E. Nelson, P. van Dokkum, N. Schreiber, M. Franx, G. Brammer, I. Momcheva, S. Wuyts, K. Whitaker, R. Skelton, M. Fumagalli and 10 other author(s). (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, and K. Dwarakanath. (2016)cite arxiv:1601.07909Comment: 5 pages, 3 figures, accepted for publication in Astrophysical Journal Letters.
C. Ly, M. Malkan, J. Rigby, and 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.
S. Offner, P. Clark, P. Hennebelle, N. Bastian, M. Bate, P. Hopkins, E. Moraux, and A. Whitworth. (2013)cite arxiv:1312.5326Comment: 24 pages, 6 figures. Accepted for publication as a chapter in Protostars and Planets VI, University of Arizona Press (2014), eds. H. Beuther, R. S. Klessen, C. P. Dullemond, Th. Henning.
V. Tamburello, L. Mayer, S. Shen, and J. Wadsley. (2014)cite arxiv:1412.3319Comment: 22 pages, 21 figures and two tables. Submitted to MNRAS. Comments welcome.