Extensive experience studying
astronomical spectroscopic data
Hyperspectral Imaging
Hyperspectral imaging (HSI) is a technique that acquires a spectrum for each pixel of an object, capturing detailed wavelength information across numerous narrow bands. The resulting data are structured as a “data cube,” which adds wavelength (λ) as a third dimension alongside the spatial x and y coordinates.
|
|
|
|---|---|---|
| Number of bands (number of wavelength ranges captured) | ||
3 bands |
~10 bands |
100+ bands |
| Amount of extractable information | ||
Significant information gaps due to only three bands |
Captures more information, but misses ranges that might be crucial |
Continuous spectrum which captures full information at each pixel |
NISS
The world’s first wide-field infrared hyperspectral imager Unveiling the formation of stars and galaxies through a wide field of view
SPHEREx
PI of the Korean team for NASA’s SPHEREx project
The first mission to map the entire sky with infrared spectroscopy
Experimental Chamber
The world’s only infrared optics laboratory instrument
Validating optical performance under cryogenic and vacuum conditions equivalent to space
Supporting the development and reliability verification of next-generation space-based observatories
Spectroscopic Data Research
Decades of expertise in unlocking the universe through large-scale spectroscopic data analysis
