activity
20132026
most citedLAMOST Spectroscopic Survey of the Galactic Anti-centre (LSS-GAC): target selection and the first release of value-added catalogues

141 citations · 272 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.SR2026

Searching for Magnetic White Dwarfs in LAMOST DR10

Si-Cheng Yu, Juan-Juan Ren, Vitaly V. Neustroev +7

Magnetic white dwarfs (MWDs) are key to understanding the origin and evolution of magnetic fields in compact stars. While large spectroscopic surveys such as SDSS have greatly expa…

astro-ph.IM2024★ 4 cited

All-sky Guide Star Catalog for CSST

Hui-Mei Feng, Zi-Huang Cao, Man I Lam +17

The China Space Station Telescope (CSST) is a two-meter space telescope with multiple back-end instruments. The Fine Guidance Sensor (FGS) is an essential subsystem of the CSST Pre…

astro-ph.HE2020★ 14 cited

Insight-HXMT observations of Swift J0243.6+6124: the evolution of RMS pulse fractions at super-Eddington luminosity

P. J. Wang, L. D. Kong, S. Zhang +116

Based on Insight-HXMT data, we report on the pulse fraction evolution during the 2017-2018 outburst of the newly discovered first Galactic ultraluminous X-ray source (ULX) Swift J0…

astro-ph.SR2018★ 14 cited

New Oe stars in LAMOST DR5

Guang-Wei Li, Jian-Rong Shi, Brian Yanny +7

Stars of spectral type Oe are very rare. To date, only 13 Oe stars have been identified within our Galaxy. In this paper, we present six new Oe stars and four new B0e stars found i…

astro-ph.IM2017★ 10 cited

Cosmic Ray Removal in Fiber Spectroscopic Image

Zhongrui Bai, Haotong Zhang, Hailong Yuan +4

Single-exposure spectra in large spectral surveys are valuable for time domain studies such as stellar variability, but there is no available method to eliminate cosmic rays for si…

astro-ph.IM2017★ 25 cited

Sky Subtraction for LAMOST

Zhong-Rui Bai, Hao-Tong Zhang, Hai-Long Yuan +7

Sky subtraction is the key technique in data reduction of multi-fiber spectra. Knowledge of the related instrument character is necessary to determine the method adopted in sky sub…

astro-ph.GA2017★ 5 cited

Candidate members of the Pal 5, GD-1, Cetus Polar, and Orphan tidal stellar halo streams from Sdss DR9, Lamost DR3 and APOGEE catalogues

Guang-Wei Li, Brian Yanny, Hao-Tong Zhang +8

We present candidate members of the Pal 5, GD-1, Cetus Polar, and Orphan tidal stellar streams found in LAMOST DR3, SDSS DR9 and APOGEE catalogs. In LAMOST DR3, we find 20, 4, 24 h…

astro-ph.SR2014★ 141 cited

LAMOST Spectroscopic Survey of the Galactic Anti-centre (LSS-GAC): target selection and the first release of value-added catalogues

Haibo Yuan, Xiaowei Liu, Zhiying Huo +16

As a major component of the LAMOST Galactic surveys, the LAMOST Spectroscopic Survey of the Galactic Anti-centre (LSS-GAC) aims to survey a significant volume of the Galactic thin/…

astro-ph.IM2014★ 24 cited

ASERA: A Spectrum Eye Recognition Assistant for Quasar Spectra

Hailong Yuan, Haotong Zhang, Yanxia Zhang +3

Spectral type recognition is an important and fundamental step of large sky survey projects in the data reduction for further scientific research, like parameter measurement and st…

astro-ph.HE2013★ 10 cited

The properties of cross-correlation and spectra of the low-mass X-ray binary 4U 1608-52

Ya-Juan Lei, Shu Zhang, Jin-Lu Qu +4

With {\it RXTE} data, we analyzed the cross-correlation function between the soft and hard X-rays of the transient atoll source 4U 1608-52. We found anti-correlations in three outb…

astro-ph.IM2013★ 10 cited

Moon night sky brightness simulation for Xinglong station

Song Yao, Hao-Tong Zhang, Hai-Long Yuan +5

With a sky brightness monitor in Xinglong station of National Astronomical Observatories of China (NAOC), we collected data from 22 dark clear nights and 90 lunar nights. We first…

astro-ph.HE2013★ 15 cited

Evolution of cross-correlation and time lag of 4U 1735-44 along the branches

Ya-Juan Lei, Hao-Tong Zhang, Cheng-Min Zhang +7

We analyze the cross-correlation function between the soft and hard X-rays of atoll source 4U 1735-44 with RXTE data, and find the anti-correlated soft and hard time lags of about…