Image Details
Caption: Figure 12.
Internal photometric precision of SAGES DDO51 derived from 5.26 million pairs of repeated observations. Top: distribution of magnitude differences (Δm) for calibrated stars. The red lines mark the ±1σ envelope, and the blue dashed line shows the median bias. Bottom: single-measurement precision (σint) as a function of magnitude. Dotted lines indicate 1% (10 mmag) and 10% precision levels.
© 2026. The Author(s). Published by the American Astronomical Society.