J. T. Mendel

TL;DR: In this article, the authors present the KMOS3D survey, a new integral field survey of over 600 galaxies at 0.7 1, implying that the star-forming main sequence is primarily composed of rotating galaxies at both redshift regimes.

TL;DR: In this paper, the authors present the KMOS^3D survey, a new integral field survey of over 600 galaxies at 0.7 1$, implying that the star-forming "main sequence" (MS) is primarily composed of rotating galaxies at both redshift regimes.

TL;DR: Rotation curves (showing rotation velocity as a function of disk radius) for the outer disks of six massive star-forming galaxies are reported, and find that the rotation velocities are not constant, but decrease with radius, a trend that appears to increase with redshift.

TL;DR: Forster Schreiber et al. as discussed by the authors used a combination of the SINS/zC-SINF, LUCI, GNIRS, and KMOS^3D spectroscopic surveys to detect broad nuclear emission (FWHM) in the Ha, [NII], and [SII] lines.

TL;DR: In this article, the authors follow up on their previous detection of nuclear ionized outflows in the most massive (log(M */M ☉) ≥ 10.9) z ~ 1-3 star-forming galaxies by increasing the sample size by a factor of six.