  We present ten $R$-band photometric observations of eight different transits
of the hot Jupiter HAT-P-33b, which has been targeted by our Transiting
Exoplanet Monitoring Project (TEMP). The data were obtained by two telescopes
at the Xinglong Station of National Astronomical Observatories of China (NAOC)
from 2013 December through 2016 January, and exhibit photometric scatter of
$1.6-3.0\,\rm{mmag}$. After jointly analyzing the previously published
photometric data, radial-velocity (RV) measurements, and our new light curves,
we revisit the system parameters and orbital ephemeris for the HAT-P-33b
system. Our results are consistent with the published values except for the
planet-to-star radius ratio ($R_{P}/R_{*}$), the ingress/egress duration
($\tau$) and the total duration ($T_{14}$), which together indicate a slightly
shallower and shorter transit shape. Our results are based on more complete
light curves, whereas the previously published work had only one complete
transit light curve. No significant anomalies in Transit Timing Variations
(TTVs) are found, and we place upper mass limits on potential perturbers,
largely supplanting the loose constraints provided by the extant RV data. The
TTV limits are stronger near mean-motion resonances, especially for the
low-order commensurabilities. We can exclude the existence of a perturber with
mass larger than 0.6, 0.3, 0.5, 0.5, and $0.3\,{\rm M_\oplus}$ near the 1:3,
1:2, 2:3, 3:2, and 2:1 resonances, respectively.
