Figure 1 from Possible Detection of an Emission Cyclotron Resonance Scattering Feature from the Accretion-powered Pulsar 4U 1626

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Possible Detection of an Emission Cyclotron Resonance Scattering Feature from the Accretion-powered Pulsar 4U 1626–67

Authors: W. B. Iwakiri, Y. Terada, T. Mihara, L. Angelini, M. S. Tashiro, T. Enoto, S. Yamada, K. Makishima, M. Nakajima, and A. Yoshida

Iwakiri et al. 2012 The Astrophysical Journal 751 35.

Provider: AAS Journals

Caption: Figure 1.

Energy-resolved light curves of 4U 1626−67 observed with Suzaku. Upper and middle panels show background-subtracted light curves obtained with XIS-0 in the 0.4–10.0 keV range and with the HXD in the 10–50 keV range, respectively. The bottom panel shows the hardness ratio of the above two panels. The gray solid line shows the average and the gray dotted lines show the ±3σ interval.

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