E. Nelson, P. van Dokkum, N. Schreiber, M. Franx, G. Brammer, I. Momcheva, S. Wuyts, K. Whitaker, R. Skelton, M. Fumagalli und 10 andere Autor(en). (2015)cite arxiv:1507.03999Comment: Submitted to ApJ. Main results: Fig. 6 shows the scale lengths of ionized gas vs. stellar disks. Fig. 9 shows where Halpha in galaxies is enhanced above and suppressed below the star-forming main sequence. Data points for Halpha profiles are available upon request.
N. Kanekar, S. Sethi, und K. Dwarakanath. (2016)cite arxiv:1601.07909Comment: 5 pages, 3 figures, accepted for publication in Astrophysical Journal Letters.
C. Ly, M. Malkan, J. Rigby, und T. Nagao. (2016)cite arxiv:1602.01098Comment: 17 pages, 11 figures, 2 tables. Submitted to ApJ on Feb 1, 2016. Paper presents first results on the evolution of the stellar mass--gas metallicity relation. The description of the survey and dataset is available in Paper I (Ly et al. ApJS, submitted). Key figures are # 4 & 5 (M-Z evolution), 7-9 (M-Z-SFR relation), and 11 (comparison with theory). Comments welcome.