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Fig. 1.

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Tiling pattern of the beams of the TRAPUM observations of NGC 6522 performed on 2020 December 23 (left) and on 2022 February 2022 (right). The tied-array beams are shown in pink up to the half-power level measured at 1284 MHz at the middle of the observation. The black dashed circle shows the half-light radius of the cluster, ∼1.15 arcmin (Baumgardt & Hilker 2018). The red dotted circles show the maximum extent of the size of the tiling in the two observations plotted for comparison. PSR J1803−3002A is shown in blue at the position measured through timing (Zhang et al. 2020), while the other pulsars are shown at position of the beam where they appeared with the highest S/N. The beams with the best detections are represented in a brighter shade of pink. The new discoveries are shown in bold. All of the beams shown have been searched for new pulsars.

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