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Visible camera cryostat design and performance for the SuMIRe Prime Focus Spectrograph (PFS)

Author(s): Smee, Stephen A; Gunn, James E; Golebiowski, Mirek; Hope, Stephen C; Madec, Fabrice; et al

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dc.contributor.authorSmee, Stephen A-
dc.contributor.authorGunn, James E-
dc.contributor.authorGolebiowski, Mirek-
dc.contributor.authorHope, Stephen C-
dc.contributor.authorMadec, Fabrice-
dc.contributor.authorGabriel, Jean-Francois-
dc.contributor.authorLoomis, Craig-
dc.contributor.authorLe Fur, Arnaud-
dc.contributor.authorDohlen, Kjetil-
dc.contributor.authorLe Mignant, David-
dc.contributor.authorBarkhouser, Robert-
dc.contributor.authorCarr, Michael-
dc.contributor.authorHart, Murdock-
dc.contributor.authorTamura, Naoyuki-
dc.contributor.authorShimono, Atsushi-
dc.contributor.authorTakato, Naruhisa-
dc.date.accessioned2023-12-12T16:06:58Z-
dc.date.available2023-12-12T16:06:58Z-
dc.date.issued2016en_US
dc.identifier.citationSmee, Stephen A, Gunn, James E, Golebiowski, Mirek, Hope, Stephen C, Madec, Fabrice, Gabriel, Jean-Francois, Loomis, Craig, Le Fur, Arnaud, Dohlen, Kjetil, Le Mignant, David, Barkhouser, Robert, Carr, Michael, Hart, Murdock, Tamura, Naoyuki, Shimono, Atsushi, Takato, Naruhisa. (2016). Visible camera cryostat design and performance for the SuMIRe Prime Focus Spectrograph (PFS). GROUND-BASED AND AIRBORNE INSTRUMENTATION FOR ASTRONOMY VI, 9908 (10.1117/12.2233185en_US
dc.identifier.issn0277-786X-
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/pr1mc8rg43-
dc.description.abstractWe describe the design and performance of the SuMIRe Prime Focus Spectrograph (PFS) visible camera cryostats. SuMIRe PFS is a massively multi-plexed ground-based spectrograph consisting of four identical spectrograph modules, each receiving roughly 600 fibers from a 2394 fiber robotic positioner at the prime focus. Each spectrograph module has three channels covering wavelength ranges 380 nm - 640 nm, 640 nm - 955 nm, and 955 nm - 1.26 um, with the dispersed light being imaged in each channel by a f/1.07 vacuum Schmidt camera. The cameras are very large, having a clear aperture of 300 mm at the entrance window, and a mass of similar to 280 kg. In this paper we describe the design of the visible camera cryostats and discuss various aspects of cryostat performance.en_US
dc.language.isoen_USen_US
dc.relation.ispartofGROUND-BASED AND AIRBORNE INSTRUMENTATION FOR ASTRONOMY VIen_US
dc.rightsAuthor's manuscripten_US
dc.titleVisible camera cryostat design and performance for the SuMIRe Prime Focus Spectrograph (PFS)en_US
dc.typeConference Articleen_US
dc.identifier.doidoi:10.1117/12.2233185-
pu.type.symplectichttp://www.symplectic.co.uk/publications/atom-terms/1.0/journal-articleen_US

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