A Programme in Astrophysical Theory and Observations at Leeds
Lead Research Organisation:
University of Leeds
Department Name: Physics and Astronomy
Abstract
This research programme principally addresses how stars and planets form from clouds of dust and gas.
Stars form from the clouds of gas that occupy interstellar space and the small dust grains mixed in them. The clouds are highly filamentary and magnetic fields, that also pervade space, are likely to have had a role in shaping them, and controlling their collapse under gravity to form stars. We will conduct computer simulations to ascertain how the beginning of the formation of stars like our Sun takes place.
The formation of stars much more massive than our Sun has proved to be much more problematic as they are rare and distant and produce prodigious amounts of radiation that blow material away rather than let it fall in. As the infalling material gets close in to the star we expect it to complete its journey in a thin disc orbiting the star. Detailed mapping of the molecular emission with the ALMA telescope is beginning to reveal these discs. We will significantly extend these initial discoveries and interpret the data with sophisticated models to find out how material flows into these discs. The rich spectra due to molecules at these wavelengths will be explored with novel data mining techniques to search for ways that we can trace changes over time as these stars form.
The inner regions of these discs where the material completes its journey on to the forming star will be studied using the techniques of infrared interferometry. This reveals spatial information at levels 10 to 100 times better than the Hubble Space Telescope, where we may start to see the material being channelled by magnetic fields instead. At the same time that material is spiralling onto a star via a disc, some of it is being ejected at high speeds along the rotation axis, again most likely by magnetic fields. To follow these jets further out we will use the highly sensitive network of radio dishes in the UK, e-MERLIN, to map their emission. Comparison with complex models will show whether particles are being accelerated to relativistic speeds in these jets, further enhancing their potential impact on their environment.
As massive stars finally begin to clear away the material from which they were born the combined effect of the winds driven by their strong radiation fields has a dramatic effect. As the winds slam into the molecular material and each other they get heated to millions of degrees and emit strongly in the X-ray region as observed with NASA's Chandra satellite. The most massive stars have such short lives of a few million years that they can blow up as supernovae whilst still surrounded by the remnants of the molecular clouds. Computer simulations will be used to tackle this problem to investigate how these processes can terminate the star formation episodes in giant molecular clouds.
The discs that surround stars like the Sun as they are forming are the sites where planets form, built up from the coalescence of dust grains. This is only thought to occur in the quieter regions of the disc where turbulence due to the magnetic fields is less strong. We will perform calculations of the chemical effects that occur where the icy grains are sublimated that then affect their charge, and hence, magnetic properties. How the charged dust particles move relative to the gas is important in the formation process and that will be examined with sophisticated computer simulations.
Near the end of the lives of stars, the very dust grains that begin the planet formation process are themselves produced. We will perform detailed chemical calculations to work out how these silicate minerals are built up from the gaseous elements in the rich, cool, atmospheres of giant stars. Many of these heavier elements themselves are first made in the exploding stars known as supernovae. We will perform state-of-the-art simulations of the thermo-nuclear detonation of these stars, and examine how this affects the production of elements in the cosmos.
Stars form from the clouds of gas that occupy interstellar space and the small dust grains mixed in them. The clouds are highly filamentary and magnetic fields, that also pervade space, are likely to have had a role in shaping them, and controlling their collapse under gravity to form stars. We will conduct computer simulations to ascertain how the beginning of the formation of stars like our Sun takes place.
The formation of stars much more massive than our Sun has proved to be much more problematic as they are rare and distant and produce prodigious amounts of radiation that blow material away rather than let it fall in. As the infalling material gets close in to the star we expect it to complete its journey in a thin disc orbiting the star. Detailed mapping of the molecular emission with the ALMA telescope is beginning to reveal these discs. We will significantly extend these initial discoveries and interpret the data with sophisticated models to find out how material flows into these discs. The rich spectra due to molecules at these wavelengths will be explored with novel data mining techniques to search for ways that we can trace changes over time as these stars form.
The inner regions of these discs where the material completes its journey on to the forming star will be studied using the techniques of infrared interferometry. This reveals spatial information at levels 10 to 100 times better than the Hubble Space Telescope, where we may start to see the material being channelled by magnetic fields instead. At the same time that material is spiralling onto a star via a disc, some of it is being ejected at high speeds along the rotation axis, again most likely by magnetic fields. To follow these jets further out we will use the highly sensitive network of radio dishes in the UK, e-MERLIN, to map their emission. Comparison with complex models will show whether particles are being accelerated to relativistic speeds in these jets, further enhancing their potential impact on their environment.
As massive stars finally begin to clear away the material from which they were born the combined effect of the winds driven by their strong radiation fields has a dramatic effect. As the winds slam into the molecular material and each other they get heated to millions of degrees and emit strongly in the X-ray region as observed with NASA's Chandra satellite. The most massive stars have such short lives of a few million years that they can blow up as supernovae whilst still surrounded by the remnants of the molecular clouds. Computer simulations will be used to tackle this problem to investigate how these processes can terminate the star formation episodes in giant molecular clouds.
The discs that surround stars like the Sun as they are forming are the sites where planets form, built up from the coalescence of dust grains. This is only thought to occur in the quieter regions of the disc where turbulence due to the magnetic fields is less strong. We will perform calculations of the chemical effects that occur where the icy grains are sublimated that then affect their charge, and hence, magnetic properties. How the charged dust particles move relative to the gas is important in the formation process and that will be examined with sophisticated computer simulations.
Near the end of the lives of stars, the very dust grains that begin the planet formation process are themselves produced. We will perform detailed chemical calculations to work out how these silicate minerals are built up from the gaseous elements in the rich, cool, atmospheres of giant stars. Many of these heavier elements themselves are first made in the exploding stars known as supernovae. We will perform state-of-the-art simulations of the thermo-nuclear detonation of these stars, and examine how this affects the production of elements in the cosmos.
Planned Impact
The proposed research has many beneficiaries, including the general public. The subjects of stellar birth and planet formation, including their astrobiological relevance, appeal to the imagination. Leeds astrophysicists are strongly committed to communicating both their own and general astronomical results to a wide audience. They do this via public appearances and the organisation of events, and through the mass media by, for example, issuing press releases and making media appearances. We make use of our full time outreach officer to coordinate activities locally, regionally and nationally and have a good working relationship with our press office.
Our outreach is built around a set portfolio of events, which continue to be developed and improved. We particularly focus events on school children and young people.
Our donation of telescopes to local astronomical societies has enhanced their outreach in joint partnerships with us.
Our leadership of the collaboration with Goonhilly Earth Station continues with the long-term aim of developing a state-of-the-art showcase for space science and radio astronomy. We also lead the use of Overseas Development Assistance funding to provide training in radio astronomy in Africa as the continent gears up to host the world's biggest radio telescope. The advanced research and technical skills will help to upskill the population and generate economic development in the long term.
The proposal concerns work that will have impact on various industries that directly benefit from the spin-offs of our research methodologies, expertise and in-house computer codes. For example, the research exploiting our state-of-the- art multifluid models is extremely relevant in a surprisingly wide range of applications. At present our codes are being applied to the study of the consequences of the rupture of a high pressure pipeline carrying carbon dioxide for sequestration to combat climate change. We are also working on magnetic confinement of plasmas for nuclear fusion. The ongoing development and improvement of computational methods and codes will ensure the continuation of existing, and the forging of new, fruitful industrial collaborations, which will ultimately aid the UK's economic competitiveness.
Our astronomical expertise is put to use in assisting planning decisions surrounding light pollution around wind farm developments. The trawling of large complex datasets associated with the observational astronomical surveys and we work with computer science colleagues to explore new analysis methods.
Our outreach is built around a set portfolio of events, which continue to be developed and improved. We particularly focus events on school children and young people.
Our donation of telescopes to local astronomical societies has enhanced their outreach in joint partnerships with us.
Our leadership of the collaboration with Goonhilly Earth Station continues with the long-term aim of developing a state-of-the-art showcase for space science and radio astronomy. We also lead the use of Overseas Development Assistance funding to provide training in radio astronomy in Africa as the continent gears up to host the world's biggest radio telescope. The advanced research and technical skills will help to upskill the population and generate economic development in the long term.
The proposal concerns work that will have impact on various industries that directly benefit from the spin-offs of our research methodologies, expertise and in-house computer codes. For example, the research exploiting our state-of-the- art multifluid models is extremely relevant in a surprisingly wide range of applications. At present our codes are being applied to the study of the consequences of the rupture of a high pressure pipeline carrying carbon dioxide for sequestration to combat climate change. We are also working on magnetic confinement of plasmas for nuclear fusion. The ongoing development and improvement of computational methods and codes will ensure the continuation of existing, and the forging of new, fruitful industrial collaborations, which will ultimately aid the UK's economic competitiveness.
Our astronomical expertise is put to use in assisting planning decisions surrounding light pollution around wind farm developments. The trawling of large complex datasets associated with the observational astronomical surveys and we work with computer science colleagues to explore new analysis methods.
