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Exoplanets in the Antarctic sky. II. 116 Transiting Exoplanet Candidates Found by AST3-II (CHESPA) within the Southern CVZ of TESS

Authors :
Zhang, Hui
Yu, Zhouyi
Liang, Ensi
Yang, Ming
Ashley, Michael C. B.
Cui, Xiangqun
Du, Fujia
Fu, Jianning
Gong, Xuefei
Gu, Bozhong
Hu, Yi
Jiang, Peng
Liu, Huigen
Lawrence, Jon
Liu, Qiang
Li, Xiaoyan
Li, Zhengyang
Ma, Bin
Mould, Jeremy
Shang, Zhaohui
Suntzeff, Nicholas B.
Tao, Charling
Tian, Qiguo
Tinney, C. G.
Uddin, Syed A.
Wang, Lifan
Wang, Songhu
Wang, Xiaofeng
Wei, Peng
Wright, Duncan
Wu, Xuefeng
Wittenmyer, Robert A.
Xu, Lingzhe
Yang, Shi-hai
Yu, Ce
Yuan, Xiangyan
Zheng, Jessica
Zhou, Hongyan
Zhou, Ji-lin
Zhu, Zhenxi
Publication Year :
2018

Abstract

We report first results from the CHinese Exoplanet Searching Program from Antarctica (CHESPA)---a wide-field high-resolution photometric survey for transiting exoplanets carried out using telescopes of the AST3 (Antarctic Survey Telescopes times 3) project. There are now three telescopes (AST3-I, AST3-II, and CSTAR-II) operating at Dome A---the highest point on the Antarctic Plateau---in a fully automatic and remote mode to exploit the superb observing conditions of the site, and its long and uninterrupted polar nights. The search for transiting exoplanets is one of the key projects for AST3. During the Austral winters of 2016 and 2017 we used the AST3-II telescope to survey a set of target fields near the southern ecliptic pole, falling within the continuous viewing zone of the TESS mission \citep{Ricker10}. The first data release of the 2016 data, including images, catalogs and lightcurves of 26578 bright stars ($7.5\le i \le15$) was presented in \citet{Zhang18}. The best precision, as measured by the RMS of the lightcurves at the optimum magnitude of the survey ($i=10$), is around 2\,mmag. We detect 222 objects with plausible transit signals from these data, 116 of which are plausible transiting exoplanet candidates according to their stellar properties as given by the TESS Input Catalog \citep{Stassun17}, Gaia DR2 \citep{Gaia18} and TESS-HERMES spectroscopy \citep{Sharma18}. With the first data release from TESS expected in late 2018, this candidate list will be a timely for improving the rejection of potential false positives.<br />Comment: 49 pages, 23 figures, 3 tables

Details

Database :
arXiv
Publication Type :
Report
Accession number :
edsarx.1809.01789
Document Type :
Working Paper
Full Text :
https://doi.org/10.3847/1538-4365/aaf583