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Predicting the Detection Yields of Giant Planets and Brown Dwarfs with CSST Astrometry

  • Authors: Yifan Xuan, 一帆 宣, Fabo Feng, 发波 冯, Zhensen Fu, 震森 傅, Shilong Liao, 石龙 廖, Zhaoxiang Qi, 朝祥 齐, Yang Chen, 洋 陈

Yifan Xuan et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 4.

CSST filter transmission curves corresponding to near-ultraviolet, u, g, r, i, z, and y bands. The limiting magnitude of the wide field survey for each band is 25.4, 25.4, 26.3, 26.0, 25.9, 25.2, 24.4 mag, shown under corresponding curves. This figure is adapted from Figure 1 in J. Lu et al. (2024).

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