High-precision interpolation of stellar atmospheres with a deep neural
network using a 1D convolutional auto encoder for feature extraction
- URL: http://arxiv.org/abs/2306.06938v1
- Date: Mon, 12 Jun 2023 08:16:26 GMT
- Title: High-precision interpolation of stellar atmospheres with a deep neural
network using a 1D convolutional auto encoder for feature extraction
- Authors: C. Westendorp Plaza, A. Asensio Ramos, C. Allende Prieto
- Abstract summary: We establish a reliable, precise, lightweight, and fast method for recovering stellar model atmospheres.
We employ a fully connected deep neural network which in turn uses a 1D convolutional auto-encoder to extract the nonlinearities of a grid.
We show a higher precision with a convolutional auto-encoder than using principal component analysis as a feature extractor.
- Score: 0.0
- License: http://creativecommons.org/licenses/by/4.0/
- Abstract: Given the widespread availability of grids of models for stellar atmospheres,
it is necessary to recover intermediate atmospheric models by means of accurate
techniques that go beyond simple linear interpolation and capture the
intricacies of the data. Our goal is to establish a reliable, precise,
lightweight, and fast method for recovering stellar model atmospheres, that is
to say the stratification of mass column, temperature, gas pressure, and
electronic density with optical depth given any combination of the defining
atmospheric specific parameters: metallicity, effective temperature, and
surface gravity, as well as the abundances of other key chemical elements. We
employed a fully connected deep neural network which in turn uses a 1D
convolutional auto-encoder to extract the nonlinearities of a grid using the
ATLAS9 and MARCS model atmospheres. This new method we call iNNterpol
effectively takes into account the nonlinearities in the relationships of the
data as opposed to traditional machine-learning methods, such as the light
gradient boosting method (LightGBM), that are repeatedly used for their speed
in well-known competitions with reduced datasets. We show a higher precision
with a convolutional auto-encoder than using principal component analysis as a
feature extractor.We believe it constitutes a useful tool for generating fast
and precise stellar model atmospheres, mitigating convergence issues, as well
as a framework for future developments. The code and data for both training and
direct interpolation are available online at
https://github.com/cwestend/iNNterpol for full reproducibility and to serve as
a practical starting point for other continuous 1D data in the field and
elsewhere.
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