Skip to main content
Go to the home page of the European Commission (opens in new window)
English English
CORDIS - EU research results
CORDIS
Content archived on 2024-06-18

The Gaia-ESO Milky Way Survey

Objective

Understanding how galaxies actually form and evolve within our dark matter and dark energy dominated [ɅCDM] universe continues to be an enormous challenge. State of the art simulations of the aggregation of cold dark matter under its own gravitational influence suggest that galaxies grow from very smooth initial conditions through a sequence of merger and accretion events. However, theoretical models of galaxy formation, which necessarily involve modelling star formation and stellar evolution, the creation and dispersal of the chemical elements, the formation and energy output of massive black holes, and the response of gas to radiation and supernova shock waves, among much more, rely more heavily on phenomenological models than on a detailed understanding of physical theory. Thus, these models require calibration with well-studied (nearby) test cases of galaxies which we can study in detail, specifically our own Milky Way Galaxy.
The Gaia-ESO Survey is Europe’s major ground-based project to meet this scientific challenge.
The Gaia-ESO Survey, which began data-taking in January 2012, has been allocated 300nights of telescope time over five years using the European Southern Observatory's Very Large Telescope (VLT-UT2) with its premier multi-object spectrograph, FLAMES. The project will obtain high-quality spectroscopy of some 100,000 faint stars, systematically covering all the major components of the Milky Way. This will provide the first homogeneous overview of the distributions of kinematics and chemical elemental abundances in the Galaxy. With well-defined samples the Survey will quantify the kinematic+ multi-chemical element abundance distribution functions of the bulge, the thick disk, the thin disc, and the halo stellar components.
This proposal is to provide the core support team for the Co-Principal Investigator of the Gaia-ESO Survey with responsibility for the Milky Way Survey.

Fields of science (EuroSciVoc)

CORDIS classifies projects with EuroSciVoc, a multilingual taxonomy of fields of science, through a semi-automatic process based on NLP techniques. See: The European Science Vocabulary.

You need to log in or register to use this function

Topic(s)

Calls for proposals are divided into topics. A topic defines a specific subject or area for which applicants can submit proposals. The description of a topic comprises its specific scope and the expected impact of the funded project.

Call for proposal

Procedure for inviting applicants to submit project proposals, with the aim of receiving EU funding.

ERC-2012-ADG_20120216
See other projects for this call

Funding Scheme

Funding scheme (or “Type of Action”) inside a programme with common features. It specifies: the scope of what is funded; the reimbursement rate; specific evaluation criteria to qualify for funding; and the use of simplified forms of costs like lump sums.

ERC-AG - ERC Advanced Grant

Host institution

THE CHANCELLOR MASTERS AND SCHOLARS OF THE UNIVERSITY OF CAMBRIDGE
EU contribution
€ 2 499 978,00
Address
TRINITY LANE THE OLD SCHOOLS
CB2 1TN CAMBRIDGE
United Kingdom

See on map

Region
East of England East Anglia Cambridgeshire CC
Activity type
Higher or Secondary Education Establishments
Links
Total cost

The total costs incurred by this organisation to participate in the project, including direct and indirect costs. This amount is a subset of the overall project budget.

No data

Beneficiaries (1)

My booklet 0 0