating to our research. These will vary with respect to audience: schools (from primary upwards), amateur astronomy societies, lecture societies, WI etc. We will also showcase the new research at events organised by the ARI (such as the annual Merseyside Astronomy Day) and, where appropriate, at the Spaceport visitor centre.
In all cases the benefits will be twofold. Obviously, an exposure to current research can stimulate inquiry and interest in any audience. However, a less obvious, but perhaps more important benefit is to use that stimulation to promote an appreciation of science as a whole. This is particularly important for engagement with schools where astronomy has a vital role to play in promoting science and other STEM subjects as potential careers.
In order to facilitate this, younger and less experienced researchers (especially PDRAs and PhD students) are encouraged to present their research to a variety of audiences, with training and support provided by the experienced Outreach team within the ARI.
We will also work with non-science organisations to find ways in which the research can be used to enhance their own work. This sort of impact is difficult to predict in advance, as it is usually opportunistic, but past examples in the ARI have involved work with arts organisations and artists (including musicians, theatre companies, street theatre performers, sculptors, photographers and writers) and organisations that promote access to education (such as Aim Higher).
Publications
McAlpine S
(2016)
The eagle simulations of galaxy formation: Public release of halo and galaxy catalogues
in Astronomy and Computing
Csengeri T
(2016)
The first Galaxy scale hunt for the youngest high-mass protostars
in EAS Publications Series
Sembolini F
(2016)
nIFTy galaxy cluster simulations - I. Dark matter and non-radiative models
in Monthly Notices of the Royal Astronomical Society
Bozorgnia N
(2016)
Predictions of hydrodynamic simulations for direct dark matter detection
in Journal of Physics: Conference Series
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
Longmore S
(2016)
Using young massive star clusters to understand star formation and feedback in high-redshift-like environments
in EAS Publications Series
Leloudas G
(2016)
The superluminous transient ASASSN-15lh as a tidal disruption event from a Kerr black hole
in Nature Astronomy
Piatti A
(2016)
Extended main sequence turn-offs in low mass intermediate-age clusters
in Astronomy & Astrophysics
Lieu M
(2016)
The XXL Survey IV. Mass-temperature relation of the bright cluster sample???
in Astronomy & Astrophysics
Barnes A
(2017)
Star formation rates on global and cloud scales within the Galactic Centre
in Proceedings of the International Astronomical Union
Holoien T
(2017)
The ASAS-SN bright supernova catalogue - I. 2013-2014
in Monthly Notices of the Royal Astronomical Society
Inserra C.
(2017)
TRACE spectroscopic classification of optical transient
in The Astronomer's Telegram
Ishida E
(2017)
Exploring the spectroscopic diversity of type Ia supernovae with Deep Learning and Unsupervised Clustering
in Proceedings of the International Astronomical Union
Parsons S
(2017)
Testing the white dwarf mass-radius relationship with eclipsing binaries
in Monthly Notices of the Royal Astronomical Society
Barnes A
(2017)
Star formation rates and efficiencies in the Galactic Centre
in Monthly Notices of the Royal Astronomical Society
Pian E
(2017)
Spectroscopic identification of r-process nucleosynthesis in a double neutron-star merger.
in Nature
Krieger N
(2017)
The Survey of Water and Ammonia in the Galactic Center (SWAG): Molecular Cloud Evolution in the Central Molecular Zone
in The Astrophysical Journal
Cikota A
(2017)
Spatially resolved analysis of superluminous supernovae PTF 11hrq and PTF 12dam host galaxies
in Monthly Notices of the Royal Astronomical Society
Henshaw J
(2017)
Erratum: Seeding the Galactic Centre gas stream: gravitational instabilities set the initial conditions for the formation of protocluster clouds
in Monthly Notices of the Royal Astronomical Society: Letters
Morokuma T
(2017)
OISTER optical and near-infrared monitoring observations of peculiar radio-loud active galactic nucleus SDSS J110006.07+442144.3
in Publications of the Astronomical Society of Japan
Steele I. A.
