Figure 2 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 2.

SEDs for the 13 Einstein@Home pulsars presented in this paper. The best-fit spectral models obtained by analyzing the full energy range are shown as red lines. The 95% confidence upper limits are calculated for energy bins with TS values below 4.

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