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Empirical H- and K-band Limb Darkening for 31 CHARA Stars: A Near-infrared Benchmark for Stellar-Atmosphere Models

  • Authors: Narsireddy Anugu, John D. Monnier, Antoine Mérand, Becky Flores, Alexandre Gallenne, Douglas R. Gies, Mayra Gutierrez, Robert Klement, Stefan Kraus, Jayadev Rajagopal, Rachael M. Roettenbacher, Gail H. Schaefer

Narsireddy Anugu et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 3.

Comparison of H- and K-band power-law coefficients from CHARA data and atmosphere-model predictions. The filled colored points show the empirical CHARA coefficients, (αHαK), measured by fitting the CHARA V2 data and color-coded by Teff. The gray sequences show the corresponding model-grid predictions. Left: direct intensity-domain model coefficients, ﹩({\alpha }_{I,H}^{g},{\alpha }_{I,K}^{g})﹩, obtained by fitting the analytic law to the passband-integrated model intensity profiles Ib(μ) (Section 4.3). Right: SVAM coefficients, ﹩({\alpha }_{{\rm{SV\; AM}},H}^{g},{\alpha }_{{\rm{SV\; AM}},K}^{g})﹩, recovered by fitting the same law to synthetic CHARA-sampled visibilities generated from each model CLV (Section 4.4). The dashed line marks equality between the H- and K-band coefficients. The systematic separation between the colored CHARA and the gray model points shows the model–data discrepancy discussed in the text.

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