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Stellar Chromospheric Activity Database of Solar-like Stars Based on the LAMOST Low-resolution Spectroscopic Survey. III. Calibrating the Chromospheric Basal Flux and the Connection to Stellar Rotation

Authors: Weitao Zhang, Han He, Jun Zhang

Weitao Zhang et al 2026 The Astrophysical Journal Supplement Series 283 .

Provider: AAS Journals

Caption: Figure 13.

The distribution of ﹩\mathrm{log}{R}_{{\rm{HK}}}^{{\prime} }﹩ values derived in this work with those reported in previous studies. The black solid line indicates ﹩\mathrm{log}{R}_{{\rm{HK}}}^{{\prime} }﹩= ﹩\mathrm{log}{R}_{{\rm{HK}},{\rm{paper}}}^{{\prime} }﹩, and the dotted line is their fitting line.

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