E. Nelson, P. van Dokkum, I. Momcheva, G. Brammer, S. Wuyts, M. Franx, N. Schreiber, K. Whitaker, и 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 и 8 other автор(ы). (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, и 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, и V. Müller. (2015)cite arxiv:1503.05201Comment: 12 pages, 7 figures, version revised by referee's comments, resubmitted to MNRAS, comments welcome.