Extended Data Fig. 1: Timing residuals of PSR J0901 − 4046.
From: Discovery of a radio-emitting neutron star with an ultra-long spin period of 76 s
The residuals from the best fit timing model given in Table 1. The orange data points are determined from the original MeerTRAP detection images, the first red diamond corresponds to a single pulse and the remaining red diamonds are determined from each of the half hour long follow-up observations with MeerKAT. The error bars are 1-σ. We used the L-band MeerKAT data for the timing analysis. The light coloured data points are from the Parkes UWL observations.
