CORDIS Project
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The SPIAKID project develops a specialized camera using Kinetic Inductance Detectors to enhance an 8-meter telescope's ability to measure the ages and metallicities of stars in Ultra Faint Dwarf galaxies. This technology aims to improve our understanding of early galaxy formation and can also be applied to other scient…
The SPIAKID project will build a camera using Kinetic Inductance Detectors (KIDs) to equip an 8 m class telescope to derive ages and metallicities for stars in Ultra Faint Dwarf galaxies (UFDs) in the Local Group.
UFDs are the key to understand early galaxy formation processes, including the properties of the first stars, and the role of environment and internal feedback in shaping the evolution of dwarf galaxies.
A full exploitation of UFDs to understand these processes requires knowledge of th…
CENTRE NATIONAL DE LA RECHERCHE SCIENTIFIQUE CNRS
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France, Paris
Type: University / higher education
Activity type: Higher or Secondary Education Establishments
SME: No
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