Joss Bland-Hawthorn

TL;DR: In this paper, the spectral energy distribution (SED) model was used to estimate the mass to light ratios of stellar populations and hence the stellar masses of galaxies, and the SED derived masses for a carefully selected sample of low redshift galaxies were compared with the prediction from stellar population synthesis models that $M_*/L ǫ = 0.15$ for all such galaxies, independent of other stellar population parameters.

TL;DR: In this paper, the apparent stellar angular momentum of 300 galaxies across the Hubble sequence, using integral-field spectroscopic data from the CALIFA survey, was measured in different apertures.

TL;DR: In this paper, a brief rebuttal to arXiv:1502.03821, which claims to provide the first observational proof of dark matter interior to the solar circle, is presented.

TL;DR: In this paper, it was shown that a clumpy outer disk of dense clouds or cloudlets is potentially detectable to much larger radii and lower HI column densities than previously discussed.

TL;DR: The OTELO survey as mentioned in this paper is the most comprehensive survey to date in terms of minimum detectable flux and emission line equivalent width in order to detect the faintest extragalactic emission line systems.