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Fig. 1.

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X-ray counterpart candidates in 0.3–2.0 keV as observed with the EPIC-pn and EPIC-MOS2 (PSR J0711-6830). The green circles are centered at the radio timing position of the pulsars, the cyan circles are centered at the position where the X-ray source has the highest significance. The images have pixel scales of 0.4″, and are smoothed with Gaussian length scales σ = 3.4″ (for PSR J1125–5825), and σ = 2.4″ (for PSRs J0745–5353 and J0711–6830). The angular separations between X-ray and radio positions are given in Table 2.

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