タイトル | The Optical Design of CHARIS: An Exoplanet IFS for the Subaru Telescope |
本文(外部サイト) | http://hdl.handle.net/2060/20140017483 |
著者(英) | Groff, Tyler; Hayashi, Masahiko; Guyone, Olivier; Takato, Naruhisa; Kasdin, N. Jeremy; Peters-Limbach, Mary; Jovanovic, Nemanja; Fagan, Rad; Galvin, Michael; LeClerc, Dave; Driscoll, Dave; Carr, Michael; Brandt, Timothy; Knapp, Gillian; Foster, Allen; Janson, Markus; McElwain, Michael; Martinache, Frantz |
著者所属(英) | NASA Goddard Space Flight Center |
発行日 | 2013-08-25 |
言語 | eng |
内容記述 | High-contrast imaging techniques now make possible both imaging and spectroscopy of planets around nearby stars. We present the optical design for the Coronagraphic High Angular Resolution Imaging Spectrograph (CHARIS), a lenslet-based, cryogenic integral field spectrograph (IFS) for imaging exoplanets on the Subaru telescope. The IFS will provide spectral information for 138138 spatial elements over a 2.07 arcsec 2.07 arcsec field of view (FOV). CHARIS will operate in the near infrared (lambda = 1.15 2.5 micrometers) and will feature two spectral resolution modes of R is approximately 18 (low-res mode) and R is approximately 73 (high-res mode). Taking advantage of the Subaru telescope adaptive optics systems and coronagraphs (AO188 and SCExAO), CHARIS will provide sufficient contrast to obtain spectra of young self-luminous Jupiter-mass exoplanets. CHARIS will undergo CDR in October 2013 and is projected to have first light by the end of 2015. We report here on the current optical design of CHARIS and its unique innovations. |
NASA分類 | Optics; Astronomy |
レポートNO | GSFC-E-DAA-TN14959 |
権利 | Copyright, Distribution as joint owner in the copyright |
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