Identifying Exoplanets with Deep Learning. V. Improved Light Curve Classification for TESS Full Frame Image Observations
Evan Tey, Dan Moldovan, Michelle Kunimoto, Chelsea X. Huang, Avi, Shporer, Tansu Daylan, Daniel Muthukrishna, Andrew Vanderburg, Anne Dattilo,, George R. Ricker, S. Seager

TL;DR
This paper introduces Astronet-Triage-v2, a deep learning model that significantly improves exoplanet light curve classification accuracy for TESS data, aiding in more effective identification of planet candidates.
Contribution
The paper presents a new neural network model trained on a curated dataset, achieving higher recall and better generalization for TESS exoplanet candidate classification.
Findings
Achieves 99.6% recall at 75.7% precision on test data.
Improves the area under the precision-recall curve by 4% over previous models.
Recovers 3577 out of 4140 TOIs, saving at least 200 planet candidates.
Abstract
The TESS mission produces a large amount of time series data, only a small fraction of which contain detectable exoplanetary transit signals. Deep learning techniques such as neural networks have proved effective at differentiating promising astrophysical eclipsing candidates from other phenomena such as stellar variability and systematic instrumental effects in an efficient, unbiased and sustainable manner. This paper presents a high quality dataset containing light curves from the Primary Mission and 1st Extended Mission full frame images and periodic signals detected via Box Least Squares (Kov\'acs et al. 2002; Hartman 2012). The dataset was curated using a thorough manual review process then used to train a neural network called Astronet-Triage-v2. On our test set, for transiting/eclipsing events we achieve a 99.6% recall (true positives over all data with positive labels) at a…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research · Gamma-ray bursts and supernovae
MethodsTest
