[1] Xiangqun CUI, Yongheng ZHAO, Yaoquan CHU et al. The large sky area multi-object fiber spectroscopic telescope(LAMOST). Research in Astron Astrophys, 12, 1197-1242(2012).

[2] Gang ZHAO, Yongheng ZHAO. LAMOST spectral survey-an overview. Research in Astronomy and Astrophysics, 12, 723-734(2012).

[3] Z T IVEZIC, W N AXELROD, W N BRANDT et al. Large synoptic survey telescope: from science drivers to reference design. Serbian Astronomical Journal, 176, 1-13(2008).

[4] B ABARESHI, J AGUILAR, S AHLEN et al. Overview of the instrumentation for the dark energy spectroscopic instrument. The Astronomical Journal, 164, 207-269(2022).

[6] E TOLSTOY, V HILL, M TOSI. Star-formation histories, abundances and kinematics of dwarf galaxies in the local group. Annual Review of Astronomy and Astrophysics, 47, 371-425(2009).

[7] A B SARAH, Xiangxiang XUE, Haijun TIAN et al. Constraints on the assembly history of the Milky Way's smooth, diffuse stellar halo from the metallicity-dependent, radially dominated velocity anisotropy profiles probed with K giants and BHB stars using LAMOST, SDSS/SEGUE, and Gaia. The Astrophysical Journal, 919, 66-93(2021).

[8] Jiwei XIE, Subo DONG, Yong ZHANG et al. Exoplanet orbital eccentricities derived from LAMOST-Kepler analysis. Proceedings of the National Academy of Sciences of the United States of America, 113, 11431-11435(2016).

[9] Subo DONG, Jiwei XIE, A LUO et al. LAMOST telescope reveals that Neptunian cousins of hot Jupiters are mostly single off spring of stars that are rich in heavy elements. Proceedings of the National Academy of Sciences of the United States of America, 115, 266-271(2018).

[10] Weimin GU, Huijun MU, Jifeng LIU et al. A method to search for black hole candidates with giant companions by LAMOST. The Astrophysical Journal Letters, 872, 20-26(2019).

[11] Tuan YI, Mouyuan SUN, Weimin GU. Mining for candidates of Galactic stellar-mass black hole binaries with LAMOST. The Astrophysical Journal, 886, 97-105(2019).

[12] Hongliang YAN, Haining LI, Yongheng ZHAO et al. Overview of the LAMOST survey in the first decade. The Innovation, 3, 100-224(2022).

[13] I S MCLEAN, C C STEIDEL, H W EPPS et al. MOSFIRE, the multi-object spectrometer for infra-red exploration at the keck observatory(2012).

[14] N SUZUKI, D TYTLER. Relative flux calibration of keck HIRES echelle spectra. Publications of the Astronomical Society of the Pacific, 115, 1050-1067(2003).

[15] T ICHIKAWA, R SUZUKI, T NISHIMURA et al. MOIRCS: multi-object infrared camera and spectrograph for SUBARU(2006).

[17] R S D JONG, S C BARDEN, O BELLIDO-TIRADO et al. 4MOST: the 4-metre multi-object spectroscopic telescope project at preliminary design review(2016).

[18] J J SALAZAR-GONZÁLEZ. Designing optimal masks for a multi-object spectrometer. Omega, 103, 1-13(2021).

[19] Feifan ZHANG, Jianping WANG, Jiaru CHU. Fiber assignment for multi-object fiber-fed spectrographs(2020).

[20] A SZENTGYORGYI, G FURESZ. Hectochelle: a multi object optical echelle spectrograph for the MMT. Publications of the a Stronomical Society of the Pacific, 123, 1188-1209(2011).

[21] S SMEDLEY, G BAKER. Sphinx: a massively multiplexed fiber positioner for MSE(2018).

[22] C BELLANGER, A BRIGNON. Design of a fiber-collimated array for beam combining. Optical Engineering, 50, 025005(2011).

[23] Xue TONG, Dong LIN, Jinping HE. Research status and application prospects of astrophotonics. Acta Astronomica Sinica, 63, 1-22(2022).