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- W4285489993 abstract "The Exoplanets at LBT with a Visible IFS for SHARK-VIS (ELVIS) is an add-on imaging spectrograph to be integrated in the new LBT high-contrast high-resolution AO-assisted imager SHARK-VIS. ELVIS is optimized for a medium/high spectral resolution of 10-20k with a limited bandwidth around the Hα, and it is planned fed by a small core (10-20 ⊘ µm) multi mode fiber bundle providing about 140 spaxels on a field of view around 300×300 sqmas. This instrument has a very compact design based on a VPH dispersing element to allow its installation within a standard 19” rack mount. As shown in the literature, young accreting sub-stellar and planetary companions are better detected and analyzed by these instruments allowing to reach contrast at least ten times fainter (in their Hα emission) with respect to standard imagers." @default.
- W4285489993 created "2022-07-15" @default.
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- W4285489993 date "2022-08-29" @default.
- W4285489993 modified "2023-09-27" @default.
- W4285489993 title "ELVIS: the exoplanets at LBT with a visible IFS for SHARK-VIS" @default.
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- W4285489993 doi "https://doi.org/10.1117/12.2629400" @default.
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