Corner plot showing the posterior distributions of the orbital, post-Keplerian parameters and the derived mass of PSR J1910−5959A obtained from ELL1 binary model using TEMPONEST. The diagonal elements show the marginalised 1D histograms of the parameters while the off-diagonal elements show the correlation between the parameters and are marked by contours that define the 39%, 86%, and 98% C.L. The shaded region in the 1D histograms indicates the nominal 68.27% C.L. as noted in Table 3.