(2017)
Medium Resolution Spectroscopy of Boyajian's Star (KIC 8462852)
in The Astronomer's Telegram
Martocchia S
(2017)
The search for multiple populations in Magellanic Cloud Clusters - III. No evidence for multiple populations in the SMC cluster NGC 419
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
Anderson L
(2017)
Galactic supernova remnant candidates discovered by THOR
in Astronomy & Astrophysics
Brown T. M.
(2017)
A Universal Transition in Atmospheric Diffusion for Hot Subdwarfs Near 18,000K
in ASTROPHYSICAL JOURNAL
Ben-Ami S.
(2017)
VizieR Online Data Catalog: Type Ic SN 2010mb optical photometry (Ben-Ami+, 2014)
in VizieR Online Data Catalog
Font A
(2017)
The Diversity of Assembly Histories Leading to Disc Galaxy Formation in a ?CDM Model
in Publications of the Astronomical Society of Australia
Lepson J
(2017)
Measurement of L-shell transitions in M-shell ions in the laboratory and identification in stellar coronae
in Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms
Ching J
(2017)
Galaxy And Mass Assembly (GAMA): the environments of high- and low-excitation radio galaxies
in Monthly Notices of the Royal Astronomical Society
Hachinger S
(2017)
Type Ia supernovae with and without blueshifted narrow Na i D lines - how different is their structure?
in Monthly Notices of the Royal Astronomical Society
Longmore S
(2017)
H2O Southern Galactic Plane Survey (HOPS): Paper III - properties of dense molecular gas across the inner Milky Way
in Monthly Notices of the Royal Astronomical Society
Barnes D
(2017)
The Cluster-EAGLE project: global properties of simulated clusters with resolved galaxies
in Monthly Notices of the Royal Astronomical Society
McCarthy I
(2017)
The bahamas project: calibrated hydrodynamical simulations for large-scale structure cosmology
in Monthly Notices of the Royal Astronomical Society
Davies L
(2017)
Galaxy And Mass Assembly: the 1.4 GHz SFR indicator, SFR-M * relation and predictions for ASKAP-GAMA
in Monthly Notices of the Royal Astronomical Society
Nettke W
(2017)
The SCUBA-2 Ambitious Sky Survey: a catalogue of beam-sized sources in the Galactic longitude range 120°-140°
in Monthly Notices of the Royal Astronomical Society
Tanvir N
(2017)
The Emergence of a Lanthanide-rich Kilonova Following the Merger of Two Neutron Stars
in The Astrophysical Journal
Henshaw J
(2017)
Erratum: Seeding the Galactic Centre gas stream: gravitational instabilities set the initial conditions for the formation of protocluster clouds: Table 1.
in Monthly Notices of the Royal Astronomical Society
Csengeri T
(2017)
ALMA survey of massive cluster progenitors from ATLASGAL Limited fragmentation at the early evolutionary stage of massive clumps?
in Astronomy & Astrophysics
Cartier R
(2017)
Early observations of the nearby Type Ia supernova SN 2015F
in Monthly Notices of the Royal Astronomical Society
Federrath C
(2017)
The link between solenoidal turbulence and slow star formation in G0.253+0.016
in Proceedings of the International Astronomical Union
Piran Tsvi
(2017)
Relativistic Jets in Core Collapse Supernovae
in arXiv e-prints
Lin Y
(2017)
Erratum: "Cloud Structure of Three Galactic Infrared Dark Star-forming Regions from Combining Ground and Space-based Bolometric Observations" (2017, ApJ, 840, 22)
in The Astrophysical Journal
Longmore S
(2017)
Adapting astronomical source detection software to help detect animals in thermal images obtained by unmanned aerial systems
in International Journal of Remote Sensing
Massari D
(2017)
The chemical composition of the low-mass Galactic globular cluster NGC 6362?
