Visiting Fellowships at Durham
Lead Research Organisation:
Durham University
Department Name: Physics
Abstract
This application seeks support to continue the successful visitors programme that we have conducted at Durham since 1983. This application covers the entire spectrum of astronomical research at Durham which includes extragalactic astronomy, cosmology, astronomical instrumentation, gamma-ray astronomy and high energy astrophysics. The current grant has supported 97 visitors over a 2.5 year period and had led to 111 joint refereed publications involving Durham researchers and visitors. Examples of research projects involving visitors are: the Virgo Consortium's programme of simulations of the formation of structure in the universe; theoretical modelling of galaxy formation; observational studies of young massive galaxies undergoing huge starbursts; investigation of accretion processes onto black holes of a wide range of sizes, from a few to a billion solar masses; the effects of the growth of supermassive black holes on forming galaxies; observations of groups and clusters at early stages of formation; the detection and interpretation of very high energy gamma rays from exotic objects including microquasars; the design of new instruments for existing telescopes like the Very Large Telescopes and future ones like the projected Extremely Large Telescope.
Organisations
- Durham University (Lead Research Organisation)
- University of Zurich (Collaboration)
- Heidelberg Institute of Technology and Science (Collaboration)
- Planetary Science Institute - Arizona (Collaboration)
- UNIVERSITY OF EDINBURGH (Collaboration)
- QUEEN MARY UNIVERSITY OF LONDON (Collaboration)
- Max Planck Society (Collaboration)
- Ohio State University (Collaboration)
- DURHAM UNIVERSITY (Collaboration)
- Cardiff University (Collaboration)
- University of Hawaii (Collaboration)
- Johns Hopkins University (Collaboration)
- Seoul National University (Collaboration)
- European Space Agency (Collaboration)
- University of Canterbury (Collaboration)
- UNIVERSITY OF SYDNEY (Collaboration)
- National Aeronautics and Space Administration (NASA) (Collaboration)
- Leiden University (Collaboration)
- HARVARD UNIVERSITY (Collaboration)
- University of Manchester (Collaboration)
- UNIVERSITY OF NOTTINGHAM (Collaboration)
- National Institute for Astrophysics (Collaboration)
- Pontifical Catholic University of Chile (Collaboration)
- University of California, Santa Cruz (Collaboration)
- UNIVERSITY OF CAMBRIDGE (Collaboration)
- UNIVERSITY OF OXFORD (Collaboration)
- University of Sussex (Collaboration)
- Los Alamos National Laboratory (Collaboration)
- National Astronomical Observatories of China (Collaboration)
- University of Massachusetts (Collaboration)
- University of Washington (Collaboration)
People |
ORCID iD |
Carlos Frenk (Principal Investigator) |
Publications
Power C
(2010)
The redshift evolution of the mass function of cold gas in hierarchical galaxy formation models Redshift evolution of cold gas mass function
in Monthly Notices of the Royal Astronomical Society
Navarro J
(2010)
The diversity and similarity of simulated cold dark matter haloes Diversity and similarity of simulated CDM haloes
in Monthly Notices of the Royal Astronomical Society
Ivison R
(2010)
BLAST: the far-infrared/radio correlation in distant galaxies Bolometric FIR/radio correlation
in Monthly Notices of the Royal Astronomical Society
Strigari L
(2010)
Kinematics of Milky Way satellites in a Lambda cold dark matter universe Kinematics of Milky Way satellites
in Monthly Notices of the Royal Astronomical Society
Gonzalez-Perez V
(2009)
Massive, red galaxies in a hierarchical universe - I. Counts of extremely red objects and basic properties
in Monthly Notices of the Royal Astronomical Society
Eke V
(2009)
The spatial distribution of polar hydrogen deposits on the Moon
in Icarus
Okamoto T
(2009)
The origin of failed subhaloes and the common mass scale of the Milky Way satellite galaxies
in Monthly Notices of the Royal Astronomical Society: Letters
Jones D
(2009)
The 6dF Galaxy Survey: final redshift release (DR3) and southern large-scale structures
in Monthly Notices of the Royal Astronomical Society
Sanderson A
(2009)
LoCuSS: the connection between brightest cluster galaxy activity, gas cooling and dynamical disturbance of X-ray cluster cores
in Monthly Notices of the Royal Astronomical Society
Wiersma R
(2009)
Chemical enrichment in cosmological, smoothed particle hydrodynamics simulations
in Monthly Notices of the Royal Astronomical Society
Cattaneo A
(2009)
The role of black holes in galaxy formation and evolution.
in Nature
Casey C
(2009)
A search for neutral carbon towards two z = 4.05 submillimetre galaxies, GN???20 and GN???20.2
in Monthly Notices of the Royal Astronomical Society
Elphic, R.C., Paige, D.A., Siegler, M.A., Eke, V.R., Teodoro, L.F.A., And Lawrence, D.J.
