activity
20122022
most citedIdentification of the brightest Lyα emitters at z=6.6: implications for the evolution of the luminosity function in the re-ionisation era

173 citations · 1.3k across the 39 of their papers we have counts for

collaborators
Showing 2020Show all

10 papers · 1 filter

astro-ph.GA20208 cited

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…

astro-ph.GA202019 cited

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…

astro-ph.GA202019 cited

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…

astro-ph.GA2020

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…

astro-ph.GA2020

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…

astro-ph.GA202018 cited

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…