Extracting science from surveys of our Galaxy

Cel

The goal is to put in place the infrastructure required to extract the promised science for large surveys of our Galaxy that are underway and will culminate in ESA's Cornerstone Mission Gaia. Dynamical models are fundamental to this process because surveys are heavily biased by the Sun's location in the Galaxy. Novel dynamical models will be built and novel methods of fitting them to the data developed. With their help we will be able to constrain the distribution of dark matter in the Galaxy. By modelling the chemical and dynamical evolution of the Galaxy we expect to be able to infer much information about how the Galaxy was assembled, and thus test the prevailing cosmological paradigm. During the grant period we will be applying our tools to ground-based surveys, but the first version of the Gaia Catalogue will become available at the end of the grant period, and our goal is to have everything ready and tested for its prompt exploitation.

System finansowania

ERC-AG - ERC Advanced Grant

Instytucja przyjmująca

THE CHANCELLOR, MASTERS AND SCHOLARS OF THE UNIVERSITY OF OXFORD

Wkład UE

€ 1 954 460,00

Adres

WELLINGTON SQUARE UNIVERSITY OFFICES
OX1 2JD Oxford
Zjednoczone Królestwo

Region

South East (England) Berkshire, Buckinghamshire and Oxfordshire Oxfordshire

Rodzaj działalności

Higher or Secondary Education Establishments

Kontakt administracyjny

Gill Wells (Ms.)

Kierownik naukowy

James Jeffrey Binney (Prof.)

Linki

Kontakt z organizacją Strona internetowa

Koszt całkowity

Brak danych

Beneficjenci (1)