Fig. 3.

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Localization of known pulsars and the new discoveries in NGC 6522 using SEEKAT. We show the likelihood map of the SEEKAT localization showing the 1σ and 2σ confidence intervals. The larger and asymmetric uncertainties for PSR J1803−3002E and PSR J1803−3002F are caused by the low S/N of the detections and the small number of beams used for the localization. The position of PSR J1803−3002A determined by timing (Zhang et al. 2020) is shown as a green star and is compatible with the SEEKAT localization of the pulsar. The red cross shows the location of the optical center of the GC, while the green dashed circle shows the core radius of the cluster of ∼12.3 arcsec (Kerber et al. 2018).
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