Same as Fig. 6 for PSR J1825−1446. The solid black line in each panel indicates the Galactic velocity assuming a radial velocity of 0 km s^-1. The velocity uncertainties at 3-σ level are smaller than the black lines. The red thin line corresponds to an hypothetical radial velocity from the Sun of  +500 km s^-1 (away from the Sun) and the blue thin line to  −500 km s^-1 (towards the Sun).