in Monthly Notices of the Royal Astronomical Society
Holoien T
(2017)
The ASAS-SN Bright Supernova Catalog - II. 2015
in Monthly Notices of the Royal Astronomical Society
Whitaker J
(2017)
MALT90 Kinematic Distances to Dense Molecular Clumps
in The Astronomical Journal
Henson M
(2017)
The impact of baryons on massive galaxy clusters: halo structure and cluster mass estimates
in Monthly Notices of the Royal Astronomical Society
Bertelli Motta C
(2017)
Observing the products of stellar evolution in the old open cluster M67 with APOGEE
in Monthly Notices of the Royal Astronomical Society
Crain R
(2017)
The EAGLE simulations: atomic hydrogen associated with galaxies
in Monthly Notices of the Royal Astronomical Society
Chen T
(2017)
The evolution of superluminous supernova LSQ14mo and its interacting host galaxy system
in Astronomy & Astrophysics
Description | Discoveries about evolution of stars, galaxies and clusters of galaxies, dark matter and dark energy. Total publication output due to new staff and associated new collaborations rose from 100 p.a. to 200 p.a. - doubling our research productivity. Over the same period research income grew from £5m to over £11m. |
Exploitation Route | Further research into unsolved problems in astrophysics. This award led to successful integration of newly appointed staff into the Consolidated submissions in 2015 and 2018. One newly appointed staff Co-I (Steve Longmore) started the Astro-ecology group at ARI. The ARI's AE project combining infrared astronomical instrumentation expertise with drone technology is impacting the way conservation agencies around the world (e.g. WWF) conduct animal surveys. The thermal-drone enables safe, routine, efficient and cost-effective monitoring and management of animal populations over large and inhospitable areas, with a factor of up to 200x increase in survey efficiency over existing methods. This provides conservation agencies greatly improved data needed to quantify and mitigate biodiversity loss. The thermal drone system is being used routinely to help local fire-fighting teams to find/extinguish annual peat fires in Indonesia which are a major contributor to anthropogenic CO2 emissions. The orders of magnitude improvement in fire extinction efficiency the system offers over existing methods will hopefully lead to substantial reduction in CO2 emissions -- a leading cause of climate change. the amount of income generated for this project has now (Feb 2020) exceeded £1.5m. |
Sectors | Communities and Social Services/Policy Education Environment Security and Diplomacy |
URL | http://www.astro.ljmu.ac.uk |
Description | Many outreach activities across all sectors, e.g. Schools, public, policy makers, flower shows. Across discipline funding for astro-ecology using 10 micron cameras on drones flown over conservation areas (Nepal, Africa, Australia) to help preservation of endangered species. Findings are disseminated in astronomical literature and through public events and schools through the National Schools' Observatory. Partly as a result of this grant NSO now has 3,000 registered schools and delivered 140,000 observations to classrooms. We carry out a range of outreach activities visiting schools, astronomical societies and social groups. We also carry out special exhibitions and events at national venues including Tate Liverpool; FACT; the Science Museum London; the London Design Biennale at Somerset House. These have showcased ARI and LJMU research to a total estimated audience in excess of 50,000. Two of our Outreach staff have fEC awards to carry out impact for two funded projects on our renewed Consolidated Grant 2018-21. Under the directorship of Professor Steve Longmore, ARI has developed a major new research area connected to environmental impact, "Astro-ecology". Longmore and team are working with conservation agencies worldwide (e.g. WWF; Endangered Wildlife Trust; Wetland Wildlife trust; National Geographic; Borneo Nature Foundation; Indonesia National Parks; Chester Zoo; Knowsley Safari Park; Morecambe Bay Search and Rescue; several universities), flying infrared instrumentation developed for astronomical purposes on drones. Applications include: animal conservation in rain forests; peat fire detection in Indonesia and human rescue at sea. Starting with an internal LJMU startup award of £25k in 2016, this work has attracted more than £1.5m of external funding (as of Feb 2020) principally through STFC/GCRF grant awards. |
