R. Naidu, P. Oesch, D. Setton, J. Matthee, C. Conroy, B. Johnson, J. Weaver, R. Bouwens, G. Brammer, P. Dayal и 15 other автор(ы). (2022)cite arxiv:2208.02794Comment: Submitted to ApJL. Fig. 1 shows the "superposed" state, Fig. 2 presents the potential z~5 protocluster, Fig. 3 shows some atypical z~5 SEDs, Fig. 4 studies the morphology, Fig. 5 summarizes the extraordinary situation at z~17, and Fig. 6 argues for why such interlopers may not be a major issue for z>10 searches. Comments warmly welcomed.
R. Naidu, P. Oesch, P. van Dokkum, E. Nelson, K. Suess, K. Whitaker, N. Allen, R. Bezanson, R. Bouwens, G. Brammer и 14 other автор(ы). (2022)cite arxiv:2207.09434Comment: Submitted to ApJL. Figs. 1 and 2 summarize the candidates, Fig. 3 places the brightness of these systems in context, Fig. 4 shows the morphology, Fig. 5 explores implications for the UVLF. Comments warmly welcomed.
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. Nelson, P. van Dokkum, N. Schreiber, M. Franx, G. Brammer, I. Momcheva, S. Wuyts, K. Whitaker, R. Skelton, M. Fumagalli и 10 other автор(ы). (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.