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. Michałowski, E. Murphy, J. Hjorth, D. Watson, C. Gall, and J. Dunlop. (2011)cite arxiv:1107.5149Comment: ASP Conference Series; proceedings of the conference 'Galaxy Evolution: Infrared to Millimeter Wavelength Perspective', Guilin, China, 25-29 October 2010; 6 pages, 1 figure.