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Webster, S.M. Sweet, T.M. Heckman, V.A. Kilborn, Z. Zheng","submitted_at":"2018-06-15T09:46:32Z","abstract_excerpt":"For the first time both H$\\alpha$ and far-ultraviolet (FUV) observations from an HI-selected sample are used to determine the dust-corrected star formation rate density (SFRD: $\\dot{\\rho}$) in the local Universe. Applying the two star formation rate indicators on 294 local galaxies we determine log($\\dot{\\rho}$$ _{H\\alpha}) = -1.68~^{+0.13}_{-0.05}$ [M$_{\\odot} $ yr$^{-1} $ Mpc$^{-3}]$ and log($\\dot{\\rho}_{FUV}$) $ = -1.71~^{+0.12}_{-0.13}$ [M$_\\odot $ yr$^{-1} $ Mpc$^{-3}]$. These values are derived from scaling H$\\alpha$ and FUV observations to the HI mass function. 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