Label Transfer From APOGEE to LAMOST and BOSS

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2022-05

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The Ohio State University

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Abstract

In this century, large spectroscopic stellar surveys observe stars in a large range of spectral types at different wavelengths, different resolutions with different data analysis methods. In order to further study Galactic evolution, measurements of stellar parameters for different surveys must be made precise and consistent. With The Cannon 2, a data driven method, we can transfer stellar parameters between two different surveys on the same scale directly. Using The Cannon 2, I investigated the effect of the training set size on the accuracy of the predicted results. As the size of the training set increasing, the accuracy of the inferred parameters increasing. The training label's quality is the other factor that influences the label transfer results. In this thesis, The Cannon 2 is also used to predicate stellar parameters for 10,000 F, G, K stars, with estimate Tef f less than 6000 K, from BOSS under the APOGEE scale to reduce the labels' inconsistencies between two surveys.

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The Cannon 2, APOGEE, LAMOST, BOSS, MaStar

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