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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 3.

Phase-channel residuals for the best fit to the data of our model with three uniform-temperature circular spots plus a modulated power law, over the full set of 32 uniformly spaced rotational phases and NICER PI channels 30–299 inclusive. Here, for a phase-channel bin i, if the data have di counts and the model predicts mi counts, we define ﹩\chi \equiv ({m}_{i}-{d}_{i})/\sqrt{{m}_{i}}﹩. In addition to the fit having an overall acceptable χ2/dof = 8335.00/8345 (for which the probability of this χ2 or higher for a correct model is 53%), there are no patterns visible and no individual phase-channel bins with an unexpectedly large ∣χ∣. This is a one-way test: our satisfactory fit does not guarantee that the model is correct, but a very low probability would indicate that we would need to look more closely at our model.

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