Output posterior distributions for PSR J1933−6211 parameters. These were obtained from TEMPONEST sampling using the T2 orbital model and a red-noise model, and were generated using the CHAINCONSUMER package. We present the orbital and post-Keplerian parameters. Full details are provided in Table 2. The obtained pulsar mass (M_p) distribution was computed using the mass function and the posterior distributions on M_c, i, x_p, and P_b.