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Reflection Spectra of the Black Hole Binary Candidate MAXI J1535-571 in the Hard State Observed by NuSTAR

  • Authors: Yanjun Xu, Fiona A. Harrison, Javier A. García, Andrew C. Fabian, Felix Fürst, Poshak Gandhi, Brian W. Grefenstette, Kristin K. Madsen, Jon M. Miller, Michael L. Parker, John A. Tomsick, and Dominic J. Walton

2018 The Astrophysical Journal Letters 852 L34.

  • Provider: AAS Journals

Caption: Figure 1.

(a) MAXI/GSC (black) and Swift/BAT (red) orbital light curves of MAXI J1535-571, scaled to the Crab count rates in the corresponding instrument bands (only BAT data points with S/N > 7 are included). The gray shaded area marks the duration of the NuSTAR observation. (b) MAXI hardness ratio calculated from count rates (4–20/2–4 keV). (c) NuSTAR hardness ratio in 100 s bins (count rates, 6–10/3–6 keV).

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