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dc.contributor.authorSeager, Sara
dc.date.accessioned2020-04-15T17:54:27Z
dc.date.available2020-04-15T17:54:27Z
dc.date.issued2019-09
dc.identifier.issn0277-786X
dc.identifier.urihttps://hdl.handle.net/1721.1/124667
dc.description.abstractThe 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. ©2019en_US
dc.language.isoen
dc.publisherSPIE-Intl Soc Optical Engen_US
dc.relation.isversionof10.1117/12.2528756en_US
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.en_US
dc.sourceSPIEen_US
dc.titleMapping the observable sky for a remote occulter working with ground-based telescopesen_US
dc.typeArticleen_US
dc.identifier.citationPeretz, Eliad, et al., "Mapping the observable sky for a remote occulter working with ground-based telescopes." Proceeding of SPIE 11117: Techniques and Instrumentation for Detection of Exoplanets IX, August 11-15, 2019, San Diego, California (2019): 111170S doi 10.1117/12.2528756 ©2019 Author(s)en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciencesen_US
dc.relation.journalProceedings of SPIE, the International Society for Optical Engineeringen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/ConferencePaperen_US
eprint.statushttp://purl.org/eprint/status/NonPeerRevieweden_US
dc.date.updated2020-04-07T12:16:15Z
dspace.orderedauthorsPeretz, Eliad ; Mather, John ; Seager, Sara ; Slonaker, Richard ; Shaklan, Stuart ; Willems, Phil ; Hildebrant, Sergeien_US
dspace.date.submission2020-04-07T12:16:17Z
mit.journal.volume11117en_US
mit.licensePUBLISHER_POLICY
mit.metadata.statusComplete


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