タイトル | Coronagraphic Imaging with HST and STIS |
本文(外部サイト) | http://hdl.handle.net/2060/20030032982 |
著者(英) | Heap, S. R.; Kimble, R. A.; Gull, T. R.; Proffitt, C.; Malumuth, E.; Bowers, C. W.; Lindler, D.; Woodgate, B. E.; Grady, C. A.; Plait, P. |
著者所属(英) | NASA Goddard Space Flight Center |
発行日 | 2002-01-01 |
言語 | eng |
内容記述 | Revealing faint circumstellar nebulosity and faint stellar or substellar companions to bright stars typically requires use of techniques for rejecting the direct, scattered, and diffracted light of the star. One such technique is Lyot coronagraphy. We summarize the performance of the white-light coronagraphic capability of the Space Telescope Imaging spectrograph, on board the Hubble Space Telescope. |
NASA分類 | Astrophysics |
権利 | Copyright, Distribution as joint owner in the copyright |
|