First Year Of Impact | 2015 |
Sector | Agriculture, Food and Drink,Education,Environment,Culture, Heritage, Museums and Collections,Security and Diplomacy,Other |
Impact Types | Cultural Societal Economic Policy & public services |
Description | Astro-ecology with drones (2015-2020) |
Geographic Reach | Multiple continents/international |
Policy Influence Type | Influenced training of practitioners or researchers |
Impact | The ARI's project combining infrared astronomical instrumentation expertise with drone technology is impacting the way conservation agencies around the world (e.g. WWF) conduct animal surveys. The thermal-drone enables safe, routine, efficient and cost-effective monitoring and management of animal populations over large and inhospitable areas, with a factor of up to 200x increase in survey efficiency over existing methods. This provides conservation agencies greatly improved data needed to quantify and mitigate biodiversity loss. The thermal drone system is being used routinely to help local fire-fighting teams to find/extinguish annual peat fires in Indonesia which are a major contributor to anthropogenic CO2 emissions. The orders of magnitude improvement in fire extinction efficiency the system offers over existing methods will hopefully lead to substantial reduction in CO2 emissions -- a leading cause of climate change. |
URL | http://www.astro.ljmu.ac.uk |
Description | NSO Presentation in House of Commons |
Geographic Reach | National |
Policy Influence Type | Influenced training of practitioners or researchers |
Description | Astro-ecology: the solution from the skies to save Earth's biodiversity |
Amount | £411,988 (GBP) |
Funding ID | ST/R002673/1 |
Organisation | Science and Technologies Facilities Council (STFC) |
Sector | Public |
Country | United Kingdom |
Start | 01/2018 |
End | 12/2021 |
Description | CO2 emission from peat fires in Indonesia |
Amount | £450,000 (GBP) |
Funding ID | ST/S00288X/1 |
Organisation | Science and Technologies Facilities Council (STFC) |
Sector | Public |
Country | United Kingdom |
Start | 03/2019 |
End | 03/2022 |
Description | Consolidated Renewal |
Amount | £1,200,000 (GBP) |
Funding ID | ST/R000484/1 |
Organisation | Science and Technologies Facilities Council (STFC) |
Sector | Public |
Country | United Kingdom |
Start | 03/2018 |
End | 03/2021 |
Description | ERC Consolidator Award |
Amount | £1,500,000 (GBP) |
Organisation | EU-T0 |
Sector | Public |
Country | European Union (EU) |
Start | 05/2018 |
End | 05/2023 |
Description | STFC Consolidated Grant Renewal |
Amount | £1,200,000 (GBP) |
Funding ID | ST/M000966/1 |
Organisation | Science and Technologies Facilities Council (STFC) |
Sector | Public |
Country | United Kingdom |
Start | 03/2015 |
End | 03/2018 |
Description | The next generation of holistic galaxy formation simulations at LJMU |
Amount | £37,942 (GBP) |
Funding ID | RGF/EA/180162 |
Organisation | Liverpool John Moores University |
Sector | Academic/University |
Country | United Kingdom |
Start | 11/2017 |
End | 10/2020 |
Description | Astro-ecology |
Organisation | World Wide Fund for Nature |
Country | Switzerland |
Sector | Charity/Non Profit |
PI Contribution | Various conservation agencies, e.g. WWF worldwide. |
Collaborator Contribution | Development of drone technology and IR data reduction techniques for various applications: rare animal species (rhino, lemur, orangutang etc..), peat fires in Indonesia; RNLI search and rescue |
Impact | Listed in publications |
Start Year | 2016 |
Description | International Research Collaboration 2015-2021 |
Organisation | California Institute of Technology |
Country | United States |
Sector | Academic/University |
