Image Details
Caption: Figure 2.
A schematic layout of the LBTI instrument, which receives the beams from both sub-telescopes, combines them, and directs them through a trichroic and beamsplitter elements onto the science and phase detectors. The star indicates the fast pathlength corrector mirror, which is used to correct the phase.
© 2022. The Author(s). Published by the American Astronomical Society.