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20072023
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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19 papers · 1 filter

astro-ph.GA2023

Ionized gas metallicity of the strong [OIII]λ emission-line compact galaxies in the LAMOST survey

Siqi Liu, A-Li Luo, Wei Zhang +2

This article reports a sample of 1830 strong [O III] λ5007 emission-line compact galaxies discovered with the LAMOST spectroscopic survey and the photometric catalog of SDSS. We ne…

astro-ph.GA202219 cited

PhotoRedshift-MML: a multimodal machine learning method for estimating photometric redshifts of quasars

Shuxin Hong, Zhiqiang Zou, A-Li Luo +3

We propose a Multimodal Machine Learning method for estimating the Photometric Redshifts of quasars (PhotoRedshift-MML for short), which has long been the subject of many investiga…

astro-ph.GA202226 cited

Strong [OIII]λ5007 emission line compact galaxies in LAMOST DR9: Blueberries, Green Peas and Purple Grapes

Siqi Liu, A-Li Luo, Huan Yang +8

Green Pea and Blueberry galaxies are well-known for their compact size, low mass, strong emission lines and analogs to high-z Lyα emitting galaxies. In this study, 1547 strong [OII…

astro-ph.GA2021

High-α-Metal-Rich stars in the LAMOST-MRS survey and its connection with the galactic bulge

Haopeng Zhang, Yuqin Chen, Gang Zhao +6

We report the detection of a large sample of high--metal-rich stars on the low giant branch with dex in the LAMOST-MRS survey. This special group corresponds to a…

astro-ph.GA2020

Central velocity dispersion catalog of LAMOST-DR7 galaxies

Nicola R. Napolitano, Giuseppe D'Ago, Crescenzo Tortora +6

The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) is a major facility to carry out spectroscopic surveys for cosmology and galaxy evolution studies. The sevent…

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…