The FOS
examined fainter objects than the High Resolution Spectrograph (HRS), and could study these objects across a much wider spectral range — from the UV (1150 Angstroms) through the visible red and the near - IR (8000 Angstroms).
Not exact matches
SOFIA's
Faint Object Infrared Camera will
examine the Milky Way's tumultuous center, star - forming regions, dust clouds, and nearby galaxies.