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An Efficient Shift-and-stack Algorithm Applied to Detection Catalogs

Authors: Steven Stetzler, Mario Jurić, Pedro H. Bernardinelli, Dino Bektešević, Colin Orion Chandler, Andrew J. Connolly, Fred C. Adams, Cesar Fuentes, David W. Gerdes, Matthew J. Holman, Hsing Wen Lin, 省文林, Larissa Markwardt, Andrew McNeill, Michael Mommert, Kevin J. Napier, William J. Oldroyd, Matthew J. Payne, Andrew S. Rivkin, Luis E. Salazar-Manzano, Hilke Schlichting, Scott S. Sheppard, Dallin Spencer, Ryder Strauss, David E. Trilling, Chadwick A. Trujillo

Steven Stetzler et al 2025 The Astronomical Journal 170 .

Provider: AAS Journals

Caption: Figure 6.

The fraction of synthetic objects recovered as a function of their magnitude for the TNO and MBA searches. Dots represent the detection fraction in bins of size 0.5 mag, and error bars represent the asymmetric uncertainty in the estimated fraction using the Wilson score interval. Two reference magnitudes are visualized as black solid and dashed vertical lines. The solid black line visualizes the estimated single-epoch m₅₀ = 23.7. The dashed black line represents the theoretical achievable depth by coadding all of the images, and it is equal to ﹩{m}_{50}^{{\rm{coadd}}}=26.2﹩.

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