TY - JOUR
T1 - Deep learning exoplanets detection by combining real and synthetic data
AU - Cuéllar, Sara
AU - Granados, Paulo
AU - Fabregas, Ernesto
AU - Curé, Michel
AU - Vargas, Héctor
AU - Dormido-Canto, Sebastián
AU - Farias, Gonzalo
N1 - Publisher Copyright:
© 2022 Cuéllar et al. This is an open access article distributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.
PY - 2022/5
Y1 - 2022/5
N2 - Scientists and astronomers have attached great importance to the task of discovering new exoplanets, even more so if they are in the habitable zone. To date, more than 4300 exoplanets have been confirmed by NASA, using various discovery techniques, including planetary transits, in addition to the use of various databases provided by space and groundbased telescopes. This article proposes the development of a deep learning system for detecting planetary transits in Kepler Telescope light curves. The approach is based on related work from the literature and enhanced to validation with real light curves. A CNN classification model is trained from a mixture of real and synthetic data. The model is then validated only with unknown real data. The best ratio of synthetic data is determined by the performance of an optimisation technique and a sensitivity analysis. The precision, accuracy and true positive rate of the best model obtained are determined and compared with other similar works. The results demonstrate that the use of synthetic data on the training stage can improve the transit detection performance on real light curves.
AB - Scientists and astronomers have attached great importance to the task of discovering new exoplanets, even more so if they are in the habitable zone. To date, more than 4300 exoplanets have been confirmed by NASA, using various discovery techniques, including planetary transits, in addition to the use of various databases provided by space and groundbased telescopes. This article proposes the development of a deep learning system for detecting planetary transits in Kepler Telescope light curves. The approach is based on related work from the literature and enhanced to validation with real light curves. A CNN classification model is trained from a mixture of real and synthetic data. The model is then validated only with unknown real data. The best ratio of synthetic data is determined by the performance of an optimisation technique and a sensitivity analysis. The precision, accuracy and true positive rate of the best model obtained are determined and compared with other similar works. The results demonstrate that the use of synthetic data on the training stage can improve the transit detection performance on real light curves.
UR - http://www.scopus.com/inward/record.url?scp=85130904073&partnerID=8YFLogxK
U2 - 10.1371/journal.pone.0268199
DO - 10.1371/journal.pone.0268199
M3 - Article
C2 - 35613093
AN - SCOPUS:85130904073
SN - 1932-6203
VL - 17
JO - PLoS ONE
JF - PLoS ONE
IS - 5 May
M1 - e0268199
ER -