Figure 3 from Broadband X-Ray Spectra of the Ultraluminous X-Ray Source Holmberg IX X-1 Observed with NuSTAR, XMM-Newton, and Suzaku

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

Broadband X-Ray Spectra of the Ultraluminous X-Ray Source Holmberg IX X-1 Observed with NuSTAR, XMM-Newton, and Suzaku

Authors: D. J. Walton, F. A. Harrison, B. W. Grefenstette, J. M. Miller, M. Bachetti, D. Barret, S. E. Boggs, F. E. Christensen, W. W. Craig, A. C. Fabian, F. Fuerst, C. J. Hailey, K. K. Madsen, M. L. Parker, A. Ptak, V. Rana, D. Stern, N. Webb, and W. W. Zhang

Walton et al. 2014 The Astrophysical Journal 793 21.

Provider: AAS Journals

Caption: Figure 3.

Data/model ratios for the XMM-Newton (black: EPIC-pn, red: EPIC-MOS), Suzaku (green: FI XIS, blue: BI XIS), and NuSTAR (magenta: FPMA, cyan: FPMB) data sets obtained during epoch 1, modeled with both a power-law continuum (top panel) and a bremsstrahlung continuum (bottom panel). The data from the various missions display consistent curvature across their common energy range (3–10 keV). The data have been rebinned for visual clarity.

Other Images in This Article

Copyright and Terms & Conditions