Y. Jeon, M. Im, S. Pak, M. Hyun, S. Kim, Y. Kim, H. Lee, and W. Park. (2016)cite arxiv:1602.02236Comment: 12 pages, 10 figures, 4 tables, accepted for publication in Journal of the Korean Astronomical Society.
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.
E. da Cunha, F. Walter, I. Smail, M. Swinbank, J. Simpson, R. Decarli, J. Hodge, A. Weiss, P. van der Werf, F. Bertoldi and 8 other author(s). (2015)cite arxiv:1504.04376Comment: 22 pages, 14 figures, 2 tables. Accepted for publication in the Astrophysical Journal. The new MAGPHYS model libraries used in this paper will appear in www.iap.fr/magphys. The SMG SED templates shown in Section 6.1 are available at http://astronomy.swinburne.edu.au/~ecunha/ecunha/SED_Templates.html.
R. Bouwens, G. Illingworth, P. Oesch, J. Caruana, B. Holwerda, R. Smit, and S. Wilkins. (2015)cite arxiv:1503.08228Comment: 16 pages, 10 figures, 3 tables, submitted to the Astrophysical Journal, Figure 6 shows the main result of the paper, Table 1 includes a compilation of the many key constraints on the ionisation state of the universe at z>6.
A. Hutter, P. Dayal, and V. Müller. (2015)cite arxiv:1503.05201Comment: 12 pages, 7 figures, version revised by referee's comments, resubmitted to MNRAS, comments welcome.