Poster + Paper
18 July 2024 Prime Focus Spectrograph (PFS) for Subaru Telescope: integration and test of the last spectrograph modules
Julien Rousselle, Yuki Moritani, Fabrice Madec, Patrick Blanchard, David Le Mignant, Michael Carle, Thibaut Crauchet, Rudy Barette, Shintaro Koshida, Matthew Wung, Kumiko Morihana, Arnaud Le Fur, Craig Loomis, Naoyuki Tamura
Author Affiliations +
Conference Poster
Abstract
PFS (Prime Focus Spectrograph) is an ultra-wide-field, multi-object spectrograph currently being commissioned at Subaru telescope. The focal plane is made of ∼2400 science fibers and fiber positioners at the telescope prime focus, covering a field of view of 1.3 deg in diameter. The science fibers will be connected to 4 identical spectrograph modules, each receiving ∼600 fibers. Every spectrograph module will host 3 cameras, covering the blue (380–650 nm), red (630–970 nm) and near-infrared (940–1260 nm) wavelengths. This presentation will focus on the completion of the PFS spectrograph modules at the Subaru telescope. We will present their integration and test processes and measured performance, as well as the technical challenges encountered along the way, and the solutions used to correct them.
(2024) Published by SPIE. Downloading of the abstract is permitted for personal use only.
Julien Rousselle, Yuki Moritani, Fabrice Madec, Patrick Blanchard, David Le Mignant, Michael Carle, Thibaut Crauchet, Rudy Barette, Shintaro Koshida, Matthew Wung, Kumiko Morihana, Arnaud Le Fur, Craig Loomis, and Naoyuki Tamura "Prime Focus Spectrograph (PFS) for Subaru Telescope: integration and test of the last spectrograph modules", Proc. SPIE 13096, Ground-based and Airborne Instrumentation for Astronomy X, 130962L (18 July 2024); https://doi.org/10.1117/12.3020408
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KEYWORDS
Cameras

Spectrographs

Near infrared

Telescopes

Vacuum

System integration

Temperature control

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