(2009)
South Pole Hydrogen Distributions for Present Lunar Conditions
in LPI Contributions
Angulo R
(2009)
The fate of substructures in cold dark matter haloes
in Monthly Notices of the Royal Astronomical Society
Crain R
(2009)
Galaxies???intergalactic medium interaction calculation ??? I. Galaxy formation as a function of large-scale environment
in Monthly Notices of the Royal Astronomical Society
Vogelsberger M
(2009)
Phase-space structure in the local dark matter distribution and its signature in direct detection experiments
in Monthly Notices of the Royal Astronomical Society
Norberg P
(2009)
Statistical analysis of galaxy surveys - I. Robust error estimation for two-point clustering statistics
in Monthly Notices of the Royal Astronomical Society
Mitchell N
(2009)
On the origin of cores in simulated galaxy clusters
in Monthly Notices of the Royal Astronomical Society
Boylan-Kolchin M
(2009)
Resolving cosmic structure formation with the Millennium-II Simulation
in Monthly Notices of the Royal Astronomical Society
Libeskind N
(2009)
How common is the Milky Way-satellite system alignment?
in Monthly Notices of the Royal Astronomical Society
Symeonidis M
(2009)
The link between SCUBA and Spitzer : cold galaxies at z ? 1
in Monthly Notices of the Royal Astronomical Society
Sánchez A
(2009)
Cosmological parameter constraints from SDSS luminous red galaxies: a new treatment of large-scale clustering
in Monthly Notices of the Royal Astronomical Society
Muxlow T. W. B.
(2009)
Discovery of a new transient radio source in the central region of M82
in The Astronomer's Telegram
Reed D
(2009)
The clustering of the first galaxy haloes
in Monthly Notices of the Royal Astronomical Society
Ludlow A
(2009)
THE UNORTHODOX ORBITS OF SUBSTRUCTURE HALOS
in The Astrophysical Journal
Description | This grant has enabled a wide range of developments including: i) Developing a model that explains the formation and structure of the stellar haloes that surround the Milky Way and other nearby galaxies as the result of the tidal stripping of stars from accreted satellite galaxies. ii) Establishing that the accretion discs around the black hold of AGN are correlated with the orientation of their surrounding host galaxy. iii) Demonstrating that Cold Dark Matter model generates dark matter substructures whose properties are compatible with the kinematic data of the dwarf galaxies surrounding the Milky Way. iv) Developed a fast method of computing the spectral energy distributions of model galaxies by employing machine learning techniques. v) Developed a technique to compute the imprint of intervening cosmic structure of the Cosmic Microwave Background. |
Exploitation Route | Enables: i) Making detailed predictions of the statistics of stellar haloes that can be tested by future ground and space based facilities. ii) Can be used to constrain the models of the growth of black holes and their accretion discs. iii) Can be used to rule out alternatives to the Cold Dark Matter model of structure formation. iv) Can be used to build large mock catalogues of galaxies with realistic spectral energy distributions which are needed to complement the analysis of future galaxy redshift surveys and investigate the environmental impact on galaxy formation. v) Can be used to allow theoretical models to be analysed in the same way as observational data in order to use the Cosmic Microwave Background to set additional constraints on models of cosmic structure formation. |
Sectors | Digital/Communication/Information Technologies (including Software) Education Other |
URL | http://adsabs.harvard.edu/abs/2010MNRAS.407..201C |
Description | Our many findings have been discussed in used by others in many subsequent scientific articles. In addition our work stellar haloes has motivated innovative wide angle ground and space borne telescopes to image the diffuse stellar haloes around nearby galaxies in order to test this key prediction of the Cold Dark Matter model. |
First Year Of Impact | 2012 |
Sector | Aerospace, Defence and Marine,Digital/Communication/Information Technologies (including Software),Education,Other |
Impact Types | Cultural Societal |
Description | High Performance Computing: The Virgo Consortium |
Amount | £1,684,000 (GBP) |
Funding ID | ST/H008519/1 |
Organisation | Science and Technologies Facilities Council (STFC) |
Sector | Public |
Country | United Kingdom |
Start | 03/2009 |
End | 03/2012 |
Description | Visiting Fellowships at Durham 2011-2014 |
Amount | £72,426 (GBP) |
Organisation | Science and Technologies Facilities Council (STFC) |
Sector | Public |
Country | United Kingdom |
Start | 03/2011 |
End | 03/2014 |
Description | Euclid |
Organisation | European Space Agency |
Country | France |
Sector | Public |
PI Contribution | Euclid is an ESA mission to map the geometry of the dark Universe. The mission will investigate the distance-redshift relationship and the evolution of cosmic structures by measuring shapes and redshifts of galaxies and clusters of galaxies out to redshifts ~2, or equivalently to a look-back time of 10 billion years. In this way, Euclid will cover the entire period over which dark energy played a significant role in accelerating the expansion. |
Collaborator Contribution | Euclid is an ESA mission to map the geometry of the dark Universe. The mission will investigate the distance-redshift relationship and the evolution of cosmic structures by measuring shapes and redshifts of galaxies and clusters of galaxies out to redshifts ~2, or equivalently to a look-back time of 10 billion years. In this way, Euclid will cover the entire period over which dark energy played a significant role in accelerating the expansion. |
