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A Chandra Proper Motion for PSR J1809–2332

  • Authors: Adam Van Etten, Roger W. Romani, and C.-Y. Ng

Van Etten, Romani, & Ng 2012 The Astrophysical Journal 755 151.

  • Provider: AAS Journals

Caption: Figure 3.

Residual source displacements between epochs (δ = new position − old position), relative to the PSF-fit frame offset (Table 3). Blue indicates wavdetect positions and errors, while red indicates positions and errors obtained from the FoM maps. Source 3, an obvious outlier, is pruned from the frame-shift fits. The pulsar shows small but significant shifts.

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