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From DESI to Euclid: A Generative Bridge to Improve Measurements of Galaxy Structure

  • Authors: Renhao Ye, 人豪 叶, Shiyin Shen, 世银 沈

Renhao Ye et al 2026 The Astrophysical Journal Letters 1009 .

  • Provider: AAS Journals

Caption: Figure 4.

Fourier-domain comparison with the held-out Euclid VIS observations over the test set (median; shaded 16th–84th-percentile intervals). (a) Azimuthally averaged power spectrum P versus angular scale for Euclid VIS, E-BGS, and the DESI r and z bands. (b) FRC with the held-out Euclid VIS observations for E-BGS and the DESI bands. The horizontal dashed line marks FRC = 0.5, and the vertical dashed lines mark the corresponding crossing scale q0.5 for each curve. Thin curves show the E-BGS FRC in three bins of DESI r-band PSF FWHM.

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