Figure 14 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 14.

Plotted line is the background-subtracted pulse profile in the 10–30 keV energy band. The circles denote the best-fit values of the normalization of the positive power-law term (i.e., the Wien hump) when fitting by NPEX model, presented as a function of the pulse phase (see the text for details). Values are normalized by each maximum value.

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