The formation and evolution of the Milky Way as read in its stars

Related content

• Activities

• Spectroscopic studies of the Milky Way, stellar ages

  Activity: Examination and supervision › Supervision of PostDoc

• Projects

• The New Milky Way

  Project: Research

• 4MOST - massive spectroscopic surveys of the Milky Way and the Universe

  Project: Research

• WEAVE - a massively multiplex spectrograph for the William Herschel Telescope and associated surveys

  Project: Research

• Research output

• Selecting accreted populations: Metallicity, elemental abundances, and ages of the Gaia-Sausage-Enceladus and Sequoia populations

  Research output: Contribution to journal › Article › peer-review

• 4MOST: Project overview and information for the First Call for Proposals

  Research output: Contribution to journal › Article › peer-review

• The Gaia -ESO Survey: Spectroscopic-asteroseismic analysis of K2 stars in Gaia -ESO

  Research output: Contribution to journal › Article › peer-review

• Vintergatan - i. The origins of chemically, kinematically, and structurally distinct discs in a simulated milky way-mass galaxy

  Research output: Contribution to journal › Article › peer-review

• Exploring the stellar age distribution of the milky way bulge using APOGEE

  Research output: Contribution to journal › Article › peer-review

• The Gaia -ESO survey: The non-universality of the age-chemical-clocks-metallicity relations in the Galactic disc

  Research output: Contribution to journal › Article › peer-review

• Spatial variations in the Milky Way disc metallicity-age relation

  Research output: Contribution to journal › Article › peer-review

• The SkyMapper-Gaia RVS view of the Gaia–Enceladus–Sausage  – an investigation of the metallicity and mass of the Milky Way’s last major merger

  Research output: Contribution to journal › Article › peer-review

• The HR 1614 moving group is not a dissolving cluster

  Research output: Contribution to journal › Article › peer-review