Open Access
Fig. 2
Timing residuals as a function of time for the best-fit timing solution of PSR J1618−3921 given in Table 3. The inset shows the residuals for the time interval when the pulsar was intensively observed to derive a phase-connected timing solution.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.