C. Cicone, M. Bothwell, J. Wagg, P. Møller, C. De Breuck, Z. Zhang, S. Martín, R. Maiolino, P. Severgnini, M. Aravena and 9 other author(s). (2017)cite arxiv:1705.05851Comment: Accepted for publication in A&A. Abstract abridged due to arXiv requirements. The APEX spectra are available via the dedicated Phase 3 query interface at the ESO Science Archive Facility: http://archive.eso.org/wdb/wdb/adp/phase3_spectral/form?collection_name=ALLSMOG.
M. Varma, M. Mhatre, M. More, and P. Ayane. International Journal on Recent and Innovation Trends in Computing and Communication, 3 (4):
2213--2216(April 2015)
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.