activity
20182021
most citedKiloparsec-scale ALMA Imaging of [CII] and Dust Continuum Emission of 27 Quasar Host Galaxies at z~6

152 citations · 504 across the 8 of their papers we have counts for

collaborators

13 papers

astro-ph.GA202152 cited

Measurements of the dust properties in z~1-3 SMGs with ALMA

E. da Cunha, J. A. Hodge, C. M. Casey +13

We present Atacama Large Millimetre Array (ALMA) 2mm continuum observations of a complete and unbiased sample of 99 870micron-selected sub-millimeter galaxies (SMGs) in the Extende…

astro-ph.GA2021

The Kinematics of z ~ 6 Quasar Host Galaxies

Marcel Neeleman, Mladen Novak, Bram P. Venemans +9

We explore the kinematics of 27 z~6 quasar host galaxies observed in [CII]-158 micron ([CII]) emission with the Atacama Large Millimeter/sub-millimeter Array at a resolution of ~0.…

astro-ph.GA2020152 cited

Kiloparsec-scale ALMA Imaging of [CII] and Dust Continuum Emission of 27 Quasar Host Galaxies at z~6

Bram Venemans, Fabian Walter, Marcel Neeleman +12

We present a study of the [CII] 158micron line and underlying far-infrared (FIR) continuum emission of 27 quasar host galaxies at z~6, traced by the Atacama Large Millimeter/submil…

astro-ph.GA202075 cited

No evidence for [CII] halos or high-velocity outflows in z>6 quasar host galaxies

Mladen Novak, Bram P. Venemans, Fabian Walter +13

We study the interstellar medium in a sample of 27 high-redshift quasar host galaxies at z>6, using the [CII] 158um emission line and the underlying dust continuum observed at ~1kp…

astro-ph.GA2020

A significant excess in major merger rate for AGNs with the highest Eddington ratios at z<0.2

V. Marian, K. Jahnke, I. Andika +16

Observational studies are increasingly finding evidence against major mergers being the dominant mechanism responsible for triggering AGN. After studying the connection between maj…

astro-ph.IM202043 cited

An astronomical institute's perspective on meeting the challenges of the climate crisis

Knud Jahnke, Christian Fendt, Morgan Fouesneau +10

Analysing greenhouse gas emissions of an astronomical institute is a first step in reducing its environmental impact. Here, we break down the emissions of the Max Planck Institute…