English

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

Instrumentation and Methods for Astrophysics 2016-12-14 v1 Instrumentation and Detectors

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 \sim280~kg. In this paper we describe the design of the visible camera cryostats and discuss various aspects of cryostat performance.

Keywords

Cite

@article{arxiv.1608.01196,
  title  = {Visible camera cryostat design and performance for the SuMIRe Prime Focus Spectrograph (PFS)},
  author = {Stephen A. Smee and James E. Gunn and Mirek Golebiowski and Stephen C. Hope and Fabrice Madec and Jean-Francois Gabriel and Craig Loomis and Arnaud Le Fur and Kjetil Dohlen and David Le Mignant and Robert Barkhouser and Michael Carr and Murdock Hart and Naoyuki Tamura and Atsushi Shimono and Naruhisa Takato},
  journal= {arXiv preprint arXiv:1608.01196},
  year   = {2016}
}
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