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 Ṗ are the observed spin period and spin period derivative in each detection. The pulsar turns out to be in an orbit with P_b ∼ 1.197 d and x  ∼ 1.43 lt-s.