Fig. 5
AV-distance relation towards PSR J1048–5832. The vertical dashed line corresponds to the DM distance to the pulsar of 2.7 kpc. The hatched region and horizontal solid line show the confidence interval of AV resulting from the uncertainty interval of NH and its best-fit value for the pulsar presented in Table 3. The entire galactic extinction is indicated by the dash-dotted line.
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