N. F. Schreiber, D. Wilman, E. Wisnioski, M. Fossati, J. Mendel, R. Bender, R. Genzel, A. Beifiori, S. Belli, G. Brammer, A. Burkert, J. Chan, R. Davies, R. L. Davies, M. Fabricius, A. Galametz, R. Herrera-Camus, P. Lang, D. Lutz, I. Momcheva, T. Naab, E. Nelson, S. Price, A. Renzini, R. Saglia, S. Seitz, Taro Shimizu, A. Sternberg, L. Tacconi, K. Tadaki, H. Übler, P. Dokkum, S. Wuyts
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引用次数: 1
Abstract
Near-infrared spectrographs are powerful tools for investigating galaxy evolution. We on our completed multi-year KMOS 3D survey of a ,
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