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No Strong Geometric Beaming in the Ultraluminous Neutron Star Binary NGC 300 ULX-1 (SN 2010da) from Swift and Gemini

  • Authors: B. Binder, E. M. Levesque, and T. Dorn-Wallenstein

2018 The Astrophysical Journal 863 141.

  • Provider: AAS Journals

Caption: Figure 5.

(a) Timing analysis plots for the Swift/XRT observations. The top panel shows the 0.3–10 keV light curve. The bottom left panel shows the photon arrival time (solid line) vs. the expectation for a constant count rate (dashed line), used to calculate the K-S probability of non-variability. (b) The bottom right panel shows the 3–200 mHz periodogram, used to calculate Fvar (see the text for details).

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