Figure 4 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 4.

Radio and gamma-ray pulse profiles for PSR J0002+6216 (left) and PSR J0631+0646 (right). Two complete cycles are shown for clarity. Weighted LAT gamma-ray pulse profiles (in red) were produced by selecting photons with weights greater than 0.05. Radio profiles (in black) correspond to 1.4 GHz observations made with the Effelsberg telescope for PSR J0002+6216 and the Arecibo telescope for PSR J0631+0646. Uncertainties in DM converted to uncertainties in the phase offset between the radio and gamma-ray peaks correspond to ∼1% of the rotational periods.

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