activity
20162022
most citedKiloparsec-scale ALMA Imaging of [CII] and Dust Continuum Emission of 27 Quasar Host Galaxies at z~6

152 citations · 934 across the 20 of their papers we have counts for

collaborators

41 papers

astro-ph.GA20221 cited

Spectroscopy of High Redshift Galaxies with the ngVLA

C. L. Carilli, M. Neeleman

We present simulations of the capabilities of the ngVLA to image at kpc resolution (), molecular line emission from star forming disk galaxies at high redshift.…

astro-ph.GA20227 cited

The Decoupled Kinematics of high-z QSO Host Galaxies and their Lya halos

Alyssa Drake, Marcel Neeleman, Bram P. Venemans +7

We present a comparison of the interstellar medium traced by [CII] (ALMA), and ionised halo gas traced by Lya (MUSE), in and around QSO host galaxies at z~6. To date, 18 QSOs at th…

astro-ph.GA2022

Dense Gas History of the Universe: from ASPECS to the ngVLA

C. L. Carilli, F. Walter, R. Decarli +7

We review the evolution of the cosmic average molecular gas density to large look-back times, using observations of rotational transitions of CO. Molecular gas is the fuel for star…

astro-ph.CO202269 cited

Co-evolution of massive black holes and their host galaxies at high redshift: discrepancies from six cosmological simulations and the key role of JWST

Melanie Habouzit, Masafusa Onoue, Eduardo Banados +7

The James Webb Space Telescope will have the power to characterize high-redshift quasars at z>6 with an unprecedented depth and spatial resolution. While the brightest quasars at s…

astro-ph.GA202256 cited

ALMA 200 pc imaging of a z~7 quasar reveals a compact, disk-like host galaxy

Fabian Walter, Marcel Neeleman, Roberto Decarli +10

We present 0".035 resolution (~200 pc) imaging of the 158 um [CII] line and the underlying dust continuum of the z=6.9 quasar J234833.34-305410.0. The 18 h ALMA observations reveal…

astro-ph.GA202111 cited

A [C II] 158m Emitter Associated with an OI Absorber at the End of the Reionization Epoch

Yunjing Wu, Zheng Cai, Marcel Neeleman +12

The physical and chemical properties of the circumgalactic medium (CGM) at have been studied successfully through the absorption in the spectra of background Quasi-Stel…