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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 3.

Distribution of ﹩\mathrm{log}{R}_{{\rm{HK}}}^{{\prime} }﹩ versus rotation period for different Teff ranges. We mark the position of the Sun with a red ⋆ symbol for comparison. The red dotted line indicates the position of Prot,sat and the red solid line is the fitted segmented function line. The error bars of ﹩\mathrm{log}{R}_{{\rm{HK}}}^{{\prime} }﹩ represent the standard deviations for stars with repeated measurements.

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