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MWGaiaDN: Revealing the Milky Way with Gaia

Lead Research Organisation: University of Cambridge
Department Name: Institute of Astronomy

Abstract

The Milky Way-Gaia Doctoral Network (MWGaiaDN): Revealing the Milky Way (MW) with Gaia - Excellent science, Extending techniques, Enhancing people skills, Effecting the next revolution in European led astronomy through leadership in astrometric-based science. What: Gaia, ESA's major space mission launched in Dec 2013, is now in its extended mission to map some two billion stars in the MW. It's upcoming data releases , that will provide chemical and physical annotation of the earlier positional releases, present major challenges in terms of complexity and size, hence research training to deliver a full science exploitation is essential, ensuring that Gaia is the `game changer' for astronomy How: Our DN will link major partners responsible for the development of Gaia, to form an effective and unique training network combining the best research training with a range of academic and industrial placements, specialist research and knowledge transfer workshops. It will develop and train a cohort of young researchers through a set of key science projects pushing the Gaia data to its limits. Our DN will train 10 ESRs located across 10 European beneficiaries, benefiting from the participation of 13 associate partners. These include major industry (e.g. AirbusDS, TAS), at the forefront of Space and Information technologies; SME Industry (e.g. DAPCOM, Suil), innovating new technologies for Space and partners leading the development of next generation astrometry missions outside of Europe (NAOJ). Relevance: It will shape the delivery of training in astrometry and the study of the MW across Europe: delivering key insights into the structure and formation of our Galaxy; delivering the roadmap for the next generation of astrometric space telescopes; equipping the ESRs with skills to drive the next innovative steps in this crucial area of space discovery, as well as enabling them to contribute to the future, growth and challenges of the big data industry and commerce. MWGaiaDN

Publications

10 25 50
 
Title WEAVE Twilight Observation mode 
Description This method allow effective use of the WEAVE spectrograph for observations of bright stars in twilight. 
Type Of Material Improvements to research infrastructure 
Year Produced 2025 
Provided To Others? No  
Impact This method is currently being submitted for publication in RAS Techniques & Instruments 
 
Description Gaia Data Processing and Analysis Consortium (Gaia DPAC) 
Organisation Leiden University
Department Leiden Observatory
Country Netherlands 
Sector Academic/University 
PI Contribution The UK team is a major member of the Gaia DPAC and is responsible for (Spectro)Photometric processing and contributions to the ESA Gaia data delivery. See https://www.cosmos.esa.int/web/gaia/dpac/consortium for details of the DPAC.
Collaborator Contribution See https://www.cosmos.esa.int/web/gaia/dpac/consortium for details of the DPAC. Note that Leiden University is listed as the partner. This is the host institute of the current Chair of the DPAC Executive. The consortium is composed on institutes from many countries.
Impact The DPAC is responsible for the delivery of the data products from the ESA Gaia mission - see https://www.cosmos.esa.int/web/gaia/data
Start Year 2006
 
Description PLATO M3 Mission 
Organisation German Aerospace Centre (DLR)
Country Germany 
Sector Public 
PI Contribution The Plato exoplanet analysis system preparation work has formed a significant element of the M3 submission package to ESA - and the subsequent successful selection of Plato as the M3 mission. As a result of the investment in the definition and preliminary phases of Plato - it will now lead the development of the Exoplanet analysis system for Plato.
Collaborator Contribution The DLR group in Berlin lead the Plato mission.
Impact Plato is now in the B1 development phase, leading to an eventual launch in 2026
Start Year 2010
 
Description WEAVE 
Organisation Isaac Newton Group of Telescopes (ING)
Country Spain 
Sector Academic/University 
PI Contribution WEAVE is a new instrument under development and construction for the ING's William Herschel Telescope. We are responsible for the development of the Data Analysis system for the instrument - and also participate in the WEAVE Science Team.
Collaborator Contribution The page at http://www.ing.iac.es/weave/consortium.html gives a list of the partners in the WEAVE consortium.
Impact The consortium is responsible for the development of the WEAVE spectrograph. This will be commissioned on the ING's WHT late 2017.
Start Year 2010