Study on the Classification of LAMOST Early Stellar Spectrum Template by Mahalanobis Distance

CHEN Shu-xin; SUN Wei-min; SONG Yi-han

doi:10.3964/j.issn.1000-0593(2019)05-1618-05

Journals >Spectroscopy and Spectral Analysis >Volume 39 >Issue 5 >Page 1618 > Article

Spectroscopy and Spectral Analysis
Vol. 39, Issue 5, 1618 (2019)

Study on the Classification of LAMOST Early Stellar Spectrum Template by Mahalanobis Distance

CHEN Shu-xin^1、2、*, SUN Wei-min¹, and SONG Yi-han³

Author Affiliations

¹[in Chinese]

²[in Chinese]

³[in Chinese]

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DOI: 10.3964/j.issn.1000-0593(2019)05-1618-05 Cite this Article

CHEN Shu-xin, SUN Wei-min, SONG Yi-han. Study on the Classification of LAMOST Early Stellar Spectrum Template by Mahalanobis Distance[J]. Spectroscopy and Spectral Analysis, 2019, 39(5): 1618 Copy Citation Text

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References

[2] Luo A L, Zhao Y H, Zhao G, et al. RAA, 2015, 15(8): 1095.

[3] Wei P, Luo A L, Li Y B, et al. The Astronomical Journal, 2014, 147（5）: 101.

[4] Bouchy F, Ségransan D, Díaz R F, et al. Astronomy Astrophysics, 2016, 585: A46.

CHEN Shu-xin, SUN Wei-min, SONG Yi-han. Study on the Classification of LAMOST Early Stellar Spectrum Template by Mahalanobis Distance[J]. Spectroscopy and Spectral Analysis, 2019, 39(5): 1618

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