Fig. 7 from A Further Study of the Luminosity‐dependent Cyclotron Resonance Energies of the Binary X‐Ray Pulsar 4U 0115+63 with the Rossi X‐Ray Timing Explorer

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A Further Study of the Luminosity‐dependent Cyclotron Resonance Energies of the Binary X‐Ray Pulsar 4U 0115+63 with the Rossi X‐Ray Timing Explorer

Authors: M. Nakajima, T. Mihara, K. Makishima, and H. Niko

Nakajima et al. 2006 The Astrophysical Journal 646 1125.

Provider: AAS Journals

Caption: Fig. 7.

Eight intensity‐sorted spectra defined in Fig. 5, fitted with the NPEX×CYAB2 (f1–f5) or the NPEX×CYAB (f6–f8) model. The middle panels show the data‐to‐model ratios, while the bottom panels are the same ratios but without incorporating the CYAB factor(s).

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