Fig. 1: Light curves of the ASKAP and MeerKAT detections. | Nature Astronomy

Fig. 1: Light curves of the ASKAP and MeerKAT detections.

From: An emission-state-switching radio transient with a 54-minute period

Fig. 1

The y axis is the pulse number. The peak flux densities of these detections are reported in Extended Data Table 1. The different colours represent the dates of the observations. Pulse detections within an observation represent consecutive rotations of the source. Although different in terms of radio properties, the MeerKAT detections appear to arrive in phase with the ASKAP detections.

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