The Automatic Recognition and Detection of Sky-Subtraction Residual Componentin the Stellar Spectra

AN Ran; PAN Jing-chang; YI Zhen-ping; WEI Peng

doi:10.3964/j.issn.1000-0593(2017)01-0273-05

Journals >Spectroscopy and Spectral Analysis >Volume 37 >Issue 1 >Page 273 > Article

Spectroscopy and Spectral Analysis
Vol. 37, Issue 1, 273 (2017)

The Automatic Recognition and Detection of Sky-Subtraction Residual Componentin the Stellar Spectra

AN Ran¹, PAN Jing-chang¹, YI Zhen-ping¹, and WEI Peng²

Author Affiliations

¹[in Chinese]

²[in Chinese]

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DOI: 10.3964/j.issn.1000-0593(2017)01-0273-05 Cite this Article

AN Ran, PAN Jing-chang, YI Zhen-ping, WEI Peng. The Automatic Recognition and Detection of Sky-Subtraction Residual Componentin the Stellar Spectra[J]. Spectroscopy and Spectral Analysis, 2017, 37(1): 273 Copy Citation Text

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References

[1] Gui X Q, Zhao Y H, Chu Y Q, et al. Research in Astronomy and Astrophysics, 2012, 12(9): 1197.

[2] Luo A L, Zhang Y X, Zhao Y H. Astronomical Telescopes and Instrumentation, International Society for Optics and Photonics, 2004, 756.

[3] Luo A L, Zhang H T, Zhao Y H, et al. Research in Astronomy and Astrophysics, 2012, 12(9): 1243.

[6] York D, Adelman J, Anderson J, et al. The Sloan Digital Sky Survey: Technical Summary, AJ, 120, 2000, 1579.

[7] Gunn J, Siegmund W, Mannery E, et al. The 2.5 m Telescope of the Sloan Digital Sky Survey, AJ, 131, 2006. 2332.

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