Figure 5 from LONG-TERM STUDY OF THE DOUBLE PULSAR J0737–3039 WITH XMM-NEWTON: PULSAR TIMING

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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 5.

Background-subtracted pulsed fraction of PSR A (top panels) and orbital modulation of the total count rate from the system (bottom panels), in the 0.15–3.0 keV energy interval, obtained by folding ∼67 orbital periods (2006+2011 EPIC-pn data) and binning at ∼40 minutes (left) and ∼20 minutes (right). The vertical dotted–dashed line represents the superior conjunction of PSR A.

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