Organisations
- University of Leeds (Lead Research Organisation)
- National Radio Astronomy Observatory (NRAO) (Collaboration)
- University of Colorado Boulder (Collaboration)
- University of Calgary (Collaboration)
- Catania Astrophysical Observatory (Collaboration)
- University of California, Berkeley (Collaboration)
- DURHAM UNIVERSITY (Collaboration)
- Spanish National Research Council (CSIC) (Collaboration)
- European Space Agency (Collaboration)
- University of Amsterdam (Collaboration)
- Saclay Nuclear Research Centre (Collaboration)
- Observatory of Paris (Collaboration)
- UNIVERSITY OF SYDNEY (Collaboration)
- UNIVERSITY OF SOUTHAMPTON (Collaboration)
- HARVARD UNIVERSITY (Collaboration)
- Leiden University (Collaboration)
- University of Wisconsin-Madison (Collaboration)
- National Institute for Astrophysics (Collaboration)
- University of Jaen (Collaboration)
- Sapienza University of Rome (Collaboration)
- Nagoya University (Collaboration)
- Armagh Observatory (Collaboration)
- QUEEN'S UNIVERSITY BELFAST (Collaboration)
- UNIVERSITY OF CAMBRIDGE (Collaboration)
- UNIVERSITY OF EXETER (Collaboration)
- Commonwealth Scientific and Industrial Research Organisation (Collaboration)
- UNIVERSITY OF OXFORD (Collaboration)
- Boston University (Collaboration)
- University of Maryland, College Park (Collaboration)
- University of Cologne (Collaboration)
- University of Rome Tor Vergata (Collaboration)
- University of Tasmania (Collaboration)
- National Astronomical Observatories of China (Collaboration)
- Marseille Observatory (Collaboration)
- Liverpool John Moores University (Collaboration)
- NRC Canada (Collaboration)
- University of Toronto (Collaboration)
- DePaul University (Collaboration)
- Monash University (Collaboration)
- California Institute of Technology (Collaboration)
- University of Hertfordshire (Collaboration)
- University of Laval (Collaboration)
- Max Planck Society (Collaboration)
- Chalmers University of Technology (Collaboration)
- National Autonomous University of Mexico (Collaboration)
- Cardiff University (Collaboration)
- UNSW Sydney (Collaboration)
- National Astronomical Research Institute of Thailand (Collaboration)
- Instituto de Radioastronomía Milimétrica (Collaboration)
- University of Barcelona (Collaboration)
- University of Bristol (Collaboration)
- European Southern Observatory (ESO) (Collaboration)
- National Aeronautics and Space Administration (NASA) (Collaboration)
- University College London (Collaboration)
- University of Manchester (Collaboration)
- Dominion Radio Astrophysical Observatory (Collaboration)
- University of Western Australia (Collaboration)
- Université Catholique de Louvain (Collaboration)
- IMPERIAL COLLEGE LONDON (Collaboration)
- Rutherford Appleton Laboratory (Collaboration)
- Laboratory of Astrophysics of Bordeaux (Collaboration)
- University of Central Lancashire (Collaboration)
- University of Leuven (Collaboration)
Publications
Johnston K
(2020)
Spiral arms and instability within the AFGL 4176 mm1 disc
in Astronomy & Astrophysics
Johnston K
(2019)
Spiral arms and instability within the AFGL 4176 mm1 disc
Kalcheva I
(2018)
The coordinated radio and infrared survey for high-mass star formation III. A catalogue of northern ultra-compact H II regions
in Astronomy & Astrophysics
Khorrami Z
(2019)
A Code to Make Your Own Synthetic ObservaTIonS (MYOSOTIS)
in Monthly Notices of the Royal Astronomical Society
Khorrami Zeinab
(2019)
A Code to Make Your Own Synthetic ObservaTIonS (MYOSOTIS)
in Monthly Notices of the Royal Astronomical Society
Khorrami Zeinab
(2021)
High contrast and resolution near-infrared photometry of the core of R136
in Monthly Notices of the Royal Astronomical Society
Klaassen P
(2018)
The evolution of young HII regions I. Continuum emission and internal dynamics
in Astronomy & Astrophysics
Koumpia E
(2019)
Resolving the MYSO binaries PDS 27 and PDS 37 with VLTI/PIONIER
in Astronomy & Astrophysics
Koumpia E
(2022)
Tracing a decade of activity towards a yellow hypergiant. The spectral and spatial morphology of IRC+10420 at au scales
in Monthly Notices of the Royal Astronomical Society
Title | Collaboration with artists Semiconductor to make artwork on radio astronomy |
Description | We collaborated with the artists Semiconductor who incorporated some of our raw e-MERLIN radio interferometric data into a video installation artwork called 'As the world turns'. Postdoc Some of the data streams were also turned in to sounds for the video. |
Type Of Art | Film/Video/Animation |
Year Produced | 2018 |
Impact | The video installation was exhibited during May 2018 at Goonhilly Earth Station Ltd in Cornwall as part of the Groundwork exhibition organised by the Cornubian Arts & Science Trust in Helston. Several hundred members of the public and artist communities visited the installation. |
URL | https://semiconductorfilms.com/art/featured-artwork/as-the-world-turns/ |
Title | Online artwork in response to Rosette Nebula Press Release |
Description | An online image influenced by the IPHAS observation of the Rosette Nebula by Michael Potter, a self-titled Ecologer/Artist in Brisbane, Queensland, Australia, released through the artist's facebook channel. |
Type Of Art | Artwork |
Year Produced | 2018 |
Impact | The image generated a number of facebook 'likes' and 'loves' from the followers of the Artist. |
URL | https://www.facebook.com/photo.php?fbid=10214152969971408&set=a.3647418957271.156621.1628341103&type... |
Description | Our theoretical work has shown that clouds of molecular gas can become unstable and collapse solely due to their thermal properties in typical instellar conditions. This is important in understanding how the process of star formation is initiated. The filamentary nature of instellar clouds was studied using magneto-hydrodynamic simulations. The understanding of the formation of dust grains in the atmospheres red giant stars was made through study of the chemical processes at work. Our observational work has revealed new details of how stars form through high spatial resolution observations. Combining 3 or 4 infrared telescopes together has shown close binaries and information on how the material accretes and is ejected during the formation process. Imaging of high-mass stars in the process of forming has shown that binarity is very common for these stars. Similarly high resolution mm-wave studies show that the disk of material accreting to form high mass stars is unstable and shows spiral arm type structure. Again the ejecting material has been studied at some of the highest resolutions to date via ionized jets with the e-Merlin array of UK radio telescopes showing collimation on structure on scales smaller than the solar system. |
Exploitation Route | The results will used as the basis for further research in to how stars form. |
Sectors | Other |
Description | The simulation codes for dusty plasmas used in the research are being applied to fusion research. Similarly the multi-fluid codes are being applied to medical areas such as liver surgery. Leeds astronomers are assisting with planning in the area of light pollution from wind farms. They also continue to bring the excitement of astronomy to the general public through numerous talks and events to encourage STEM take up. |
First Year Of Impact | 2017 |
Sector | Education,Energy,Healthcare |
Impact Types | Societal Economic |
Description | Scottish Government Working Group |
Geographic Reach | National |
Policy Influence Type | Participation in a guidance/advisory committee |
Description | Accelerating the development of radio astronomy at Goonhilly Earth Station |
Amount | £36,000 (GBP) |
Organisation | Science and Technologies Facilities Council (STFC) |
Sector | Public |
Country | United Kingdom |
Start | 01/2018 |
End | 03/2018 |
Description | STFC IAA Award Accelerating Dish Conversions at Goonhilly Earth Station |
Amount | £63,587 (GBP) |
Organisation | Science and Technologies Facilities Council (STFC) |
Sector | Public |
Country | United Kingdom |
Start | 03/2018 |
End | 03/2019 |
Title | CORNISH Database |
Description | Public online catalogue of the radio sources found during the CORNISH survey of the Galactic plane with the VLA. |
Type Of Material | Database/Collection of data |
Year Produced | 2012 |
Provided To Others? | Yes |
Impact | Been used to select targets for follow-up observations with frontline facilities such as ALMA, JVLA and e-MERLIN. Being used to study the ultra-compact H II region population of the northern Galactic plane. |
URL | http://cornish.leeds.ac.uk/public/index.php |
Title | Data associated with the paper "Particle acceleration and non-thermal emission in colliding-wind binary systems" to be published in Monthly Notices of the Royal Astronomical Society |
Description | The data is associated with a paper to be published in Monthly Notices of the Royal Astronomical Society. The paper abstract is: "We present a model for the creation of non-thermal particles via diffusive shock acceleration in a colliding-wind binary. Our model accounts for the oblique nature of the global shocks bounding the wind-wind collision region and the finite velocity of the scattering centres to the gas. It also includes magnetic field amplification by the cosmic ray induced streaming instability and the dynamical back reaction of the amplified field. We assume that the injection of the ions and electrons is independent of the shock obliquity and that the scattering centres move relative to the fluid at the Alfven velocity (resulting in steeper non-thermal particle distributions). We find that the Mach number, Alfvenic Mach number, and transverse field strength vary strongly along and between the shocks, resulting in significant and non-linear variations in the particle acceleration efficiency and shock nature (turbulent vs. non-turbulent). We find much reduced compression ratios at the oblique shocks in most of our models compared to our earlier work, though total gas compression ratios that exceed 20 can still be obtained in certain situations. We also investigate the dependence of the non-thermal emission on the stellar separation and determine when emission from secondary electrons becomes important. We finish by applying our model to WR146, one of the brightest colliding wind binaries in the radio band. We are able to match the observed radio emission and find that roughly 30 per cent of the wind power at the shocks is channelled into non-thermal particles." |
Type Of Material | Database/Collection of data |
Year Produced | 2021 |
Provided To Others? | Yes |
URL | http://archive.researchdata.leeds.ac.uk/836/ |
Title | Data for the paper "How D-type Hii region expansion depends on numerical resolution" |
Description | This dataset contains theoretical data described in the journal paper http://doi.org/10.1093/mnras/stab3707. The data is organized into 2 zip files: data.zip - this contains 8 directories containing data from the simulations presented in the paper. Each directory contains a set of ASCII data files containing details on the fluid variables, as well as 2 ASCII data files which log the evolution of particular properties of the HII region. It also contains a gnuplot script for generating the figures. figures.zip - this contains the pdf files of all of the figures in the paper. |
Type Of Material | Database/Collection of data |
Year Produced | 2022 |
Provided To Others? | Yes |
URL | https://archive.researchdata.leeds.ac.uk/918/ |
Title | Dataset to accompany 'Striations, integrals, hourglasses and collapse - thermal instability driven magnetic simulations of molecular clouds' |
Description | This is the dataset to accompany the publication "Striations, integrals, hourglasses and collapse - thermal instability driven magnetic simulations of molecular clouds" |
Type Of Material | Database/Collection of data |
Year Produced | 2020 |
Provided To Others? | Yes |
URL | http://archive.researchdata.leeds.ac.uk/739/ |
Title | ESO Large Programme on Multiplicity of Young Stars |
Description | GRAVITY+ large programme awarded in 2022, observations on-going |
Type Of Material | Database/Collection of data |
Year Produced | 2023 |
Provided To Others? | No |
Impact | Understanding of Massive Star Formation |
Title | Fried Egg Nebula AMBER and GRAVITY observations |
Description | VizieR online Data Catalogue associated with article published in journal Astronomy & Astrophysics with title 'Optical/near-infrared observations of the Fried Egg Nebula. Multiple shell ejections on a 100 yr timescale from a massive yellow hypergiant.' (bibcode: 2020A&A...635A.183K) |
Type Of Material | Database/Collection of data |
Year Produced | 2020 |
Provided To Others? | Yes |
URL | https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/635/A183 |
Title | Massive YSOs VLTI observations |
Description | VizieR online Data Catalogue associated with article published in journal Astronomy & Astrophysics with title 'The first interferometric survey of massive YSOs in the K-band. Hot dust, ionised gas, and binarity at au scales.' (bibcode: 2021A&A...654A.109K) |
Type Of Material | Database/Collection of data |
Year Produced | 2021 |
Provided To Others? | Yes |
URL | https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/654/A109 |
Title | Prestellar cores H2D+ and N2H+ maps |
Description | VizieR online Data Catalogue associated with article published in journal Astronomy & Astrophysics with title 'Mapping the H_2_D^+^ and N_2_H^+^ emission towards prestellar cores. Testing dynamical models of the collapse using gas tracers.' (bibcode: 2020A&A...643A..61K) |
Type Of Material | Database/Collection of data |
Year Produced | 2020 |
Provided To Others? | Yes |
URL | https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/643/A61 |
Title | RMS Database |
Description | Public online database of the catalogue of massive young stellar objects and other objects found during the Red MSX Source survey. |
Type Of Material | Database/Collection of data |
