Figure 7.
Trend with redshift of automated vote fractions for ‘Smooth or Featured’. Featured likelihood drops significantly from z = 0 for all galaxy subsets. Split by radius, the largest galaxies (≈9 kpc) have a similar likelihood of featured votes to typical (≈5 kpc) galaxies but have a slower drop in featured likelihood as redshift increases. Markers indicate vote fractions in 20 equal-count photo-z bins. Statistical errors are negligible throughout.

Trend with redshift of automated vote fractions for ‘Smooth or Featured’. Featured likelihood drops significantly from z = 0 for all galaxy subsets. Split by radius, the largest galaxies (≈9 kpc) have a similar likelihood of featured votes to typical (≈5 kpc) galaxies but have a slower drop in featured likelihood as redshift increases. Markers indicate vote fractions in 20 equal-count photo-z bins. Statistical errors are negligible throughout.

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