E. Nelson, P. van Dokkum, I. Momcheva, G. Brammer, S. Wuyts, M. Franx, N. Schreiber, K. Whitaker, and R. Skelton. (2015)cite arxiv:1511.04443Comment: Submitted to ApJ Letters. Fig. 2. shows measured radial Balmer decrement profiles. Fig. 3 shows inferred dust gradients. Fig. 4 shows dust-corrected radial profiles of star formation and the likely growth of bulges in high mass galaxies through in-situ star formation.
M. Murphy, and M. Bernet. (2015)cite arxiv:1510.05667Comment: Accepted to MNRAS. 18 pages, 17 figures, 5 tables. Tables 1-4 available in the published electronic version or from http://astronomy.swin.edu.au/~mmurphy/publications . Code emulating the SDSS colour-selection algorithm is available at doi:10.5281/zenodo.31470 (http://dx.doi.org/10.5281/zenodo.31470) and hosted on GitHub (https://github.com/mbernet79/SDSS_QSOsel_Bernet).