Impact | Not yet |
Start Year | 2010 |
Description | GAMA: Galaxy And Mass Assembly survey |
Organisation | University of Sydney |
Country | Australia |
Sector | Academic/University |
PI Contribution | GAMA is a major redshift and multi-wavelength survey started in 2008 and for which we are still actively collecting data using 2dF and AAOmega on the Anglo-Australian Telescope. GAMA is governed by formal and informal agreements. |
Collaborator Contribution | Publication of 40 GAMA refereed papers |
Impact | Publication of 40 GAMA refereed papers |
Start Year | 2009 |
Description | HST Legacy Extragalactic UV Survey (LEGUS) |
Organisation | University of Massachusetts |
Country | United States |
Sector | Academic/University |
PI Contribution | I am part of a large HST Legacy Extragalactic UV Survey (LEGUS). The collaboration started in 2013, and it is still active. The first paper from the collaboration was recently accepted (Calzetti et al., 2014 AJ in press). As part of the collaboration, I am contributing to the data analysis and modeling. |
Collaborator Contribution | The collaboration has also a rich outreach programme: one highlight is the realization of 3D models with different textures to help visually impaired students to learn about galaxies. |
Impact | See webpage https://legus.stsci.edu/ |
Start Year | 2013 |
Description | Herschel ATLAS consortium |
Organisation | Cardiff University |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Research projects analysing data from Herschel-ATLAS survey, to investigate dependence of galaxy far-IR luminosities and star formation rates on environment in low-redshift universe. |
Collaborator Contribution | Contributions by other partners: planning and data reduction for Herschel-ATLAS survey. |
Impact | 1 paper published by us so far: Guo et al 2011, MNRAS 412, 2277 "Which haloes host Herschel-ATLAS galaxies in the local Universe?" |
Start Year | 2008 |
Description | Herschel ATLAS consortium |
Organisation | University of Canterbury |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Research projects analysing data from Herschel-ATLAS survey, to investigate dependence of galaxy far-IR luminosities and star formation rates on environment in low-redshift universe. |
Collaborator Contribution | Contributions by other partners: planning and data reduction for Herschel-ATLAS survey. |
Impact | 1 paper published by us so far: Guo et al 2011, MNRAS 412, 2277 "Which haloes host Herschel-ATLAS galaxies in the local Universe?" |
Start Year | 2008 |
Description | Lunar radar collaboration |
Organisation | National Aeronautics and Space Administration (NASA) |
Country | United States |
Sector | Public |
PI Contribution | Produced a paper submitted to Icarus |
Collaborator Contribution | Produced a paper submitted to Icarus |
Impact | Produced a paper submitted to Icarus |
Start Year | 2013 |
Description | Moon-forming Impact simulation collaboration |
Organisation | Los Alamos National Laboratory |
Country | United States |
Sector | Public |
PI Contribution | produced a conference proceedings |
Collaborator Contribution | produced a conference proceedings |
Impact | produced a conference proceedings |
Start Year | 2013 |
Description | Moon-forming Impact simulation collaboration |
Organisation | National Aeronautics and Space Administration (NASA) |
Country | United States |
Sector | Public |
PI Contribution | produced a conference proceedings |
Collaborator Contribution | produced a conference proceedings |
Impact | produced a conference proceedings |
Start Year | 2013 |
Description | Moon-forming Impact simulation collaboration |
Organisation | University of California, Santa Cruz |
Country | United States |
Sector | Academic/University |
PI Contribution | produced a conference proceedings |
Collaborator Contribution | produced a conference proceedings |
Impact | produced a conference proceedings |
Start Year | 2013 |
Description | Neutron spectroscopy collaboration |
Organisation | Johns Hopkins University |
Country | United States |
Sector | Academic/University |
PI Contribution | Has produced a paper in press at JGR Planets |
Collaborator Contribution | research contributions |
Impact | Has produced a paper in press at JGR Planets |
Start Year | 2013 |
Description | Neutron spectroscopy collaboration |
Organisation | National Aeronautics and Space Administration (NASA) |
Country | United States |
Sector | Public |
PI Contribution | Has produced a paper in press at JGR Planets |
Collaborator Contribution | research contributions |
Impact | Has produced a paper in press at JGR Planets |
Start Year | 2013 |
Description | Neutron spectroscopy collaboration |
Organisation | Planetary Science Institute - Arizona |
Country | United States |
Sector | Academic/University |
PI Contribution | Has produced a paper in press at JGR Planets |
Collaborator Contribution | research contributions |
Impact | Has produced a paper in press at JGR Planets |
Start Year | 2013 |
Description | Pan-STARRS |
Organisation | Harvard University |
Department | Harvard-Smithsonian Center for Astrophysics |
Country | United States |
Sector | Academic/University |
PI Contribution | Pan-STARRS is an international collaboration, involving teams in Germany (Heidelberg and Munich), the USA (Harvard, Hawaii, Johns Hopkins) and the UK (Durham, Edinburgh, Belfast) to exploit data from the novel PS1 telescope. |
Impact | White paper, outreach materials |
Start Year | 2008 |
Description | Pan-STARRS |
Organisation | Harvard University |
Department | Harvard-Smithsonian Center for Astrophysics |
