Mingyang Wang, Peng Liu, Jianping Yuan, Ang Li

We report the detection of a spin-down glitch with a fractional frequency change of $\Delta\nu/\nu=-3.46(6)\times10^{-9}$ in the rotation-powered pulsar PSR J1835$-$1106 at MJD 55813, based on timing observations collected with the Nanshan 26-m and Parkes 64-m radio telescopes from January 2000 to July 2022. A comparison of the average pulse profiles within $\pm300$ d of the event reveals no significant morphological changes. We also estimate the angular velocity lag between the normal and superfluid components at the time of the glitch, demonstrating that one of the spin-down glitch models proposed by Kantor & Gusakov (2014) is not applicable to PSR J1835$-$1106.