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Over ons Praktische zaken Waar vindt u ons prof. dr. E. (Else) Starkenburg

Research interests

My main research interests concern the early history of the Milky Way and surrounding galaxies. I am using both photometric and spectroscopic observations as well as modelling to study these systems. In particular, several of my projects focus on the first generations of stars in these systems that contain valuable information about our Galaxy’s childhood as well as conditions in the early Universe in general. The search for such most pristine (and presumably extremely old) stars has justifiably been compared with finding needles in a haystack as these stars are extremely rare. I am the founder and Principal Investigator for the "Pristine Survey", an international collaboration uncovering and studying these rare earliest generation stars in the Galaxy with unprecedented efficiency and success. The Pristine survey collaboration is an international team of over 30 scientists and the project to date has already resulted in 18 peer-reviewed articles and 5 successful PhD theses, with more in preparation. I am furthermore deeply involved in upcoming and future instrumentation and surveys in my field, for instance as co-lead for one of the ten 4MOST consortium surveys and co-lead for the very metal-poor (early generation) star working group for the WEAVE spectrograph.

Publicaties

Charting the Galactic Acceleration Field. II. A Global Mass Model of the Milky Way from the STREAMFINDER Atlas of Stellar Streams Detected in Gaia DR3

Gaia's brightest very metal-poor (VMP) stars: Metallicity catalogue of a thousand VMP stars from Gaia's radial velocity spectrometer spectra

Improving metallicity estimates for very metal-poor stars in the Gaia DR3 GSP-Spec catalog

Probing the early Milky Way with GHOST spectra of an extremely metal-poor star in the Galactic disc

Stellar Metallicities and Gradients in the Faint M31 Satellites Andromeda XVI and Andromeda XXVIII

Stellar Metallicities and Gradients in the Isolated, Quenched Low-mass Galaxy Tucana

Swarming in stellar streams: Unveiling the structure of the Jhelum stream with ant colony-inspired computation

The 33 M black hole Gaia BH3 is part of the disrupted ED-2 star cluster

The metal-poor edge of the Milky Way' s thin disc

The Pristine Inner Galaxy Survey (PIGS): IX. The largest detailed chemical analysis of very metal-poor stars in the Sagittarius dwarf galaxy

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