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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Full metadata record
DC Field | Value | Language |
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dc.contributor.author | Smee, Stephen A | - |
dc.contributor.author | Gunn, James E | - |
dc.contributor.author | Golebiowski, Mirek | - |
dc.contributor.author | Hope, Stephen C | - |
dc.contributor.author | Madec, Fabrice | - |
dc.contributor.author | Gabriel, Jean-Francois | - |
dc.contributor.author | Loomis, Craig | - |
dc.contributor.author | Le Fur, Arnaud | - |
dc.contributor.author | Dohlen, Kjetil | - |
dc.contributor.author | Le Mignant, David | - |
dc.contributor.author | Barkhouser, Robert | - |
dc.contributor.author | Carr, Michael | - |
dc.contributor.author | Hart, Murdock | - |
dc.contributor.author | Tamura, Naoyuki | - |
dc.contributor.author | Shimono, Atsushi | - |
dc.contributor.author | Takato, Naruhisa | - |
dc.date.accessioned | 2023-12-12T16:06:58Z | - |
dc.date.available | 2023-12-12T16:06:58Z | - |
dc.date.issued | 2016 | en_US |
dc.identifier.citation | Smee, 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 (10.1117/12.2233185 | en_US |
dc.identifier.issn | 0277-786X | - |
dc.identifier.uri | http://arks.princeton.edu/ark:/88435/pr1mc8rg43 | - |
dc.description.abstract | We 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.iso | en_US | en_US |
dc.relation.ispartof | GROUND-BASED AND AIRBORNE INSTRUMENTATION FOR ASTRONOMY VI | en_US |
dc.rights | Author's manuscript | en_US |
dc.title | Visible camera cryostat design and performance for the SuMIRe Prime Focus Spectrograph (PFS) | en_US |
dc.type | Conference Article | en_US |
dc.identifier.doi | doi:10.1117/12.2233185 | - |
pu.type.symplectic | http://www.symplectic.co.uk/publications/atom-terms/1.0/journal-article | en_US |
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