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Update on the LBTI: a versatile high-contrast and high-resolution infrared imager for a 23-m telescope

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Academic year: 2021

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Figure

Figure 1.: Components of the LBTI shown with the optical path through the beam combiner and the NIC cryostat
Figure 2.: Optical layout of NOMIC. The light enters from the left side, is reflected by the beam diverter and reimaged by LWBC 1
Figure 3.: Optical layout of Phasecam. The outputs of the nulling beamsplitter are directed via several lenses to two quadrants of a PICNIC detector.
Figure 4.: Fizeau interferometric PSF at 4.0 µm and 11.0 µm obtained respec- respec-tively with LMIRcam and NOMIC.
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