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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 10.

The predicted IPs on two dates. From left to right, the IPs correspond to central wavelengths of 4046.57, 4358.34, 4678.15, 4799.91, 5085.82, 5460.75, and 5790.67 Å. Solid lines indicate profiles from an exposure on the left side of the red dashed line in Figure 9, while dashed lines correspond to ones on the right side.

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