Year Produced | 2010 |
Provided To Others? | Yes |
Impact | Used by other researchers studying massive star formation throughout the Galaxy and to select targets for follow-up with frontline facilities such as ALMA, e-MERLIN and VLTI. |
URL | http://rms.leeds.ac.uk/cgi-bin/public/RMS_DATABASE.cgi |
Description | ATOMIUM |
Organisation | Chalmers University of Technology |
Department | Onsala Space Observatory |
Country | Sweden |
Sector | Academic/University |
PI Contribution | Plane developed the chemical networks to model the ALMA observations of small molecules (e.g. FeO, AlO, AlOH, AlCl, AlF) around a number of AGB stars. Relevant rate coefficients were either measured in the laboratory at Leeds, or calculated using theoretical methods. |
Collaborator Contribution | Other partners led the ALMA observations, reduction and analysis. |
Impact | Plane has published 7 papers with the consortium. |
Start Year | 2019 |
Description | ATOMIUM |
Organisation | Harvard University |
Department | Harvard-Smithsonian Center for Astrophysics |
Country | United States |
Sector | Academic/University |
PI Contribution | Plane developed the chemical networks to model the ALMA observations of small molecules (e.g. FeO, AlO, AlOH, AlCl, AlF) around a number of AGB stars. Relevant rate coefficients were either measured in the laboratory at Leeds, or calculated using theoretical methods. |
Collaborator Contribution | Other partners led the ALMA observations, reduction and analysis. |
Impact | Plane has published 7 papers with the consortium. |
Start Year | 2019 |
Description | ATOMIUM |
Organisation | Imperial College London |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Plane developed the chemical networks to model the ALMA observations of small molecules (e.g. FeO, AlO, AlOH, AlCl, AlF) around a number of AGB stars. Relevant rate coefficients were either measured in the laboratory at Leeds, or calculated using theoretical methods. |
Collaborator Contribution | Other partners led the ALMA observations, reduction and analysis. |
Impact | Plane has published 7 papers with the consortium. |
Start Year | 2019 |
Description | ATOMIUM |
Organisation | Instituto de Radioastronomía Milimétrica |
Country | Spain |
Sector | Public |
PI Contribution | Plane developed the chemical networks to model the ALMA observations of small molecules (e.g. FeO, AlO, AlOH, AlCl, AlF) around a number of AGB stars. Relevant rate coefficients were either measured in the laboratory at Leeds, or calculated using theoretical methods. |
Collaborator Contribution | Other partners led the ALMA observations, reduction and analysis. |
Impact | Plane has published 7 papers with the consortium. |
Start Year | 2019 |
Description | ATOMIUM |
Organisation | Laboratory of Astrophysics of Bordeaux |
Country | France |
Sector | Public |
PI Contribution | Plane developed the chemical networks to model the ALMA observations of small molecules (e.g. FeO, AlO, AlOH, AlCl, AlF) around a number of AGB stars. Relevant rate coefficients were either measured in the laboratory at Leeds, or calculated using theoretical methods. |
Collaborator Contribution | Other partners led the ALMA observations, reduction and analysis. |
Impact | Plane has published 7 papers with the consortium. |
Start Year | 2019 |
Description | ATOMIUM |
Organisation | Max Planck Society |
Department | Max Planck Institute for Radio Astronomy |
Country | Germany |
Sector | Academic/University |
PI Contribution | Plane developed the chemical networks to model the ALMA observations of small molecules (e.g. FeO, AlO, AlOH, AlCl, AlF) around a number of AGB stars. Relevant rate coefficients were either measured in the laboratory at Leeds, or calculated using theoretical methods. |
Collaborator Contribution | Other partners led the ALMA observations, reduction and analysis. |
Impact | Plane has published 7 papers with the consortium. |
Start Year | 2019 |
Description | ATOMIUM |
Organisation | Monash University |
Department | Monash Centre for Astrophysics |
Country | Australia |
Sector | Academic/University |
PI Contribution | Plane developed the chemical networks to model the ALMA observations of small molecules (e.g. FeO, AlO, AlOH, AlCl, AlF) around a number of AGB stars. Relevant rate coefficients were either measured in the laboratory at Leeds, or calculated using theoretical methods. |
Collaborator Contribution | Other partners led the ALMA observations, reduction and analysis. |
Impact | Plane has published 7 papers with the consortium. |
Start Year | 2019 |
Description | ATOMIUM |
Organisation | National Aeronautics and Space Administration (NASA) |
Department | Jet Propulsion Laboratory |
Country | United States |
Sector | Public |
PI Contribution | Plane developed the chemical networks to model the ALMA observations of small molecules (e.g. FeO, AlO, AlOH, AlCl, AlF) around a number of AGB stars. Relevant rate coefficients were either measured in the laboratory at Leeds, or calculated using theoretical methods. |
Collaborator Contribution | Other partners led the ALMA observations, reduction and analysis. |
Impact | Plane has published 7 papers with the consortium. |
Start Year | 2019 |
Description | ATOMIUM |
Organisation | Observatory of Paris |
Country | France |
Sector | Academic/University |
PI Contribution | Plane developed the chemical networks to model the ALMA observations of small molecules (e.g. FeO, AlO, AlOH, AlCl, AlF) around a number of AGB stars. Relevant rate coefficients were either measured in the laboratory at Leeds, or calculated using theoretical methods. |
Collaborator Contribution | Other partners led the ALMA observations, reduction and analysis. |
Impact | Plane has published 7 papers with the consortium. |
Start Year | 2019 |
Description | ATOMIUM |
Organisation | Queen's University Belfast |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Plane developed the chemical networks to model the ALMA observations of small molecules (e.g. FeO, AlO, AlOH, AlCl, AlF) around a number of AGB stars. Relevant rate coefficients were either measured in the laboratory at Leeds, or calculated using theoretical methods. |
Collaborator Contribution | Other partners led the ALMA observations, reduction and analysis. |
Impact | Plane has published 7 papers with the consortium. |
Start Year | 2019 |
Description | ATOMIUM |
Organisation | University of Amsterdam |
Department | Anton Pannekoek Institute for Astronomy |
Country | Netherlands |
Sector | Academic/University |
PI Contribution | Plane developed the chemical networks to model the ALMA observations of small molecules (e.g. FeO, AlO, AlOH, AlCl, AlF) around a number of AGB stars. Relevant rate coefficients were either measured in the laboratory at Leeds, or calculated using theoretical methods. |
Collaborator Contribution | Other partners led the ALMA observations, reduction and analysis. |
Impact | Plane has published 7 papers with the consortium. |
Start Year | 2019 |
Description | ATOMIUM |
Organisation | University of Cologne |
Country | Germany |
Sector | Academic/University |
PI Contribution | Plane developed the chemical networks to model the ALMA observations of small molecules (e.g. FeO, AlO, AlOH, AlCl, AlF) around a number of AGB stars. Relevant rate coefficients were either measured in the laboratory at Leeds, or calculated using theoretical methods. |
Collaborator Contribution | Other partners led the ALMA observations, reduction and analysis. |
Impact | Plane has published 7 papers with the consortium. |
Start Year | 2019 |
Description | ATOMIUM |
Organisation | University of Leuven |
Country | Belgium |
Sector | Academic/University |
PI Contribution | Plane developed the chemical networks to model the ALMA observations of small molecules (e.g. FeO, AlO, AlOH, AlCl, AlF) around a number of AGB stars. Relevant rate coefficients were either measured in the laboratory at Leeds, or calculated using theoretical methods. |
Collaborator Contribution | Other partners led the ALMA observations, reduction and analysis. |
Impact | Plane has published 7 papers with the consortium. |
Start Year | 2019 |
Description | ATOMIUM |
Organisation | University of Manchester |
Department | Jodrell Bank Centre for Astrophysics |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Plane developed the chemical networks to model the ALMA observations of small molecules (e.g. FeO, AlO, AlOH, AlCl, AlF) around a number of AGB stars. Relevant rate coefficients were either measured in the laboratory at Leeds, or calculated using theoretical methods. |
Collaborator Contribution | Other partners led the ALMA observations, reduction and analysis. |
Impact | Plane has published 7 papers with the consortium. |
Start Year | 2019 |
Description | CUGA |
Organisation | Durham University |
Department | Department of Physics |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | The Consortium of Universities for Goonhilly Astronomy (CUGA) works with the SME Goonhilly Earth Station Ltd. to develop radio astronomy capability at the Goonhilly site in Cornwall, UK. Each main partner has contributed £125k net either in cash or in kind. Oxford has contributed a C-band receiver and digital backed. Manchester are making available an L-band receiver. The 29 m class Ghy-3 dish has been refurbished and brought back in to use as a dual-purpose radio telescope and deep space communications dish. Leeds has contributed to the drive upgrades and peripheral components for the L-band receiver. There is an ambition to link them into the existing e-MERLIN network in the UK and EVN in Europe. UCLan joined the effort in 2018 and will provide and in-kind contribution of the mount for the L-band receiver on the Ghy-1 dish. In 2022 a Space AI Institute is being developed at Goonhilly where academics from CUGA can utilize the GPU cluster in the new data centre facility at Goonhilly and work on applied problems with space sector clients. Funds from ST/W507994/1 have been used to augment the GPU cluster and upgrade the digital back end for the radio telescope to enable maser monitoring. |
Collaborator Contribution | As above. University of Hertfordshire acts as the legal entity for CUGA. |
Impact | A JANET REACH grant has been awarded to GES Ltd, Adaptive Array Systems Ltd and CUGA to enable a datalink between Goonhilly and Jodrell Bank to allow the connection into e-MERLIN. Various joint outreach events have taken place. |
Start Year | 2011 |
Description | CUGA |
Organisation | University of Bristol |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | The Consortium of Universities for Goonhilly Astronomy (CUGA) works with the SME Goonhilly Earth Station Ltd. to develop radio astronomy capability at the Goonhilly site in Cornwall, UK. Each main partner has contributed £125k net either in cash or in kind. Oxford has contributed a C-band receiver and digital backed. Manchester are making available an L-band receiver. The 29 m class Ghy-3 dish has been refurbished and brought back in to use as a dual-purpose radio telescope and deep space communications dish. Leeds has contributed to the drive upgrades and peripheral components for the L-band receiver. There is an ambition to link them into the existing e-MERLIN network in the UK and EVN in Europe. UCLan joined the effort in 2018 and will provide and in-kind contribution of the mount for the L-band receiver on the Ghy-1 dish. In 2022 a Space AI Institute is being developed at Goonhilly where academics from CUGA can utilize the GPU cluster in the new data centre facility at Goonhilly and work on applied problems with space sector clients. Funds from ST/W507994/1 have been used to augment the GPU cluster and upgrade the digital back end for the radio telescope to enable maser monitoring. |
Collaborator Contribution | As above. University of Hertfordshire acts as the legal entity for CUGA. |
Impact | A JANET REACH grant has been awarded to GES Ltd, Adaptive Array Systems Ltd and CUGA to enable a datalink between Goonhilly and Jodrell Bank to allow the connection into e-MERLIN. Various joint outreach events have taken place. |
Start Year | 2011 |
Description | CUGA |
Organisation | University of Central Lancashire |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | The Consortium of Universities for Goonhilly Astronomy (CUGA) works with the SME Goonhilly Earth Station Ltd. to develop radio astronomy capability at the Goonhilly site in Cornwall, UK. Each main partner has contributed £125k net either in cash or in kind. Oxford has contributed a C-band receiver and digital backed. Manchester are making available an L-band receiver. The 29 m class Ghy-3 dish has been refurbished and brought back in to use as a dual-purpose radio telescope and deep space communications dish. Leeds has contributed to the drive upgrades and peripheral components for the L-band receiver. There is an ambition to link them into the existing e-MERLIN network in the UK and EVN in Europe. UCLan joined the effort in 2018 and will provide and in-kind contribution of the mount for the L-band receiver on the Ghy-1 dish. In 2022 a Space AI Institute is being developed at Goonhilly where academics from CUGA can utilize the GPU cluster in the new data centre facility at Goonhilly and work on applied problems with space sector clients. Funds from ST/W507994/1 have been used to augment the GPU cluster and upgrade the digital back end for the radio telescope to enable maser monitoring. |
Collaborator Contribution | As above. University of Hertfordshire acts as the legal entity for CUGA. |
Impact | A JANET REACH grant has been awarded to GES Ltd, Adaptive Array Systems Ltd and CUGA to enable a datalink between Goonhilly and Jodrell Bank to allow the connection into e-MERLIN. Various joint outreach events have taken place. |
Start Year | 2011 |
Description | CUGA |