PI Contribution | The New Applicants Award and subsequent consolidated grants in 2015 and 2018 led to many international collaborations, for example: Harvard - Star Formation and PhD Exchange Programme. Caltech - supernovae and (iPTF/ZTF) transient surveys Virgo consortium membership in Cosmological Simulations - High Performance Computing SLOAN Digitised Survey - IV: UK Participation membership. Virgo-Ligo GW electromagnetic followup MPE, MPA Munch, Penn State, University of Tokyo, IAC Tenerife, and partners in the UK. |
Collaborator Contribution | Partners contribute through refereed papers (ARI publishes 200 p.a.) |
Impact | More than 200 refereed papers p.a. and £12m of external grant income. |
Start Year | 2015 |
Description | ARI Engagement |
Form Of Engagement Activity | A talk or presentation |
Part Of Official Scheme? | No |
Geographic Reach | National |
Primary Audience | Public/other audiences |
Results and Impact | The ARI Outreach team delivers 50 events per year in addition to School based activities. These include, astronomy and science societies and associations, public open events, theatre, street theatre etc..art exhibitions, church societies, cubs, scouts, brownies etc.. |
Year(s) Of Engagement Activity | 2009,2010,2011,2012,2013,2014,2015,2016 |
Description | Exhibitions at national venues |
Form Of Engagement Activity | Participation in an activity, workshop or similar |
Part Of Official Scheme? | No |
Geographic Reach | International |
Primary Audience | Public/other audiences |
Results and Impact | Special exhibitions and events at national venues including: Tate Liverpool, Foundation for Art and Creative Technology (FACT), the Science Museum, the London Design Biennale at Somerset House. |
Year(s) Of Engagement Activity | 2016,2017,2018,2019 |
URL | http://www.astro.ljmu.ac.uk/ |
Description | NSO-Garden Chelsea |
Form Of Engagement Activity | Participation in an activity, workshop or similar |
Part Of Official Scheme? | No |
Geographic Reach | International |
Primary Audience | Public/other audiences |
Results and Impact | In 2015 the NSO exhibited a garden called Dark Matter; at the Chelsea Flower Show winning a Gold medal and Best in Class" (Fresh Gardens). The aggregate audience was estimated at 211 million. The garden has an extensive legacy value at the STFC Daresbury Laboratory and is highlighted on the front cover of the 2015 STFC Impact Report. |
Year(s) Of Engagement Activity | 2015 |
URL | http://www.stfc.ac.uk/files/impact-report-2015/ |
Description | National Schools Observatory |
Form Of Engagement Activity | Participation in an activity, workshop or similar |
Part Of Official Scheme? | No |
Geographic Reach | International |
Primary Audience | Schools |
Results and Impact | Enhanced interest and uptake of STEM subjects Each year the NSO delivers just over 40 different events or visits to or involving schools. This reaches a total of about 4,500 pupils per year in about 80 different schools. Increasing schools registration on NSO - more than 4000 currently |
Year(s) Of Engagement Activity | Pre-2006,2006,2007,2008,2009,2010,2011,2012,2013,2014,2015,2016 |
URL | http://www.schoolsobservatory.org.uk/ |
Description | National Schools' Observatory |
Form Of Engagement Activity | Participation in an activity, workshop or similar |
Part Of Official Scheme? | No |
Geographic Reach | National |
Primary Audience | Schools |
Results and Impact | The NSO has 3,000 registered schools. More than 100,000 discrete observations with the LT have been returned to schools for projects within the classroom. Full evaluation of the impact of the NSO is currently underway. Two of the NSO staff team now have FeC on our renewed Consolidated Grant (2018-2021) |
Year(s) Of Engagement Activity | 2006,2007,2008,2009,2010,2011,2012,2013,2014,2015,2016,2017,2018,2019 |
URL | http://www.astro.ljmu.ac.uk/ |
Description | National Schools' Observatory |
Form Of Engagement Activity | Participation in an activity, workshop or similar |
Part Of Official Scheme? | No |
Geographic Reach | International |
Primary Audience | Public/other audiences |
Results and Impact | Local Schools, Exhibitions (Tate Liverpool, Chelsea Flower Show (audience 200 million) ; FACT; London Design Biennale |
Year(s) Of Engagement Activity | 2014,2015,2016,2017,2018,2019,2020 |
URL | http://www.astro.ljmu.ac.uk/ |