Open Access

Fig. 4.

image

Download original image

Period vs. acceleration for timing observations taken on 27 November 2017; 18, 21, and 28 January, 2020; and 5, 14, and 15 February 2020. Line-of-sight acceleration is calculated using observed period derivatives, where P and are the observed spin period and spin period derivative in each detection. The pulsar turns out to be in an orbit with Pb ∼ 1.197 d and x  ∼ 1.43 lt-s.

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.