152 citations · 1.2k across the 22 of their papers we have counts for
42 papers
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…
Physical constraints on the extended interstellar medium of the z=6.42 quasar J1148+5251: [CII] 158um, [NII] 205um and [OI] 146um observations
Romain A. Meyer, Fabian Walter, Claudia Cicone +7
We report new Northern Extended Millimeter Array (NOEMA) observations of the [CII], [NII] and [OI] atomic fine structure lines and dust continuum emission of J1148+5251, a z=6.42 q…
The Impact of Powerful Jets on the Far-infrared Emission of an Extreme Radio Quasar at z~6
Sofía Rojas-Ruiz, Eduardo Bañados, Marcel Neeleman +9
The interactions between radio jets and the interstellar medium play a defining role for the co-evolution of central supermassive black holes and their host galaxies, but observati…
The XXL Survey: XLIII. The quasar radio loudness dichotomy exposed via radio luminosity functions obtained by combining results from COSMOS and XXL-S X-ray selected quasars
Lana Ceraj, Vernesa Smolčić, Ivan Delvecchio +13
We studied a sample of 274 radio and X-ray selected quasars (XQSOs) detected in the COSMOS and XXL-S radio surveys at 3 GHz and 2.1 GHz, respectively. This sample was identified by…
An ALMA multi-line survey of the ISM in two quasar host-companion galaxy pairs at
A. Pensabene, R. Decarli, E. Bañados +15
We present a multi-line survey of the interstellar medium (ISM) in two quasar (QSO) host galaxies, PJ231-20 () and PJ308-21 (), and their two companion galaxi…
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.…