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LONG-TERM STUDY OF THE DOUBLE PULSAR J0737–3039 WITH XMM-NEWTON: PULSAR TIMING

  • Authors: M. N. Iacolina, A. Pellizzoni, E. Egron, A. Possenti, R. Breton, M. Lyutikov, M. Kramer, M. Burgay, S. E. Motta, A. De Luca, and A. Tiengo

2016 The Astrophysical Journal 824 87.

  • Provider: AAS Journals

Caption: Figure 2.

Result of phasing of the PSR A’s pulsed profile. The X-ray profile obtained for 0.15–3.0 keV is represented by the solid blue line. The green line shows the radio profile at 820 MHz in arbitrary units. While the dotted–dashed red vertical lines indicate the phase value of the maximum of the γ-ray pulses. Two rotational phases are displayed for clarity.

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