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20072022
most citedThe SEGUE Stellar Parameter Pipeline. I. Description and Initial Validation Tests

511 citations · 1k across the 26 of their papers we have counts for

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Showing 2019Show all

8 papers · 1 filter

astro-ph.IM20197 cited

DEEM, a versatile platform of FRD measurement for highly multiplexed fibre systems in astronomy

Yunxiang Yan, Qi Yan, Gang Wang +6

We present a new method of DEEM, the direct energy encircling method, for characterising the performance of fibres in most astronomical spectroscopic applications. It's a versatile…

astro-ph.IM201910 cited

A modified method for determining the FRD and length properties of optical fibres in astronomy

Yunxiang Yan, Gang Wang, Weimin Sun +4

Focal ratio degradation (FRD) is a major contributor to throughput and light loss in a fibre spectroscopic telescope system. We combine the guided mode theory in geometric optics a…

astro-ph.SR20192 cited

Spectroscopically Identified Cataclysmic Variables from LAMOST survey. I. The Sample

Wen Hou, A-Li Luo, Yin-Bi Li +1

A sample of Cataclysmic Variables (CVs) is presented including spectroscopically identified 380 spectra of 245 objects, of which 58 CV candidates are new discoveries. The BaggingTo…

astro-ph.GA2019

Bivariate Luminosity Function of Galaxy Pairs

Shuai Feng, Shi-Yin Shen, Fang-Ting Yuan +8

We measure the bivariate luminosity function (BLF) of galaxy pairs and use it to probe and characterize the galaxy-galaxy interaction between pair members. The galaxy pair sample i…

astro-ph.GA2019

Stellar population analysis on the stacked spectra of double-peaked emission-line galaxies

Meng-Xin Wang, A-Li Luo

The double-peaked emission-line galaxies has long been perceived as objects related with merging galaxies or other phenomena of disturbed dynamical activities, such as outflows and…

astro-ph.SR201932 cited

Metallic-Line Stars Identified from Low Resolution Spectra of LAMOST DR5

Li Qin, A-Li Luo, Wen Hou +6

LAMOST DR5 released more than 200,000 low resolution spectra of early-type stars with S/N>50. Searching for metallic-line (Am) stars in such a large database and study of their sta…