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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

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

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

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

A 3D view of dwarf galaxies with Gaia and VLT/FLAMES. I. The Sculptor dwarf spheroidal

Hidden deep in the halo: selection of a reduced proper motion halo catalogue and mining retrograde streams in the velocity space

Metallicity Distribution Functions of 13 Ultra-faint Dwarf Galaxy Candidates from Hubble Space Telescope Narrowband Imaging

The Pristine dwarf galaxy survey-V. The edges of the dwarf galaxy Hercules

The Pristine Inner Galaxy Survey (PIGS) - V. A chemo-dynamical investigation of the early assembly of the Milky Way with the most metal-poor stars in the bulge

The Pristine Inner Galaxy Survey (PIGS) - VI. Different vertical distributions between two DIBs at 442.8 nm and 862.1 nm

The Pristine survey - XX. GTC follow-up observations of extremely metal-poor stars identified from Pristine and LAMOST

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