翻訳と辞書 |
Optical System for Imaging and low Resolution Integrated Spectroscopy : ウィキペディア英語版 | Optical System for Imaging and low Resolution Integrated Spectroscopy OSIRIS (Optical System for Imaging and low Resolution Integrated Spectroscopy) is the Spanish Day One instrument for the Gran Telescopio Canarias (GTC). Sensitive in the wavelength range from 365 through 1000 nm, OSIRIS is a multiple purpose instrument for imaging and low-resolution long slit and multiple object spectroscopy (MOS). Imaging can be done using broad-band filters or narrow-band tunable filters with FWHM ranging from 0.2 to 0.9 nm at 365 nm, through 0.9 to 1.2 at 1000 nm. OSIRIS observing modes include also fast photometry and spectroscopy. OSIRIS field of view is of 8.5×8.5 arcminutes and the maximum nominal spectral resolution is of 5000 for a slit width of 0.6 arcsec. MOS incorporates detector charge shuffling co-ordinated with telescope nodding for an excellent sky subtraction. The use of tunable filters is a completely new feature in 8 to 10 m class telescopes that will allow observing the very faint and distant emission line objects. The OSIRIS scientific Key Project is OTELO. ==External links==
*(Gran Telescopio CANARIAS OSIRIS instrument page ) *(OSIRIS Home Page (IAC) )
抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)』 ■ウィキペディアで「Optical System for Imaging and low Resolution Integrated Spectroscopy」の詳細全文を読む
スポンサード リンク
翻訳と辞書 : 翻訳のためのインターネットリソース |
Copyright(C) kotoba.ne.jp 1997-2016. All Rights Reserved.
|
|