E-Elt/Metis

B. Brandl,S. Quanz, M. Feldt, A. Glasse, M. Guedel,M. Meyer, E. Pantin,C. Waelkens,K. Pontoppidan,E. Van Dishoeck,O. Absil,R. Van Boekel, T. Ratzka, T. Henning

6TH ZERMATT ISM-SYMPOSIUM: CONDITIONS AND IMPACT OF STAR FORMATION: FROM LAB TO SPACE: IN MEMORY OF CHARLES H. TOWNES(2016)

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摘要
The Mid-infrared E-ELT Imager and Spectrograph (METIS) will be one of the first three scientific instruments on the European Extremely Large Telescope (E-ELT). It will be the only instrument to cover the thermal/mid-infrared wavelength range from 3-19 m. METIS offers a number of scientifically important observing modes, including diffraction-limited imaging, low resolution slit spectroscopy, coronagraphy, and high resolution (R similar to 100,000) integral field spectroscopy at very high sensitivity.This paper gives a brief summary of METIS and focuses on its unique discovery space in the area of protoplanetary disks, where METIS is quite complementary to ALMA and JWST.
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