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The Tail of PSR J0002+6216 and the Supernova Remnant CTB 1

  • Authors: F. K. Schinzel, M. Kerr, U. Rau, S. Bhatnagar, and D. A. Frail

2019 The Astrophysical Journal Letters 876 L17.

  • Provider: AAS Journals

Caption: Figure 1.

Histogram (orange) of the photon weights using pulse phase from the best-fit timing model (see the main text). Shown as solid black lines are the six wrapped Gaussian components of the analytic profile. The faint blue lines show 200 randomly chosen realizations of the template from the Monte Carlo Markov chain (MCMC) fits with the template parameters allowed to vary.

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