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20112026
most citedFour-hundred Very Metal-Poor Stars Studied with LAMOST and Subaru. II. Elemental abundances

120 citations · 946 across the 56 of their papers we have counts for

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astro-ph.SR2022★ 30 cited

Hot subdwarf stars identified in LAMOST DR8 with single-lined and composite spectra

Zhenxin Lei, Ruijie He, Peter Nemeth +6

222 hot subdwarf stars were identified with LAMOST DR8 spectra, among which 131 stars show composite spectra and have been decomposed, while 91 stars present single-lined spectra.…

astro-ph.GA2022★ 6 cited

Existence of Tidal Tails for the Globular Cluster NGC 5824

Yong Yang, Jing-Kun Zhao, Miho N. Ishigaki +5

Context. Several dynamically cold streams have been associated with certain globular clusters (GCs) based on orbital energies and angular momenta. Some of these streams are surpris…

astro-ph.GA2022★ 5 cited

A New Cold Stream near the Southern Galactic Pole

Yong Yang, Jing-Kun Zhao, Xiang-Xiang Xue +2

We report the discovery of a cold stream near the southern Galactic pole (dubbed as SGP-S) detected in Early Data Release 3. The stream is at a heliocentric distance of $\si…

astro-ph.GA2022★ 9 cited

Revisit of open clusters UPK 39, UPK 41 and PHOC 39 : a new binary open cluster found

Xianhao Ye, Jingkun Zhao, Terry D. Oswalt +2

We investigate the three open clusters near Aquila Rift cloud, named as UPK 39 (\texttt{c1} hereafter), UPK 41 (\texttt{c2} hereafter) in Sim et al. (2019) and PHOC 39 (\texttt{c3}…

astro-ph.GA2022★ 27 cited

The stellar parameters and elemental abundances from low-resolution spectra I: 1.2 million giants from LAMOST DR8

Zhuohan Li, Gang Zhao, Yuqin Chen +2

As a typical data-driven method, deep learning becomes a natural choice for analysing astronomical data nowadays. In this study, we built a deep convolutional neural network to est…

astro-ph.GA2022★ 22 cited

A spectroscopic study of blue supergiant stars in Local Group spiral galaxies: Andromeda and Triangulum

Cheng Liu, Rolf-Peter Kudritzki, Gang Zhao +4

Low-resolution LAMOST and Keck spectra of blue supergiant stars distributed over the disks of the Local Group spiral galaxies M 31 and M 33 are analyzed to determine stellar effect…

astro-ph.SR2022★ 120 cited

Four-hundred Very Metal-Poor Stars Studied with LAMOST and Subaru. II. Elemental abundances

Haining Li, Wako Aoki, Tadafumi Matsuno +9

We present homogeneous abundance analysis of over 20 elements for 385 very metal-poor (VMP) stars based on the LAMOST survey and follow-up observations with the Subaru Telescope. I…

astro-ph.SR2022★ 29 cited

Four-hundred Very Metal-poor Stars studied with LAMOST and Subaru. I. Survey Design, Follow-up Program, and Binary Frequency

Wako Aoki, Haining Li, Tadafumi Matsuno +11

The chemical abundances of very metal-poor stars provide important constraints on the nucleosynthesis of the first generation of stars and early chemical evolution of the Galaxy. W…

astro-ph.GA2022★ 32 cited

High-precision chemical abundances of Galactic building blocks. II. Revisiting the chemical distinctness of the Helmi streams

Tadafumi Matsuno, Emma Dodd, Helmer H. Koppelman +6

Context: The Helmi streams are a kinematic substructure whose progenitor is likely a dwarf galaxy. Although 20 years have passed since their discovery, it is still unclear whether…