Organisation | University of Manchester |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | The Consortium of Universities for Goonhilly Astronomy (CUGA) works with the SME Goonhilly Earth Station Ltd. to develop radio astronomy capability at the Goonhilly site in Cornwall, UK. Each main partner has contributed £125k net either in cash or in kind. Oxford has contributed a C-band receiver and digital backed. Manchester are making available an L-band receiver. The 29 m class Ghy-3 dish has been refurbished and brought back in to use as a dual-purpose radio telescope and deep space communications dish. Leeds has contributed to the drive upgrades and peripheral components for the L-band receiver. There is an ambition to link them into the existing e-MERLIN network in the UK and EVN in Europe. UCLan joined the effort in 2018 and will provide and in-kind contribution of the mount for the L-band receiver on the Ghy-1 dish. In 2022 a Space AI Institute is being developed at Goonhilly where academics from CUGA can utilize the GPU cluster in the new data centre facility at Goonhilly and work on applied problems with space sector clients. Funds from ST/W507994/1 have been used to augment the GPU cluster and upgrade the digital back end for the radio telescope to enable maser monitoring. |
Collaborator Contribution | As above. University of Hertfordshire acts as the legal entity for CUGA. |
Impact | A JANET REACH grant has been awarded to GES Ltd, Adaptive Array Systems Ltd and CUGA to enable a datalink between Goonhilly and Jodrell Bank to allow the connection into e-MERLIN. Various joint outreach events have taken place. |
Start Year | 2011 |
Description | CUGA |
Organisation | University of Oxford |
Department | Department of Physics |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | The Consortium of Universities for Goonhilly Astronomy (CUGA) works with the SME Goonhilly Earth Station Ltd. to develop radio astronomy capability at the Goonhilly site in Cornwall, UK. Each main partner has contributed £125k net either in cash or in kind. Oxford has contributed a C-band receiver and digital backed. Manchester are making available an L-band receiver. The 29 m class Ghy-3 dish has been refurbished and brought back in to use as a dual-purpose radio telescope and deep space communications dish. Leeds has contributed to the drive upgrades and peripheral components for the L-band receiver. There is an ambition to link them into the existing e-MERLIN network in the UK and EVN in Europe. UCLan joined the effort in 2018 and will provide and in-kind contribution of the mount for the L-band receiver on the Ghy-1 dish. In 2022 a Space AI Institute is being developed at Goonhilly where academics from CUGA can utilize the GPU cluster in the new data centre facility at Goonhilly and work on applied problems with space sector clients. Funds from ST/W507994/1 have been used to augment the GPU cluster and upgrade the digital back end for the radio telescope to enable maser monitoring. |
Collaborator Contribution | As above. University of Hertfordshire acts as the legal entity for CUGA. |
Impact | A JANET REACH grant has been awarded to GES Ltd, Adaptive Array Systems Ltd and CUGA to enable a datalink between Goonhilly and Jodrell Bank to allow the connection into e-MERLIN. Various joint outreach events have taken place. |
Start Year | 2011 |
Description | CUGA |
Organisation | University of Southampton |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | The Consortium of Universities for Goonhilly Astronomy (CUGA) works with the SME Goonhilly Earth Station Ltd. to develop radio astronomy capability at the Goonhilly site in Cornwall, UK. Each main partner has contributed £125k net either in cash or in kind. Oxford has contributed a C-band receiver and digital backed. Manchester are making available an L-band receiver. The 29 m class Ghy-3 dish has been refurbished and brought back in to use as a dual-purpose radio telescope and deep space communications dish. Leeds has contributed to the drive upgrades and peripheral components for the L-band receiver. There is an ambition to link them into the existing e-MERLIN network in the UK and EVN in Europe. UCLan joined the effort in 2018 and will provide and in-kind contribution of the mount for the L-band receiver on the Ghy-1 dish. In 2022 a Space AI Institute is being developed at Goonhilly where academics from CUGA can utilize the GPU cluster in the new data centre facility at Goonhilly and work on applied problems with space sector clients. Funds from ST/W507994/1 have been used to augment the GPU cluster and upgrade the digital back end for the radio telescope to enable maser monitoring. |
Collaborator Contribution | As above. University of Hertfordshire acts as the legal entity for CUGA. |
Impact | A JANET REACH grant has been awarded to GES Ltd, Adaptive Array Systems Ltd and CUGA to enable a datalink between Goonhilly and Jodrell Bank to allow the connection into e-MERLIN. Various joint outreach events have taken place. |
Start Year | 2011 |
Description | Hi-GAL Survey |
Organisation | California Institute of Technology |
Department | Infrared Processing and Analysis Center |
Country | United States |
Sector | Academic/University |
PI Contribution | Hoare and Caselli contributed to the science case for this Herschel survey of the galactic plane and exploit the resulting data. |
Collaborator Contribution | Carried out the survey, reduced and analysed the data. |
Impact | Publications New knowledge Data acquisition Data analysis |
Description | Hi-GAL Survey |
Organisation | Cardiff University |
Department | School of Physics and Astronomy |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Hoare and Caselli contributed to the science case for this Herschel survey of the galactic plane and exploit the resulting data. |
Collaborator Contribution | Carried out the survey, reduced and analysed the data. |
Impact | Publications New knowledge Data acquisition Data analysis |
Description | Hi-GAL Survey |
Organisation | Catholic University of Louvain |
Country | Belgium |
Sector | Academic/University |
PI Contribution | Hoare and Caselli contributed to the science case for this Herschel survey of the galactic plane and exploit the resulting data. |
Collaborator Contribution | Carried out the survey, reduced and analysed the data. |
Impact | Publications New knowledge Data acquisition Data analysis |
Description | Hi-GAL Survey |
Organisation | Harvard University |
Department | Harvard-Smithsonian Center for Astrophysics |
Country | United States |
Sector | Academic/University |
PI Contribution | Hoare and Caselli contributed to the science case for this Herschel survey of the galactic plane and exploit the resulting data. |
Collaborator Contribution | Carried out the survey, reduced and analysed the data. |
Impact | Publications New knowledge Data acquisition Data analysis |
Description | Hi-GAL Survey |
Organisation | Liverpool John Moores University |
Department | Astrophysics Research Institute |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Hoare and Caselli contributed to the science case for this Herschel survey of the galactic plane and exploit the resulting data. |
Collaborator Contribution | Carried out the survey, reduced and analysed the data. |
Impact | Publications New knowledge Data acquisition Data analysis |
Description | Hi-GAL Survey |
Organisation | Marseille Observatory |
Country | France |
Sector | Academic/University |
PI Contribution | Hoare and Caselli contributed to the science case for this Herschel survey of the galactic plane and exploit the resulting data. |
Collaborator Contribution | Carried out the survey, reduced and analysed the data. |
Impact | Publications New knowledge Data acquisition Data analysis |
Description | Hi-GAL Survey |
Organisation | Max Planck Society |
Department | Max Planck Institute for Nuclear Physics |
Country | Germany |
Sector | Academic/University |
PI Contribution | Hoare and Caselli contributed to the science case for this Herschel survey of the galactic plane and exploit the resulting data. |
Collaborator Contribution | Carried out the survey, reduced and analysed the data. |
Impact | Publications New knowledge Data acquisition Data analysis |
Description | Hi-GAL Survey |
Organisation | Max Planck Society |
Department | Max Planck Institute for Radio Astronomy |
Country | Germany |
Sector | Academic/University |
PI Contribution | Hoare and Caselli contributed to the science case for this Herschel survey of the galactic plane and exploit the resulting data. |
Collaborator Contribution | Carried out the survey, reduced and analysed the data. |
Impact | Publications New knowledge Data acquisition Data analysis |
Description | Hi-GAL Survey |
Organisation | Nagoya University |
Country | Japan |
Sector | Academic/University |
PI Contribution | Hoare and Caselli contributed to the science case for this Herschel survey of the galactic plane and exploit the resulting data. |
Collaborator Contribution | Carried out the survey, reduced and analysed the data. |
Impact | Publications New knowledge Data acquisition Data analysis |
Description | Hi-GAL Survey |
Organisation | National Astronomical Observatories of China |
Country | China |
Sector | Public |
PI Contribution | Hoare and Caselli contributed to the science case for this Herschel survey of the galactic plane and exploit the resulting data. |
Collaborator Contribution | Carried out the survey, reduced and analysed the data. |
Impact | Publications New knowledge Data acquisition Data analysis |
Description | Hi-GAL Survey |
Organisation | National Institute for Astrophysics |
Country | Italy |
Sector | Academic/University |
PI Contribution | Hoare and Caselli contributed to the science case for this Herschel survey of the galactic plane and exploit the resulting data. |
Collaborator Contribution | Carried out the survey, reduced and analysed the data. |
Impact | Publications New knowledge Data acquisition Data analysis |
Description | Hi-GAL Survey |
Organisation | Rutherford Appleton Laboratory |
Department | Space Science and Technology Department |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Hoare and Caselli contributed to the science case for this Herschel survey of the galactic plane and exploit the resulting data. |
Collaborator Contribution | Carried out the survey, reduced and analysed the data. |
Impact | Publications New knowledge Data acquisition Data analysis |
Description | Hi-GAL Survey |
Organisation | Saclay Nuclear Research Centre |
Country | France |
Sector | Public |
PI Contribution | Hoare and Caselli contributed to the science case for this Herschel survey of the galactic plane and exploit the resulting data. |
Collaborator Contribution | Carried out the survey, reduced and analysed the data. |
Impact | Publications New knowledge Data acquisition Data analysis |
Description | Hi-GAL Survey |
Organisation | Sapienza University of Rome |
Country | Italy |
Sector | Academic/University |
PI Contribution | Hoare and Caselli contributed to the science case for this Herschel survey of the galactic plane and exploit the resulting data. |
Collaborator Contribution | Carried out the survey, reduced and analysed the data. |
Impact | Publications New knowledge Data acquisition Data analysis |
Description | Hi-GAL Survey |
Organisation | Spanish National Research Council (CSIC) |
Country | Spain |
Sector | Public |
PI Contribution | Hoare and Caselli contributed to the science case for this Herschel survey of the galactic plane and exploit the resulting data. |
Collaborator Contribution | Carried out the survey, reduced and analysed the data. |
Impact | Publications New knowledge Data acquisition Data analysis |
Description | Hi-GAL Survey |
Organisation | University College London |
Department | Department of Physics & Astronomy |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Hoare and Caselli contributed to the science case for this Herschel survey of the galactic plane and exploit the resulting data. |
Collaborator Contribution | Carried out the survey, reduced and analysed the data. |
Impact | Publications New knowledge Data acquisition Data analysis |
Description | Hi-GAL Survey |
Organisation | University of Calgary |
Country | Canada |
Sector | Academic/University |
PI Contribution | Hoare and Caselli contributed to the science case for this Herschel survey of the galactic plane and exploit the resulting data. |
Collaborator Contribution | Carried out the survey, reduced and analysed the data. |
Impact | Publications New knowledge Data acquisition Data analysis |
Description | Hi-GAL Survey |
Organisation | University of California, Berkeley |
Country | United States |
Sector | Academic/University |
PI Contribution | Hoare and Caselli contributed to the science case for this Herschel survey of the galactic plane and exploit the resulting data. |
Collaborator Contribution | Carried out the survey, reduced and analysed the data. |
Impact | Publications New knowledge Data acquisition Data analysis |
Description | Hi-GAL Survey |
Organisation | University of Colorado |
Country | United States |
Sector | Academic/University |
PI Contribution | Hoare and Caselli contributed to the science case for this Herschel survey of the galactic plane and exploit the resulting data. |
Collaborator Contribution | Carried out the survey, reduced and analysed the data. |
Impact | Publications New knowledge Data acquisition Data analysis |
Description | Hi-GAL Survey |
Organisation | University of Exeter |
Department | Physics and Astronomy |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Hoare and Caselli contributed to the science case for this Herschel survey of the galactic plane and exploit the resulting data. |
Collaborator Contribution | Carried out the survey, reduced and analysed the data. |
Impact | Publications New knowledge Data acquisition Data analysis |
Description | Hi-GAL Survey |
Organisation | University of Hertfordshire |
Department | Centre for Astrophysics Research (CAR) |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Hoare and Caselli contributed to the science case for this Herschel survey of the galactic plane and exploit the resulting data. |
