Near-identical star formation rate densities from H$��$ and FUV at redshift zero

For the first time both H$��$ and far-ultraviolet (FUV) observations from an HI-selected sample are used to determine the dust-corrected star formation rate density (SFRD: $\dot��$) in the local Universe. Applying the two star formation rate indicators on 294 local galaxies we determine log($\dot��$$ _{H��}) = -1.68~^{+0.13}_{-0.05}$ [M$_{\odot} $ yr$^{-1} $ Mpc$^{-3}]$ and log($\dot��_{FUV}$) $ = -1.71~^{+0.12}_{-0.13}$ [M$_\odot $ yr$^{-1} $ Mpc$^{-3}]$. These values are derived from scaling H$��$ and FUV observations to the HI mass function. Galaxies were selected to uniformly sample the full HI mass (M$_{HI}$) range of the HI Parkes All-Sky Survey (M$_{HI} \sim10^{7}$ to $\sim10^{10.7}$ M$_{\odot}$). The approach leads to relatively larger sampling of dwarf galaxies compared to optically-selected surveys. The low HI mass, low luminosity and low surface brightness galaxy populations have, on average, lower H$��$/FUV flux ratios than the remaining galaxy populations, consistent with the earlier results of Meurer. The near-identical H$��$- and FUV-derived SFRD values arise with the low H$��$/FUV flux ratios of some galaxies being offset by enhanced H$��$ from the brightest and high mass galaxy populations. Our findings confirm the necessity to fully sample the HI mass range for a complete census of local star formation to include lower stellar mass galaxies which dominate the local Universe.
17 pages, 7 figures