Acta Optica Sinica, Volume. 42, Issue 1, 0112002(2022)
Improvement of Wavelength Calibration Accuracy of Astronomical High-Resolution Spectrometers with Fabry-Perot Etalons
Fig. 5. Optical path compensation function fitting, which is derived from the measured 2D spectra of FPE and ThAr shown in
Fig. 6. Residuals between the wavelength of spectral lines and the wavelength calculated by wavelength solutions, which are derived from the measured 2D spectra of FPE and ThAr shown in
Fig. 7. Residuals between the locked wavelength of LFC spectral lines and the wavelength calculated by wavelength solutions, which are derived from the measured 2D spectra of FPE and ThAr shown in
Fig. 8. Optical path compensation functions for different (m0,d0) degenerate solutions
Fig. 9. FPE wavelength solution for S-2 minus that for S0 and FPE wavelength solution for S+2 minus that for S0
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Zhibo Hao, Huiqi Ye, Liang Tang, Jun Hao, Jian Han, Yang Zhai, Dong Xiao. Improvement of Wavelength Calibration Accuracy of Astronomical High-Resolution Spectrometers with Fabry-Perot Etalons[J]. Acta Optica Sinica, 2022, 42(1): 0112002
Category: Instrumentation, Measurement and Metrology
Received: Jun. 21, 2021
Accepted: Jul. 19, 2021
Published Online: Jan. 17, 2022
The Author Email: Ye Huiqi (hqye@niaot.ac.cn)