A Method to Fit Low-Quality Stellar Spectrum

WU Ming-lei; PAN Jing-chang; YI Zhen-ping; WEI Peng

doi:10.3964/j.issn.1000-0593(2018)03-0963-05

Journals >Spectroscopy and Spectral Analysis >Volume 38 >Issue 3 >Page 963 > Article

Spectroscopy and Spectral Analysis
Vol. 38, Issue 3, 963 (2018)

A Method to Fit Low-Quality Stellar Spectrum

WU Ming-lei^1、2、*, PAN Jing-chang¹, YI Zhen-ping¹, and WEI Peng³

Author Affiliations

¹[in Chinese]

²[in Chinese]

³[in Chinese]

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DOI: 10.3964/j.issn.1000-0593(2018)03-0963-05 Cite this Article

WU Ming-lei, PAN Jing-chang, YI Zhen-ping, WEI Peng. A Method to Fit Low-Quality Stellar Spectrum[J]. Spectroscopy and Spectral Analysis, 2018, 38(3): 963 Copy Citation Text

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References

[2] Cui X Q, Zhao Y H, Chu Y Q, et al. RAA, 2012, 12(9): 1197.

[7] Marziani M, Gambaccini M, Di Domenico G, et al. Applied Radiation and Isotopes, 2014, 92(6): 32.

[9] Sahoo G S, Tripathy S P, Molokanov A G, et al. Nuclear Instruments and Methods in Physics Research A, 2016, 38(2): 14.

WU Ming-lei, PAN Jing-chang, YI Zhen-ping, WEI Peng. A Method to Fit Low-Quality Stellar Spectrum[J]. Spectroscopy and Spectral Analysis, 2018, 38(3): 963

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