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We report the photometry of six transits of the hot Jupiter HAT-P-29bobtained from 2013 October to 2015 January. We analyze the new light curves, incombination with the published photometric, and Doppler velocimetric, andspectroscopic measurements, finding an updated orbital ephemeris for theHAT-P-29 system, $T_{\rm C}[0]= 2456170.5494(15)\,[\rm{BJD_{TDB}}]$ and$P=5.723390(13) \,{\rm days}$. It is $17.63\,{\rm s}$ ($4.0\,\sigma$) longerthan the previously published value, amounting to errors exceeding$2.5\,\rm{hrs}$ at the time of writing (on UTC 2018 June 1). The measuredtransit mid-times for HAT-P-29b show no compelling evidence of timing anomaliesfrom a linear model, which rules out the presence of a perturbers with massesgreater than $0.6$, $0.7$, $0.5$, and $0.4\,{\rm M_\oplus}$ near the $1:2$,$2:3$, $3:2$, and $2:1$ resonances with HAT-P-29b, respectively.

Transiting Exoplanet Monitoring Project (TEMP). I. Refined System Parameters and Transit Timing Variations of HAT-P-29b