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Revisiting Ca II Activity Indices in FGK Stars: Systematic Biases in Infrared Triplet Measurements

  • Authors: Xiaozhen Yang, 肖振 杨, Xiaoting Fu, 晓婷 符, Mingjie Jian, 明杰 简, Jingkun Zhao, 景昆 赵, Hailong Yuan, 海龙 袁, Zhongrui Bai, 仲瑞 白, Mengxin Wang, 梦欣 汪, Yiqiao Dong, 义乔 董, Mingkuan Yang, 明宽 杨, Ziyue Jiang, 子悦 蒋, Qian Liu, 倩 刘, Ganyu Li, 甘雨 李, Haotong Zhang, 昊彤 张

Xiaozhen Yang et al 2026 The Astrophysical Journal Supplement Series 287 .

  • Provider: AAS Journals

Caption: Figure 17.

Shown here are the 5th percentile curves of ﹩{R}_{{\rm{HK}}}^{+}﹩ and ﹩{R}_{8542}^{+}﹩ for the LAMOST solar-like sample. The upper two rows show ﹩{R}_{{\rm{HK}}}^{+}﹩, and the lower two rows show ﹩{R}_{8542}^{+}﹩. In each panel, the title lists the radiative transfer code and model atmosphere, while the colors distinguish the combinations of solar abundance scale and line list. Each curve corresponds to a different synthesis configuration. The A1 5th percentile curve is shown as a red solid line and is included in all panels for reference. For visual clarity, the BT-Settl and GSL curves are shifted upward by 0.025 in ﹩{R}_{{\rm{HK}}}^{+}﹩ and by 0.1 in ﹩{R}_{8542}^{+}﹩, respectively.

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