Image Details
Caption: Figure 2.
The 3σ depth and wavelength range of the multiband data used by PRIMER-COSMOS (upper panel) and PRIMER-UDS (lower panel). All depths of point sources are measured using empty circular apertures and have been corrected to consider aperture losses. We use the apertures with the highest sensitivity (among 0﹩\mathop{.}\limits^{^{\prime\prime} }﹩2, 0﹩\mathop{.}\limits^{^{\prime\prime} }﹩5, and Kron apertures) for the JWST and HST data, and apertures with d = 3.5 × FWHMPSF for the other low-resolution data.
© 2026. The Author(s). Published by the American Astronomical Society.