The KMOS^3D Survey: data release and final survey paper

E. Wisnioski; N. M. Förster Schreiber; M. Fossati; J. T. Mendel; D. Wilman; R. Genzel; R. Bender; S. Wuyts; R. L. Davies; H. Übler; K. Bandara; A. Beifiori; S. Belli; G. Brammer; J. Chan; R. I. Davies; M. Fabricius; A. Galametz; P. Lang; D. Lutz; E. J. Nelson; I. Momcheva; S. Price; D. Rosario; R. Saglia; S. Seitz; T. Shimizu; L. J. Tacconi; K. Tadaki; P. G. van Dokkum; E. Wuyts

doi:10.3847/1538-4357/ab4db8

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arXiv · 1909.11096

The KMOS^3D Survey: data release and final survey paper

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Abstract

We present the completed KMOS$^\mathrm{3D}$ survey $-$ an integral field spectroscopic survey of 739, $\log(M_{\star}/M_{\odot})>9$, galaxies at $0.6 10.5$). We confirm our first year results of a high rotation dominated fraction (monotonic velocity gradient and $v_\mathrm{rot}$/$\sigma_0 > \sqrt{3.36}$) of 77% for the full KMOS$^\mathrm{3D}$ H$\alpha$sample. The rotation-dominated fraction is a function of both stellar mass and redshift with the strongest evolution measured over the redshift range of the survey for galaxies with $\log(M_{\star}/M_{\odot})<10.5$. With this paper we include a final data release of all 739 observed objects.

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E. Wisnioski, N. M. Förster Schreiber, M. Fossati, J. T. Mendel, D. Wilman, R. Genzel, R. Bender, S. Wuyts, R. L. Davies, H. Übler, K. Bandara, A. Beifiori, S. Belli, G. Brammer, J. Chan, R. I. Davies, M. Fabricius, A. Galametz, P. Lang, D. Lutz, E. J. Nelson, I. Momcheva, S. Price, D. Rosario, R. Saglia, S. Seitz, T. Shimizu, L. J. Tacconi, K. Tadaki, P. G. van Dokkum, E. Wuyts. 2019-09-24. The KMOS^3D Survey: data release and final survey paper. https://doi.org/10.3847/1538-4357/ab4db8

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