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Stellar spectral classification using automated schemes

Ravi K. Gulati, Ranjan Gupta, Pradeep Gothoskar, S. Khobragade

Open publisher page 67 citations

Abstract

Classification of stellar spectra by human experts, in the past, has been subjective, leading to many non-unique databases. However, with the availability of large spectral databases, automated classification schemes offer an alternative to visual classification. Here, we present two schemes for automated classification of stellar spectra, namely, chi-square - minimization and Artificial Neural Network. These techniques have been applied to classify a complete set of 158 test spectra into 55 spectral types of a reference library. Using these methods, we have successfully classified the test library on the basis of a reference library to an accuracy of two spectral subclasses. Such automated schemes would in the future provide fast, uniform, and almost on-line classification of stellar spectra.

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What this paper is about

Classification of stellar spectra by human experts, in the past, has been subjective, leading to many non-unique databases. However, with the availability of large spectral databases, automated classification schemes offer an alternative to visual classification. Here, we present two schemes for automated classification of stellar spectra, namely, chi-square - minimization and Artificial Neural Network. These techniques have been applied to classify a complete set of 158 test spectra into 55 spectral types of a reference library. Using these methods, we have successfully classified the test library on the basis of a reference library to an accuracy of two spectral subclasses. Such automated schemes would in the future provide fast, uniform, and almost on-line classification of stellar spectra.

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OpenAlex reports 67 citations for this work. Citation counts describe recorded attention and do not establish research quality.

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Available abstract

Classification of stellar spectra by human experts, in the past, has been subjective, leading to many non-unique databases. However, with the availability of large spectral databases, automated classification schemes offer an alternative to visual classification. Here, we present two schemes for automated classification of stellar spectra, namely, chi-square - minimization and Artificial Neural Network. These techniques have been applied to classify a complete set of 158 test spectra into 55 spectral types of a reference library. Using these methods, we have successfully classified the test library on the basis of a reference library to an accuracy of two spectral subclasses. Such automated schemes would in the future provide fast, uniform, and almost on-line classification of stellar spectra.

Key concepts: Stellar classification, Physics, Astronomical spectroscopy, Luminosity, Data reduction, Stars, Spectral line, LAMOST

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