activity
20042024
most citedA Dust-Obscured Massive Maximum-Starburst Galaxy at a Redshift of 6.34

609 citations · 5.8k across the 89 of their papers we have counts for

collaborators
Showing 2018Show all

25 papers · 1 filter

astro-ph.GA201824 cited

The ISM Properties and Gas Kinematics of a Redshift 3 Massive Dusty Star-forming Galaxy

T. K. Daisy Leung, Dominik A. Riechers, Andrew J. Baker +9

We present CO(J= 1-0; 3-2; 5-4; 10-9) and 1.2-kpc resolution [CII] line observations of the dusty star-forming galaxy (SFG) HXMM05 -- carried out with the Karl G. Jansky Very Large…

astro-ph.GA2018

Low star formation efficiency in typical galaxies at z=5-6

Riccardo Pavesi, Dominik A. Riechers, Andreas L. Faisst +2

Using the VLA and ALMA, we have obtained CO(2-1), [C II], [N II] line emission and multiple dust continuum measurements in a sample of "normal" galaxies at . We report the h…

astro-ph.GA2018

No evidence for enhanced [OIII] 88um emission in a z~6 quasar compared to its companion starbursting galaxy

Fabian Walter, Dominik Riechers, Mladen Novak +14

We present ALMA band 8 observations of the [OIII] 88um line and the underlying thermal infrared continuum emission in the z=6.08 quasar CFHQS J2100-1715 and its dust-obscured starb…

astro-ph.GA2018

Dust emission in an accretion-rate-limited sample of z>6 quasars

Bram Venemans, Roberto Decarli, Fabian Walter +9

We present Atacama Large Millimeter Array 1mm observations of the rest-frame far-infrared (FIR) dust continuum in 27 quasars at redshifts 6.0 < z < 6.7. We detect FIR emission at >…

astro-ph.GA2018

Science with an ngVLA: Imaging Cold Gas to 1 kpc Scales in High-Redshift Galaxies with the ngVLA

Caitlin M. Casey, Desika Narayanan, Chris Carilli +9

The next generation Very Large Array (ngVLA) will revolutionize our understanding of the distant Universe via the detection of cold molecular gas in the first galaxies. Its impact…

astro-ph.GA2018

Science with an ngVLA. Cold gas in High-z Galaxies: The dense ISM

R. Decarli, C. Carilli, C. Casey +7

The goal of this science case is to study physical conditions of the interstellar medium (ISM) in distant galaxies. In particular, its densest component is associated with the inne…