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The Radius of PSR J0437–4715 from NICER Data

  • Authors: M. C. Miller, A. J. Dittmann, I. M. Holt, F. K. Lamb, C. Chirenti, Z. Arzoumanian, J. Berteaud, S. Bogdanov, K. C. Gendreau, W. C. G. Ho, S. M. Morsink, P. S. Ray, R. A. Remillard, Z. Wadiasingh, M. T. Wolff

M. C. Miller et al 2026 The Astrophysical Journal Letters 1000 .

  • Provider: AAS Journals

Caption: Figure 1.

Radius posteriors for each of our three models with a modulated power law (the vertical axis is linear in the probability density); from top to bottom in the legend, the model numbers are 5, 4, and 3. The dotted line shows the prior. There is a large overlap of the posteriors of all three models, which shows that among the models with a modulated power law, the posterior is not especially sensitive to the model chosen.

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