Poster + Paper
23 August 2024 Spectral response of the SPHEREx telescope
Howard Hui, Phillip M. Korngut, Samuel Condon, Chi Nguyen, Stephen Padin, Jamie J. Bock, Charles D. Dowell, Woong-Seob Jeong, Youngsoo Jo, Kenneth Manatt, Hien Nguyen, Sung-Joon Park, Jeonghyun Pyo, Yujin Yang
Author Affiliations +
Conference Poster
Abstract
The Spectro-Photometer for the History of the Universe, Epoch of Reionization, and Ices Explorer (SPHEREx) is an upcoming all-sky near-infrared spectroscopic survey satellite designed to address all three primary science goals of NASA’s Astrophysics Division. SPHEREx employs a series of Linear Variable Filters (LVFs) to create 102 spectral channels across the wavelength range of 0.75 to 5 µm, with spectral resolutions R between 35 and 120. This paper presents the spectral calibration setup used for SPHEREx and discusses the various challenges encountered during the measurement process. Ultimately, we demonstrate the spectral responses for all 25 million pixels in SPHEREx.
© (2024) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Howard Hui, Phillip M. Korngut, Samuel Condon, Chi Nguyen, Stephen Padin, Jamie J. Bock, Charles D. Dowell, Woong-Seob Jeong, Youngsoo Jo, Kenneth Manatt, Hien Nguyen, Sung-Joon Park, Jeonghyun Pyo, and Yujin Yang "Spectral response of the SPHEREx telescope", Proc. SPIE 13092, Space Telescopes and Instrumentation 2024: Optical, Infrared, and Millimeter Wave, 130923N (23 August 2024); https://doi.org/10.1117/12.3018463
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KEYWORDS
Sensors

Spectral response

Telescopes

Monochromators

Spectral calibration

Spectral resolution

Cryogenics

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