Figure 4 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 4.

4.5–78.4 keV NuSTAR FPMA (black) and NuSTAR FPMB (red) spectra and the 0.7–10 keV Swift (blue) spectrum of 4U 1728-34, fit with the continuum model: disk blackbody + blackbody + power law. The residuals between 6–8 keV indicate the presence of iron emission.

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