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The stellar-substellar limit in the large scale survey EuclidClosing date: 2024-04-15
Contact: Celine Reyle
The successful applicant will work on the identification of ultra cool dwarfs in Euclid fields, and may propose new identification techniques and explore the possibility of using the precise PSF of Euclid to identify close binaries. Other challenges can be addressed, such as to determine the luminosity function, infer the most likely low-mass end of the initial mass function and explore its degree of universality in different components of the Milky Way.

The candidate will be working with the international Euclid UCD group within the consortium, as well as the Gaia UCD team.

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