Overview of the LAMOST survey in the first decade

H Yan, H Li, S Wang, W Zong, H Yuan, M Xiang… - The Innovation, 2022 - cell.com
The Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST), also known as
the Guoshoujing Telescope, is a major national scientific facility for astronomical research …

The Pristine survey–I. Mining the Galaxy for the most metal-poor stars

E Starkenburg, N Martin, K Youakim… - Monthly Notices of …, 2017 - academic.oup.com
We present the Pristine survey, a new narrow-band photometric survey focused on the
metallicity-sensitive Ca H&K lines and conducted in the Northern hemisphere with the wide …

ASPCAP: the APOGEE stellar parameter and chemical abundances pipeline

AEG Pérez, CA Prieto, JA Holtzman… - The Astronomical …, 2016 - iopscience.iop.org
ABSTRACT The Apache Point Observatory Galactic Evolution Experiment (APOGEE) has
built the largest moderately high-resolution (R≈ 22,500) spectroscopic map of the stars …

The first data release (DR1) of the LAMOST regular survey

AL Luo, YH Zhao, G Zhao, LC Deng… - … in Astronomy and …, 2015 - iopscience.iop.org
Abstract The Large sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) general
survey is a spectroscopic survey that will eventually cover approximately half of the celestial …

The radial velocity experiment (RAVE): fifth data release

A Kunder, G Kordopatis, M Steinmetz… - The Astronomical …, 2017 - iopscience.iop.org
ABSTRACT Data Release 5 (DR5) of the Radial Velocity Experiment (RAVE) is the fifth data
release from a magnitude-limited ($9\lt I\lt 12$) survey of stars randomly selected in the …

Abundance estimates for 16 elements in 6 million stars from LAMOST DR5 low-resolution spectra

M Xiang, YS Ting, HW Rix, N Sandford… - The Astrophysical …, 2019 - iopscience.iop.org
We present the determination of stellar parameters and individual elemental abundances for
6 million stars from∼ 8 million low-resolution (R∼ 1800) spectra from LAMOST DR5. This is …

3D kinematics and age distribution of the open cluster population

Y Tarricq, C Soubiran, L Casamiquela… - Astronomy & …, 2021 - aanda.org
Context. Open clusters (OCs) trace the evolution of the Galactic disc with great accuracy.
Gaia and large ground-based spectroscopic surveys make it possible to determine their …

The Milky Way's rotation curve out to 100 kpc and its constraint on the Galactic mass distribution

Y Huang, XW Liu, HB Yuan, MS Xiang… - Monthly Notices of …, 2016 - academic.oup.com
The rotation curve (RC) of the Milky Way out to∼ 100 kpc has been constructed using∼ 16
000 primary red clump giants (PRCGs) in the outer disc selected from the LAMOST …

Stellar labels for hot stars from low-resolution spectra-I. The HotPayne method and results for 330 000 stars from LAMOST DR6

M Xiang, HW Rix, YS Ting, RP Kudritzki… - Astronomy & …, 2022 - aanda.org
We set out to determine stellar labels from low-resolution survey spectra of hot stars,
specifically OBA stars with T eff≳ 7500 K. This fills a gap in the scientific analysis of large …

Milky Way mass with K giants and BHB stars using LAMOST, SDSS/SEGUE, and Gaia: 3D spherical Jeans equation and tracer mass estimator

SA Bird, XX Xue, C Liu, C Flynn, J Shen… - Monthly Notices of …, 2022 - academic.oup.com
We measure the enclosed Milky Way mass profile to Galactocentric distances of∼ 70 and∼
50 kpc using the smooth, diffuse stellar halo samples of Bird et al. The samples are Large …