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A 0.03 Hz Radio Quasiperiodic Oscillation during the 2025 Flare of GRS 1915+105

  • Authors: Ya Xing Li, 亚星 李, Lei Liu, 磊 刘, Wu Jiang, 悟 江, Zhen Yan, 震 闫, Bo Xia, 博 夏, Zhi Qiang Shen, 志强 沈

Ya Xing Li et al 2026 The Astrophysical Journal 1004 .

  • Provider: AAS Journals

Caption: Figure 3.

The distributions of the maximum TR from each simulated data for the corresponding wave bands. ﹩{T}_{{\rm{R}}}={\rm{\max }}(2{I}_{j}/{S}_{j})﹩ is calculated from each simulated PDS and LS periodogram, where Ij is the power at frequency fj and Sj is the best-fit power-law value at that frequency. The dashed red and green lines indicate ﹩{T}_{{\rm{R}}}^{{\rm{obs}}}﹩ at the fundamental and harmonic frequencies, respectively.

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