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

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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 1.

Light curves obtained for Holmberg IX X-1 in 5 ks bins with Suzaku (top panels), NuSTAR (middle panels), and XMM-Newton (bottom panels) during our observing program in late 2012, indicating the relative coordination of the various observations utilized in this work.

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