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Fig. 2.

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Ter5 field shown with each axis approximately spanning 1.5 times the core radius of the cluster. The positions of the X-ray sources (black rings), known pulsars (blue dots) as well new discoveries (red dots) are also overlaid. Particular emphasis is made on the VLA-38 source (brown star) obtained from radio imaging and whose coordinates are reported in Urquhart et al. (2020). The timing position of Ter5ar (green star) is shown to overlap significantly with VLA-38 as well as with an X-ray source (CXOU J174804.63−244645.2) in the backdrop. The dashed lines surrounding the X-ray sources and VLA-38 are the 3-σ positional uncertainties.

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