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Disk Truncation Triggers Relativistic Jet Launching of a Highly Accreting Supermassive Black Hole

  • Authors: Hirofumi Noda, Kazuhiro Hada, Hiroto Maruyama, Taishu Kayanoki, Kenji Toma, Taiki Kawamuro, Yoshiyuki Inoue, Tomohisa Kawashima, Soyeon Yeo, Ilje Cho, Keiichi Asada, Yasushi Fukazawa, Yoshihiro Ueda

Hirofumi Noda et al 2026 The Astrophysical Journal Letters 1010 .

  • Provider: AAS Journals

Caption: Figure A1.

(a) XRISM Xtend light curve in the 0.5–10 keV band, showing the temporal evolution of the X-ray flux. (b) Power spectral density (PSD) derived from the light curve, exhibiting a significant peak at approximately 1.2 × 10−5 Hz. The solid blue line represents the best-fit model (red noise plus Poisson noise), and the dashed red line indicates the global 95% confidence level. The detection of the peak above this threshold confirms its statistical significance against the underlying red-noise continuum.

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