Country | United States |
Sector | Academic/University |
PI Contribution | Pan-STARRS is an international collaboration, involving teams in Germany (Heidelberg and Munich), the USA (Harvard, Hawaii, Johns Hopkins) and the UK (Durham, Edinburgh, Belfast) to exploit data from the novel PS1 telescope. |
Collaborator Contribution | na |
Impact | Many collaborative papers published in scientific journals; Astronomical Survey data beign made public via a database at the Hubble Space Telescope Science Institute |
Start Year | 2008 |
Description | Pan-STARRS |
Organisation | Johns Hopkins University |
Department | Department of Physics & Astronomy |
Country | United States |
Sector | Academic/University |
PI Contribution | Pan-STARRS is an international collaboration, involving teams in Germany (Heidelberg and Munich), the USA (Harvard, Hawaii, Johns Hopkins) and the UK (Durham, Edinburgh, Belfast) to exploit data from the novel PS1 telescope. |
Impact | White paper, outreach materials |
Start Year | 2008 |
Description | Pan-STARRS |
Organisation | Johns Hopkins University |
Department | Department of Physics & Astronomy |
Country | United States |
Sector | Academic/University |
PI Contribution | Pan-STARRS is an international collaboration, involving teams in Germany (Heidelberg and Munich), the USA (Harvard, Hawaii, Johns Hopkins) and the UK (Durham, Edinburgh, Belfast) to exploit data from the novel PS1 telescope. |
Collaborator Contribution | na |
Impact | Many collaborative papers published in scientific journals; Astronomical Survey data beign made public via a database at the Hubble Space Telescope Science Institute |
Start Year | 2008 |
Description | Pan-STARRS |
Organisation | Max Planck Society |
Country | Germany |
Sector | Charity/Non Profit |
PI Contribution | Pan-STARRS is an international collaboration, involving teams in Germany (Heidelberg and Munich), the USA (Harvard, Hawaii, Johns Hopkins) and the UK (Durham, Edinburgh, Belfast) to exploit data from the novel PS1 telescope. |
Collaborator Contribution | na |
Impact | Many collaborative papers published in scientific journals; Astronomical Survey data beign made public via a database at the Hubble Space Telescope Science Institute |
Start Year | 2008 |
Description | Pan-STARRS |
Organisation | Max Planck Society |
Country | Germany |
Sector | Charity/Non Profit |
PI Contribution | Pan-STARRS is an international collaboration, involving teams in Germany (Heidelberg and Munich), the USA (Harvard, Hawaii, Johns Hopkins) and the UK (Durham, Edinburgh, Belfast) to exploit data from the novel PS1 telescope. |
Impact | White paper, outreach materials |
Start Year | 2008 |
Description | Pan-STARRS |
Organisation | Queen Mary University of London |
Department | School of Physics and Astronomy |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Pan-STARRS is an international collaboration, involving teams in Germany (Heidelberg and Munich), the USA (Harvard, Hawaii, Johns Hopkins) and the UK (Durham, Edinburgh, Belfast) to exploit data from the novel PS1 telescope. |
Collaborator Contribution | na |
Impact | Many collaborative papers published in scientific journals; Astronomical Survey data beign made public via a database at the Hubble Space Telescope Science Institute |
Start Year | 2008 |
Description | Pan-STARRS |
Organisation | Queen Mary University of London |
Department | School of Physics and Astronomy |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Pan-STARRS is an international collaboration, involving teams in Germany (Heidelberg and Munich), the USA (Harvard, Hawaii, Johns Hopkins) and the UK (Durham, Edinburgh, Belfast) to exploit data from the novel PS1 telescope. |
Impact | White paper, outreach materials |
Start Year | 2008 |
Description | Pan-STARRS |
Organisation | University of Edinburgh |
Department | Institute for Astronomy |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Pan-STARRS is an international collaboration, involving teams in Germany (Heidelberg and Munich), the USA (Harvard, Hawaii, Johns Hopkins) and the UK (Durham, Edinburgh, Belfast) to exploit data from the novel PS1 telescope. |
Impact | White paper, outreach materials |
Start Year | 2008 |
Description | Pan-STARRS |
Organisation | University of Edinburgh |
Department | Institute for Astronomy |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | Pan-STARRS is an international collaboration, involving teams in Germany (Heidelberg and Munich), the USA (Harvard, Hawaii, Johns Hopkins) and the UK (Durham, Edinburgh, Belfast) to exploit data from the novel PS1 telescope. |
Collaborator Contribution | na |
Impact | Many collaborative papers published in scientific journals; Astronomical Survey data beign made public via a database at the Hubble Space Telescope Science Institute |
Start Year | 2008 |
Description | Pan-STARRS |
Organisation | University of Hawaii |
Department | Institute for Astronomy |
Country | United States |
Sector | Academic/University |
PI Contribution | Pan-STARRS is an international collaboration, involving teams in Germany (Heidelberg and Munich), the USA (Harvard, Hawaii, Johns Hopkins) and the UK (Durham, Edinburgh, Belfast) to exploit data from the novel PS1 telescope. |
Collaborator Contribution | na |
Impact | Many collaborative papers published in scientific journals; Astronomical Survey data beign made public via a database at the Hubble Space Telescope Science Institute |
Start Year | 2008 |
Description | Pan-STARRS |
Organisation | University of Hawaii |
Department | Institute for Astronomy |
Country | United States |
