NASA NTRS · 20030032982
Coronagraphic Imaging with HST and STIS
Abstract
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.
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Grady, C. A., Proffitt, C., Malumuth, E., Woodgate, B. E., Gull, T. R., Bowers, C. W., Heap, S. R., Kimble, R. A., Lindler, D., Plait, P.. 2002-01-01. Coronagraphic Imaging with HST and STIS. https://ntrs.nasa.gov/citations/20030032982
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