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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 11.

Distribution of ﹩\mathrm{log}{R}_{{\rm{HK}}}^{{\prime} }﹩ versus Prot (upper left), ﹩\mathrm{log}{R}_{{\rm{HK}},L}^{+}﹩ versus Prot (upper right), ﹩\mathrm{log}{R}_{{\rm{HK}}}^{{\prime} }﹩ versus Ro (bottom left), and ﹩\mathrm{log}{R}_{{\rm{HK}},L}^{+}﹩ versus Ro (bottom right) for stars observed more than twice. The red dotted line indicates the position of Prot,sat and the red solid line is the fitted segmented function line. The light red interval represents the error interval of the fitting curve.

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