Schmidt AI in Science Fellow · CITA Fellow · University of Toronto

Modelling and measuring the Universe

Christian Kragh Jespersen

03

Data-driven science with spectra

Spectra are the most information-rich data type we have, and they are the cornerstone of galaxy property inference. Whether for galaxy evolution or instrument calibration, we can do better science and make better models by using them more effectively.

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04

Instrument optimization

Calibration from the Earth's sky itself. Airglow, sky subtraction and wavelength solutions for the Prime Focus Spectrograph, plus PSF work for COSMOS2020.

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