Poster + Paper
20 August 2024 Prime focus spectrograph (PFS) for Subaru Telescope: modeling of the 2D point spread function using commissioning data
Kota Hayashi, Neven Caplar, Kiyoto Yabe, Robert H. Lupton, James E. Gunn, Masahiro Takada, Naoyuki Tamura, Yuki Moritani, Satoshi Kawanomoto, Naoki Yasuda
Author Affiliations +
Conference Poster
Abstract
Prime Focus Spectrograph is a next-generation spectroscopic instrument being installed on Subaru Telescope. The key to the success of its cosmological survey is accurate sky subtraction to extract galaxy emission lines from very bright night-sky emissions. We model the two-dimensional point spread function considering various e↵ects such as optical aberrations in the spectrographs and vignetting on the telescope prime focal plane. We are developing models using commissioning data, and currently we have achieved 1 % precision in one-dimensional spectra for the aberration model.
© (2024) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Kota Hayashi, Neven Caplar, Kiyoto Yabe, Robert H. Lupton, James E. Gunn, Masahiro Takada, Naoyuki Tamura, Yuki Moritani, Satoshi Kawanomoto, and Naoki Yasuda "Prime focus spectrograph (PFS) for Subaru Telescope: modeling of the 2D point spread function using commissioning data", Proc. SPIE 13096, Ground-based and Airborne Instrumentation for Astronomy X, 130969R (20 August 2024); https://doi.org/10.1117/12.3019024
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KEYWORDS
Data modeling

Spectrographs

Telescopes

Point spread functions

Vignetting

Optical aberrations

Modeling

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