Sector | Academic/University |
PI Contribution | Pan-STARRS is an international collaboration, involving teams in Germany (Heidelberg and Munich), the USA (Harvard, Hawaii, Johns Hopkins) and the UK (Durham, Edinburgh, Belfast) to exploit data from the novel PS1 telescope. |
Impact | White paper, outreach materials |
Start Year | 2008 |
Description | Probing the origin of the accelerated expansion of our Universe |
Organisation | National Astronomical Observatories of China |
Country | China |
Sector | Public |
PI Contribution | Sharing my simulation data and helping interpreting their analysis outputs of the data, test various theories to explain the cosmic acceleration |
Collaborator Contribution | expertise in various areas of analysing simulation data and helps in making connections with observations |
Impact | We analysed a variety of cosmological probes of the origin of the acceleration and assessed their viability, potential and possible difficulties. |
Start Year | 2013 |
Description | Probing the origin of the accelerated expansion of our Universe |
Organisation | National Institute for Astrophysics |
Country | Italy |
Sector | Academic/University |
PI Contribution | Sharing my simulation data and helping interpreting their analysis outputs of the data, test various theories to explain the cosmic acceleration |
Collaborator Contribution | expertise in various areas of analysing simulation data and helps in making connections with observations |
Impact | We analysed a variety of cosmological probes of the origin of the acceleration and assessed their viability, potential and possible difficulties. |
Start Year | 2013 |
Description | Probing the origin of the accelerated expansion of our Universe |
Organisation | Ohio State University |
Country | United States |
Sector | Academic/University |
PI Contribution | Sharing my simulation data and helping interpreting their analysis outputs of the data, test various theories to explain the cosmic acceleration |
Collaborator Contribution | expertise in various areas of analysing simulation data and helps in making connections with observations |
Impact | We analysed a variety of cosmological probes of the origin of the acceleration and assessed their viability, potential and possible difficulties. |
Start Year | 2013 |
Description | Probing the origin of the accelerated expansion of our Universe |
Organisation | Pontifical Catholic University of Chile |
Country | Chile |
Sector | Academic/University |
PI Contribution | Sharing my simulation data and helping interpreting their analysis outputs of the data, test various theories to explain the cosmic acceleration |
Collaborator Contribution | expertise in various areas of analysing simulation data and helps in making connections with observations |
Impact | We analysed a variety of cosmological probes of the origin of the acceleration and assessed their viability, potential and possible difficulties. |
Start Year | 2013 |
Description | Probing the origin of the accelerated expansion of our Universe |
Organisation | Seoul National University |
Country | Korea, Republic of |
Sector | Academic/University |
PI Contribution | Sharing my simulation data and helping interpreting their analysis outputs of the data, test various theories to explain the cosmic acceleration |
Collaborator Contribution | expertise in various areas of analysing simulation data and helps in making connections with observations |
Impact | We analysed a variety of cosmological probes of the origin of the acceleration and assessed their viability, potential and possible difficulties. |
Start Year | 2013 |
Description | Probing the origin of the accelerated expansion of our Universe |
Organisation | University of Zurich |
Country | Switzerland |
Sector | Academic/University |
PI Contribution | Sharing my simulation data and helping interpreting their analysis outputs of the data, test various theories to explain the cosmic acceleration |
Collaborator Contribution | expertise in various areas of analysing simulation data and helps in making connections with observations |
Impact | We analysed a variety of cosmological probes of the origin of the acceleration and assessed their viability, potential and possible difficulties. |
Start Year | 2013 |
Description | SCUBA-2 Cosmology Legacy Survey |
Organisation | Durham University |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | The SCUBA2 Cosmology Legacy Survey (S2CLS) is a collaboration of ~100 scientists across the three partner countries who run the James Clerk Maxwell Telescope (JCMT): Canada, the UK and the Netherlands (with a few individuals based in other countries). The survey will exploit the immense increase in mapping speed, fidelity and sensitivity of the new SCUBA2 submillimeter camera on the JCMT. |
Collaborator Contribution | n/a |
Impact | outcomes in last year: published 1 paper: The SCUBA-2 Cosmology Legacy Survey: blank-field number counts of 450-?-selected galaxies and their contribution to the cosmic infrared background Geach, J. E.; et al MNRAS 432, 53 |
Description | The Ordered Universe |
Organisation | University of Oxford |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | AHRC funding: network grant |
Collaborator Contribution | Each team member, from whatever discipline, contributes to editions, translations, analyses and presentations. In so doing, we are pioneering new ways of working across and between our disciplines. Trusting one another, and learning to learn from the past have presented creative demands. We have challenged academic and public preconceptions regarding the value of past science as 'irrelevant'. Funding for the project has been provided by Durham University's Institute of Medieval and Early Modern Studies, the Arts and Humanities Research Council, UK, and the Mahfouz Foundation for Interdisciplinary Research, Pembroke College, Oxford |
