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HARMONI: the ELT's First-Light Near-infrared and Visible Integral Field Spectrograph

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arxiv 2103.11215 v1 pith:GB6NKGI2 submitted 2021-03-20 astro-ph.IM

HARMONI: the ELT's First-Light Near-infrared and Visible Integral Field Spectrograph

classification astro-ph.IM
keywords adaptivefieldharmoniintegralnear-infraredopticsspectrographchoices
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The High Angular Resolution Monolithic Optical and Near-infrared Integral field spectrograph (HARMONI) is the visible and near-infrared (NIR), adaptive-optics-assisted, integral field spectrograph for ESO's Extremely Large Telescope (ELT). It will have both a single-conjugate adaptive optics (SCAO) mode (using a single bright natural guide star) and a laser tomographic adaptive optics (LTAO) mode (using multiple laser guide stars), providing near diffraction-limited hyper-spectral imaging with high performance and good sky coverage, respectively. A unique high-contrast adaptive optics (HCAO) capability has recently been added for exoplanet characterisation. A large detector complement of eight HAWAII-4RG arrays, four choices of spaxel scale, and 11 grating choices with resolving powers ranging from R~3000 to R~17000 make HARMONI a very versatile instrument that can cater to a wide range of observing programmes.

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