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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 5.

Distribution of WN (essentially pulsar timing precision) for 10 realizations of the disk MSP population in the virtual LAT. As in previous plots, the solid line indicates the mean, while the shaded region indicates the range of the simulations. The green trace gives the distribution of observed WN values.

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