Chinese Optics Letters, Volume. 23, Issue 3, 031301(2025)

High-resolution waveguide array-based astronomical spectrograph with cascaded phase modulation

Yunxian Zhong1,2,3, Dong Lin1,2,3, Biao Xu1,2,4, Zhuangzhuang Zhu1,2,3, Xue Tong1,2,3, Qing Zhong1,2,3, Jijun Feng5、*, and Jinping He1,2,4、**
Author Affiliations
  • 1Laboratory of Solar and Space Instruments, Nanjing Institute of Astronomical Optics & Technology, Chinese Academy of Sciences, Nanjing 210042, China
  • 2CAS Key Laboratory of Astronomical Optics & Technology, Nanjing Institute of Astronomical Optics & Technology, Chinese Academy of Sciences, Nanjing 210042, China
  • 3University of Chinese Academy of Sciences, Beijing 100049, China
  • 4University of Chinese Academy of Sciences, Nanjing 211135, China
  • 5Shanghai Key Laboratory of Modern Optical System, Engineering Research Center of Optical Instrument and System, Ministry of Education, School of Optical-Electrical and Computer Engineering, University of Shanghai for Science and Technology, Shanghai 200093, China
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    Figures & Tables(7)
    (a) Schematic diagram of the CPMWA structure. Inset (i) shows variable output waveguide spacing. Inset (ii) shows the design and optical field mode of the waveguide. (b) Schematic diagram of the star coupler. (c) Schematic diagram of the reconfigurable module.
    (a) Electric field amplitude obtained through the beam propagation simulation of the star coupler. (b) The electric field amplitude at the end of the simulated region shows the Gaussian envelope of the illumination pattern of the tapered waveguide as sampled by the waveguide array.
    Experimental setup of the CPMWA spectrograph. MO, microscope objectives; SL, spherical lens.
    (a) Captured spectral lines at different wavelengths of the CPMWA spectrograph. (b) Spectrum measured with the CPMWA spectrograph. (c) Measured and fitted spectrum with an FWHM of 2.0 pixels at 1550 nm.
    (a) Near-field images of the output facet of the CPMWA. (b) Normalized light transmission of the 80 waveguides in the CPMWA chip. (c) The line spread function of the CPMWA spectrograph is calculated from the theoretical (blue line) and measured transmission (red line).
    (a) Spectrum reconstruction overall process. Li represents the designed length of the ith waveguide. (b) Phase error detection. (c) Spectrum reconstruction process.
    (a) Ideal spectrum. (b) Measured spectrum. (c) Corrected spectrum, contrast up to 20 dB.
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    Yunxian Zhong, Dong Lin, Biao Xu, Zhuangzhuang Zhu, Xue Tong, Qing Zhong, Jijun Feng, Jinping He, "High-resolution waveguide array-based astronomical spectrograph with cascaded phase modulation," Chin. Opt. Lett. 23, 031301 (2025)

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    Paper Information

    Category: Integrated Optics

    Received: May. 31, 2024

    Accepted: Aug. 30, 2024

    Posted: Aug. 30, 2024

    Published Online: Mar. 13, 2025

    The Author Email: Jijun Feng (fjijun@usst.edu.cn), Jinping He (jphe@niaot.ac.cn)

    DOI:10.3788/COL202523.031301

    CSTR:32184.14.COL202523.031301

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