Image Details
Caption: Figure 13.
Cumulative and differential completeness of the absolute magnitude, C(H V < ), at the end of 2022 as a result of the KOM for 10 instances of the reference model with the minimum size set to 40 m. The differential completeness is shown as the light gray solid lines, while cumulative completeness is shown as the dark gray solid lines. The cumulative and differential completenesses as a function of absolute magnitude as derived by Harris & Chodas (2021) are shown as the solid and dashed red lines, respectively. The missing completeness in the KOM at H V < 20 mag is due to the KOM not modeling the low solar elongation surveys and NEOWISE.
© 2023. The Author(s). Published by the American Astronomical Society.