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Optical–Near-infrared Multiband Photometric Analysis and Characterization of Giant Exoplanets with CPI-C

  • Authors: Yiming Zhu, Gang Zhao, Xi Zhang, Gang Wang, Bingli Niu, Zhonghua Lv, Jiangpei Dou

Yiming Zhu et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 13.

A posterior comparison for the synthetic warm giant. The upper panels show Gaussian kernel-density estimates of the joint posterior distributions in the TeffRp, Teff–﹩\mathrm{log}g﹩, and Rp–﹩\mathrm{log}g﹩ planes. The contours enclose 68% and 95% of the posterior probability. The lower panels show the corresponding one-dimensional marginal distributions of Teff, ﹩\mathrm{log}g﹩, and Rp. Gray, orange, and blue denote the H/K/L-only, CPI-C NIR4-only, and combined fits, respectively. Colored vertical lines mark the posterior medians, and the shaded regions indicate the central 68% credible intervals. The black stars and vertical dashed lines mark the input-model parameters.

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