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Future Space-based γ-Ray Pulsar Timing Arrays

  • Authors: M. Kerr, Z. Wadiasingh, A. Laviron, C. Kalapotharakos, H. T. Cromartie, T. Cohen

M. Kerr et al 2026 The Astrophysical Journal Letters 1001 .

  • Provider: AAS Journals

Caption: Figure 2.

Predicted cutoff energy (Ec, left) and γ-ray efficiency (right) distributions for one realization of the disk population (S1), showing three regimes. The orange points indicate the direct application of the relation to the synthesized P and ﹩\dot{P}﹩, and the blue points indicate the introduction of scatter on both Ec and ﹩{{ \mathcal L }}_{\gamma }﹩. The former captures the observed observational spread in Ec, and the latter captures beaming and other neglected physical influences on the luminosity/flux (e.g., magnetic inclination).

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