Chinese Optics Letters, Volume. 13, Issue 11, 111101(2015)

Optical design for Antarctic Bright Star Survey Telescope

Zhengyang Li1,2、*, Haipin Lu1,2, and Xiangyan Yuan1,2
Author Affiliations
  • 1National Astronomical Observatories/Nanjing Institute of Astronomical Optics and Technology, Chinese Academy of Sciences, Nanjing 210042, China
  • 2Key Laboratory of Astronomical Optics & Technology, Nanjing Institute of Astronomical Optics and Technology, Chinese Academy of Sciences, Nanjing 210042, China
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    Figures & Tables(13)
    Schematic drawing of R–C telescope.
    BSST optical layout of open-band configuration. (The filter is located before the insulated window).
    Image spot diagram of BSST (the box is 60 μm).
    Diffraction-encircled energy layout.
    Resulting 80% encircled energy diameters.
    Residual astigmatism and coma field behavior (the arrows on the maps show the amplitude and direction of the aberrations sampling from various fields).
    Astigmatism and coma field behavior of tilting secondary mirror around the CFP.
    Astigmatism and coma field behavior of translating secondary mirror.
    BSST image of 120 s exposure in the R band (1200 pixels×1200 pixels).
    • Table 1. Initial Optical Configuration of BSST

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      Table 1. Initial Optical Configuration of BSST

      Optical ElementRadius (mm)Conic CoefficientDistance (mm)
      Primary Mirror−800−1.33227.1
      Secondary Mirror−639.9−14.16357.1
    • Table 2. Optical Configuration of BSST

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      Table 2. Optical Configuration of BSST

      Optical ElementRadius (mm)Conic CoefficientThickness (mm)Diameter (mm)Glass
      Defrost WindowInfinity20324Fused silica
      Infinity280
      Primary Mirror−800−1.519235315Zerodur
      Secondary Mirror−606−14.443222113Zerodur
      Lens 13581590Fused silica
      −159.910
      Lens 2−159.9884TF3
      −239.6613
      Lens 3−123.59880Fused silica
      Infinity40
      Insulated WindowInfinity890Fused silica
      Infinity18.5
      CCD WindowInfinity9.590Fused silica
      Infinity8
      Focal PlaneInfinity70
    • Table 3. Parameters of Filters

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      Table 3. Parameters of Filters

      FilterCentral Wavelength (nm)Bandwidth (nm)Transmission (%)Diameter (mm)
      B440100>5050
      V55090>7050
      R760250>7050
      Hα656.310>5025
      Hβ486.110>4025
      O–3500.710>6025
    • Table 4. Tolerance Values of BSST

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      Table 4. Tolerance Values of BSST

      Manufactory Error Budget
      ItemsThickness (mm)Radius (mm)ConicNominal
      Primary±1mm±0.0001(−800; −1.519)
      Secondary±1mm±0.0001(−606; −14.443)
      Lens−0.10(15, 8, 8)
      Alignment Error Budget
      DOFDecenter (mm)TiltPosition (mm)
      PrimaryDATUM
      Secondary±0.06±1±0.4
      Corrector±0.1±3.6±0.4
      Lens Space±0.1
      Use Focal Length as Compensator
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    Zhengyang Li, Haipin Lu, Xiangyan Yuan, "Optical design for Antarctic Bright Star Survey Telescope," Chin. Opt. Lett. 13, 111101 (2015)

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    Paper Information

    Category: Atomic and Molecular Physics

    Received: Jun. 24, 2015

    Accepted: Sep. 18, 2015

    Published Online: Sep. 13, 2018

    The Author Email: Zhengyang Li (zyli@niaot.ac.cn)

    DOI:10.3788/COL201513.111101

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