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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 2.

PSG-based albedo spectra adopting an HST Jupiter template as a baseline, illustrating the impact of controlled perturbations in key atmospheric parameters. The examples shown include (1) a standard Jupiter-like atmosphere, (2) methane abundance increased by a factor of 5, (3) ammonia abundance increased by a factor of 5, (4) water-vapor abundance increased by a factor of 5, (5) carbon-monoxide abundance increased by a factor of 5, and (6) water-cloud abundance increased by a factor of 100. Within this setup, methane produces the strongest modulation of the reflectance at longer optical wavelengths and motivates methane-sensitive band placement in our optical diagnostics.

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