An Ultra-Stable Mid-Infrared Sensor for the Detection of Bio-Signatures by Means of Transit Spectroscopy
2019 IEEE AEROSPACE CONFERENCE（2019）
Key words
Trappist-1 system,ultra cool M-dwarf star,habitable zone,planetary systems,dwarf stars,exoplanets,high-priority science goal,future space missions,spectral range,planets atmosphere,Mid-IR transit spectrometers,Origins Space Telescope,M-dwarfs,mid-IR detectors,impurity band conduction devices,exposure dependent response,IBC detectors,ultra-stable Mid-IR Array Spectrometer demonstration,Exoplanet Transits,atmospheric bio-signatures,habitable-zone planets,Transition Edge Sensor detectors,mid-IR transit spectroscopy,high-accuracy calibration system,stable reference source,in-band calibration,detector gain,OST space telescope,spectral lines,wavelength 3.0 micron to 15.0 micron,wavelength 0.5 mum
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