Kota Hayashi,1,2 Neven Caplar,3 Kiyoto Yabe,4 Robert H. Lupton,5 James E. Gunn,5 Masahiro Takada,1 Naoyuki Tamura,4 Yuki Moritanihttps://orcid.org/0000-0003-2541-1052,4 Satoshi Kawanomoto,6 Naoki Yasuda1
1Kavli Institute for the Physics and Mathematics of the Universe (Japan) 2The Univ. of Tokyo (Japan) 3Univ. of Washington (United States) 4Subaru Telescope, National Astronomical Observatory of Japan (United States) 5Princeton Univ. (United States) 6National Astronomical Observatory of Japan (Japan)
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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.
Kota Hayashi,Neven Caplar,Kiyoto Yabe,Robert H. Lupton,James E. Gunn,Masahiro Takada,Naoyuki Tamura,Yuki Moritani,Satoshi Kawanomoto, andNaoki 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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Kota Hayashi, Neven Caplar, Kiyoto Yabe, Robert H. Lupton, James E. Gunn, Masahiro Takada, Naoyuki Tamura, Yuki Moritani, Satoshi Kawanomoto, 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