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Characterizing the Instrumental Profile of LAMOST

  • Authors: Qian Liu, 倩 刘, Zhongrui Bai, 仲瑞 白, Ming Zhou, 明 周, Mingkuan Yang, 明宽 杨, Xiaozhen Yang, 肖振 杨, Ziyue Jiang, 子悦 蒋, Hailong Yuan, 海龙 袁, Ganyu Li, 甘雨 李, Yuji He, 玉吉 何, Mengxin Wang, 梦欣 汪, Yiqiao Dong, 义乔 董, Haotong Zhang, 昊彤 张

Qian Liu et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 1.

This figure shows the variation of the lamp line profile parameters for LAMOST Spectrograph No. 1 at a given time (indicated in the title of each panel). From top to bottom, the panels show 2D maps of the FWHM, skewness, and kurtosis of the profiles, with fiber ID on the x-axis and wavelength on the y-axis.

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