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Items: 1 to 20 of 99

1.

[A new automated method to identify emission line star from massive spectra].

Pan JC, Zhang CM, Wei P, Luo AL, Zhao YH.

Guang Pu Xue Yu Guang Pu Fen Xi. 2012 Jun;32(6):1689-93. Chinese.

PMID:
22870668
2.

[A method for auto-recognizing the stars based on spectral feature].

Liu ZT, Qiu KM.

Guang Pu Xue Yu Guang Pu Fen Xi. 2010 Jan;30(1):274-7. Chinese.

PMID:
20302131
3.

[Searching for Rare Celestial Objects Automatically from Stellar Spectra of the Sloan Digital Sky Survey Data Release Eight].

Si JM, Luo AL, Wu FZ, Wu YH.

Guang Pu Xue Yu Guang Pu Fen Xi. 2015 Mar;35(3):834-40. Chinese.

PMID:
26117907
4.

[A method for automatic recognition of stellar spectra based on feature matching of spectral lines].

Liu ZT, Qiu KM, Zhao RZ.

Guang Pu Xue Yu Guang Pu Fen Xi. 2008 Jun;28(6):1435-8. Chinese.

PMID:
18800743
5.

[The radial velocity measurement accuracy of different spectral type low resolution stellar spectra at different signal-to-noise ratio].

Wang FF, Luo AL, Zhao YH.

Guang Pu Xue Yu Guang Pu Fen Xi. 2014 Feb;34(2):565-8. Chinese.

PMID:
24822441
6.

Exploring the SDSS Dataset with Linked Scatter Plots: I. EMP, CEMP, and CV Stars.

Carbon DF, Henze C, Nelson BC.

Astrophys J Suppl Ser. 2017 Feb;228(2). pii: 19. doi: 10.3847/1538-4365/228/2/19. Epub 2017 Feb 9.

PMID:
28684884
7.

[An automated method to fit stellar continuum based on statistic windows].

Pan JC, Wang XX, Wei P, Jiang B, Tu LP, Luo AL.

Guang Pu Xue Yu Guang Pu Fen Xi. 2012 Aug;32(8):2260-3. Chinese.

PMID:
23156794
8.

[Atmospheric parameter estimation for LAMOST/GUOSHOUJING spectra].

Lu Y, Li XR, Yang T.

Guang Pu Xue Yu Guang Pu Fen Xi. 2014 Nov;34(11):3127-31. Chinese.

PMID:
25752072
9.

[Searching QSO candidates and calculating their redshfit from a flood of spectra].

Song YH, Luo AL, Zhao YH.

Guang Pu Xue Yu Guang Pu Fen Xi. 2011 Sep;31(9):2578-81. Chinese.

PMID:
22097876
10.

[Stellar spectral outliers detection based on Isomap].

Bu YD, Pan JC, Chen FQ.

Guang Pu Xue Yu Guang Pu Fen Xi. 2014 Jan;34(1):267-73. Chinese.

PMID:
24783574
11.

[An automated stellar spectra classification system based on non-parameter regression and nearest neighbor method].

Zhang JN, Zhao YH, Liu R.

Guang Pu Xue Yu Guang Pu Fen Xi. 2009 Dec;29(12):3424-8. Chinese.

PMID:
20210186
12.

[Efficient computation of spectral flux normalization].

Li XR.

Guang Pu Xue Yu Guang Pu Fen Xi. 2012 Jan;32(1):179-82. Chinese.

PMID:
22497154
13.

[An automated measurement of the galaxies spectra of LAMOST].

Zhu GH, Luo AL, Zhao YH.

Guang Pu Xue Yu Guang Pu Fen Xi. 2005 Jun;25(6):1002-5. Chinese.

PMID:
16201393
14.

[Galaxy/quasar classification based on nearest neighbor method].

Li XR, Lu Y, Zhou JM, Wang YJ.

Guang Pu Xue Yu Guang Pu Fen Xi. 2011 Sep;31(9):2582-5. Chinese.

PMID:
22097877
15.

[Comparison of different template matching methods of automatic stellar spectrum parameter measurement].

Liu J, Pan JC, Liu M, Wei P, Luo AL.

Guang Pu Xue Yu Guang Pu Fen Xi. 2013 Feb;33(2):558-61. Chinese.

PMID:
23697154
16.

[Data mining for cataclysmic variables candidates in SDSS-DR8].

Jiang B, Pan JC, Wang W.

Guang Pu Xue Yu Guang Pu Fen Xi. 2013 Feb;33(2):464-7. Chinese.

PMID:
23697133
17.

[A method for obtaining redshifts of quasars based on wavelet multi-scaling feature matching].

Liu ZT, Li XR, Wu FC, Zhao YH.

Guang Pu Xue Yu Guang Pu Fen Xi. 2006 Sep;26(9):1738-41. Chinese.

PMID:
17112059
18.

[The backgroud sky subtraction around [OIII] line in LAMOST QSO spectra].

Shi ZX, Comte G, Luo AL, Tu LP, Zhao YH, Wu FC.

Guang Pu Xue Yu Guang Pu Fen Xi. 2014 Nov;34(11):3132-5. Chinese.

PMID:
25752073
19.

[Searching for WDMS Candidates In SDSS-DR10 With Automatic Method].

Jiang B, Wang CY, Wang WY, Wang W.

Guang Pu Xue Yu Guang Pu Fen Xi. 2015 May;35(5):1428-31. Chinese.

PMID:
26415473
20.

[Wavelet transform zero-crossing method for auto-extraction of spectral lines].

Zhao RZ, Hu ZY, Zhao YH.

Guang Pu Xue Yu Guang Pu Fen Xi. 2005 Jan;25(1):153-6. Chinese.

PMID:
15852843

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