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124667 |
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|a Seager, Sara
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|a Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
|e contributor
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|a Mapping the observable sky for a remote occulter working with ground-based telescopes
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|b SPIE-Intl Soc Optical Eng,
|c 2020-04-15T17:54:27Z.
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|z Get fulltext
|u https://hdl.handle.net/1721.1/124667
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|a The Remote Occulter (Orbiting Starshade) is a proposed 100-meter class starshade working with a ground-based telescope, designed for visible-band imaging and spectroscopy of temperate planets around sun-like stars. With advanced adaptive optics and the largest telescopes like the 39 m ELT, it would enable the study of planetary systems and a wide variety of exoplanets. In this paper, we describe the geometrical constraints and establish which parts of the sky are observable. ©2019
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|a Article
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|t 10.1117/12.2528756
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|t Proceedings of SPIE, the International Society for Optical Engineering
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