We report the photometry of six transits of the hot Jupiter HAT-P-29b obtained from 2013 October to 2015 January. We analyze the new light curves, in combination with the published photometric, and Doppler velocimetric, and spectroscopic measurements, finding an updated orbital ephemeris for the HAT-P-29 system, TC[0]=2456170.5494(15)[BJDTDB] and P=5.723390(13)days. It is 17.63s (4.0σ) longer than the previously published value, amounting to errors exceeding 2.5hrs at the time of writing (on UTC 2018 June 1). The measured transit mid-times for HAT-P-29b show no compelling evidence of timing anomalies from a linear model, which rules out the presence of a perturbers with masses greater than 0.6, 0.7, 0.5, and 0.4M⊕ near the 1:2, 2:3, 3:2, and 2:1 resonances with HAT-P-29b, respectively.
@article{arxiv.1807.10107,
title = {Transiting Exoplanet Monitoring Project (TEMP). I. Refined System Parameters and Transit Timing Variations of HAT-P-29b},
author = {Songhu Wang and Xian-Yu Wang and Yong-Hao Wang and Hui-Gen Liu and Tobias C. Hinse and Jason Eastman and Daniel Bayliss and Yasunori Hori and Shao-Ming Hu and Kai Li and Jinzhong Liu and Norio Narita and Xiyan Peng and R. A. Wittenmyer and Zhen-Yu Wu and Hui Zhang and Xiaojia Zhang and Haibin Zhao and Ji-Lin Zhou and George Zhou and Xu Zhou and Gregory Laughlin},
journal= {arXiv preprint arXiv:1807.10107},
year = {2018}
}