Speaker
William Gillard
Description
The Euclid mission aims to deliver high-precision spectroscopic measurements to probe the geometry and evolution of the Universe. Achieving this objective requires a detailed understanding and mitigation of detector-induced effects that can bias spectroscopic data products. This work investigates the impact of key detector effects on the Euclid Near-Infrared Spectrometer and Photometer (NISP) spectroscopic data processing chain. We assess how these effects propagate through calibration and extraction steps.
Author
William Gillard