Acta Photonica Sinica, Volume. 52, Issue 5, 0552206(2023)

Optical Design of a High-efficiency Medium-low Dispersion Spectrograph with Wide-band Based on FOSC Type(Invited)

Hangxin JI1,2、*, Guoxin BA1,2,3, Jun LI1,2, and Haoran YU1,2
Author Affiliations
  • 1National Astronomical Observatories/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, Nanjing 210042, China
  • 3University of Chinese Academy of Sciences, Beijing 100049, China
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    Figures & Tables(12)
    The working principle of the double channel spectrograph based on FOSC type
    The working principle of two straight-through GRISMS
    The optical layout of the double channel multi-mode spectrograph
    The spot diameter of different wavelength at 4 spectral modes in the blue channel
    The spot diameter of different wavelength at 4 spectral modes in the red channel
    Different straight- through grisms,the relationship between spectral resolution and wavelength(left),the relationship between the spectrum position on the CCD in dispersion direction and wavelength(right)
    The spectrograph efficiency curve with different straight-through grisms(GRISM or VPHG)
    The camera design comparison for the red channel of multi-mode astronomical spectrometer
    The spot diameter of different wavelength at 4 spectral modes in the red channel with curved detector
    • Table 1. The main requirements of the double channel medium-low dispersion spectrograph

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      Table 1. The main requirements of the double channel medium-low dispersion spectrograph

      Technical indexIndex requirements
      Working band

      Blue channel:310~560 nm

      Red channel:540~1 000 nm

      Spectral resolutionR=500,2 000,5 500@0.8″slit
      Operating temperature-30 ℃~20 ℃
      Peak efficiency(without slit loss)≥40%
      Minimum efficiency≥15%(goal)
      Image qualityRMS radius ≤ 10 μm
    • Table 2. The initial configuration parameters of the spectrograph

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      Table 2. The initial configuration parameters of the spectrograph

      Spectrograph parameterValues
      Collimator focal length400 mm
      Pupil diameter50 mm
      Camera focal length215 mm
      Camera focal ratio & field of viewF/4.3 & φ≥16°
      CCD4 K@15 μm
      Channel working band

      Blue channel:310~560 nm

      Red channel:540~1 000 nm

    • Table 3. The main parameters of grisms for the blue & red-channel

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      Table 3. The main parameters of grisms for the blue & red-channel

      Resolution modeLine density/(l·mm-1Groove anglePrism angle & materialsOrder
      B-GRISM 5002008.95°10.6° & fused silica1
      B-GRISM 2 00060028.7°33.1° & fused silica1
      B-VPHG 2 00077520°20° & fused silica1
      B-GRISM >5 00097.1156°56° & LF5HTI9~17
      R-GRISM 50015010.8°10.8° & LF5HTI1
      R-GRISM 2 00030026.7°23.5° & LF5HTI1
      R-VPHG 2 00045021°21° & LF5HTI1
      R-GRISM >5 00091.758.9°58.9° & LF5HTI5~10
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    Hangxin JI, Guoxin BA, Jun LI, Haoran YU. Optical Design of a High-efficiency Medium-low Dispersion Spectrograph with Wide-band Based on FOSC Type(Invited)[J]. Acta Photonica Sinica, 2023, 52(5): 0552206

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    Paper Information

    Category: Special Issue for Advanced Science and Technology of Astronomical Optics

    Received: Dec. 27, 2022

    Accepted: Feb. 20, 2023

    Published Online: Jul. 19, 2023

    The Author Email: JI Hangxin (hxji@niaot.ac.cn)

    DOI:10.3788/gzxb20235205.0552206

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