摘要: Deep learning techniques have been well explored in the transiting exoplanet
field; however, previous work mainly focuses on classification and inspection.
In this work, we develop a novel detection algorithm based on a well proven
object detection framework in the computer vision field. Through training the
network on the light curves of the confirmed Kepler exoplanets, our model
yields about 90% precision and recall for identifying transits with
signal-to-noise ratio higher than 6 (set the confidence threshold to 0.6).
Giving a slightly lower confidence threshold, recall can reach higher than 95%.
We also transfer the trained model to the TESS data and obtain similar
performance. The results of our algorithm match the intuition of the human
visual perception and make it useful to find single-transiting candidates.
Moreover, the parameters of the output bounding boxes can also help to find
multiplanet systems. Our network and detection functions are implemented in the
Deep-Transit toolkit, which is an open-source Python package hosted on GitHub
and PyPI.