Figure 1 from The Einstein@Home Gamma-ray Pulsar Survey. II. Source Selection, Spectral Analysis, and Multiwavelength Follow-up

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The Einstein@Home Gamma-ray Pulsar Survey. II. Source Selection, Spectral Analysis, and Multiwavelength Follow-up

Authors: J. Wu, C. J. Clark, H. J. Pletsch, L. Guillemot, T. J. Johnson, P. Torne, D. J. Champion, J. Deneva, P. S. Ray, D. Salvetti, M. Kramer, C. Aulbert, C. Beer, B. Bhattacharyya, O. Bock, F. Camilo, I. Cognard, A. Cuéllar, H. B. Eggenstein, H. Fehrmann, E. C. Ferrara, M. Kerr, B. Machenschalk, S. M. Ransom, S. Sanpa-Arsa, and K. Wood

2018 The Astrophysical Journal 854 99.

Provider: AAS Journals

Caption: Figure 1.

Results of the decomposition of gamma-ray pulse profiles into Bayesian blocks, as discussed in Section 4.1. Blue histograms represent the pulse profiles, red lines the Bayesian block decompositions, and shaded regions the off-pulse phase intervals determined from this analysis. Dashed black lines represent the estimated background levels, calculated as ﹩B={\sum }_{i}^{N}(1-{w}_{i})﹩, where w_i is the weight associated with photon i (Guillemot et al. 2012b).

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