Figure 8 from A NuSTAR OBSERVATION OF THE REFLECTION SPECTRUM OF THE LOW-MASS X-RAY BINARY 4U 1728-34

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A NuSTAR OBSERVATION OF THE REFLECTION SPECTRUM OF THE LOW-MASS X-RAY BINARY 4U 1728-34

Authors: Clio C. Sleator, John A. Tomsick, Ashley L. King, Jon M. Miller, Steven E. Boggs, Matteo Bachetti, Didier Barret, Jérôme Chenevez, Finn E. Christensen, William W. Craig, Charles J. Hailey, Fiona A. Harrison, Farid Rahoui, Daniel K. Stern, Dominic J. Walton, and William W. Zhang

2016 The Astrophysical Journal 827 134.

Provider: AAS Journals

Caption: Figure 8.

Change in χ² vs. the change in inner radius, showing that the model is consistent with the disk extending to the ISCO. The dashed blue line marks 90% confidence and the dashed red line marks 99.7% confidence (3σ). (a) Results of the reflionx model (model 1). (b) Results of the relxill model (model 5).

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