173 citations · 1.3k across the 39 of their papers we have counts for
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The First Integral Field Unit Spectroscopic View of Shocked Cluster Galaxies
Andra Stroe, Maryam Hussaini, Bernd Husemann +2
Galaxy clusters grow by merging with other clusters, giving rise to Mpc-wide shock waves that travel at 1000-2500 km/s through the intra-cluster medium. To study the effects of mer…
Dust, gas, and metal content in star-forming galaxies at revealed with ALMA and Near-IR spectroscopy
Tomoko L. Suzuki, Masato Onodera, Tadayuki Kodama +8
We conducted sub-millimeter observations with the Atacama Large Millimeter/sub-millimeter Array (ALMA) of star-forming galaxies at , whose gas-phase metallicities have be…
A kpc-scale resolved study of unobscured and obscured star-formation activity in normal galaxies at z = 1.5 and 2.2 from ALMA and HiZELS
Cheng Cheng, Edo Ibar, Ian Smail +12
We present Atacama Large Millimeter/Submillimeter Array (ALMA) continuum observations of a sample of nine star-forming galaxies at redshifts 1.47 and 2.23 selected from the High-$z…
Tightly coupled morpho-kinematic evolution for massive star-forming and quiescent galaxies across 7 Gyr of cosmic time
Anna de Graaff, Rachel Bezanson, Marijn Franx +11
We use the Fundamental Plane (FP) to measure the redshift evolution of the dynamical mass-to-light ratio () and the dynamical-to-stellar mass ratio ($M_{\mathrm…
Dust Attenuation Curves at z 0.8 from LEGA-C: Precise Constraints on the Slope and 2175 Bump Strength
Ivana Barisic, Camila Pacifici, Arjen van der Wel +11
We present a novel approach to measure the attenuation curves of 485 individual star-forming galaxies with M 10 M based on deep optical spectra from the VL…
The nature of CR7 revealed with MUSE: a young starburst powering extended Lyman- emission at z=6.6
Jorryt Matthee, Gabriele Pezzulli, Ruari Mackenzie +11
CR7 is among the most luminous Lyman- emitters (LAEs) known at and consists of at least three UV components that are surrounded by Lyman- (Ly) emission. Previous…