2020
DOI: 10.1093/mnras/staa3642
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Mode angular degree identification in subgiant stars with convolutional neural networks based on power spectrum

Abstract: The identification of the angular degrees l of oscillation modes is essential for asteroseismology and it depends on visual tagging before fitting power spectra in a so-called peakbagging analysis. In oscillating subgiants, radial (l = 0) mode frequencies are distributed linearly in frequency, while non-radial (l ≥ 1) modes are p–g mixed modes that have a complex distribution in frequency that increases the difficulty of identifying l. In this study, we trained a one-dimensional convolutional neural network to… Show more

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Cited by 3 publications
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“…e larger and deeper the foundation pit project, the more difficult it will be for the support structure of the foundation pit project [25].…”
Section: Construction Of the Spatial Topological Relationship Ofmentioning
confidence: 99%
“…e larger and deeper the foundation pit project, the more difficult it will be for the support structure of the foundation pit project [25].…”
Section: Construction Of the Spatial Topological Relationship Ofmentioning
confidence: 99%
“…The ReLU function can alleviate the problem of vanishing gradients in the neural network. The dropout technique was introduced to prevent overfitting [73,74]. By relying on the powerful prediction performance of onedimensional convolution [75] and using the data set obtained by finite element analysis to train 1D-CNN, a model equivalent to the overdetermined equation can be obtained.…”
Section: The Potential For Ann Use In Ioamentioning
confidence: 99%