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The Stellar Abundances and Galactic Evolution Survey (SAGES). V. The First Data Release of the DDO51 Band

  • Authors: Qiqian Zhang, Zhou Fan, Gang Zhao, Kai Xiao, Wei Wang, Hongrui Gu, Jie Zheng, Jingkun Zhao, Chun Li, Yuqin Chen, Haibo Yuan, Haining Li, Kefeng Tan, Yihan Song, Ali Luo, Nan Song, Yujuan Liu, Yaqian Wu, Ali Esamdin, Hubiao Niu, Jinzhong Liu, Guojie Feng, Yu Zhang

Qiqian Zhang et al 2026 The Astrophysical Journal Supplement Series 284 .

  • Provider: AAS Journals

Caption: Figure 10.

DDO51 photometric depth and precision of the merged catalog. (a) Histogram of DDO51 magnitudes for all sources and “clean” subsample in the final catalog, showing the number of objects per 0.1 mag bin. (b) Photometric uncertainty (σ) as a function of DDO51 magnitude for individual sources. The background is a two-dimensional histogram color coded by the logarithmic number of sources per bin, while the red curve traces the running median σ. The red circles mark the magnitudes at which the median uncertainty reaches ∼0.01, 0.05, and 0.10 mag. (c) Same as panel (b), but for the “clean” subsample after applying the quality cuts.

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