Impact | Bringing together a unique configuration of natural scientists, social scientists and arts and humanities scholars, the project integrates the conceptual tools of modern science with the textual methods of the humanities to explore the richness of Grosseteste's thought. Our translations, many for the first time, and which incorporate the groundbreaking concept of translation into mathematics, enable wider access to this wonderful mind, compelling us to make new assessments of his perceptive and inventive imagination. |
Start Year | 2013 |
Description | Training opportunities for postgraduate students in Durham |
Organisation | Johns Hopkins University |
Country | United States |
Sector | Academic/University |
PI Contribution | Vince Eke: I collaborate with researchers at NASA Ames Research Centre, Johns Hopkins Applied Physics Lab, the Planetary Science Institute in Tucson, Los Alamos National Lab and Washington University in St Louis on analysis of radar, gamma ray and neutron remote sensing data of other solar system bodies, and numerical simulations of giant impacts in the early solar system. These ongoing informal academic collaborations have been active for up to 8 years. They provide training opportunities for postgraduate students in Durham, as well as access to data that are not publicly available. |
Collaborator Contribution | I make contributions that range from ideas for areas to study, through technical expertise and data analysis, to paper writing and giving talks, as do the other members of the collaborations. |
Impact | All of these collaborations have produced conference proceedings and led to talks at international conferences. Almost all have led to papers in the major peer-reviewed planetary science journals. |
Start Year | 2006 |
Description | Training opportunities for postgraduate students in Durham |
Organisation | Los Alamos National Laboratory |
Country | United States |
Sector | Public |
PI Contribution | Vince Eke: I collaborate with researchers at NASA Ames Research Centre, Johns Hopkins Applied Physics Lab, the Planetary Science Institute in Tucson, Los Alamos National Lab and Washington University in St Louis on analysis of radar, gamma ray and neutron remote sensing data of other solar system bodies, and numerical simulations of giant impacts in the early solar system. These ongoing informal academic collaborations have been active for up to 8 years. They provide training opportunities for postgraduate students in Durham, as well as access to data that are not publicly available. |
Collaborator Contribution | I make contributions that range from ideas for areas to study, through technical expertise and data analysis, to paper writing and giving talks, as do the other members of the collaborations. |
Impact | All of these collaborations have produced conference proceedings and led to talks at international conferences. Almost all have led to papers in the major peer-reviewed planetary science journals. |
Start Year | 2006 |
Description | Training opportunities for postgraduate students in Durham |
Organisation | National Aeronautics and Space Administration (NASA) |
Department | NASA Ames Exploration Center |
Country | United States |
Sector | Public |
PI Contribution | Vince Eke: I collaborate with researchers at NASA Ames Research Centre, Johns Hopkins Applied Physics Lab, the Planetary Science Institute in Tucson, Los Alamos National Lab and Washington University in St Louis on analysis of radar, gamma ray and neutron remote sensing data of other solar system bodies, and numerical simulations of giant impacts in the early solar system. These ongoing informal academic collaborations have been active for up to 8 years. They provide training opportunities for postgraduate students in Durham, as well as access to data that are not publicly available. |
Collaborator Contribution | I make contributions that range from ideas for areas to study, through technical expertise and data analysis, to paper writing and giving talks, as do the other members of the collaborations. |
Impact | All of these collaborations have produced conference proceedings and led to talks at international conferences. Almost all have led to papers in the major peer-reviewed planetary science journals. |
Start Year | 2006 |
Description | Training opportunities for postgraduate students in Durham |
Organisation | Planetary Science Institute - Arizona |
Country | United States |
Sector | Academic/University |
PI Contribution | Vince Eke: I collaborate with researchers at NASA Ames Research Centre, Johns Hopkins Applied Physics Lab, the Planetary Science Institute in Tucson, Los Alamos National Lab and Washington University in St Louis on analysis of radar, gamma ray and neutron remote sensing data of other solar system bodies, and numerical simulations of giant impacts in the early solar system. These ongoing informal academic collaborations have been active for up to 8 years. They provide training opportunities for postgraduate students in Durham, as well as access to data that are not publicly available. |
Collaborator Contribution | I make contributions that range from ideas for areas to study, through technical expertise and data analysis, to paper writing and giving talks, as do the other members of the collaborations. |