Collaborator Contribution | Carried out the survey, reduced and analysed the data. |
Impact | Publications New knowledge Data acquisition Data analysis |
Description | Hi-GAL Survey |
Organisation | University of Laval |
Country | Canada |
Sector | Academic/University |
PI Contribution | Hoare and Caselli contributed to the science case for this Herschel survey of the galactic plane and exploit the resulting data. |
Collaborator Contribution | Carried out the survey, reduced and analysed the data. |
Impact | Publications New knowledge Data acquisition Data analysis |
Description | Hi-GAL Survey |
Organisation | University of Manchester |
Department | School of Physics and Astronomy Manchester |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Hoare and Caselli contributed to the science case for this Herschel survey of the galactic plane and exploit the resulting data. |
Collaborator Contribution | Carried out the survey, reduced and analysed the data. |
Impact | Publications New knowledge Data acquisition Data analysis |
Description | Hi-GAL Survey |
Organisation | University of New South Wales |
Country | Australia |
Sector | Academic/University |
PI Contribution | Hoare and Caselli contributed to the science case for this Herschel survey of the galactic plane and exploit the resulting data. |
Collaborator Contribution | Carried out the survey, reduced and analysed the data. |
Impact | Publications New knowledge Data acquisition Data analysis |
Description | Hi-GAL Survey |
Organisation | University of Rome Tor Vergata |
Country | Italy |
Sector | Academic/University |
PI Contribution | Hoare and Caselli contributed to the science case for this Herschel survey of the galactic plane and exploit the resulting data. |
Collaborator Contribution | Carried out the survey, reduced and analysed the data. |
Impact | Publications New knowledge Data acquisition Data analysis |
Description | Hi-GAL Survey |
Organisation | University of Toronto |
Country | Canada |
Sector | Academic/University |
PI Contribution | Hoare and Caselli contributed to the science case for this Herschel survey of the galactic plane and exploit the resulting data. |
Collaborator Contribution | Carried out the survey, reduced and analysed the data. |
Impact | Publications New knowledge Data acquisition Data analysis |
Description | Multifluid models for star formation |
Organisation | Max Planck Society |
Department | Max Planck Institute For Extraterrestrial Physics (MPE) |
Country | Germany |
Sector | Academic/University |
PI Contribution | The collaboration focuses on the multifluid effects in the interstellar medium and protostellar discs. My team is developing a multifluid code including dust grain physics such as sputtering and grain-grain collisions. |
Collaborator Contribution | The Center for Astrochemistry is partly supporting a PhD student and is providing observational data. |
Impact | No outputs yet. |
Start Year | 2017 |
Description | The CORNISH Radio Survey |
Organisation | Boston University |
Department | Department of Astronomy |
Country | United States |
Sector | Academic/University |
PI Contribution | Hoare leads the team, was PI of the proposal that was awarded the Large VLA Project time, carried out the observations, manages the team and organizes workshops. |
Collaborator Contribution | Contributed to the science case and the exploitation of the data. |
Impact | Data acquisition Data analysis New knowledge Project leadership Publications Online catalogue |
Start Year | 2006 |
Description | The CORNISH Radio Survey |
Organisation | Dominion Radio Astrophysical Observatory |
Country | Canada |
Sector | Public |
PI Contribution | Hoare leads the team, was PI of the proposal that was awarded the Large VLA Project time, carried out the observations, manages the team and organizes workshops. |
Collaborator Contribution | Contributed to the science case and the exploitation of the data. |
Impact | Data acquisition Data analysis New knowledge Project leadership Publications Online catalogue |
Start Year | 2006 |
Description | The CORNISH Radio Survey |
Organisation | Liverpool John Moores University |
Department | Astrophysics Research Institute |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Hoare leads the team, was PI of the proposal that was awarded the Large VLA Project time, carried out the observations, manages the team and organizes workshops. |
Collaborator Contribution | Contributed to the science case and the exploitation of the data. |
Impact | Data acquisition Data analysis New knowledge Project leadership Publications Online catalogue |
Start Year | 2006 |
Description | The CORNISH Radio Survey |
Organisation | National Autonomous University of Mexico |
Department | Radio Astronomy |
Country | Mexico |
Sector | Academic/University |
PI Contribution | Hoare leads the team, was PI of the proposal that was awarded the Large VLA Project time, carried out the observations, manages the team and organizes workshops. |
Collaborator Contribution | Contributed to the science case and the exploitation of the data. |
Impact | Data acquisition Data analysis New knowledge Project leadership Publications Online catalogue |
Start Year | 2006 |
Description | The CORNISH Radio Survey |
Organisation | National Radio Astronomy Observatory (NRAO) |
Country | United States |
Sector | Public |
PI Contribution | Hoare leads the team, was PI of the proposal that was awarded the Large VLA Project time, carried out the observations, manages the team and organizes workshops. |
Collaborator Contribution | Contributed to the science case and the exploitation of the data. |
Impact | Data acquisition Data analysis New knowledge Project leadership Publications Online catalogue |
Start Year | 2006 |
Description | The CORNISH Radio Survey |
Organisation | University of Barcelona |
Department | Faculty of Physics |
Country | Spain |
Sector | Academic/University |
PI Contribution | Hoare leads the team, was PI of the proposal that was awarded the Large VLA Project time, carried out the observations, manages the team and organizes workshops. |
Collaborator Contribution | Contributed to the science case and the exploitation of the data. |
Impact | Data acquisition Data analysis New knowledge Project leadership Publications Online catalogue |
Start Year | 2006 |
Description | The CORNISH Radio Survey |
Organisation | University of Hertfordshire |
Department | Centre for Astrophysics Research (CAR) |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Hoare leads the team, was PI of the proposal that was awarded the Large VLA Project time, carried out the observations, manages the team and organizes workshops. |
Collaborator Contribution | Contributed to the science case and the exploitation of the data. |
Impact | Data acquisition Data analysis New knowledge Project leadership Publications Online catalogue |
Start Year | 2006 |
Description | The CORNISH Radio Survey |
Organisation | University of Jaen |
Department | Department of Physics |
Country | Spain |
Sector | Academic/University |
PI Contribution | Hoare leads the team, was PI of the proposal that was awarded the Large VLA Project time, carried out the observations, manages the team and organizes workshops. |
Collaborator Contribution | Contributed to the science case and the exploitation of the data. |
Impact | Data acquisition Data analysis New knowledge Project leadership Publications Online catalogue |
Start Year | 2006 |
Description | The CORNISH Radio Survey |
Organisation | University of Manchester |
Department | School of Physics and Astronomy Manchester |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Hoare leads the team, was PI of the proposal that was awarded the Large VLA Project time, carried out the observations, manages the team and organizes workshops. |
Collaborator Contribution | Contributed to the science case and the exploitation of the data. |
Impact | Data acquisition Data analysis New knowledge Project leadership Publications Online catalogue |
Start Year | 2006 |
Description | The CORNISH Radio Survey |
Organisation | University of Maryland |
Department | Department of Astronomy |
Country | United States |
Sector | Academic/University |
PI Contribution | Hoare leads the team, was PI of the proposal that was awarded the Large VLA Project time, carried out the observations, manages the team and organizes workshops. |
Collaborator Contribution | Contributed to the science case and the exploitation of the data. |
Impact | Data acquisition Data analysis New knowledge Project leadership Publications Online catalogue |
Start Year | 2006 |
Description | The CORNISH Radio Survey |
Organisation | University of Southampton |
Department | Physics and Astronomy |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Hoare leads the team, was PI of the proposal that was awarded the Large VLA Project time, carried out the observations, manages the team and organizes workshops. |
Collaborator Contribution | Contributed to the science case and the exploitation of the data. |
Impact | Data acquisition Data analysis New knowledge Project leadership Publications Online catalogue |
Start Year | 2006 |
Description | The CORNISH Radio Survey |
Organisation | University of Wisconsin-Madison |
Department | Department of Astronomy |
Country | United States |
Sector | Academic/University |
PI Contribution | Hoare leads the team, was PI of the proposal that was awarded the Large VLA Project time, carried out the observations, manages the team and organizes workshops. |
Collaborator Contribution | Contributed to the science case and the exploitation of the data. |
Impact | Data acquisition Data analysis New knowledge Project leadership Publications Online catalogue |
Start Year | 2006 |
Description | The CORNISH-South Radio Survey |
Organisation | Boston University |
Country | United States |
Sector | Academic/University |
PI Contribution | Hoare led the collaboration and was PI of the application for the ATCA Large Project. He conducted the observations and manages the team. Lumsden and Oudmaijer are team members. |
Collaborator Contribution | Contributed to the science case for the proposal and developed science teams to exploit the data. |
Impact | Data acquisition - 450 hours of ATCA survey data Data analysis New knowledge Project Leadership |
Start Year | 2009 |
Description | The CORNISH-South Radio Survey |
Organisation | California Institute of Technology |
Department | Infrared Processing and Analysis Center |
Country | United States |
Sector | Academic/University |
PI Contribution | Hoare led the collaboration and was PI of the application for the ATCA Large Project. He conducted the observations and manages the team. Lumsden and Oudmaijer are team members. |
Collaborator Contribution | Contributed to the science case for the proposal and developed science teams to exploit the data. |
Impact | Data acquisition - 450 hours of ATCA survey data Data analysis New knowledge Project Leadership |
Start Year | 2009 |
Description | The CORNISH-South Radio Survey |
Organisation | Catania Astrophysical Observatory |
Country | Italy |
Sector | Public |
PI Contribution | Hoare led the collaboration and was PI of the application for the ATCA Large Project. He conducted the observations and manages the team. Lumsden and Oudmaijer are team members. |
Collaborator Contribution | Contributed to the science case for the proposal and developed science teams to exploit the data. |
Impact | Data acquisition - 450 hours of ATCA survey data Data analysis New knowledge Project Leadership |
Start Year | 2009 |
Description | The CORNISH-South Radio Survey |
Organisation | Commonwealth Scientific and Industrial Research Organisation |
Country | Australia |
Sector | Public |
PI Contribution | Hoare led the collaboration and was PI of the application for the ATCA Large Project. He conducted the observations and manages the team. Lumsden and Oudmaijer are team members. |
Collaborator Contribution | Contributed to the science case for the proposal and developed science teams to exploit the data. |
Impact | Data acquisition - 450 hours of ATCA survey data Data analysis New knowledge Project Leadership |
Start Year | 2009 |
Description | The CORNISH-South Radio Survey |
Organisation | Dominion Radio Astrophysical Observatory |
Country | Canada |
Sector | Public |
PI Contribution | Hoare led the collaboration and was PI of the application for the ATCA Large Project. He conducted the observations and manages the team. Lumsden and Oudmaijer are team members. |
Collaborator Contribution | Contributed to the science case for the proposal and developed science teams to exploit the data. |
Impact | Data acquisition - 450 hours of ATCA survey data Data analysis New knowledge Project Leadership |
Start Year | 2009 |
Description | The CORNISH-South Radio Survey |
Organisation | Liverpool John Moores University |
Department | Astrophysics Research Institute |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Hoare led the collaboration and was PI of the application for the ATCA Large Project. He conducted the observations and manages the team. Lumsden and Oudmaijer are team members. |
Collaborator Contribution | Contributed to the science case for the proposal and developed science teams to exploit the data. |
Impact | Data acquisition - 450 hours of ATCA survey data Data analysis New knowledge Project Leadership |
Start Year | 2009 |
Description | The CORNISH-South Radio Survey |
Organisation | National Autonomous University of Mexico |
Country | Mexico |
Sector | Academic/University |
PI Contribution | Hoare led the collaboration and was PI of the application for the ATCA Large Project. He conducted the observations and manages the team. Lumsden and Oudmaijer are team members. |
Collaborator Contribution | Contributed to the science case for the proposal and developed science teams to exploit the data. |
