A statistical analysis of the structure of the interstellar medium in the disc of the milky way
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DOI: 10.1093/mnras/stad1450
Abstract: We construct Convolutional Neural Networks (CNNs) trained on exponentiated fractional Brownian motion (xfBm) images, and use these CNNs to analyse Hi-GAL images of surface-density in the Galactic Plane. The CNNs estimate the Hurst parameter, ${\cal… read more here.
Keywords: density; structure; statistical analysis; surface density ... See more keywords