Ground-Based and Airborne Instrumentation for Astronomy IX 2022
DOI: 10.1117/12.2630427
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METIS: final design of the Imager sub-system

Abstract: METIS, the Mid-infrared Imager and Spectrograph for the Extremely Large Telescope (ELT), is one of the three firstgeneration science instruments and about to complete its final design phase [1]. The Imager sub-system provides diffraction-limited imaging capabilities and low-resolution grism-spectroscopy in two channels: one covers the atmospheric L&M bands with a field of view of 11x11 arcsec, and the second covers the N band, with a field of view of 14x14 arcsec.Both channels have a common collimator and a di… Show more

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“…The imager covers the wavelength range from L to N band (approximately 3 -13 µm). For optimal performance, this wavelength range is split into two channels, which are equipped with two different science detectors [23]. The imager has a collimator, that is common to both channels, and two camera optics optimized for the field of view (Figure 1), defined by the science detectors and the required sampling (5.5 marcsec pixels at L/M band and 6.8 marcsec pixels at Nband).…”
Section: Imagermentioning
confidence: 99%
“…The imager covers the wavelength range from L to N band (approximately 3 -13 µm). For optimal performance, this wavelength range is split into two channels, which are equipped with two different science detectors [23]. The imager has a collimator, that is common to both channels, and two camera optics optimized for the field of view (Figure 1), defined by the science detectors and the required sampling (5.5 marcsec pixels at L/M band and 6.8 marcsec pixels at Nband).…”
Section: Imagermentioning
confidence: 99%