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Evidence for a Delayed Ultraviolet Counterpart to X-Ray Quasiperiodic Eruptions in Ansky

  • Authors: Hengxiao Guo, Zhen Yan, Ya-Ping Li, Joheen Chakraborty, Paula Sánchez-Sáez, Lorena Hernández-García, Wenda Zhang, Jingbo Sun, Shuang-Liang Li, Hongping Deng, Wenwen Zuo, Hiromichi Tagawa, Xin Pan, Minghao Zhang, Patricia Arévalo, Paulina Lira, Chichuan Jin, Minfeng Gu

Hengxiao Guo et al 2026 The Astrophysical Journal Letters 1000 .

  • Provider: AAS Journals

Caption: Figure 2.

Correlation between the soft X-ray (0.3–2 keV) and UV light curves of Ansky. Left panels: the X-ray light curves are obtained from Swift XRT and XMM-Newton EPIC-pn, while the UVW2 light curves are from Swift UVOT and XMM-Newton OM. The XMM-Newton data are binned to 0.2 days to match the Swift cadence (original data shown in Figure A1). The original Swift UV data and the 0.2 day binned XMM-Newton data are used for lag measurements (light gray); both are additionally binned to 1 day for clarity. Right panels: cross-correlation results show the centroid lag (top), peak-lag distribution (bottom), and the corresponding CCF and lag posterior distributions. The maximum correlation coefficient is ﹩{r}_{{\rm{\max }}}=0.56\pm 0.04﹩.

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