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A Systematic Analysis of the X-Ray Emission in Optically Selected Tidal Disruption Events: Observational Evidence for the Unification of the Optically and X-Ray-selected Populations

  • Authors: Muryel Guolo, Suvi Gezari, Yuhan Yao, Sjoert van Velzen, Erica Hammerstein, S. Bradley Cenko, Yarone M. Tokayer

Muryel Guolo et al 2024 The Astrophysical Journal 966 .

  • Provider: AAS Journals

Caption: Figure 4.

Comparison between X-ray spectral properties of TDEs (green) and AGN (type I in red and type II in gold) from BASS (Ricci et al. 2017). In the left panels, we compare the Swift/XRT or XMM-Newton HR (see text for definition); in the right panels, we compare the Γ power-law index when TDEs are fitted with an absorbed power-law model. The top panels show the cumulative distribution of the parameters, while the bottom panels show the distribution of samples in the L X vs. HR and L X vs. Γ parameter space. For AGNs, the contours represent 68% and 90% of the sample distribution; for TDEs, each point is an XMM-Newton or Swift/XRT stacked spectrum.

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