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FATHOMER Survey. III. Preliminary H I Galaxy Identification Results

  • Authors: Shuanghao Shu, Yichao Li, Wenxiu Yang, Jiaxin Wang, Wenkai Hu, Furen Deng, Shifan Zuo, Yougang Wang, Xuelei Chen

Shuanghao Shu et al 2026 The Astrophysical Journal 1001 .

  • Provider: AAS Journals

Caption: Figure 2.

Frequency dependence of the noise level (blue curve, left axis) and the corresponding fraction of RFI-masked pixels (red dashed curve, right axis). The bottom axis shows the observed frequency in MHz, while the top axis indicates the corresponding redshift of the HI line. The secondary y-axis illustrates the fraction of RFI-masked pixels over the same frequency range. The gray curve represents the expected rms increase induced by RFI flagging, which is estimated via Equation (6).

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