Impact | All of these collaborations have produced conference proceedings and led to talks at international conferences. Almost all have led to papers in the major peer-reviewed planetary science journals. |
Start Year | 2006 |
Description | Training opportunities for postgraduate students in Durham |
Organisation | University of Washington |
Country | United States |
Sector | Academic/University |
PI Contribution | Vince Eke: I collaborate with researchers at NASA Ames Research Centre, Johns Hopkins Applied Physics Lab, the Planetary Science Institute in Tucson, Los Alamos National Lab and Washington University in St Louis on analysis of radar, gamma ray and neutron remote sensing data of other solar system bodies, and numerical simulations of giant impacts in the early solar system. These ongoing informal academic collaborations have been active for up to 8 years. They provide training opportunities for postgraduate students in Durham, as well as access to data that are not publicly available. |
Collaborator Contribution | I make contributions that range from ideas for areas to study, through technical expertise and data analysis, to paper writing and giving talks, as do the other members of the collaborations. |
Impact | All of these collaborations have produced conference proceedings and led to talks at international conferences. Almost all have led to papers in the major peer-reviewed planetary science journals. |
Start Year | 2006 |
Description | Virgo Consortium for Cosmological Simulations |
Organisation | Heidelberg Institute of Technology and Science |
Country | Germany |
Sector | Academic/University |
PI Contribution | The Virgo consortium is the world-leading collaboration on supercomputer simulations of the formation of cosmic structure |
Impact | Publications (see list), outreach materials (see list) |
Description | Virgo Consortium for Cosmological Simulations |
Organisation | Heidelberg Institute of Technology and Science |
Country | Germany |
Sector | Academic/University |
PI Contribution | The Virgo consortium is the world-leading collaboration on supercomputer simulations of the formation of cosmic structure |
Collaborator Contribution | -- |
Impact | Publications (see list), outreach materials (see list) |
Start Year | 2006 |
Description | Virgo Consortium for Cosmological Simulations |
Organisation | Heidelberg Institute of Technology and Science |
Country | Germany |
Sector | Academic/University |
PI Contribution | The Virgo consortium is the world-leading collaboration on supercomputer simulations of the formation of cosmic structure |
Impact | Publications (see list), outreach materials (see list) |
Description | Virgo Consortium for Cosmological Simulations |
Organisation | Leiden University |
Department | Leiden Observatory |
Country | Netherlands |
Sector | Academic/University |
PI Contribution | The Virgo consortium is the world-leading collaboration on supercomputer simulations of the formation of cosmic structure |
Impact | Publications (see list), outreach materials (see list) |
Description | Virgo Consortium for Cosmological Simulations |
Organisation | Leiden University |
Department | Leiden Observatory |
Country | Netherlands |
Sector | Academic/University |
PI Contribution | The Virgo consortium is the world-leading collaboration on supercomputer simulations of the formation of cosmic structure |
Collaborator Contribution | -- |
Impact | Publications (see list), outreach materials (see list) |
Start Year | 2006 |
Description | Virgo Consortium for Cosmological Simulations |
Organisation | Leiden University |
Department | Leiden Observatory |
Country | Netherlands |
Sector | Academic/University |
PI Contribution | The Virgo consortium is the world-leading collaboration on supercomputer simulations of the formation of cosmic structure |
Impact | Publications (see list), outreach materials (see list) |
Description | Virgo Consortium for Cosmological Simulations |
Organisation | Max Planck Society |
Department | Max Planck Institute for Astrophysics |
Country | Germany |
Sector | Academic/University |
PI Contribution | The Virgo consortium is the world-leading collaboration on supercomputer simulations of the formation of cosmic structure |
Impact | Publications (see list), outreach materials (see list) |
Description | Virgo Consortium for Cosmological Simulations |
Organisation | Max Planck Society |
Department | Max Planck Institute for Astrophysics |
Country | Germany |
Sector | Academic/University |
PI Contribution | The Virgo consortium is the world-leading collaboration on supercomputer simulations of the formation of cosmic structure |
Impact | Publications (see list), outreach materials (see list) |
Description | Virgo Consortium for Cosmological Simulations |
Organisation | Max Planck Society |
Department | Max Planck Institute for Astrophysics |
Country | Germany |
Sector | Academic/University |
PI Contribution | The Virgo consortium is the world-leading collaboration on supercomputer simulations of the formation of cosmic structure |
Collaborator Contribution | -- |
Impact | Publications (see list), outreach materials (see list) |
Start Year | 2006 |
Description | Virgo Consortium for Cosmological Simulations |
Organisation | University of Cambridge |
Department | Institute of Astronomy |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | The Virgo consortium is the world-leading collaboration on supercomputer simulations of the formation of cosmic structure |
Collaborator Contribution | -- |
Impact | Publications (see list), outreach materials (see list) |
Start Year | 2006 |
Description | Virgo Consortium for Cosmological Simulations |
