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A GeV Gamma-Ray Spectral Excess in the Fermi Blazar 4FGL J0136.5+3906

  • Authors: Shi-Ju Kang, Yue Yin, Yong-Gang Zheng, Qingwen Wu, Junhui Fan

Shi-Ju Kang et al 2026 The Astrophysical Journal Letters 1009 .

  • Provider: AAS Journals

Caption: Figure 1.

Spectral energy distribution (SED) and spectral excess signal of 4FGL J0136.5+3906 in the 100 MeV to 1 TeV range, using 17 yr of data (left panel: 35 bins, right panel: 45 bins). The SED is fitted with a pure log-parabola model (null hypothesis, red dashed line) and with a log-parabola plus Gaussian model (signal hypothesis, blue dotted–dashed line). Blue points denote SED bins with TS > 25; gray downward arrows indicate upper limits. The blue dotted line represents the Gaussian excess component.

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