Deep learning interpretable analysis for carbon star identification in Gaia DR3

Context. A large fraction of Asymptotic Giant Branch (AGB) stars develop carbon-rich atmospheres during their evolution. Based on their color and luminosity, these carbon stars can be easily distinguished from many other kinds of stars. However, a large number of G, K, and M giants are also distributed in the same region as carbon stars on the HR diagram. Their spectra have differences, especially in the prominent CN molecular bands. Aims. We aim to distinguish carbon stars from other kinds of stars using Gaia's XP spectra, while providing attribution explanations of key features necessary for identification, and even discovering additional new spectral key features. Methods. We proposed a classification model named `GaiaNet', an improved one-dimensional convolutional neural network specifically designed for handling Gaia's XP spectra. We utilized the SHAP interpretability model to calculate the SHAP value for each feature point in a spectrum, enabling us to explain the output of the `GaiaNet' model and provide further meaningful analysis Results. Compared to four traditional machine-learning methods, the `GaiaNet' model exhibits an average classification accuracy improvement of approximately 0. 3% on the validation set, with the highest accuracy even reaching 100%. Utilizing the SHAP algorithm, we present a clear spectroscopic heatmap highlighting molecular band absorption features primarily distributed mainly around CN773. 3 and CN895. 0, and summarize five crucial feature regions for carbon star identification. Upon applying the trained classification model to the CSTAR sample with Gaia `xpₛampledₘean' spectra, we obtained 451 new candidate carbon stars as a by-product.