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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 2.

Distribution of ﹩\mathrm{log}{R}_{{\rm{HK}}}^{{\prime} }﹩ versus Teff for different [Fe/H] ranges. The color bar indicates the number density. The red solid line represents the results of Equation (11) using the median [Fe/H] value for each metallicity range, while the red dotted line corresponds to the solar metallicity case ([Fe/H] = 0) for comparison.

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