Optical Design of the SuMIRe PFS Spectrograph
Sandrine Pascal, Sebastien Vives, Robert Barkhouser, James Gunn

TL;DR
This paper details the optical design of the SuMIRe PFS spectrograph, highlighting innovative features like the Mangin-Schmidt camera and optimized optical architecture for high image quality across multiple spectral channels.
Contribution
It introduces a novel optical design for the PFS spectrograph, including the use of a Mangin-Schmidt camera to achieve wide field-of-view and high performance.
Findings
Optimized optical design achieves high image quality.
Innovative Mangin-Schmidt camera enables large field-of-view.
Performance analysis confirms design effectiveness.
Abstract
The SuMIRe Prime Focus Spectrograph (PFS), developed for the 8-m class SUBARU telescope, will consist of four identical spectrographs, each receiving 600 fibers from a 2394 fiber robotic positioner at the telescope prime focus. Each spectrograph includes three spectral channels to cover the wavelength range 0.38-1.26 um with a resolving power ranging between 2000 and 4000. A medium resolution mode is also implemented to reach a resolving power of 5000 at 0.8 um. Each spectrograph is made of 4 optical units: the entrance unit which produces three corrected collimated beams and three camera units (one per spectral channel). The beam is split by using two large dichroics; and in each arm, the light is dispersed by large VPH gratings. The proposed optical design was optimized to achieve the requested image quality while simplifying the manufacturing of the whole optical system. The camera…
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