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ULTIMATE Deblending. I. A 50-band Ultraviolet to Mid-infrared Photometric Catalog Combining Space- and Ground-based Data in the JWST/PRIMER Survey

  • Authors: Hanwen Sun, Tao Wang, Ke Xu, David Elbaz, Emiliano Merlin, Cheng Cheng, Emanuele Daddi, Shuowen Jin, Wei-hao Wang, Longyue Chen, Adriano Fontana, Zhen-Kai Gao, Jiasheng Huang, Benjamin Magnelli, Valentina Sangalli, Yijun Wang, Tiancheng Yang, Yuheng Zhang, Luwenjia Zhou

Hanwen Sun et al 2026 The Astrophysical Journal Supplement Series 285 .

  • Provider: AAS Journals

Caption: Figure 5.

Source number counts and detection completeness. The red line in the upper panel presents the source number count density as a function of F444W magnitude. The blue line shows the number count density from the JADES survey (M. J. Rieke et al. 2023; D. J. Eisenstein et al. 2026), whose 5σ limiting magnitude in F444W is 29.8. The lower panel shows the ratio between the number count density of our work and JADES, which presents the detection completeness of our catalog.

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