Image Details
Caption: Figure 11.
The left panel shows the difference in magnitude between the 80% detection threshold obtained with DETECT (m80%,DETECT) and the default 5σ upper limit from Rubin (m5σ,Rubin) for all epochs analyzed in this work (see Figures 9 and 10). This sample contains targets that are located on top of bright host galaxies (see Section 5.1). The right panel shows the difference in flux (F80%,DETECT − F5σ,Rubin).
© 2026. The Author(s). Published by the American Astronomical Society.