Impact | Data acquisition - 450 hours of ATCA survey data Data analysis New knowledge Project Leadership |
Start Year | 2009 |
Description | The CORNISH-South Radio Survey |
Organisation | National Institute for Astrophysics |
Department | Arcetri Observatory |
Country | Italy |
Sector | Public |
PI Contribution | Hoare led the collaboration and was PI of the application for the ATCA Large Project. He conducted the observations and manages the team. Lumsden and Oudmaijer are team members. |
Collaborator Contribution | Contributed to the science case for the proposal and developed science teams to exploit the data. |
Impact | Data acquisition - 450 hours of ATCA survey data Data analysis New knowledge Project Leadership |
Start Year | 2009 |
Description | The CORNISH-South Radio Survey |
Organisation | National Institute for Astrophysics |
Department | IFSI Rome |
Country | Italy |
Sector | Academic/University |
PI Contribution | Hoare led the collaboration and was PI of the application for the ATCA Large Project. He conducted the observations and manages the team. Lumsden and Oudmaijer are team members. |
Collaborator Contribution | Contributed to the science case for the proposal and developed science teams to exploit the data. |
Impact | Data acquisition - 450 hours of ATCA survey data Data analysis New knowledge Project Leadership |
Start Year | 2009 |
Description | The CORNISH-South Radio Survey |
Organisation | National Radio Astronomy Observatory (NRAO) |
Country | United States |
Sector | Public |
PI Contribution | Hoare led the collaboration and was PI of the application for the ATCA Large Project. He conducted the observations and manages the team. Lumsden and Oudmaijer are team members. |
Collaborator Contribution | Contributed to the science case for the proposal and developed science teams to exploit the data. |
Impact | Data acquisition - 450 hours of ATCA survey data Data analysis New knowledge Project Leadership |
Start Year | 2009 |
Description | The CORNISH-South Radio Survey |
Organisation | University of Barcelona |
Department | Faculty of Physics |
Country | Spain |
Sector | Academic/University |
PI Contribution | Hoare led the collaboration and was PI of the application for the ATCA Large Project. He conducted the observations and manages the team. Lumsden and Oudmaijer are team members. |
Collaborator Contribution | Contributed to the science case for the proposal and developed science teams to exploit the data. |
Impact | Data acquisition - 450 hours of ATCA survey data Data analysis New knowledge Project Leadership |
Start Year | 2009 |
Description | The CORNISH-South Radio Survey |
Organisation | University of Hertfordshire |
Department | Centre for Astrophysics Research (CAR) |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Hoare led the collaboration and was PI of the application for the ATCA Large Project. He conducted the observations and manages the team. Lumsden and Oudmaijer are team members. |
Collaborator Contribution | Contributed to the science case for the proposal and developed science teams to exploit the data. |
Impact | Data acquisition - 450 hours of ATCA survey data Data analysis New knowledge Project Leadership |
Start Year | 2009 |
Description | The CORNISH-South Radio Survey |
Organisation | University of Jaen |
Department | Department of Physics |
Country | Spain |
Sector | Academic/University |
PI Contribution | Hoare led the collaboration and was PI of the application for the ATCA Large Project. He conducted the observations and manages the team. Lumsden and Oudmaijer are team members. |
Collaborator Contribution | Contributed to the science case for the proposal and developed science teams to exploit the data. |
Impact | Data acquisition - 450 hours of ATCA survey data Data analysis New knowledge Project Leadership |
Start Year | 2009 |
Description | The CORNISH-South Radio Survey |
Organisation | University of Manchester |
Department | School of Physics and Astronomy Manchester |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Hoare led the collaboration and was PI of the application for the ATCA Large Project. He conducted the observations and manages the team. Lumsden and Oudmaijer are team members. |
Collaborator Contribution | Contributed to the science case for the proposal and developed science teams to exploit the data. |
Impact | Data acquisition - 450 hours of ATCA survey data Data analysis New knowledge Project Leadership |
Start Year | 2009 |
Description | The CORNISH-South Radio Survey |
Organisation | University of Maryland |
Country | United States |
Sector | Academic/University |
PI Contribution | Hoare led the collaboration and was PI of the application for the ATCA Large Project. He conducted the observations and manages the team. Lumsden and Oudmaijer are team members. |
Collaborator Contribution | Contributed to the science case for the proposal and developed science teams to exploit the data. |
Impact | Data acquisition - 450 hours of ATCA survey data Data analysis New knowledge Project Leadership |
Start Year | 2009 |
Description | The CORNISH-South Radio Survey |
Organisation | University of New South Wales |
Department | School of Physics |
Country | Australia |
Sector | Academic/University |
PI Contribution | Hoare led the collaboration and was PI of the application for the ATCA Large Project. He conducted the observations and manages the team. Lumsden and Oudmaijer are team members. |
Collaborator Contribution | Contributed to the science case for the proposal and developed science teams to exploit the data. |
Impact | Data acquisition - 450 hours of ATCA survey data Data analysis New knowledge Project Leadership |
Start Year | 2009 |
Description | The CORNISH-South Radio Survey |
Organisation | University of Southampton |
Department | Physics and Astronomy |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Hoare led the collaboration and was PI of the application for the ATCA Large Project. He conducted the observations and manages the team. Lumsden and Oudmaijer are team members. |
Collaborator Contribution | Contributed to the science case for the proposal and developed science teams to exploit the data. |
Impact | Data acquisition - 450 hours of ATCA survey data Data analysis New knowledge Project Leadership |
Start Year | 2009 |
Description | The CORNISH-South Radio Survey |
Organisation | University of Sydney |
Department | School of Physics |
Country | Australia |
Sector | Academic/University |
PI Contribution | Hoare led the collaboration and was PI of the application for the ATCA Large Project. He conducted the observations and manages the team. Lumsden and Oudmaijer are team members. |
Collaborator Contribution | Contributed to the science case for the proposal and developed science teams to exploit the data. |
Impact | Data acquisition - 450 hours of ATCA survey data Data analysis New knowledge Project Leadership |
Start Year | 2009 |
Description | The CORNISH-South Radio Survey |
Organisation | University of Tasmania |
Department | Discipline of Mathematics and Physics |
Country | Australia |
Sector | Academic/University |
PI Contribution | Hoare led the collaboration and was PI of the application for the ATCA Large Project. He conducted the observations and manages the team. Lumsden and Oudmaijer are team members. |
Collaborator Contribution | Contributed to the science case for the proposal and developed science teams to exploit the data. |
Impact | Data acquisition - 450 hours of ATCA survey data Data analysis New knowledge Project Leadership |
Start Year | 2009 |
Description | The CORNISH-South Radio Survey |
Organisation | University of Wisconsin-Madison |
Department | Department of Astronomy |
Country | United States |
Sector | Academic/University |
PI Contribution | Hoare led the collaboration and was PI of the application for the ATCA Large Project. He conducted the observations and manages the team. Lumsden and Oudmaijer are team members. |
Collaborator Contribution | Contributed to the science case for the proposal and developed science teams to exploit the data. |
Impact | Data acquisition - 450 hours of ATCA survey data Data analysis New knowledge Project Leadership |
Start Year | 2009 |
Description | The RMS Survey |
Organisation | Liverpool John Moores University |
Department | Astrophysics Research Institute |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Hoare, Lumsden and Oudmaijer are the co-PIs of the RMS survey that has conducted a mid-IR search for massive YSOs in the Galaxy and an extensive follow-up campaign. |
Collaborator Contribution | Contributed to the data taking and exploitation. |
Impact | Publications Project Leadership. New Knowledge Data acquisition Data analysis |
Description | The RMS Survey |
Organisation | University of New South Wales |
Department | School of Physics |
Country | Australia |
Sector | Academic/University |
PI Contribution | Hoare, Lumsden and Oudmaijer are the co-PIs of the RMS survey that has conducted a mid-IR search for massive YSOs in the Galaxy and an extensive follow-up campaign. |
Collaborator Contribution | Contributed to the data taking and exploitation. |
Impact | Publications Project Leadership. New Knowledge Data acquisition Data analysis |
Description | X-Shooting Herbig Ae/Be stars |
Organisation | Armagh Observatory and Planetarium |
Department | Armagh Observatory |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Oudmaijer leads this collaboration to use the VLT in a spectroscopic survey. PI of the proposal, manages the team and organises the work. |
Collaborator Contribution | Contribute to the science case and the exploitation. |
Impact | Publications New knowledge Data acquistion Data analysis. |
Description | X-Shooting Herbig Ae/Be stars |
Organisation | European Southern Observatory (ESO) |
Country | Germany |
Sector | Charity/Non Profit |
PI Contribution | Oudmaijer leads this collaboration to use the VLT in a spectroscopic survey. PI of the proposal, manages the team and organises the work. |
Collaborator Contribution | Contribute to the science case and the exploitation. |
Impact | Publications New knowledge Data acquistion Data analysis. |
Description | X-Shooting Herbig Ae/Be stars |
Organisation | European Space Agency |
Department | European Space Astronomy Centre (ESAC) |
Country | Spain |
Sector | Public |
PI Contribution | Oudmaijer leads this collaboration to use the VLT in a spectroscopic survey. PI of the proposal, manages the team and organises the work. |
Collaborator Contribution | Contribute to the science case and the exploitation. |
Impact | Publications New knowledge Data acquistion Data analysis. |
Description | X-Shooting Herbig Ae/Be stars |
Organisation | University of Hertfordshire |
Department | Centre for Astrophysics Research (CAR) |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Oudmaijer leads this collaboration to use the VLT in a spectroscopic survey. PI of the proposal, manages the team and organises the work. |
Collaborator Contribution | Contribute to the science case and the exploitation. |
Impact | Publications New knowledge Data acquistion Data analysis. |
Description | e-Merlin Legacy Survey on Feedback in Massive Star Formation |
Organisation | Armagh Observatory and Planetarium |
Department | Armagh Observatory |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Hoare is the Principal Investigator for this radio continuum survey. He led the international team that proposed for this survey and is the main point of contact for the observatory carrying out the observations. The Leeds group leads the target selection, data reduction and analysis. |
Collaborator Contribution | The international team contributed to the original proposal for the survey and will contribute to the interpretation of the results. A subset of partners lead the methanol maser polarization data that is taken simultaneously with the radio continuum data. |
Impact | No yet. |
Start Year | 2008 |
Description | e-Merlin Legacy Survey on Feedback in Massive Star Formation |
Organisation | Chalmers University of Technology |
Country | Sweden |
Sector | Academic/University |
PI Contribution | Hoare is the Principal Investigator for this radio continuum survey. He led the international team that proposed for this survey and is the main point of contact for the observatory carrying out the observations. The Leeds group leads the target selection, data reduction and analysis. |
Collaborator Contribution | The international team contributed to the original proposal for the survey and will contribute to the interpretation of the results. A subset of partners lead the methanol maser polarization data that is taken simultaneously with the radio continuum data. |
Impact | No yet. |
Start Year | 2008 |
Description | e-Merlin Legacy Survey on Feedback in Massive Star Formation |
Organisation | DePaul University |
Country | United States |
Sector | Academic/University |
PI Contribution | Hoare is the Principal Investigator for this radio continuum survey. He led the international team that proposed for this survey and is the main point of contact for the observatory carrying out the observations. The Leeds group leads the target selection, data reduction and analysis. |
Collaborator Contribution | The international team contributed to the original proposal for the survey and will contribute to the interpretation of the results. A subset of partners lead the methanol maser polarization data that is taken simultaneously with the radio continuum data. |
Impact | No yet. |
Start Year | 2008 |
Description | e-Merlin Legacy Survey on Feedback in Massive Star Formation |
Organisation | Leiden University |
Country | Netherlands |
Sector | Academic/University |
PI Contribution | Hoare is the Principal Investigator for this radio continuum survey. He led the international team that proposed for this survey and is the main point of contact for the observatory carrying out the observations. The Leeds group leads the target selection, data reduction and analysis. |
