Fig. 2.
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Number of galaxies observed in each filter. The most frequently observed filter combination–F090W, F115W, F150W, F200W, F277W, F356W, F410M, and F444W–is shared by 739 galaxies (51% of the sample), meaning these galaxies were observed in all these filters. The orange dots indicate the empirical PSF FWHM in each filter. To reduce overcrowding, we omitted F250M and F300M, which contain only ten galaxies each.
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