At Hopkins / STScI, I have been part of a core science team that will use JWST GTO time to study star formation in a wide range of environments, from ‘extreme’ to more ‘quiescent’ regions, spanning almost two orders of magnitude in metallicity. I’ve been responsible for defining and planning these observations, maximizing the scientific output from various JWST instruments (MIRI/NIRCam/NIRSpec) and observational modes (imaging, IFU spectroscopy, MOS).

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