Collaborator Contribution | The international team contributed to the original proposal for the survey and will contribute to the interpretation of the results. A subset of partners lead the methanol maser polarization data that is taken simultaneously with the radio continuum data. |
Impact | No yet. |
Start Year | 2008 |
Description | e-Merlin Legacy Survey on Feedback in Massive Star Formation |
Organisation | Liverpool John Moores University |
Department | Astrophysics Research Institute |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Hoare is the Principal Investigator for this radio continuum survey. He led the international team that proposed for this survey and is the main point of contact for the observatory carrying out the observations. The Leeds group leads the target selection, data reduction and analysis. |
Collaborator Contribution | The international team contributed to the original proposal for the survey and will contribute to the interpretation of the results. A subset of partners lead the methanol maser polarization data that is taken simultaneously with the radio continuum data. |
Impact | No yet. |
Start Year | 2008 |
Description | e-Merlin Legacy Survey on Feedback in Massive Star Formation |
Organisation | Max Planck Society |
Department | Max Planck Institute for Astronomy |
Country | Germany |
Sector | Academic/University |
PI Contribution | Hoare is the Principal Investigator for this radio continuum survey. He led the international team that proposed for this survey and is the main point of contact for the observatory carrying out the observations. The Leeds group leads the target selection, data reduction and analysis. |
Collaborator Contribution | The international team contributed to the original proposal for the survey and will contribute to the interpretation of the results. A subset of partners lead the methanol maser polarization data that is taken simultaneously with the radio continuum data. |
Impact | No yet. |
Start Year | 2008 |
Description | e-Merlin Legacy Survey on Feedback in Massive Star Formation |
Organisation | NRC Canada |
Country | Canada |
Sector | Public |
PI Contribution | Hoare is the Principal Investigator for this radio continuum survey. He led the international team that proposed for this survey and is the main point of contact for the observatory carrying out the observations. The Leeds group leads the target selection, data reduction and analysis. |
Collaborator Contribution | The international team contributed to the original proposal for the survey and will contribute to the interpretation of the results. A subset of partners lead the methanol maser polarization data that is taken simultaneously with the radio continuum data. |
Impact | No yet. |
Start Year | 2008 |
Description | e-Merlin Legacy Survey on Feedback in Massive Star Formation |
Organisation | National Astronomical Research Institute Of Thailand |
Country | Thailand |
Sector | Public |
PI Contribution | Hoare is the Principal Investigator for this radio continuum survey. He led the international team that proposed for this survey and is the main point of contact for the observatory carrying out the observations. The Leeds group leads the target selection, data reduction and analysis. |
Collaborator Contribution | The international team contributed to the original proposal for the survey and will contribute to the interpretation of the results. A subset of partners lead the methanol maser polarization data that is taken simultaneously with the radio continuum data. |
Impact | No yet. |
Start Year | 2008 |
Description | e-Merlin Legacy Survey on Feedback in Massive Star Formation |
Organisation | National Autonomous University of Mexico |
Department | Radio Astronomy |
Country | Mexico |
Sector | Academic/University |
PI Contribution | Hoare is the Principal Investigator for this radio continuum survey. He led the international team that proposed for this survey and is the main point of contact for the observatory carrying out the observations. The Leeds group leads the target selection, data reduction and analysis. |
Collaborator Contribution | The international team contributed to the original proposal for the survey and will contribute to the interpretation of the results. A subset of partners lead the methanol maser polarization data that is taken simultaneously with the radio continuum data. |
Impact | No yet. |
Start Year | 2008 |
Description | e-Merlin Legacy Survey on Feedback in Massive Star Formation |
Organisation | National Institute for Astrophysics |
Country | Italy |
Sector | Academic/University |
PI Contribution | Hoare is the Principal Investigator for this radio continuum survey. He led the international team that proposed for this survey and is the main point of contact for the observatory carrying out the observations. The Leeds group leads the target selection, data reduction and analysis. |
Collaborator Contribution | The international team contributed to the original proposal for the survey and will contribute to the interpretation of the results. A subset of partners lead the methanol maser polarization data that is taken simultaneously with the radio continuum data. |
Impact | No yet. |
Start Year | 2008 |
Description | e-Merlin Legacy Survey on Feedback in Massive Star Formation |
Organisation | National Radio Astronomy Observatory (NRAO) |
Country | United States |
Sector | Public |
PI Contribution | Hoare is the Principal Investigator for this radio continuum survey. He led the international team that proposed for this survey and is the main point of contact for the observatory carrying out the observations. The Leeds group leads the target selection, data reduction and analysis. |
Collaborator Contribution | The international team contributed to the original proposal for the survey and will contribute to the interpretation of the results. A subset of partners lead the methanol maser polarization data that is taken simultaneously with the radio continuum data. |
Impact | No yet. |
Start Year | 2008 |
Description | e-Merlin Legacy Survey on Feedback in Massive Star Formation |
Organisation | University of Barcelona |
Department | Institute for Space Studies of Catalonia (IEEC) |
Country | Spain |
Sector | Academic/University |
PI Contribution | Hoare is the Principal Investigator for this radio continuum survey. He led the international team that proposed for this survey and is the main point of contact for the observatory carrying out the observations. The Leeds group leads the target selection, data reduction and analysis. |
Collaborator Contribution | The international team contributed to the original proposal for the survey and will contribute to the interpretation of the results. A subset of partners lead the methanol maser polarization data that is taken simultaneously with the radio continuum data. |
Impact | No yet. |
Start Year | 2008 |
Description | e-Merlin Legacy Survey on Feedback in Massive Star Formation |
Organisation | University of Cambridge |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Hoare is the Principal Investigator for this radio continuum survey. He led the international team that proposed for this survey and is the main point of contact for the observatory carrying out the observations. The Leeds group leads the target selection, data reduction and analysis. |
Collaborator Contribution | The international team contributed to the original proposal for the survey and will contribute to the interpretation of the results. A subset of partners lead the methanol maser polarization data that is taken simultaneously with the radio continuum data. |
Impact | No yet. |
Start Year | 2008 |
Description | e-Merlin Legacy Survey on Feedback in Massive Star Formation |
Organisation | University of Manchester |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Hoare is the Principal Investigator for this radio continuum survey. He led the international team that proposed for this survey and is the main point of contact for the observatory carrying out the observations. The Leeds group leads the target selection, data reduction and analysis. |
Collaborator Contribution | The international team contributed to the original proposal for the survey and will contribute to the interpretation of the results. A subset of partners lead the methanol maser polarization data that is taken simultaneously with the radio continuum data. |
Impact | No yet. |
Start Year | 2008 |
Description | e-Merlin Legacy Survey on Feedback in Massive Star Formation |
Organisation | University of Tasmania |
Country | Australia |
Sector | Academic/University |
PI Contribution | Hoare is the Principal Investigator for this radio continuum survey. He led the international team that proposed for this survey and is the main point of contact for the observatory carrying out the observations. The Leeds group leads the target selection, data reduction and analysis. |
Collaborator Contribution | The international team contributed to the original proposal for the survey and will contribute to the interpretation of the results. A subset of partners lead the methanol maser polarization data that is taken simultaneously with the radio continuum data. |
Impact | No yet. |
Start Year | 2008 |
Description | e-Merlin Legacy Survey on Feedback in Massive Star Formation |
Organisation | University of Western Australia |
Country | Australia |
Sector | Academic/University |
PI Contribution | Hoare is the Principal Investigator for this radio continuum survey. He led the international team that proposed for this survey and is the main point of contact for the observatory carrying out the observations. The Leeds group leads the target selection, data reduction and analysis. |
Collaborator Contribution | The international team contributed to the original proposal for the survey and will contribute to the interpretation of the results. A subset of partners lead the methanol maser polarization data that is taken simultaneously with the radio continuum data. |
Impact | No yet. |
Start Year | 2008 |
Description | A media interview for international news with CNN by email |
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 | Responding to an enquiry from a CNN writer & producer, Ashley Strickland, Dr Wareing providing the answers to several questions by email, which led to a high impact CNN article, published online and syndicated around the US and internationally (e.g. CNN Phillipines). |
Year(s) Of Engagement Activity | 2018 |
URL | https://edition.cnn.com/2018/02/14/world/rosette-nebula-heart/index.html |
Description | A media interview for international news with Cosmos Magazine by email |
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 | Responding to an email enquiry following the Rosette Nebula Press Release, Dr Wareing replied to questions by email from Phil Dooley, a freelance journalist for Australian magazine Cosmos. |
Year(s) Of Engagement Activity | 2018 |
URL | https://cosmosmagazine.com/space/solving-the-riddle-at-a-nebula-s-heart |
Description | A phone interview for the press release on massive young stellar binaries PDS 27 and PDS 37 for Live Science in the United States |
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 | Public/other audiences |
Results and Impact | A Press article (see URL) was prepared based on our official press release and phone interview for our paper on the massive young stellar objects PDS 27 and PDS 37. |
Year(s) Of Engagement Activity | 2019 |
URL | https://www.livescience.com/64972-twin-baby-giant-stars.html |
Description | A talk for Huddersfield Astronomical Society |
Form Of Engagement Activity | A talk or presentation |
Part Of Official Scheme? | No |
Geographic Reach | Local |
Primary Audience | Public/other audiences |
Results and Impact | This was a general presentation on the interesting aspects of my recent Rosette Nebula research, given to an astronomical society with members who have a special interest in astronomy, but generally no professional qualifications in the area. |
Year(s) Of Engagement Activity | 2019 |
Description | A talk for Leeds Astronomical Society |
Form Of Engagement Activity | A talk or presentation |
Part Of Official Scheme? | No |
Geographic Reach | Local |
Primary Audience | Public/other audiences |
Results and Impact | This was a general presentation on the interesting aspects of my recent Rosette Nebula research, given to an astronomical society with members who have a special interest in astronomy, but generally no professional qualifications in the area. |
Year(s) Of Engagement Activity | 2018 |
Description | An interview for BBC Local Radio Yorkshire and Lincolnshire - Paul Hudson Weather Show |
Form Of Engagement Activity | A press release, press conference or response to a media enquiry/interview |
Part Of Official Scheme? | No |
Geographic Reach | Regional |
Primary Audience | Media (as a channel to the public) |
Results and Impact | Following the Rosette Nebula Press Release, Dr Wareing was interviewed for the Paul Hudson Weather Show on BBC Local Radio for Yorkshire and Lincolnshire, broadcast on 17th March 2018. |
Year(s) Of Engagement Activity | 2018 |
URL | http://www.bbc.co.uk/programmes/p016jv8d |
Description | Be stars come in triples |
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 | press releae altmetric score 516 |
Year(s) Of Engagement Activity | 2023 |
URL | https://www.leeds.ac.uk/news-1/news/article/5460/new-insight-into-stellar-evolution |
Description | Demonstrated a 3D hologram screen for teaching and outreach |
Form Of Engagement Activity | Participation in an activity, workshop or similar |
Part Of Official Scheme? | No |
Geographic Reach | National |
Primary Audience | Professional Practitioners |
Results and Impact | Demonstrated a 3D hologram screen for teaching and outreach in astronomy (designed and built at Leeds) during a 1-hr workshop at the Advance HE STEM Conference 2019 (Jan 2019). Attendees reported that they may use this method/equipment in their own teaching in other disciplines. |
