  Timing observations from the Nanshan 26-m radio telescope for nine pulsars
between 2000 and 2014 have been used to search for glitches. The data span for
nine pulsars ranges from 11.6 to 14.2 years. From the total of 114 yr of pulsar
rotational history, 16 new glitches were identified in 9 pulsars. Glitch
parameters were measured by fitting the timing residuals data. All 16 glitches
have a small fractional size. Six new glitches have been detected in PSR
J1833-0827, making it another frequent glitching pulsar. Some of the 16
glitches may experience exponential or linear recovery, but it is unlikely for
us to make further analyses with the large gap in the data set. All the glitch
rates obtained from Nanshan are higher than that from Jodrell Bank Observatory.
The small glitch size and high glitch rate could possibly attribute to the high
observation cadence.
