Figure 3 from The Einstein@Home Gamma-ray Pulsar Survey. II. Source Selection, Spectral Analysis, and Multiwavelength Follow-up

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

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 3.

Best-fit power-law index Γ vs. cutoff energy E_cut for the new pulsars (red squares), other selected 3FGL sources that were searched in our survey (blue circles), and known gamma-ray pulsars from 2PC (green triangles). 3FGL sources with cutoff energies above 10 GeV are not plotted and uncertainties are not displayed, to improve readability.

Other Images in This Article

Copyright and Terms & Conditions