Year(s) Of Engagement Activity | 2019 |
URL | https://www.advance-he.ac.uk/programmes-events/calendar/stem-teaching-and-learning-conference-2019 |
Description | GoStargazing 2018 |
Form Of Engagement Activity | A talk or presentation |
Part Of Official Scheme? | No |
Geographic Reach | Local |
Primary Audience | Public/other audiences |
Results and Impact | Hoare and Lumsden gave a talk and Q&A session at the GoStargazing event organised by Leeds Astronomical Society on Feb 16th 2018. |
Year(s) Of Engagement Activity | 2018 |
Description | Groundwork Schools Event |
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 | One day event for several local schools in Cornwall at Goonhilly Earth Station linked to the Groundwork art exhibition in which we contributed e-MERLIN data to a video installation. Hoare presented a talk on radio astronomy and the dish conversion work at Goonhilly. |
Year(s) Of Engagement Activity | 2018 |
URL | https://groundwork.art/ |
Description | HF Holiday February 2020 |
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 | 15 members of the public attended a 3 day astronomy leisure holiday led by Hoare. Audience were all elderly including one person who lives in Switzerland. All reported new interest in astronomy and requested further resources. |
Year(s) Of Engagement Activity | 2020 |
Description | HF Holiday March 2019 |
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 | 6 members of the public attended a 3 day astronomy leisure activity holiday led by Hoare. Audience mostly elderly. |
Year(s) Of Engagement Activity | 2019 |
Description | HF Holiday November 2019 |
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 | 7 members of the public attended a 3 day astronomy leisure holiday led by Hoare. Audience were all elderly and reported new interest in the astronomy. |
Year(s) Of Engagement Activity | 2019 |
Description | Invited talk at Advanced Cooling with Carbon Dioxide - CO2 machining applications, Nuclear AMRC, Sheffield |
Form Of Engagement Activity | A talk or presentation |
Part Of Official Scheme? | No |
Geographic Reach | International |
Primary Audience | Industry/Business |
Results and Impact | Following successful collaborative work in 2017, Dr Wareing was invited to present at this one-day forum (Monday 15th January 2018) which brought together technology providers - including USA-based Fusion Coolant Systems, supplier of the Nuclear AMRC's system - with industrial users and researchers to discuss the opportunities and challenges of CO2 coolants in cryogenic machining scenarios. The talk was entitled "Numerical simulation of cryogenic machining with CO2 - applying expertise from the carbon capture and storage sector". The talk was well received, with audience clearly changing their view and questions from industry (Fusion Coolant Systems, SECO tools and BOC gases) and academia. Requests have followed for involvement in planned INNOVATE and EPSRC projects. |
Year(s) Of Engagement Activity | 2018 |
URL | http://namrc.co.uk/wp-content/uploads/2018/01/CO2-event-Jan18.pdf |
Description | Organisation and participation as host/demonstrator for Pint of Science, Leeds |
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 | Organisation of and participation in three events in pubs presenting work being carried out by researchers at University of Leeds to the general public, concentrating on reaching audiences who would not normally be interested in science. Katharine Johnston hosted the astronomy event in 2017 and prepared/built a interactive demonstration of how astronomers search for exoplanets. |
Year(s) Of Engagement Activity | 2016,2017 |
URL | https://pintofscience.co.uk/ |
Description | Physics 6th Form Conference 2017 |
Form Of Engagement Activity | Participation in an activity, workshop or similar |
Part Of Official Scheme? | No |
Geographic Reach | Regional |
Primary Audience | Schools |
Results and Impact | Dr Wareing presented the poster created as part of Work Experience Week 2017 at the School of Physics and Astronomy's Physics 6th Form Conference at a lunchtime Poster Session on Monday 4th December 2017. Many students asked questions about the work, as well as the odd undergrad/postgrad and member of the general public as the event was in the Parkinson Court public reception space at the University of Leeds. |
Year(s) Of Engagement Activity | 2017 |
URL | https://www.eventbrite.co.uk/e/physics-sixth-form-conference-registration-38532435552 |
Description | Popular astronomy talk at Cleveland & Darlington Astronomical 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 | Talk given by Katharine Johnston in May 2018. The talk increased interest in this research field (star formation with radio telescopes) amongst astronomy enthusiasts in the region. This also led to other astronomy societies booking talks on the same topic. |
Year(s) Of Engagement Activity | 2018 |
Description | Popular astronomy talk at Doncaster Astronomical Society |
Form Of Engagement Activity | A talk or presentation |
Part Of Official Scheme? | No |
Geographic Reach | Local |
Primary Audience | Public/other audiences |
Results and Impact | Gave popular astronomy talk on ALMA and star formation to Doncaster Astronomical Society, which disseminated information and sparked interest in my field of research. |
Year(s) Of Engagement Activity | 2020 |
URL | https://www.donastro.org.uk/meetings/ |
Description | Popular astronomy talk at Harrogate Astronomical 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 | Talk given by Katharine Johnston in March 2019. The talk increased interest in this research field (star formation with radio telescopes) amongst Harrogate astronomy enthusiasts. |
Year(s) Of Engagement Activity | 2019 |
Description | Presenting a holographic screen with astronomy animations at "Eureka! Late" at Eureka! The National Children's Museum, Halifax |
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 | Presented a 3D holographic screen to adult visitors to this event (Eureka! Late), increasing their interest in astronomy and optics. Participants also got to make their own holographic projectors for their smart phones. |
Year(s) Of Engagement Activity | 2019 |
Description | Presenting a holographic screen with astronomy animations at "The Shape of Games to Come Workshop: Launch of the Centre for Immersive Technologies & Virtuocity" at Leeds |
Form Of Engagement Activity | Participation in an activity, workshop or similar |
Part Of Official Scheme? | No |
Geographic Reach | National |
Primary Audience | Professional Practitioners |
Results and Impact | Presented the 3D holographic screen designed and developed at Leeds to aid teaching and outreach at a networking event with >100 participants at "The Shape of Games to Come Workshop: Launch of the Centre for Immersive Technologies & Virtuocity" at Leeds. Explained astronomy and optics to participants, and increased their knowledge of this type of virtual display and astronomy research being carried out at the University of Leeds. |
Year(s) Of Engagement Activity | 2019 |
Description | Presenting animated holograms and poster at NAM 2019: "Engaging the public and schools with science through the solar system" session, Lancaster University, UK |
Form Of Engagement Activity | Participation in an activity, workshop or similar |
Part Of Official Scheme? | No |
Geographic Reach | National |
Primary Audience | Professional Practitioners |
Results and Impact | Presented poster and 3D animated holograms designed and developed at Leeds to aid teaching and outreach at a networking event with >100 participants at "Engaging the public and schools with science through the solar system" session at NAM taking place in Lancaster. Explained astronomy and optics to participants, and increased their knowledge of this type of virtual display and astronomy research being carried out at the University of Leeds. |
Year(s) Of Engagement Activity | 2019 |
URL | https://nam2019.org/press-releases/179-nam2019-3d-holograms-bringing-astronomy-to-life |
Description | Press Release - Rosette Nebula |
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 | A Press Release (see URL) was prepared to accompany the publication of our paper on the Rosette Nebula (see DOI). The Release was timed to coincide with Valentine's Day 2018 as the heart shape of the Rosette Nebula is an often-reproduced image at this time. This was an exceptionally effective approach, resulting in an Altmetric score of 156, in the "top 5% of all research outputs scored by Altmetric". In context, as of 21st February 2018, for quality and quantity of online attention received, this placed the paper in the top 60,000 of 9 million outputs ever tracked and 101st of 7,050 outputs ever tracked from the Monthly Notices of the Royal Astronomical Society. Altmetrics note that "MNRAS outputs typically receive a lot more attention than average, with a mean attention score of 12.5, but this work has done particularly well, scoring higher than 98% of its peers". Altmetrics saw 16 news stories from 16 outlets, but our own tracking of individual news pieces saw more than 100 news stories from 100 different outlets, albeit many of which were syndicated from CNN. At the time of the Press Release, journalists from CNN (USA) and Cosmos Magazine (Australia) contacted Dr Wareing for further interview by email and since then, Dr Wareing has been recorded (on 14th March 2018) to appear on the Paul Hudson Weather show for BBC local radio in Yorkshire and Lincolnshire, UK (to be broadcast 17th March 2018). News stories have appeared internationally, including in the UK, many states of the USA, Spain, Italy, Finland, Romania, Poland, Russia, Iran, India, the Philippines, Australia and unconfirmed in China. We have tracked public discussion of the work following the news and blog articles in the UK, USA and Russia, and in the sincerest form of flattery, production of online art based on the key imagery of the Press Release [by Michael Petter, an Ecologer/Artist living in Brisbane, Queensland, Australia https://www.facebook.com/photo.php?fbid=10214152969971408&set=a.3647418957271.156621.1628341103&type=3&theater ]. |
Year(s) Of Engagement Activity | 2018 |
URL | https://www.leeds.ac.uk/news/article/4183/new_models_give_insight_into_the_heart_of_the_rosette_nebu... |
Description | Press release - massive young stellar binaries PDS 27 and PDS 37 |
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 | Public/other audiences |
Results and Impact | A Press Release (see URL) was prepared to accompany the publication of our paper on the massive young stellar objects PDS 27 and PDS 37 (see DOI). The story was redistributed via more journals, blogs and tweets (at least 16 outlets, 3 blogs and 9 tweeters) targeting a general audience and in more countries (e.g., Germany, Canada, US, Russia). Few examples : Phys.org, the Register, Infowars, University news story and more. The story triggered dialogs and engangement among the public. According to Atmetric, it reached about 90% public audience and 10% scientists. According to atmetric scores, this research output has an Altmetric Attention Score of 141, higher than 98% of its contemporaries. |
Year(s) Of Engagement Activity | 2019 |
URL | https://www.leeds.ac.uk/news/article/4379/massive_twin_star_snuggles_close_to_its_stellar_sibling |
Description | Public Talk |
Form Of Engagement Activity | A talk or presentation |
Part Of Official Scheme? | No |
Geographic Reach | Regional |
Primary Audience | Public/other audiences |
Results and Impact | Talk on massive star formation to Harrogate Astronomical Society on 28/10/21 |
Year(s) Of Engagement Activity | 2021 |
Description | Public Talk in Hull |
Form Of Engagement Activity | A talk or presentation |
Part Of Official Scheme? | No |
Geographic Reach | Regional |
Primary Audience | Public/other audiences |
Results and Impact | Talk on massive star formation to the Hull and East Riding Astronomical Society on 14/3/22 |
Year(s) Of Engagement Activity | 2022 |
Description | School Visit (Cavendish Primary School Manchester) |
Form Of Engagement Activity | A talk or presentation |
Part Of Official Scheme? | No |
Geographic Reach | Local |
Primary Audience | Schools |
Results and Impact | 7th June 2019. Visited a Primary School to talk to Year 1 (3 classes; 1 teacher, 1 or 2 TAs and 30 children per class) at the start of their Space topic this term. Short presentations per class (5-10 minutes), followed by 20-30 minutes of questions per class. Each Teacher reported pre-formulated questions from classes and high interest from the children during and following the event, even in this Key Stage 1 age group. |
Year(s) Of Engagement Activity | 2019 |
Description | Scottish Government Working Group |
Form Of Engagement Activity | A formal working group, expert panel or dialogue |
Part Of Official Scheme? | No |
Geographic Reach | National |
Primary Audience | Policymakers/politicians |
Results and Impact | I am a member of the Scottish Government working group on Aviation Lighting for Windfarms. I provide expert advice on the propogation and appearance of light at night, and the effects of light pollution and how to mitigate them. The group comprises representative of the Scottish Government, industry, NatureScot, the CAA and MOD and local council planning officers. |
Year(s) Of Engagement Activity | 2021,2022 |
Description | Taster physics lecture for Physics taster day at University of Leeds |
Form Of Engagement Activity | A talk or presentation |
Part Of Official Scheme? | No |
Geographic Reach | Local |
Primary Audience | Schools |
Results and Impact | Gave example first year lecture on astronomy to final year pupils from local schools to show them a taster of what it is like to be an undergraduate student. |
Year(s) Of Engagement Activity | 2019 |
URL | https://www.stem.leeds.ac.uk/physics/tasterday/ |