Organisation | University of Cambridge |
Department | Institute of Astronomy |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | The Virgo consortium is the world-leading collaboration on supercomputer simulations of the formation of cosmic structure |
Impact | Publications (see list), outreach materials (see list) |
Description | Virgo Consortium for Cosmological Simulations |
Organisation | University of Cambridge |
Department | Institute of Astronomy |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | The Virgo consortium is the world-leading collaboration on supercomputer simulations of the formation of cosmic structure |
Impact | Publications (see list), outreach materials (see list) |
Description | Virgo Consortium for Cosmological Simulations |
Organisation | University of Edinburgh |
Department | Institute for Astronomy |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | The Virgo consortium is the world-leading collaboration on supercomputer simulations of the formation of cosmic structure |
Impact | Publications (see list), outreach materials (see list) |
Description | Virgo Consortium for Cosmological Simulations |
Organisation | University of Edinburgh |
Department | Institute for Astronomy |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | The Virgo consortium is the world-leading collaboration on supercomputer simulations of the formation of cosmic structure |
Collaborator Contribution | -- |
Impact | Publications (see list), outreach materials (see list) |
Start Year | 2006 |
Description | Virgo Consortium for Cosmological Simulations |
Organisation | University of Edinburgh |
Department | Institute for Astronomy |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | The Virgo consortium is the world-leading collaboration on supercomputer simulations of the formation of cosmic structure |
Impact | Publications (see list), outreach materials (see list) |
Description | Virgo Consortium for Cosmological Simulations |
Organisation | University of Manchester |
Department | School of Physics and Astronomy Manchester |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | The Virgo consortium is the world-leading collaboration on supercomputer simulations of the formation of cosmic structure |
Collaborator Contribution | -- |
Impact | Publications (see list), outreach materials (see list) |
Start Year | 2006 |
Description | Virgo Consortium for Cosmological Simulations |
Organisation | University of Manchester |
Department | School of Physics and Astronomy Manchester |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | The Virgo consortium is the world-leading collaboration on supercomputer simulations of the formation of cosmic structure |
Impact | Publications (see list), outreach materials (see list) |
Description | Virgo Consortium for Cosmological Simulations |
Organisation | University of Manchester |
Department | School of Physics and Astronomy Manchester |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | The Virgo consortium is the world-leading collaboration on supercomputer simulations of the formation of cosmic structure |
Impact | Publications (see list), outreach materials (see list) |
Description | Virgo Consortium for Cosmological Simulations |
Organisation | University of Nottingham |
Department | School of Physics and Astronomy |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | The Virgo consortium is the world-leading collaboration on supercomputer simulations of the formation of cosmic structure |
Collaborator Contribution | -- |
Impact | Publications (see list), outreach materials (see list) |
Start Year | 2006 |
Description | Virgo Consortium for Cosmological Simulations |
Organisation | University of Nottingham |
Department | School of Physics and Astronomy |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | The Virgo consortium is the world-leading collaboration on supercomputer simulations of the formation of cosmic structure |
Impact | Publications (see list), outreach materials (see list) |
Description | Virgo Consortium for Cosmological Simulations |
Organisation | University of Nottingham |
Department | School of Physics and Astronomy |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | The Virgo consortium is the world-leading collaboration on supercomputer simulations of the formation of cosmic structure |
Impact | Publications (see list), outreach materials (see list) |
Description | Virgo Consortium for Cosmological Simulations |
Organisation | University of Sussex |
Department | Astronomy Centre |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | The Virgo consortium is the world-leading collaboration on supercomputer simulations of the formation of cosmic structure |
Impact | Publications (see list), outreach materials (see list) |
Description | Virgo Consortium for Cosmological Simulations |
Organisation | University of Sussex |
Department | Physics and Astronomy Department |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | The Virgo consortium is the world-leading collaboration on supercomputer simulations of the formation of cosmic structure |
Collaborator Contribution | -- |
Impact | Publications (see list), outreach materials (see list) |
Start Year | 2006 |
Description | Virgo Consortium for Cosmological Simulations |
Organisation | University of Sussex |
Department | Physics and Astronomy Department |
Country | United Kingdom |
Sector | Academic/University |
PI Contribution | The Virgo consortium is the world-leading collaboration on supercomputer simulations of the formation of cosmic structure |
Impact | Publications (see list), outreach materials (see list) |